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                    ETNA.

   [Illustration: View of Etna from Catania]




                   ETNA

       _A HISTORY OF THE MOUNTAIN AND
              OF ITS ERUPTIONS._


                    BY

               G. F. RODWELL,

     SCIENCE MASTER IN MARLBOROUGH COLLEGE.

         WITH MAPS AND ILLUSTRATIONS.

                [Illustration]

                    LONDON

   C. KEGAN PAUL & CO., 1, PATERNOSTER SQUARE

                     1878

[_The rights of translation and of reproduction are reserved._]




          I  DEDICATE  THIS  BOOK

                     TO

                 MY  MOTHER.




PREFACE.


While preparing an account of MOUNT ETNA for the Encyclopaedia
Britannica, I was surprised to find that there exists no single work in
the English language devoted to the history of the most famous volcano
in the world. I was consequently induced to considerably enlarge the
Encyclopaedia article, and the following pages are the result. The facts
recorded have been collected from various sources--German, French,
Italian, and English, and from my own observations made during the
summer of 1877. I desire to express my indebtedness to Mr. Frank Rutley,
of H.M. Geological Survey, for his careful examination of the lavas
which were collected during my ascent of the mountain, and for the
account which he has written of them; also to Mr. John Murray for
permission to copy figures from Lyell's "Principles of Geology." My
thanks are also due to Mr. George Dennis, H.M. Consul-General in Sicily;
Mr. Robert O. Franck, Vice-Consul in Catania; and to Prof. Orazio
Silvestri, for information with which they have severally supplied me.

G. F. RODWELL.

MARLBOROUGH,

_September 6th, 1878._




CONTENTS.


CHAPTER I.

HISTORY OF THE MOUNTAIN.                                         1

    Position.--Name.--Mention of Etna by early writers.--Pindar.--
    AEschylus.--Thucydides.--Virgil.--Strabo.--Lucretius.--Lucilius
    Junior.--Etna the home of early myths.--Cardinal Bembo.--Fazzello.--
    Filoteo.--Early Maps of the Mountain.--Hamilton.--Houel.--Brydone.--
    Ferrara.--Recupero.--Captain Smyth.--Gemellaro; his Map of Etna.--
    Elie de Beaumont.--Abich.--Hoffmann.--Von Waltershausen's _Atlas
    des Aetna_.--Lyell.--Map of the Italian Stato Maggiore.--Carlo
    Gemellaro.--Orazio Silvestri.


CHAPTER II.

PHYSICAL FEATURES OF THE MOUNTAIN.                              26

    Height.--Radius of Vision from the summit.--Boundaries.--Area.--
    Population.--General aspect of Etna.--The Val del Bove.--Minor
    Cones.--Caverns.--Position and extent of the three Regions.--
    Regione Coltivata.--Regione Selvosa.--Regione Deserta.--Botanical
    Regions.--Divisions of Rafinesque-Schmaltz, and of Presl.--Animal
    life in the upper Regions.


CHAPTER III.

ASCENT OF THE MOUNTAIN.                                         43

    The most suitable time for ascending Etna.--The Ascent commenced.--
    Nicolosi.--Etna mules.--Night journey through the upper Regions of
    the mountain.--Brilliancy of the Stars.--Proposed Observatory on
    Etna.--The Casa Inglesi.--Summit of the Great Crater.--Sunrise
    from the summit.--The Crater.--Descent from the Mountain.--
    Effects of Refraction.--Fatigue of the Ascent.


CHAPTER IV.

TOWNS SITUATED ON THE MOUNTAIN.                                 62

    Paterno.--Ste. Maria di Licodia.--The site of the ancient town of
    Aetna.--Biancavilla.--Aderno.--Sicilian Inns.--Adranum.--Bronte.--
    Randazzo.--Mascali.--Giarre.--Aci Reale.--Its position.--The
    Scogli de'Ciclopi.--Catania, its early history, and present
    condition.


CHAPTER V.

ERUPTIONS OF THE MOUNTAIN.                                      79

    Their frequency within the historical period.--525 B.C.--477 B.C.--
    426 B.C.--396 B.C.--140 B.C.--134 B.C.--126 B.C.--122 B.C.--
    49 B.C.--43 B.C.--38 B.C.--32 B.C.--40 A.D.--72.--253.--420.--812.--
    1169.--1181.--1285.--1329.--1333.--1371.--1408.--1444.--1446.--1447.--
    Close of the Fifteenth Century.--1536.--1537.--1566.--1579.--1603.--
    1607.--1610.--1614.--1619.--1633.--1646.--1651.--1669.--1682.--
    1688.--1689.--1693.--1694.--1702.--1723.--1732.--1735.--1744.--1747.--
    1755.--Flood of 1755.--1759.--1763.--1766.--1780.--1781.--1787.--
    1792.--1797.--1798.--1799.--1800.--1802.--1805.--1808.--1809.--1811.--
    1819.--1831.--1832.--1838.--1842.--1843.--1852.--1865.--1874.--
    General character of the Eruptions.


CHAPTER VI.

GEOLOGY AND MINERALOGY OF THE MOUNTAIN.                        114

    Elie de Beaumont's classification of the rocks of Etna.--Hoffman's
    geological map.--Lyell's researches.--The period of earliest
    eruption.--The Val del Bove.--Two craters of eruption.--Antiquity of
    Etna.--The lavas of Etna.--Labradorite.--Augite.--Olivine.--
    Analcime.--Titaniferous iron.--Mr. Rutley's examination of Etna
    lavas under the microscope.




LIST OF ILLUSTRATIONS.


    View of Etna from Catania                _To face Title._
    Topographical Map of Etna                 _To face page_           1
    Sections of Etna                                "                 30
    Grotto delle Palombe                            "                 36
    The Casa Inglesi and Cone of Etna               "                 52
    View of the Val de Bove                         "                 58
    View of Etna from Bronte                        "                 66
    Island of Columnar Basalt off Trezza            "                 74
    Geological Map of Etna                          "                114
    Map of the Val del Bove (woodcut)                                117
    Ideal Section of Mount Etna                                      119
    Profile of Etna                                                  121
    Sections of Etna Lavas seen under the Microscope, _to face p._   138

[Illustration: Topographical Map of Etna]




ETNA.

A HISTORY OF THE MOUNTAIN AND OF ITS ERUPTIONS.




CHAPTER I.

HISTORY OF THE MOUNTAIN.

    Position.--Name.--Mention of Etna by early writers.--Pindar.--
    AEschylus.--Thucydides.--Virgil.--Strabo.--Lucretius.--Lucilius
    Junior.--Etna the home of early myths.--Cardinal Bembo.--Fazzello.--
    Filoteo.--Early Maps of the Mountain.--Hamilton.--Houel.--Brydone.--
    Ferrara.--Recupero.--Captain Smyth.--Gemellaro; his Map of Etna.--
    Elie de Beaumont.--Abich.--Hoffmann.--Von Waltershausen's _Atlas
    des Aetna_.--Lyell.--Map of the Italian Stato Maggiore.--Carlo
    Gemellaro.--Orazio Silvestri.


The principal mountain chain of Sicily skirts the North and a portion of
the North-eastern coast, and would appear to be a prolongation of the
Apennines. An inferior group passes through the centre of the island,
diverging towards the South, as it approaches the East coast. Between
the two ranges, and completely separated from them by the valleys of
the Alcantara and the Simeto, stands the mighty mass of Mount Etna,
which rises in solitary grandeur from the eastern sea-board of the
island. Volcanoes, by the very mode of their formation, are frequently
completely isolated; and, if they are of any magnitude, they thus
acquire an imposing contour and a majesty, which larger mountains,
forming parts of a chain, do not possess. This specially applies to
Etna. "Coelebs degit," says Cardinal Bembo, "et nullius montis dignata
conjugium, caste intra suos terminos continetur." It is not alone the
conspicuous appearance of the mountain which has made it the most famous
volcano either of ancient or modern times:--the number and violence of
its eruptions, the extent of its lava streams, its association with
antiquity, and its history prolonged over more than 2400 years, have all
tended to make it celebrated.

The geographical position of Etna was first accurately determined by
Captain Smyth in 1814. He estimated the latitude of the highest point of
the bifid peak of the great crater at 37 deg. 43' 31" N.; and the longitude
at 15 deg. East of Greenwich. Elie de Beaumont repeated the observations in
1834 with nearly the same result; and these determinations have been
very generally adopted. In the new Italian map recently constructed by
the Stato Maggiore, the latitude of the centre of the crater is stated
to be 37 deg. 44' 55" N., and the longitude 44' 55" E. of the meridian of
Naples, which passes through the Observatory of Capo di Monte.

According to Bochart the name of Etna is derived from the Phoenician
_athana_--a furnace; others derive it from ~aitho~--to burn.
Professor Benfey of Gottingen, a great authority on the subject,
considers that the word was created by one of the early Indo-Germanic
races. He identifies the root _ait_ with the Greek ~aith~ and the
Latin _aed_--to burn, as in _aes_-tu. The Greek name ~Aitna~ was
known to Hesiod. The more modern name, _Mongibello_, by which the
mountain is still commonly known to the Sicilians, is a combination of
the Arabic _Gibel_, and the Italian _Monte_. During the Saracenic
occupation of Sicily, Etna was called _Gibel Uttamat_--the mountain of
fire; and the last syllables of Mongibello are a relic of the Saracenic
name. A mountain near Palermo is still called Gibel Rosso--the red
mountain; and names may not unfrequently be found in the immediate
neighbourhood of Etna which are partly, or sometimes even entirely,
composed of Arabic words; such, for example, as _Alcantara_--the river
of _the bridge_. Etna is also often spoken of distinctively as _Il
Monte_--the mountain _par excellence_; a name which, in its capacity of
the largest mountain in the kingdom of Italy, and the loftiest volcano
in Europe, it fully justifies.

Etna is frequently alluded to by classical writers. By the poets it was
sometimes feigned to be the prison of the giant Enceladus or Typhon,
sometimes the forge of Hephaistos, and the abode of the Cyclops.

It is strange that Homer, who has so minutely described certain portions
of the contiguous Sicilian coast, does not allude to Etna. This has been
thought by some to be a proof that the mountain was in a quiescent state
during the period which preceded and coincided with the time of Homer.

Pindar (B.C. 522-442) is the first writer of antiquity who has described
Etna. In the first of the Pythian Odes for Hieron, of the town of Aitna,
winner in the chariot race in B.C. 474, he exclaims:

... "He (Typhon) is fast bound by a pillar of the sky, even by snowy
Etna, nursing the whole year's length her dazzling snow. Whereout pure
springs of unapproachable fire are vomited from the inmost depths: in
the daytime the lava-streams pour forth a lurid rush of smoke; but in
the darkness a red rolling flame sweepeth rocks with uproar to the wide
deep sea.... That dragon-thing (Typhon) it is that maketh issue from
beneath the terrible fiery flood."[1]

[1] Translated by Ernest Myers, M.A., 1874.

AEschylus (B.C. 525-456) speaks also of the "mighty Typhon,"
(_Prometheus_ V.):

                            . . . . . "He lies
    A helpless, powerless carcase, near the strait
    Of the great sea, fast pressed beneath the roots
    Of ancient Etna, where on highest peak
    Hephaestos sits and smites his iron red hot,
    From whence hereafter streams of fire shall burst,
    Devouring with fierce jaws the golden plains
    Of fruitful, fair Sikelia."[2]

[2] Translated by E. Myers.

Herein he probably refers to the eruption which had occurred a few years
previously (B.C. 476).

Thucydides (B.C. 471-402) alludes in the last lines of the Third Book to
several early eruptions of the mountain in the following terms: "In the
first days of this spring, the stream of fire issued from Etna, as on
former occasions, and destroyed some land of the Catanians, who live
upon Mount Etna, which is the largest mountain in Sicily. Fifty years,
it is said, had elapsed since the last eruption, there having been three
in all since the Hellenes have inhabited Sicily."[3]

[3] Translated by E. Crawley.

Virgil's oft-quoted description of the mountain (_Eneid_, Bk. 3) we give
in the spirited translation of Conington:

    "But Etna with her voice of fear
    In weltering chaos thunders near.
    Now pitchy clouds she belches forth
    Of cinders red, and vapour swarth;
    And from her caverns lifts on high
    Live balls of flame that lick the sky:
    Now with more dire convulsion flings
    Disploded rocks, her heart's rent strings,
    And lava torrents hurls to-day
    A burning gulf of fiery spray."

Many other early writers speak of the mountain, among them Theokritos,
Aristotle, Ovid, Livy, Seneca, Lucretius, Pliny, Lucan, Petronius,
Cornelius Severus, Dion Cassius, Strabo, Diodorus Siculus, and Lucilius
Junior. Seneca makes various allusions to Etna, and mentions the fact
that lightning sometimes proceeded from its smoke.

Strabo has given a very fair description of the mountain. He asserts
that in his time the upper part of it was bare, and covered with ashes,
and in winter with snow, while the lower <DW72>s were clothed with
forests. The summit was a plain about twenty stadia in circumference,
surrounded by a ridge, within which there was a small hillock, the smoke
from which ascended to a considerable height. He further mentions a
second crater. Etna was commonly ascended in Strabo's time from the
south-west.

While the poets on the one hand had invested the mountain with various
supernatural attributes, and had made it the prison-house of a chained
giant, and the workshop of a swart god, Lucretius endeavoured to show
that the eruptions and other phenomena could be easily explained by the
ordinary operations of nature. "And now at last," he writes, "I will
explain in what ways yon flame, roused to fury in a moment, blazes forth
from the huge furnaces of Aetna. And, first, the nature of the whole
mountain is hollow underneath, underpropped throughout with caverns of
basalt rocks. Furthermore, in all caves are wind and air, for wind is
produced when the air has been stirred and put in motion. When this air
has been thoroughly heated, and, raging about, has imparted its heat to
all the rocks around, wherever it comes in contact with them, and to the
earth, and has struck out from them fire burning with swift flames, it
rises up and then forces itself out on high, straight through the
gorges; and so carries its heat far, and scatters far its ashes, and
rolls on smoke of a thick pitchy blackness, and flings out at the same
time stones of prodigious weight--leaving no doubt that this is the
stormy force of air. Again, the sea, to a great extent, breaks its waves
and sucks back its surf at the roots of that mountain. Caverns reach
from this sea as far as the deep gorges of the mountain below. Through
these you must admit [that air mixed up with water passes; and] the
nature of the case compels [this air to enter in from that] open sea,
and pass right within, and then go out in blasts, and so lift up flame,
and throw out stones, and raise clouds of sand; for on the summit are
craters, as they name them in their own language, what we call gorges
and mouths."[4]

[4] _De Natura Rerum_, Book 6, p. 580. Translated by E. Munro 1864.

These ideas were developed by Lucilius Junior in a poem consisting of
644 hexameters entitled _Aetna_. The authorship of this poem has long
been a disputed point; it has been attributed to Virgil, Claudian,
Quintilius Varus, Manilius, and, by Joseph Scaliger[5] and others, to
Cornelius Severus. Wensdorff was the first to adduce reasons for
attributing the poem to Lucilius Junior, and his views are generally
adopted. Lucilius Junior was Procurator of Sicily under Nero, and, while
resident in the Island, he ascended Etna; and it is said that he
proposed writing a detailed history of the mountain. He adopted the
scientific opinions of Epicurus, as established in Rome by Lucretius,
and was more immediately a disciple of Seneca. The latter dedicated to
him his _Quaestiones Naturales_, in which he alludes more than once to
Etna. M. Chenu speaks of the poem of Lucilius Junior as "sans doute
tres-poetique, mais assez souvent dur, heurte, concis, et parcela meme,
d'une obscurite parfois desesperante."[6] At the commencement of the
poem, Lucilius ridicules the ideas of the poets as regards the
connection of Etna with Vulcan and the Cyclops. He has no belief in the
practice, which apparently prevailed in his time, of ascending to the
edge of the crater and there offering incense to the tutelary gods of
the mountain. He adopts to a great extent the tone and style of
Lucretius, in his explanation of the phenomena of the mountain. Water
filters through the crevices and cracks in the rocks, until it comes
into contact with the internal fires, when it is converted into vapour
and expelled with violence. The internal fires are nourished by the
winds which penetrate into the mountain. He traces some curious
connection between the plants which grow upon the mountain, and the
supply of sulphur and bitumen to the interior, which is, at best, but
partly intelligible.

[5] See Lucilius Junioris AETNA. Recensuit notasque Jos. Scaligeri,
Frid. Lindenbruchii et suas addidit Fridericus Jacob. Lipsiae, 1826.

[6] L'Etna de Lucilius Junior. Traduction nouvelle par Jules Chenu.
Paris, 1843.

    "Nunc superant, quacunque regant incendia silvae
    Quae flammis alimenta vacent, quid nutriat Aetnam.
    Incendi patiens illis vernacula caulis
    Materia, appositumque igni genus utile terrae est,
    Uritur assidue calidus nunc sulfuris humor,
    Nunc spissus crebro praebetur flumine succus,
    Pingue bitumen adest, et quidquid cominus acres
    Irritat flammas; illius corporis AEtna est.
    Atque hanc materiam penitus discurrere fontes
    Infectae erumpunt et aquae radice sub ipsa."

Many of the myths developed by the earlier poets had their home in the
immediate neighbourhood, sometimes upon the very sides, of Etna--Demeter
seeking Persephone; Acis and Galatea; Polyphemus and the Cyclops. Mr.
Symonds tells us that the one-eyed giant Polyphemus was Etna itself,
with its one great crater, while the Cyclops were the many minor cones.
"Persephone was the patroness of Sicily, because amid the billowy
corn-fields of her mother Demeter, and the meadow-flowers she loved in
girlhood, are ever found sulphurous ravines, and chasms breathing vapour
from the pit of Hades."[7]

[7] Sketches in Italy and Greece, p. 201.

It is said that both Plato and the Emperor Hadrian ascended Etna in
order to witness the sunrise from its summit. The story of

            "He who to be deemed
    A god, leaped fondly into Etna flames,
    Empedokles"

is too trite to need repetition. A ruined tower near the head of the Val
del Bove, 9,570 feet above the sea, has from time immemorial been called
the _Torre del Filosofo_, and is asserted to have been the observatory
of Empedokles. Others regard it as the remains of a Roman tower, which
was possibly erected on the occasion of Hadrian's ascent of the
mountain.

During the Middle Ages Etna is frequently alluded to, among others by
Dante, Petrarch, Boccaccio, and Cardinal Bembo. The latter gives a
description of the mountain in the form of a dialogue, which Ferrara
characterises as "_erudito, e grecizzante, ma sensa nervi_." He
describes its general appearance, its well-wooded sides, and sterile
summit. When he visited the mountain it had two craters about a stone's
throw apart; the larger of the two was said to be about three miles in
circumference, and it stood somewhat above the other.[8]

[8] Petri Bembi DE AETNA. Ad Angelum Chabrielem Liber Impressum Venetiis
Aedibus Aldi Romani. Mense Februario anno M.V.D. (1495).

In 1541 Fazzello made an ascent of the mountain, which he briefly
describes in the fourth chapter of his bulky volume _De Rebus
Siculis_.[9] This chapter is entitled "_De Aetna monte et ejus
ignibus_;" it contains a short history of the mountain, and some mention
of the principal towns which he enumerates in the following order:
Catana, Tauromenium, Caltabianco, Linguagrossa, Castroleone,
Francavilla, Rocella, Randatio (Randazzo), Bronte, Adrano, Paterno, and
Motta. Fazzello speaks of only one crater.

[9] Fazzellus T. DE REBUS SICULIS. Panormi, 1558; folio.

In 1591 Antonio Filoteo, who was born on Etna, published a work in
Venice in which he describes the general features of the mountain, and
gives a special account of an eruption which he witnessed in 1536.[10]
The mountain was then, as now, divided into three _Regions_. The first
and uppermost of these, he asserts, is very arid, rugged, and uneven,
and full of broken rocks; the second is covered with forests; and the
third is cultivated in the ordinary manner. Of the height he remarks,
"Ascensum triginta circiter millia passuum ad plus habet." In regard to
the name, _Mongibello_, he makes a curious error, deriving it from
_Mulciber_, one of the names of Vulcan, who, as we have seen, was
feigned by the earlier poets to have had his forge within the mountain.

[10] Antonii Philothei de Homodeis Siculi, AETNAE TOPOGRAPHIA,
incendiorum Aetnaeorum Historia. Venetiis. 1591. Preface dated September,
1590.

In 1636 Carrera gave an account of Etna, followed by that of the Jesuit
Kircher, in 1638. The great eruption of 1669 was described at length by
various eye-witnesses, and furnished the subject of the first detailed
description of the eruptive phenomena of the mountain. Public attention
was now very generally drawn to the subject in all civilised countries.
It was described by the naturalist, Borelli, and in our own
_Philosophical Transactions_. Lord Winchelsea, our ambassador at
Constantinople, was returning to England by way of the Straits of
Messina at the time of the eruption, and he forwarded to Charles II "A
true and exact relation of the late prodigious earthquake and eruption
of Mount AEtna, or Monte Gibello."

The first map of the mountain which we have been able to meet with,
was published in reference to the eruption of 1669; it is entitled,
"Plan du Mont Etna communenent dit Mount Gibel en l'Isle de Scicille
et de t'incedie arrive par un treblement de terre le 8me Mars dernier
1669." This plan is in the Bibliotheque Nationale, in Paris; it was
probably drawn from a simple description, or perhaps altogether from
the imagination, as it is utterly unlike the mountain, the sides of
which possess an impossible steepness. Another very inaccurate map was
published in Nuremberg about 1680, annexed to a map of Sicily, which
is entitled, "_Regnorum Siciliae et Sardiniae, Nova Tabula_." Again, in
1714 H. Moll, "geographer in Devereux Street, Strand," published a new
map of Italy, in which there is a representation of Etna during the
eruption of 1669. This also was probably drawn from the imagination;
no one who has ever seen the mountain would recognise it, for it has
a small base, and sides which rival the Matterhorn in abruptness.
Over against the coast of Sicily, and near the mountain, is
written:--"Mount Etna, or Mount Gibello. This mountain sometimes
issues out pure flame, and at other times a thick smoak with ashes;
streams of fire run down with great quantities of burning stones, and
has made many eruptions."

During the eighteenth century Etna was frequently ascended, and as
frequently described. We have the accounts of Massa (1703), Count
D'Orville (1727), Riedesel (1767), Sir William Hamilton (1769), Brydone
(1776), Houel (1786), Dolomieu (1788), Spallanzani (1790), and many
minor writers, such as Borch, Brocchi, Swinburne, Denon, and Faujas de
Saint Fond. There is great sameness in all of these narratives, and much
repetition of the same facts; some of them, however, merit a passing
notice.

Sir William Hamilton's _Campi Phlegraei_ relates mainly to Vesuvius and
the surrounding neighbourhood; but one of the letters "addressed to the
Secretary of the Royal Society on October 17th, 1769," describes an
ascent of Etna. Hamilton ascended on June 24th with the Canon Recupero
and other companions; the few observations of any value which he made
have been alluded to elsewhere under the head of the special subjects to
which they refer. The illustrations of the _Campi Phlegraei_, specially
the original water-colours which are contained in one of the British
Museum copies, are magnificent, and convey a better idea of volcanic
phenomena than any amount of simple reading. From them we can well
realise the opening of a long rift extending down the sides of a
mountain during its eruption, and the formation of subsidiary craters
along the line of fire thus opened. Various volcanic products are also
admirably painted. In the picture of Etna, however, which was drawn by
Antonio Fabris, the artist has scarcely been more successful than his
predecessors, and the <DW72> of the sides of the mountain has been
greatly exaggerated.

M. Houel, in his _Voyage pittoresque dans les Deux Siciles_, 1781-1786,
has given a fairly good account of Etna, accompanied by some really
excellent engravings.

In 1776 Patrick Brydone, a clever Irishman with a good deal of native
shrewdness and humour, published two volumes of a _Tour in Sicily and
Malta_, in which he devoted several chapters to Mount Etna. He made the
ascent of the mountain, and collected from the Canon Recupero, and from
others, many facts concerning its then present, and its past history. He
also made observations as to the height, temperature of the air at
various elevations, brightness of the stars, and so on. Sir William
Hamilton calls Brydone "a very ingenious and accurate observer," and
adds that he was well acquainted with Alpine measurements. M. Elie de
Beaumont, writing in 1836, speaks of him as _le celebre Brydone_; while,
on the other hand, the Abbe Spallanzani, displeased at certain remarks
which he made concerning Roman Catholicism in Sicily, never fails to
deprecate his work, and deplores "his trivial and insipid pleasantries."
Albeit Brydone's chapters on Etna furnished a more complete account of
the volcano than any which had appeared in English up to that time; his
remarks are frequently very sound and just, and we shall have occasion
more than once to quote him.

It was reserved, however, for the Abate Francesco Ferrara, Professor of
Physical Science in the University of Catania, to furnish the first
history of Etna and of its eruptions, which had any just claim to
completeness. It is entitled, _Descrizione dell' Etna, con la Storia
delle Eruzioni e il Catalogo del prodotti_. The first edition appeared
in 1793, and a second was printed in Palermo in 1818. The author had an
enthusiastic love for his subject:--"Nato sopra l'Etna," he writes, "che
io conobbi ben presto palmo a palmo la mia passione per lo studio fisso
la mia attenzione sul bello, e terribile fenomeno che avea avanti agli
occhi." The work commences with a general description of the
mountain--its height, the temperature of the different regions, the view
from the summit, the mass, the water-springs, the vegetable and animal
life, and the internal fires. This extends over sixty-nine octavo pages.
The second part of the book--eighty pages--gives a history of the
eruptions from the earliest times to the year 1811; the third
part--sixty-seven pages--treats of the nature of the volcanic products;
and the fourth part--thirty-four pages--discusses certain geological and
physical considerations concerning the mountain. At the end there are a
few badly drawn and engraved woodcuts, and a map which, although the
trend of the coast-line is quite wrong, is otherwise fairly good. The
engravings represent the mountain as seen from Catania; the Isole dei
Ciclopi, and the neighbouring coast; the Montagna della Motta; and a
view from Catania of the eruption of 1787. This work has evidently to a
great extent been a labour of love; it is full of personal observations,
and also embodies the results of many other observers. It has furnished
the foundation of much that has since been written concerning Etna.

The Canon Recupero has been alluded to above; he accompanied Hamilton,
Brydone, and others to the summit of the mountain, and he was employed
by the Government to report on the flood which, in 1755, descended with
extraordinary violence through the Val del Bove. Beyond this, Recupero
does not appear to have published anything concerning Etna, although it
was well known that he had plenty of materials. He died in 1778, and it
was not till the year 1815 that his results were published under the
title of _Storia Naturale et Generale dell' Etna, del Canonico Giuseppe
Recupero.--Opera Postuma_. This work consists of two bulky quarto
volumes, the first of which is devoted to a general description of the
mountain, the second to a history of the eruptions, and an account of
the products of eruptions. Some idea may be formed of the extreme
prolixity of the author if we mention that two chapters, together
containing twelve quarto pages, are devoted to the discussion of the
height of Etna, while the first volume is terminated by sixty-three
closely printed pages of annotations. A few rough woodcuts accompany the
volumes; a view of the mountain which, as usual, is out of all reason
as regards abruptness of ascent, and a _carta oryctographia di
Mongibello_ in which the trend of the coast-line between Catania and
Taormina is altogether inexact, complete the illustrations of this most
detailed of histories.

During the years 1814-1816 Captain Smyth, acting under orders from the
Admiralty, made a survey of the coast of Sicily, and of the adjacent
islands. At this time the Mediterranean charts were very defective; some
places on the coast of Sicily were mapped as much as twenty miles out of
their true position, and even the exact positions of the observatories
at Naples, Palermo, and Malta were not known. Among other results, Smyth
carefully determined the latitude and longitude of Etna, accurately
measured its height, and examined the surroundings of the mountain. His
results were published in 1824, and are often regarded as the most
accurate that we possess.

In 1824 Dr. Joseph Gemellaro, who lived all his life on the mountain,
and made it his constant study, published an "Historical and
Topographical Map of the Eruptions of Etna from the era of the Sicani to
the year 1824." In it he delineates the extent of the three Regions,
_Coltivata_, _Selvosa_, and _Deserta_; he places the minor cones, to the
number of seventy-four, in their proper places, and he traces the course
of the various lava-streams which have flowed from them and from the
great crater. This map is the result of much patient labour and study,
and it is a great improvement upon those of Ferrara and Recupero, but of
course it is impossible for one man to survey with much accuracy an area
of nearly 500 square miles, and to trace the tortuous course of a large
number of lava-streams. Hence we must be prepared for inaccuracies, and
they are not uncommon--the coast line is altogether wrong as to its
bearings, some of the small towns on the sides of the mountain are
misplaced, and but little attention has been paid to scale. Still the
map is very useful, as it is the only one which shows the course of the
lava-streams.

Mario Gemellaro, brother of the preceding, made almost daily
observations of the condition of Etna, between the years 1803 and 1832.
These results were tabulated, and they are given in the _Vulcanologia
dell' Etna_ of his brother, Professor Carlo Gemellaro, under the title of
_Registro di Osservazioni del Sigr. Mario Gemellaro_.

Carlo Gemellaro contributed many memoirs on subjects connected with the
mountain. They are chiefly to be found in the _Atti dell' Accademia
Gioenia_ of Catania, and they extend over a number of years. Perhaps the
most important is the treatise entitled "_La Vulcanologia dell' Etna che
comprende la Topographia, la Geologia, la Storia, delle sue Eruzioni_."
It was published in Catania in 1858, and is dedicated to Sir Charles
Lyell, who ascended the mountain under the guidance of the author. The
latter also published a _Breve Raggualio della Eruzione dell' Etna, del
21 Agosto 1852_, which contains the most authentic account of this
important eruption, accompanied by some graphic sketches made on the
spot. The last contribution of Carlo Gemellaro to the history of Etna,
is fitly entitled _Un Addio al Maggior Vulcano di Europa_. It was
published in 1866, and with pardonable vanity the author reviews his
work in connection with the mountain, extending over a period of more
than forty years. He commences his somewhat florid farewell with the
following apostrophe:--"O Etna! splendida e perenne manifestazione della
esistenza dei Fuochi sotteranei massimo fra quanti altri monti, dalle
coste meridionali di Europa, dalle orientali dell' Asia e delle
settentrionali dell' Africa si specchiano nel Mediterraneo: tremendo pei
tuoi incendii: benigno per la fertilita del vulcanico tuo terreno
ridotto a prospera coltivazione ... io, nato appie del vasto tuo cono,
in quella Citta che hai minacciato piu d'una volta di sepellire sotto le
tue infocate correnti: allogato, nella mia prima eta, in una stanza
della casa paterna, che signoreggiava in allora piu basse abizioni
vicine, ed intiera godeva la veduta della estesa parte meridionale della
tua mole, io non potera non averti di continuo sotto gli occhi, e non
essere spettatore dei tuoi visibili fenomeni!"

In 1834, M. Elie de Beaumont commenced a minute geological examination
of the mountain. His results were published in 1838, under the title of
_Recherches sur la structure et sur l'origine du Mont Etna_, and they
extend over 225 pages.[11] He re-determined the latitude and longitude
of the mountain, measured the <DW72> of the cone, and the diameter of the
great crater, and minutely examined the structure of the rocks at the
base of the mountain. He also gives a good sectional view, elevations
taken from each quarter of the compass, and a geological map, which
although accurate in its general details, can scarcely be considered
very satisfactory. A relief map of Etna, a copy of which is in the Royal
School of Mines, was afterwards constructed from the flat map, and this
was, we believe, at the same time, the first geological map, and the
first map in relief, which had been made of the mountain. Elie de
Beaumont considers granite as the basis of the mountain, because it is
sometimes ejected from the crater; old basaltic rocks appear in the
Isole dei Ciclopi, and near Paterno, Licodia, and Aderno; _cailloux
roules_ near Motta; ancient lavas on each side of the Val del Bove;
modern lavas in every part of the mountain, and calcareous and
arenaceous rocks in the surrounding mountains.

[11] Printed in vol. IV. of _Memoires pour servir a une description
Geologique de la France_. Par M.M. Dufrenoy et Elie de Beaumont.

In 1836, Abich published some excellent sections of Etna, and an
accurate view of the interior of the crater, in a work entitled _Vues
illustratives de quelques Phenomenes Geologiques prises sur le Vesuve et
l'Etna pendant les annees 1833 and 1834_.

The whole of the thirteenth volume (1839) of the Berlin _Archiv fuer
Mineralogie, Geognosie, Berghau und Huettenkunde_, is occupied by an
elaborate memoir on the geology of Sicily[12] by Friedrich Hoffmann,
accompanied by an excellent geological map. A long account of the
geology of Etna is given, and an enlarged map of the mountain was
afterwards constructed and published in the _Vulkanen Atlas_ of Dr.
Leonhard in 1850.[13]

[12] Entitled _Geognostiche Beobachtungen Gesammelt auf einer Reise
durch Italian und Sicilien, in den jahren 1830 bis 1832, von Friedrich
Hoffmann_.

[13] _Vulkanen Atlas zur naturgeschichte der Erde von K. G. Von
Leonhard._ Stuttgardt. 1850.

In 1836 Baron Sartorius Von Waltershausen commenced a minute survey of
Etna, preparatory to a complete description of the mountain, both
geological and otherwise. He was assisted by Professor Cavallari of
Palermo, Professor Peters of Hensbourg, and Professor Roos of Mayence.
The survey occupied six years, (1836-1842), and the results of direct
observation in the form of maps and drawings, occupied a hundred sheets
160 millimetres (6-1/4 inches) long, by 133 m.m. (5-1/4 inches) broad.
Twenty-nine separate points were made use of in the triangulation; and
the scale chosen was 1 in 50,000. The results were published in a large
folio atlas, which appeared in eight parts; the first in 1845 and the
last in 1861, when the death of Von Waltershausen put an end to the
further publication. There are 26 fine  maps, and 31 engravings.
The cost of the atlas is L12. The maps are both geological and
topographical, and they are accompanied by outline engravings of various
details of special interest. The _Atlas des Aetna_ furnishes the most
exhaustive history of any one mountain on the face of the earth, and
Sartorius Von Waltershausen will always be the principal authority on
the subject of Etna.

Sir Charles Lyell visited Etna in 1824, 1857, and again in 1858. He
embodied his researches in a paper presented to the Royal Society in
1859, and in a lengthy chapter in the _Principles of Geology_. His
investigations have added much to our knowledge of the formation and
geological characteristics of the mountain, especially of that part of
it called the Val del Bove.

Later writers usually quote Von Waltershausen and Lyell, and do not add
much original matter. The facts of all subsequent writers are taken more
or less directly from these authors. The latest addition to the
literature of the mountain, is the _Wanderungen am Aetna_ of Dr.
Baltzer, in the journal of the Swiss Alpine Club for 1874.[14]

[14] Jahrbuch des Schweizer Alpen Club. Neunter Jahrgang, 1873-1874.
Bern 1874.

A fine map of Sicily, on the unusually large scale of 1 in 50,000, or
1.266 inch to a mile, was constructed by the Stato Maggiore of the
Italian government, between 1864 and 1868. The portion relating to Etna,
and its immediate surroundings occupies four sheets. All the small roads
and rivulets are introduced; the minor cones and monticules are placed
in their proper positions, and the elevation of the ground is given at
short intervals of space over the entire map. An examination of this map
shows us that distances, areas, and heights, have been repeatedly
misstated, the minor cones misplaced, and the trend of the coast line
misrepresented. For example, if we draw a line due north and south
through Catania, and a second line from the Capo di Taormina, (the
north-eastern limit of the base of Etna), until it meets the first line
at Catania, the lines, will be found to enclose an angle of 26 deg.. If we
adopt the same plan with Gemellaro's map, the included angle is found to
be 53 deg., and in the case of the maps of Ferrara and Recupero more than
60 deg.. Again, it has been stated on good authority, that the lava of 396
B.C. which enters the sea at Capo di Schiso flowed for a distance of
nearly 30 miles; the map shows us that its true course was less than 16
miles. Lyell in 1858 gives a section of the mountain from West 20 deg. N.,
to East 20 deg. S., but a comparison with the new map proves that the
section is really taken from West 35 deg. N. to East 35 deg. S., an error which
at a radius of ten miles from the crater would amount to a difference of
nearly three miles.

The mantle of Carlo Gemellaro appears to have fallen upon Cav. Orazio
Silvestri, Professor of Chemistry in the University of Catania. He has
devoted himself with unwearying vigour to the study of the mountain, and
his memoirs have done much to elucidate its past and present history.
His most recent work of importance on the subject is entitled _I
Fenomeni Vulcanici presentati dall'Etna nel 1863-64-65-66_. It was
published in Catania in 1867, and contains an account of some very
elaborate chemico-geological researches.




CHAPTER II.

PHYSICAL FEATURES OF THE MOUNTAIN.

    Height.--Radius of Vision from the summit.--Boundaries.--Area.--
    Population.--General aspect of Etna.--The Val del Bove.--Minor
    Cones.--Caverns.--Position and extent of the three Regions.--Regione
    Coltivata.--Regione Selvosa.--Regione Deserta.--Botanical Regions.--
    Divisions of Rafinesque-Schmaltz, and of Presl.--Animal life in the
    upper Regions.


In the preceding chapter we have discussed the history of Mount Etna;
the references to its phenomena afforded by writers of various periods;
and the present state of the literature of the subject. We have now to
consider the general aspect and physical features of the mountain,
together with the divisions of its surface into distinct regions.

The height of Etna has been often determined. The earlier writers had
very extravagant notions on the subject, and three miles has sometimes
been assigned to it. Brydone, Saussure, Shuckburgh, Irvine, and others,
obtained approximations to the real height; it must be borne in mind,
however, that the cone of a volcano is liable to variations in height at
different periods, and a diminution of as much as 300 feet occurred
during one of the eruptions of Etna, owing to the falling in of the
upper portion of the crater. During the last sixty years, however, the
height of the mountain has been practically constant. In 1815 Captain
Smyth determined it to be 10,874 feet. In 1824 Sir John Herschel, who
was unacquainted with Smyth's results, estimated it at 10,872-1/2 feet.
The new map of the Stato Maggiore gives 3312.61 metres = 10867.94 feet.

When the Canon Recupero devoted two chapters of his quarto volume to a
discussion of the height of Etna, no such exact observations had been
made, consequently he compared, and critically examined, the various
determinations which then existed. The almost perfect concordance of the
results given by Smyth, Herschel, and the Stato Maggiore, render it
unnecessary for us to further discuss a subject about which there can
now be no difference of opinion.

Professor Jukes says, "If we were to put Snowdon, the highest mountain
in Wales, on the top of Ben Nevis, the highest in Scotland, and
Carrantuohill, the highest in Ireland, on the summit of both, we should
make a mountain but a very little higher than Etna, and we should
require to heap up a great number of other mountains round the flanks of
our new one in order to build a gentle sloping pile which should equal
Etna in bulk."

The extent of radius of vision from the summit of Etna is very variously
stated. The exaggerated notions of the earlier writers, that the coast
of Africa and of Greece are sometimes visible, may be at once set aside.
Lord Ormonde's statement that he saw the Gulf of Taranta, and the
mountains of Terra di Lecce beyond it--a distance of 245 miles--must be
received with caution. It is, however, a fact that Malta, 130 miles
distant, is often visible; and Captain Smyth asserts that a considerable
portion of the upper part of the mountain may sometimes be seen, and
that he once saw more than half of it, from Malta, although that island
is usually surrounded by a sea-horizon. It is stated on good authority
that Monte S. Giuliano above Trapani, and the OEgadean Isles, 160 miles
distant, are sometimes seen. Other writers give 128 miles as the limit.
The fact is, that atmospheric refraction varies so much with different
conditions of the atmosphere that it is almost impossible to give any
exact statement. The more so when we remember that there may be many
layers of atmosphere of different density between the observer and the
horizon. Distant objects seem to be just under one's feet when seen from
the summit of the mountain. Smyth gives the radius of vision as 150.7
miles: and this we are inclined to adopt as the nearest approach to the
truth, because Smyth was an accurate observer, and he made careful
corrections both for error of instruments and for refraction. This
radius gives an horizon of 946.4 miles of circumference, and an
included area of 39,900 square miles--larger than the area of Ireland.
If a circle be traced with the crater of Etna as a centre, and a radius
of 150.7 miles, it will be found to take in the whole of Sicily and
Malta, to cut the western coast of Italy at Scalca in Calabria, leaving
the south-east coast near Cape Rizzuto. Such a circle will include the
whole of Ireland, or if we take Derby as the centre, its circumference
will touch the sea beyond Yarmouth on the East, the Isle of Wight on the
South, the Irish Channel on the West, and it will pass beyond Carlisle
and Newcastle-on-Tyne on the North.

The road which surrounds the mountain is carried along its lower <DW72>s,
and is 87 miles in length. It passes through the towns of Paterno,
Aderno, Bronte, Randazzo, Linguaglossa, Giarre, and Aci Reale. It is
considered by some writers to define the base of the mountain, which is
hence most erroneously said to have a circumference of 87 miles; but the
road frequently passes over high beds of lava, and winds considerably.
It is about 10 miles from the crater on the North, East, and West sides,
increasing to 15-1/2 miles at Paterno, (S.W.). The elevation on the North
and West flanks of the mountain is nearly 2,500 feet, while on the South
it falls to 1,500 feet, and on the East to within 50 feet of the level
of the sea. It is quite clear that it cannot be asserted with any
degree of accuracy to define the base of the mountain.

[Illustration: Sections of Etna]

The "natural boundaries" of Etna are the rivers Alcantara and Simeto on
the North, West, and South, and the sea on the East to the extent of 23
miles of coast, along which lava streams have been traced, sometimes
forming headlands several hundred feet in height. The base of the
mountain, as defined by these natural boundaries, is said to have a
circumference of "at least 120 miles," an examination of the new map,
however, proves that this is over-estimated.

If we take the sea as the eastern boundary, the river Alcantara,
(immediately beyond which Monte di Mojo, the most northerly minor cone
of Etna is situated), as the northern boundary, and the river Simeto as
the boundary on the west and south, we obtain a circumference of 91
miles for the base of Etna. In this estimate the small sinuosities of
the river have been neglected, and the southern circuit has been
completed by drawing a line from near Paterno to Catania, because the
Simeto runs for the last few miles of its course through the plain of
Catania, quite beyond the most southerly stream of lava. The Simeto
(anciently _Simaethus_) is called the Giaretta along the last three miles
of its course, after its junction with the Gurna Longa.

The area of the region enclosed by these boundaries is approximately 480
square miles. Reclus gives the area of the mountain as 1,200 square
kilometres--461 square miles. (_Nouvelle Geographie Universelle_, 1875.)
The last edition of a standard Gazetteer states it as "849 square
miles;" but this estimate is altogether absurd. This would require a
circle having a radius of between sixteen and seventeen miles. If a
circle be drawn with a radius of sixteen miles from the crater, it will
pass out to sea to a distance of 4-1/2 miles on the East, while on the
West and North it will pass through limestone and sandstone formations
far beyond the Alcantara and the Simeto, and beyond the limit of the
lava streams.

There are two cities, Catania and Aci Reale, and sixty-two towns or
villages on Mount Etna. It is far more thickly populated than any other
part of Sicily or Italy, for while the population of the former is 228
per square mile, and of the latter 233, the population of the habitable
zone of Etna amounts to 1,424 per square mile. More than 300,000 persons
live on the <DW72>s of the mountain. Thus with an area rather larger than
that of Bedfordshire (462 square miles) the mountain has more than
double the population; and with an area equal to about one-third that of
Wiltshire, the population of the mountain is greater by nearly 50,000
inhabitants. We have stated above that the area of Etna is 480 square
miles, but it must be borne in mind that the habitable zone only
commences at a distance of about 9-1/4 miles from the crater. A circle,
having a radius of 9-1/4 miles, encloses an area of 269 square miles;
and 480 minus 269 leaves 211 square miles as the approximate area of the
habitable zone. Only a few insignificant villages on the East side are
nearer to the crater than 9-1/4 miles. Taking the inhabitants as
300,000, we find, by dividing this number by 211, (the area of the
habitable zone), that the population amounts to 1,424 per square mile.
Even Lancashire, the most populous county in Great Britain, (of course
excepting Middlesex), and the possessor of two cities, which alone
furnish more than a million inhabitants, has a population of only 1,479
to the square mile.

Some idea of the closeness of the towns and villages may be found by
examining the south-east corner of the map. If we draw a line from Aci
Reale to Nicolosi, and from Nicolosi to Catania, we enclose a nearly
equilateral triangle, having the coast line between Aci Reale and
Catania as its third side.

Starting from Aci Reale with 24,151 inhabitants, and moving westwards to
Nicolosi, we come in succession to Aci S. Lucia, Aci Catena, Aci S.
Antonio, Via Grande, Tre Castagni, Pedara, Nicolosi, completing the
first side of the triangle; then turning to the south-east and following
the Catania road, we pass Torre di Grifo, Mascalucia, Gravina, and reach
Catania with 85,055 inhabitants; while on the line of coast between
Catania and Aci Reale we have Ognina, Aci Castello, and Trezza. Within
the triangle we find Aci Patane, Aci S. Filippo, Valverde, Bonacorsi, S.
Gregorio, Tremestieri, Piano, S. Agata, Trappeto, and S. Giovanni la
Punta: in all twenty-five, two of which are cities, several of the
others towns of about 3,000 inhabitants, and the rest villages. These
are all included within an area of less than thirty square miles, which
constitutes the most populous portion of the habitable zone of Etna.

That the population is rapidly increasing is well shown by a comparison
of the number of inhabitants of some of the more important towns in 1824
and in 1876.[15]

                     _1824_  _1876_

    Catania          45,081  85,055
    Aci Reale        14,094  24,151
    Giarre           13,705  17,965
    Paterno           9,808  16,512
    Aderno            6,623  15,657
    Bronte            9,153  15,081
    Biancavilla       5,870  13,261
    Linguaglossa      2,415   9,120
    Randazzo          4,700   8,378
    Piedimonte Etnea  1,404   4,924
    Zaffarana Etnea     700   3,884
    Pedara            2,068   3,181
    Trecastagni       2,406   3,061

[15] I am indebted for these figures to Mr. George Dennis, H.M. Consul
General for Sicily.

The general aspect of Etna is that of a pretty regular cone, covered
with vegetation, except near the summit. The regularity is broken on the
East side by a slightly oval valley, four or five miles in diameter,
called the _Val del Bove_, or in the language of the district Val del
_Bue_. This commences about two miles from the summit, and is bounded on
three sides by nearly vertical precipices from 3,000 to 4,000 feet in
height. The bottom of the valley is covered with lavas of various date,
and several minor craters have from time to time been upraised from it.
Many eruptions have commenced in the immediate neighbourhood of the Val
del Bove, and Lyell believes that there formerly existed a centre of
permanent eruption in the valley. The Val del Bove is altogether
sterile; but the mountain at the same level is, on other sides, clothed
with trees. The vast mass of the mountain is realised by the fact that,
after twelve miles of the ascent from Catania, the summit looks as far
off as it did at starting. Moreover, Mount Vesuvius might be almost
hidden away in the Val del Bove.

A remarkable feature of Etna is the large number of minor craters which
are scattered over its sides. They look small in comparison with the
great mass of the mountain, but in reality some of them are of large
dimensions. Monte Minardo, near Bronte, the largest of these minor
cones, is still 750 feet high, although its base has been raised by
modern lava-streams which have flowed around it. There are 80 of the
more conspicuous of these minor cones, but Von Waltershausen has mapped
no less than 200 within a ten mile radius from the great crater, while
neglecting many monticules of ashes. As to the statement made by Reclus
to the effect that there are 700 minor cones, and by Jukes, that the
number is 600, it is to be supposed that they include not only the most
insignificant monticules and heaps of cinders, but also the _bocche_ and
_boccarelle_ from which at any time lava or fire has issued. If these be
included, no doubt these numbers are not exaggerations.

[Illustration: Grotto delle Palombe]

The only important minor cone which has been produced during the
historical period, is the double mountain known as Monti Rossi, from the
red colour of the cinders which compose it. This was raised from the
plain of Nicolosi during the eruption of 1669; it is 450 feet in height,
and two miles in circumference at the base. In a line between the Monti
Rossi and the great crater, thirty-three minor cones may be counted.
Hamilton counted forty-four, looking down from the summit towards
Catania, and Captain Smyth was able to discern fifty at once from an
elevated position on the mountain. Many of these parasitic cones are
covered with vegetation, as the names Monte Faggi, Monte Ilice, Monte
Zappini, indicate. The names have not been happily chosen; thus there
are several cones in different parts of the mountain called by the same
name--Monte Arso, Monte Nero, Monte Rosso, Monte Frumento, are the most
common of the duplicates. Moreover, the names have from time to time
been altered, and it thus sometimes becomes difficult to trace a cone
which has been alluded to under a former name, or by an author who wrote
before the name was changed. In addition to the minor cones from which
lava once proceeded, there are numerous smaller vents for the
subterranean fires called _Bocche_, or if very small, _Boccarelle_, _del
Fuoco_. In the eruption of 1669, thirteen mouths opened in the course of
a few days; and in the eruption of 1809, twenty new mouths opened one
after the other in a line about six miles long. Two new craters were
formed in the Val del Bove in 1852, and seven craters in 1865. The
outbursts of lava from lateral cones are no doubt due to the fact that
the pressure of lava in the great crater, which is nearly 1000 feet in
depth, becomes so great that the lava is forced out at some lower point
of less resistance. The most northerly of the minor cones is Monte di
Mojo, from whence issued the lava of 396 B.C., it is 11-1/2 miles from
the crater; the most southerly cone is Monte Ste Sofia, 16 miles from
the crater. Nearly all the minor cones are within 10 miles of the
crater, and the majority are collected between south-east, and west,
that is, in an angular space of 135 deg., starting midway between east and
south, (45 deg. south of due east) to due west, (90 deg. west of due south).
Lyell speaks of the minor cones "as the most grand and original feature
in the physiognomy of Etna."

A number of caverns are met with in various parts of Etna; Boccacio
speaks of the Cavern of Thalia, and several early writers allude to the
Grotto delle Palombe near Nicolosi. The latter is situated in front of
Monte Fusara, and the entrance to it is evidently the crater of an
extinct monticule. It descends for 78 feet, and at the bottom a cavern
is entered by a long shaft; this leads to a second cavern, which
abruptly descends, and appears to be continued into the heart of the
neighbouring Monti Rossi. Brydone says that people have lost their
senses in these caverns, "imagining that they saw devils, and the
spirits of the damned; for it is still very generally believed that Etna
is the mouth of Hell." Many of the caverns near the upper part of the
mountain are used for storing snow, and sometimes as places of shelter
for shepherds. We have already seen to what extent Lucretius attributed
the eruptions to air pent up within the interior caverns of the
mountains.

The surface of the mountain has been divided into three zones or
regions--the _Piedimontana_ or _Coltivata_; the _Selvosa_ or _Nemorosa_;
and the _Deserta_ or _Discoperta_. Sometimes the name of _Regione del
Fuoco_ is given to the central cone and crater. As regards temperature,
the zones correspond more or less to the Torrid, Temperate, and Frigid.
The lowest of these, the _Cultivated Region_, yields in abundance all
the ordinary Sicilian products. The soil, which consists of decomposed
lava, is extremely fertile, although of course large tracts of land are
covered by recent lavas, or by those which decompose slowly. In this
region the vine flourishes, and abundance of corn, olives, pistachio
nuts, oranges, lemons, figs, and other fruit trees.

The breadth of this region varies; it terminates at an approximate
height of 2000 feet. A circle drawn with a radius of 10 miles from the
crater, roughly defines the limit. The elevation of this on the north is
2,310 feet near Randazzo; on the south, 2,145 feet near Nicolosi; on the
east, 600 feet near Mascali; and on the west, 1,145 feet near Bronte.
The breadth of this cultivated zone is about 2 miles on the north, east,
and west, and 9 or 10 on the south, if we take for the base of the
mountain the limits proposed above.

The _Woody Region_ commences where the cultivated region ends, and
extends as a belt of varying width to an approximate height of 6,300
feet. It is terminated above by a circle having a radius of nearly 1-1/2
miles from the crater. There are fourteen separate forests in this
region: some abounding with the oak, beech, pine, and poplar, others
with the chestnut, ilex, and cork tree.

The celebrated _Castagno di Cento Cavalli_, one of the largest and
oldest trees in the world, is in the Forest of Carpinetto, on the East
side of the mountain, five miles above Giarre. This tree has the
appearance of five separate trunks united into one, but Ferrara declares
that by digging a very short distance below the surface he found one
single stem. The public road now passes through the much-decayed trunk.
Captain Smyth measured the circumference a few feet from the ground, and
found it to be 163 feet, which would give it a diameter of more than 50
feet. The tree derives its name from the story that one of the Queens of
Arragon took shelter in its trunk with a suite of 100 horsemen. Near
this patriarch are several large chestnuts, which, without a shadow of
doubt, are single trees; one of these is 18 feet in diameter, and a
second 15 feet, while the _Castagno della Galea_, higher up on the
mountain, is 25 feet in diameter, and probably more than 1000 years old.
The breadth of the Regione Selvosa varies considerably, as may be seen
by reference to the accompanying map; in the direction of the Val del
Bove it is very narrow, while elsewhere it frequently has a breadth of
from 6 to 8 miles.

The Desert Region is embraced between the limit of 6,300 feet and the
summit. It occupies about 10 square miles, and consists of a dreary
waste of black sand, scoriae, ashes, and masses of ejected lava. In
winter it remains permanently covered with snow, and even in the height
of summer snow may be found in certain rifts.

Botanists have divided the surface of Etna into seven regions. The first
extends from the level of the sea to 100 feet above it, and in it
flourishes the palm, banana, Indian fig or prickly pear, sugar-cane,
mimosa, and acacia. It must be remembered, however, that it is only on
the east side of the mountain that the level within the base sinks to
100 feet above the sea; and, moreover, that the palm, banana, and
sugar-cane, are comparative rarities in this part of Sicily. Prickly
pears and vines are the most abundant products of the lower <DW72>s of
the eastern side of Etna. The second, or hilly region, reaches from 100
to 2000 feet above the sea, and therefore constitutes, with the
preceding, the _Regione Coltivata_ of our former division. In it are
found cotton, maize, orange, lemon, shaddock, and the ordinary Sicilian
produce. The culture of the vine ceases near its upward limit. The
third, or woody region, reaches from 2000 to 4000 feet, and the
principal trees within it are the cork, oak, maple, and chestnut. The
fourth region extends from 4000 to 6000 feet, and contains the beech,
Scotch fir, birch, dock, plaintain, and sandworth. The fifth, or
sub-Alpine region, extending from 6000 to 7000 feet, contains the
barberry, soapwort, toad-flax, and juniper. In the sixth region, 7,500
to 9000 feet, are found soapwort, sorrel, and groundsel; while the last
narrow zone, 9000 to 9,200 feet, contains a few lichens, the commonest
of which is the _Stereocaulon Paschale_. The flora of Etna comprises 477
species, only 40 of which are found between 7000 feet and the summit,
while in the last 2000 feet only five phanerogamous species are found,
viz., Anthemis Etnensis, Senecio Etnensis, Robertsia taraxacoides,
(which are peculiar to Etna), Tanacetum vulgare, and Astragulus Siculus.
Common ferns, such as the _pteris aquilina_, are found in abundance
beneath the trees in the Regione Selvosa.

This division has been advocated by Presl in his _Flora Sicula_.[16] He
names the different regions beginning from below: _Regio Subtropica_,
_Regio Collina_, _Regio Sylvatica inferior_, _Regio fagi Sylvestris_.
These four are common to all Sicily. The three remaining regions, _Regio
Subalpina_, _Regio Alpina_, and _Regio Lichenum_, together extending
from 6000 to 9,200 feet, belong to Etna alone.

[16] "Flora sicula: exhibens Plantas vasculosas in Sicilia aut sponte
crescentes aut frequentissime cultas, secundum systema naturale
digestas." Auctore G. B. Presl. Pragae, 1824.

At the conclusion of the first volume of Recupero's _Storia Naturale et
Generale dell' Etna_ we find a somewhat different botanical division
proposed by Signor Rafinesque-Schmaltz.[17] He makes his divisions in
the following manner:--

    1. Florula Piedemontana.
    2. Florula Nemorosa.
    3. Florula excelsa o della Regione Discoperta.
    4. Florula Arenosa o della Regione delle Scorie.

[17] Chloris Aetnensis: o le quattro Florule dell' Etna, opusculo del
Sig. C. S. Rafinesque-Schmaltz, Palermo. Dicembre, 1813.

In the latter region, (to which he assigns no limit as to height), he
found Potentilla Argentea, Rumex Scutatus, Tanacetum Vulgare, Anthemis
Montana, Jacobaea Chrysanthemifolia, Seriola Uniflora, and Phalaris
Alpina.

As regards the animal life on Etna, of course it is the same as that of
the eastern sea-board of Sicily, except in the higher regions, where it
becomes more sparse. The only living creatures in the upper regions are
ants, a little lower down Spallanzani found a few partridges, jays,
thrushes, ravens, and kites.

Brydone says of the three regions: "Besides the corn, the wine, the oil,
the silk, the spice, and delicious fruits of its lower region; the
beautiful forests, the flocks, the game, the tar, the cork, the honey of
its second; the snow and ice of its third; it affords from its caverns a
variety of minerals and other productions--cinnabar, mercury, sulphur,
alum, nitre, and vitriol; so that this wonderful mountain at the same
time produces every necessary, and every luxury of life."




CHAPTER III.

ASCENT OF THE MOUNTAIN.

    The most suitable time for ascending Etna.--The ascent commenced.--
    Nicolosi.--Etna mules.--Night journey through the upper Regions of
    the mountain.--Brilliancy of the Stars.--Proposed Observatory on
    Etna.--The Casa Inglesi.--Summit of the Great Crater.--Sunrise from
    the summit.--The Crater.--Descent from the Mountain.--Effects of
    Refraction.--Fatigue of the Ascent.


The ascent of Mount Etna has been described many times during the last
eighteen centuries, from Strabo in the second century to Dr. Baltzer in
1875. One of the most interesting accounts is certainly that of Brydone,
and in this century perhaps that of Mr. Gladstone. Of course the
interest of the expedition is greatly increased if it can be combined
with that spice of danger which is afforded by the fact of the mountain
being in a state of eruption at the time.

The best period for making the ascent is between May and September,
after the melting of the winter snows, and before the autumnal rains. In
winter snow frequently extends from the summit downwards for nine or
ten miles; the paths are obliterated, and the guides refuse to accompany
travellers. Even so late in the spring as May 29th Brydone had to
traverse seven miles of snow before reaching the summit. Moreover,
violent storms often rage in the upper regions of the mountain, and the
wind acquires a force which it is difficult to withstand, and is at the
same time piercingly cold. Sir William Hamilton, in relating his ascent
on the night of June 26th, 1769, remarks that, if they had not kindled a
fire at the halting place, and put on much warm clothing, they would
"surely have perished with the cold." At the same time the wind was so
violent that they had several times to throw themselves on their faces
to avoid being overthrown. Yet the guides said that the wind was not
unusually violent. Some writers, well used to Alpine climbing, have
asserted that the cold on Etna was more severe than anything they have
ever experienced in the Alps.

The writer of this memoir made the ascent of the mountain in August
1877, accompanied by a courier and a guide. We took with us two mules;
some thick rugs; provisions consisting of bread, meat, wine, coffee, and
brandy; wooden staves for making the ascent of the cone; a geological
hammer; a bag for specimens; and a few other requisites. It has to be
remembered that absolutely nothing is to be met with at the Casa
Inglesi, where the halt is made for the night; even firewood has to be
taken, a fire being most necessary in those elevated regions even during
a midsummer's night. For some time previous to our ascent the weather
had been uniformly bright and fine, and there had been no rain for more
than three months. The mean temperature in the shade at Catania, and
generally along the eastern sea-base of the mountain, was 82 deg. F.

As we desired to see the sunrise from the summit of the mountain, we
determined to ascend during the cool of the evening, resting for an hour
or two before sunrise at the Casa Inglesi at the foot of the cone.
Accordingly we left Catania soon after midday, and drove to Nicolosi,
twelve miles distant, and 2,288 feet above the sea. The road for some
distance passed through a very fertile district; on either side there
were corn fields and vineyards, and gardens of orange and lemon trees,
figs and almonds, growing luxuriantly in the decomposed lava. About half
way between Catania and Nicolosi stands the village of Gravina, and a
mile beyond it Mascalucia, a small town containing nearly 4000
inhabitants. Near this is the ruined church of St. Antonio, founded in
1300. Nine miles from Catania the village of Torre di Grifo is passed,
and the road then enters a nearly barren district covered with the lava
and scoriae of 1527. The only prominent form of vegetation is a peculiar
tall broom--_Genista Etnensis_--which here flourishes. We are now
entering the region of minor cones; the vineclad cone of Monpilieri is
visible on the left, and just above it Monti Rossi, 3,110 feet above the
sea; to the right of the latter we see Monte San Nicola, Serrapizzuta,
and Monte Arso. We reach Nicolosi at half-past four; for although the
distance is short, the road is very rugged and steep.

Nicolosi has a population of less than 3,000; it consists of a long
street, bordered by one-storied cottages of lava. In the church the
priests were preparing for a _festa_ in honour of S. Anthony of Padua.
They politely took us into the sacristy, and exhibited with much pride
some graven images of rather coarse workmanship, which were covered with
gilding and bright  paint. Near Nicolosi stands the convent of
S. Nicola dell' Arena, once inhabited by Benedictine monks, who however
were compelled to abandon it in consequence of the destruction produced
by successive shocks of earthquake. Nicolosi itself has been more than
once shaken to the ground. We dined pretty comfortably, thanks to the
courier who acted as cook, in the one public room of the one primitive
inn of the town; starting for the Casa Inglesi at 6 o'clock. The good
people of the inn surrounded us at our departure and with much warmth
wished us a safe and successful journey.

For a short distance above Nicolosi, stunted vines are seen growing in
black cinders, but these soon give place to a large tract covered with
lava and ashes, with here and there patches of broom. There was no
visible path, but the mules seemed to know the way perfectly, and they
continued to ascend with the same easy even pace without any guidance,
even after the sun had disappeared behind the western flank of the
mountain. In fact, you trust yourself absolutely to your mule, which
picks his way over the roughest ground, and rarely stumbles or changes
his even step. I found it quite easy to write notes while ascending, and
even to use a pocket spectroscope at the time of the setting sun.
Subsequently we saw a man extended at full length, and fast asleep upon
a mule, which was leisurely plodding along the highway. The same
confidence must not however be extended to the donkeys of Etna, as I
found to my cost a few days later at Taormina. Here the only animal to
be procured to carry me down to the sea-shore, 800 feet below, was a
donkey. It was during the hottest part of the day, and it was necessary
to carry an umbrella in one hand, and comfortable to wear a kind of
turban of many folds of thin muslin round one's cap. The donkey after
carefully selecting the roughest and most precipitous part of the road,
promptly fell down, leaving me extended at full length on the road, with
the open umbrella a few yards off. At the same time the turban came
unfolded, and stretched itself for many a foot upon the ground.
Altogether it was a most comical sight, and it reminded me forcibly, and
at the instant, of a picture which I once saw over the altar of a
church in Pisa, and which represented S. Thomas Aquinas discomfiting
Plato, Aristotle, and Averroees. The latter was completely overthrown,
and in the most literal sense, for he was grovelling in the dust at the
feet of S. Thomas, while his disarranged turban had fallen from him.

The district of lava and ashes above Nicolosi is succeeded by forests of
small trees, and we are now fairly within the _Regione Selvosa_. At
half-past 8 o'clock the temperature was 66 deg., at Nicolosi at 4 o'clock it
was 80 deg.. About 9 o'clock we arrived at the Casa del Bosco, (4,216 feet),
a small house in which several men in charge of the forest live. Here we
rested till 10 o'clock, and then after I had put on a great-coat and a
second waistcoat, we started for the higher regions. At this time the
air was extraordinarily still, the flame of a candle placed near the
open door of the house did not flicker. The ascent from this point
carried us through forests of pollard oaks, in which it was quite
impossible to see either a path or any obstacles which might lie in
one's way. The guide carried a lantern, and the mules seemed well
accustomed to the route. At about 6,300 feet we entered the _Regione
Deserta_, a lifeless waste of black sand, ashes, and lava; the ascent
became more steep, and the air was bitterly cold. There was no moon, but
the stars shone with an extraordinary brilliancy, and sparkled like
particles of white-hot steel. I had never before seen the heavens
studded with such myriads of stars. The milky-way shone like a path of
fire, and meteors flashed across the sky in such numbers that I soon
gave up any attempt to count them. The vault of heaven seemed to be much
nearer than when seen from the earth, and more flat, as if only a short
distance above our heads, and some of the brighter stars appeared to be
hanging down from the sky. Brydone, in speaking of his impressions under
similar circumstances says:

"The sky was clear, and the immense vault of heaven appeared in awful
majesty and splendour. We found ourselves more struck with veneration
than below, and at first were at a loss to know the cause, till we
observed with astonishment that the number of the stars seemed to be
infinitely increased, and the light of each of them appeared brighter
than usual. The whiteness of the milky-way was like a pure flame that
shot across the heavens, and with the naked eye we could observe
clusters of stars that were invisible in the regions below. We did not
at first attend to the cause, nor recollect that we had now passed
through ten or twelve thousand feet of gross vapour, that blunts and
confuses every ray before it reaches the surface of the earth. We were
amazed at the distinctness of vision, and exclaimed together, 'What a
glorious situation for an observatory! had Empedocles had the eyes of
Galileo, what discoveries must he not have made!' We regretted that
Jupiter was not visible, as I am persuaded we might have discovered some
of his satellites with the naked eye, or at least with a small glass
which I had in my pocket."

Brydone wrote a hundred years ago, but his idea of erecting an
observatory on Mount Etna was only revived last year, when Prof.
Tacchini the Astronomer Royal at Palermo, communicated a paper to the
Accademia Gioenia, entitled "_Della Convenienza ed utilita di erigere
sull' Etna una Stazione Astronomico-Meteorologico_." Tacchini mentions
the extraordinary blueness of the sky as seen from Etna, and the
appearance of the sun, which is "whiter and more tranquil" than when
seen from below. Moreover, the spectroscopic lines are defined with
wonderful distinctness. In the evening at 10 o'clock, Sirius appeared to
rival Venus, the peculiarities of the ring of Saturn were seen far
better than at Palermo; and Venus emitted a light sufficiently powerful
to cast shadows; it also scintillated. When the chromosphere of the sun
was examined the next morning by the spectroscope, the inversion of the
magnesium line, and of the line 1474 was immediately apparent, although
it was impossible to obtain this effect at Palermo. Tacchini proposes
that an observatory should be established at the Casa Inglesi, in
connection with the University of Catania, and that it be provided with
a good six-inch refracting telescope, and with meteorological
instruments. In this observatory, constant observations should be made
from the beginning of June to the end of September, and the telescope
should then be transported to Catania, where a duplicate mounting might
be provided for it, and observations continued for the rest of the year.
There seems to be every probability that this scheme will be carried out
in the course of next year.

During this digression we have been toiling along the <DW72>s of the
_Regione Deserta_ and looking at the sky; at length we reach the _Piano
del Lago_ or Plain of the Lake, so called because a lake produced by the
melting of the snows existed here till 1607, when it was filled up by
lava. The air is now excessively cold, and a sharp wind is blowing.
Progress is very slow, the soil consists of loose ashes, and the mules
frequently stop; the guide assures us that the Casa Inglesi is quite
near, but the stoppages become so frequent that it seems a long way off;
at length we dismount, and drag the mules after us, and after a toilsome
walk the small lava-built house, called the Casa Inglesi, is reached
(1.30 a.m., temperature 40 deg. F.) It stands at a height of 9,652 feet
above the sea, near the base of the cone of the great crater, and it
takes its name from the fact that it was erected by the English officers
stationed in Sicily in 1811. It has suffered severely from time to time
from the pressure of snow and from earthquakes, but it was thoroughly
repaired in 1862, on the occasion of the visit of Prince Humbert, and is
now in tolerable preservation. It consists of three rooms, containing a
few deal chairs, a table, and several shelves like the berths of ships
furnished with plain straw mattresses; there is also a rough fireplace.
We had no sooner reached this house, very weary and so cold that we
could scarcely move, than it was discovered that the courier had omitted
to get the key from Nicolosi, and there seemed a prospect of spending
the hours till dawn in the open air. Fortunately we had with us a chisel
and a geological hammer, and by the aid of these we forced open the
shutter serving as a window, and crept into the house; ten minutes later
a large wood fire was blazing up the chimney, our eatables were
unpacked, some hot coffee was made, and we were supremely comfortable.

[Illustration: The Casa Inglesi and Cone of Etna]

At 3 a.m. we left the Casa Inglesi for the summit of the great crater,
1,200 feet above us, in order to be in time to witness the sunrise. Our
road lay for a short distance over the upper portion of the Piano del
Lago, and the walking was difficult. The brighter stars had disappeared,
and it was much darker than it had been some hours before. The guide led
the way with a lantern. The ascent of the cone was a very stiff piece of
work; it consists of loose ashes and blocks of lava, and <DW72>s at an
angle of "45 deg. or more" according to one writer, and of 33 deg. according to
another; probably the <DW72> varies on different sides of the cone: we do
not think that the <DW72> much exceeds 33 deg. anywhere on the side of the
cone which we ascended. Fortunately there was no strong wind, and we did
not suffer from the sickness of which travellers constantly complain in
the rarefied air of the summit. We reached the highest point at 4.30
a.m., and found a temperature of 47 deg. F.

When Sir William Hamilton ascended towards the end of June the
temperature at the base of the mountain was 84 deg. F., and at the summit
56 deg. F. When Brydone left Catania on May 26th, 1770, the temperature was
76 deg. F., Bar. 29 in. 8-1/2 lines; at Nicolosi at midday on the 27th it
was 73 deg. F., Bar. 27 in. 1-1/2 lines; at the Spelonca del Capriole (6,200
feet), 61 deg. F., Bar. 26 in. 5-1/2 lines; at the foot of the crater, temp.
33 deg. F., Bar. 20 in. 4-1/2 lines, and at the summit of the crater just
before sunrise, temp. 27 deg. F., Bar. 19 in. 4 lines.

On reaching the summit we noticed that a quantity of steam and
sulphurous acid gas issued from the ground under our feet, and in some
places the cinders were so hot that it was necessary to choose a cool
place to sit down upon. A thermometer inserted just beneath the soil
from which steam issued registered 182 deg. F. For a short time we anxiously
awaited the rising of the sun. Nearly all the stars had faded away; the
vault of heaven was a pale blue, becoming a darker and darker grey
towards the west, where it appeared to be nearly black. Just before
sunrise the sky had the appearance of an enormous arched spectrum,
extremely extended at the blue end. Above the place where the sun would
presently appear there was a brilliant red, shading off in the direction
of the zenith to orange and yellow; this was succeeded by pale green,
then a long stretch of pale blue, darker blue, dark grey, ending
opposite the rising sun with black. This effect was quite distinct, it
lasted some minutes, and was very remarkable. This was succeeded by the
usual rayed appearance of the rising sun, and at ten minutes to 5
o'clock the upper limb of the sun was seen above the mountains of
Calabria. Examined by the spectroscope the Fraunhofer lines were
extremely distinct, particularly two lines near the red end of the
spectrum.

The top of the mountain was now illuminated, while all below was in
comparative darkness, and a light mist floated over the lower regions.
We were so fortunate as to witness a phenomenon which is not always
visible, viz., the projection of the triangular shadow of the mountain
across the island, a hundred miles away. The shadow appeared vertically
suspended in space at or beyond Palermo, and resting on a slightly misty
atmosphere; it gradually sank until it reached the surface of the
island, and as the sun rose it approached nearer and nearer to the base
of the mountain. In a short time the flood of light destroyed the first
effects of light and shadow. The mountains of Calabria and the west
coast of Italy appeared very close, and Stromboli and the Lipari Islands
almost under our feet; the east coast of Sicily could be traced until it
ended at Cape Passaro and turned to the west, forming the southern
boundary of the island, while to the west distant mountains appeared. No
one would have the hardihood to attempt to describe the various
impressions which rapidly float through the mind during the
contemplation of sunrise from the summit of Etna. Brydone, who is by no
means inclined to be rapturous or ecstatic in regard to the many
wonderful sights he saw in the course of his tour, calls this "the most
wonderful and most sublime sight in nature." "Here," he adds,
"description must ever fall short, for no imagination has dared to form
an idea of so glorious and so magnificent a scene. Neither is there on
the surface of this globe any one point that unites so many awful and
sublime objects. The immense elevation from the surface of the earth,
drawn as it were to a single point, without any neighbouring mountains
for the senses and imagination to rest upon, and recover from their
astonishment in their way down to the world. This point or pinnacle,
raised on the brink of a bottomless gulph, as old as the world, often
discharging rivers of fire and throwing out burning rocks with a noise
that shakes the whole island. Add to this, the unbounded extent of the
prospect, comprehending the greatest diversity and the most beautiful
scenery in nature, with the rising sun advancing in the east to
illuminate the scene."

When the sun had risen we had time to examine the crater, a vast abyss
nearly 1000 feet in depth, and with very precipitous sides. Its
dimensions vary, but it is now between two and three miles in
circumference. Sometimes it is nearly full of lava, at other times it
appears to be bottomless. At the present time it is like an inverted
cone; its sides are covered with incrustations of sulphur and ammonia
salts, and jets of steam perpetually issue from crevices. Near the
summit we found a deposit, several inches in thickness, of a white
substance, apparently lava decomposed by the hot issuing gases.
Hydrochloric acid is said to frequently issue from the crater; the gases
that were most abundant appeared to be sulphurous acid and steam. The
interior of the crater appeared to be very similar to that of the
Solfatara near Puzzuoli. During the descent from the cone we collected
various specimens of ash and cinder, some red, others black and very
vesicular, others crystalline, some pale pink. The steep <DW72> of the
cone was well shown by the fact that, although the surface is either
extremely rugged owing to the accumulation of masses of lava, or soft
and yielding on account of the depth of cinders, a large mass of lava
set rolling at the top rushes down with increasing velocity until it
bounds off to the level plain below.

[Illustration: View of the Val de Bove]

The great cone is formed by the accumulation of sand, scoriae, and masses
of rock ejected from the crater; it is oval in form, and has varied both
in shape and size in the course of centuries. When we saw it, it was not
full of smoke or steam; but it was possible to see to the bottom of it,
in spite of small jets of steam which issued from the sides. It
presented the appearance of a profound funnel-shaped abyss; the sides of
which were covered with an efflorescence of a red or yellow, and
sometimes nearly white, colour. The crater presented the same appearance
when it was seen by Captain Smyth in 1814, but he was so fortunate as to
witness it in a less quiescent state. "While making these observations,"
he writes, "on a sudden the ground trembled under our feet, a harsh
rumbling with sonorous thunder was heard, and volumes of heavy smoke
rolled over the side of the crater, while a lighter one ascended
vertically, with the electric fluid escaping from it in frequent flashes
in every direction.... During some time the ground shook so violently
that we apprehended the whole cone would tumble into the burning gulf
(as it actually had done several times before) and destroy us in the
horrible consequences; however, in less than a couple of hours all was
again clear above and quiet within." When Mr. Gladstone ascended in
1838, the volcano was in a slight state of eruption: "The great
features of this action," he writes, "are the sharp and loud claps,
which perceptibly shook from time to time the ground of the mountain
under our feet; the sheet of flame which leapt up with a sudden
momentary blast, and soon disappeared in smoke; then the shower of
red-hot stones and lava. At this time, as we found on our way down, lava
masses of 150 or 200 pound weight were being thrown a distance of
probably a mile and a half; smaller ones we found even more remote.
These showers were most copious, and often came in the most rapid
succession. Even while we were ascending the exterior of the cone, we
saw them alighting on its <DW72>, and sometimes bounding down with
immense rapidity within, perhaps, some thirty or forty yards of our
rickety footing on the mountain side. They dispersed like the sparks of
a rocket; they lay beneath the moon, over the mountain, thicker than
ever the stars in heaven; the larger ones ascended as it were with
deliberation, and descended, first with speed and then with fury. Now
they passed even over our heads, and we could pick up some newly fallen,
and almost intolerably hot. Lastly, there was the black grey column,
which seemed smoke, and was really ash, and which was shot from time to
time out of the very bowels of the crater, far above its edge, in
regular unbroken form."

At the Casa Inglesi we remounted the mules, and made a slight detour to
the east in order to look down into the Val del Bove, which is here seen
as a gigantic valley, bounded on the north by the precipitous cliffs of
the Serra delle Concazze, and on the South by the Serra del Solfizio. It
is believed by Lyell and others that in the Balzo di Trifoglietto, at
which point the precipices are most profound and abrupt, there was a
second permanent crater of eruption. The Torre del Filosofo, a ruined
tower, traditionally the observatory of Empedocles, stands near the Casa
Inglesi. Not far from this a great deposit of ice was found in 1828. It
was preserved from melting by a layer of ashes and sand, which had
covered it, soon after its first existence, as a glacier: a stream of
lava subsequently flowed over the ashes, and completely protected the
ice; the non-conducting power of the ashes prevented the lava from
melting the ice. The snow which falls on the mountain is stowed away in
caves, and used by the Sicilians during summer. A ship load is also sent
to Malta, and the Archbishop of Catania derives a good deal of his
income from the sale of Etna snow.

During our descent from the mountain we were much struck by the apparent
nearness of the minor cones beneath us, and of the villages at the base
of the mountain. They seemed to be painted on a vertical wall in front
of us, and although from ten to fifteen miles distant they appeared to
be almost within a stone's throw. This curious effect, which has often
been observed before, is due to refraction. At the summit of Etna we
have left one-third of the atmosphere beneath us, and the air is now
pressing upon the surface of the earth with a weight of ten pounds on
the square inch, instead of the usual fifteen pounds experienced at the
level of the sea. In looking towards the base of the mountain we are
consequently looking from a rarer to a denser medium; and it is a law of
optics, that when light passes from a denser to a rarer medium it is
refracted away from the perpendicular, and thus the object, from which
it emanates, appears raised, and nearer to us than it really is. The
objects around Etna appear near to us and raised vertically from the
horizon for the same reason that a stick plunged in water appears bent.

We reached Nicolosi again about noon, having left it eighteen hours
before. The ascent of the mountain, although it does not involve much
hard walking, is somewhat trying on account of the extremes of
temperature which have to be endured. In the course of the morning of
our descent we had experienced a difference equal to more than 40 deg. F. As
to the ascent, you are moving upwards nearly all night; you have six
hours of riding on a mule, some of it in a bitterly cold atmosphere; you
get very much heated by the final steep climb of 1100 feet, and you find
at the summit a piercing wind; of course there is no shelter, and you
sit down to wait for sunrise on cinders which are gently giving off
steam and sulphurous acid; the former condenses to water as soon as it
meets the cold air, and you find your great coat, or the rug on which
you have sat down, speedily saturated with moisture.




CHAPTER IV.

TOWNS SITUATED ON THE MOUNTAIN.

    Paterno.--Ste. Maria di Licodia.--The site of the ancient town of
    Aetna.--Biancavilla.--Aderno.--Sicilian Inns.--Adranum.--Bronte.--
    Randazzo.--Mascali.--Giarre.--Aci Reale.--Its position.--The Scogli
    de'Ciclopi.--Catania, its early history, and present condition.


We have before alluded to the fact that Etna is far more thickly
populated than any other part of Sicily or Italy; in fact, more so than
almost any equal area in the world, of course excepting large cities and
their neighbourhood. This is due to the wonderful fertility of the soil,
the salubrity of the climate, and, on the eastern base, to the proximity
of a sea-coast indented with excellent harbours. The habitable zone of
Etna is restricted to the _Regione Coltivata_, nevertheless some of the
towns on the north and west have a considerable elevation; thus Bronte
is 2,782 feet above the sea, and Randazzo 2,718. All the principal towns
are situated on the base road of the mountain, which was indeed
constructed in order to connect them. Out of the sixty-four towns and
villages on the mountain, the following are the most important:
Catania, Aci Reale, Paterno, Aderno, Bronte, Randazzo, Aci S. Antonio,
Biancavilla, Calatabiano, Giarre, Francavilla, Linguagrossa, Licodia,
Mascali, Misterbianco, Nicolosi, Pedara, Piedemonte, Trecastagne, and
Tremestieri.

On our return from the summit, we rested for awhile at Nicolosi, and in
the cool of the evening started to make a _giro_ of the mountain by way
of the base road. Descending by the Nicolosi road as far as Mascalucia,
we branched off to the west, and made for Paterno, passing near the town
of Belpasso, which was destroyed by the earthquake of 1669, and
subsequently erected on a new site. It still contains more than 7,000
inhabitants, although the district is extremely unhealthy.

Paterno, the second largest town on the flanks of Etna after Catania and
Aci Reale, stands in the very heart of the Regione Coltivata, and
possesses more than 16,000 inhabitants. According to Cluverius, it is
the site of the city of Hybla Major (~Hybla Megale~), a Sikelian
city which was unsuccessfully attacked by the Athenians soon after they
first landed in Sicily. During the second Punic War, the inhabitants
went over to the Carthagenians, but the city was speedily recovered by
the Romans. Pliny, Cicero, and Pausanias allude to it, but its later
history has not come down to us. An altar was lately found in Paterno
dedicated to _Veneri Victrici Hyblensi_. Several towns in Sicily were
called Hybla, probably--according to Pausanias--in honour of a local
deity. Paterno was founded by Roger I. in 1073: it was once a feudal
city of some importance, and possessed a cathedral and castle, and
several large monasteries. Although much fallen to decay, it still
possesses a good deal of vitality, and the population is on the
increase.

On leaving Paterno the road turns to the North-west, and passes through
the village of Ste. Maria di Licodia. Here originally stood the Sikelian
City of Inessa (~Inessa~), which, after the death of Hiero I.,
was peopled by colonists from Katana (then called ~Aitne~). The
new occupants of the city changed its name from Inessa to Aetna, which
it retained. The town later fell into the hands of the Syracusans, and
in 462 B.C. the Athenians in vain attempted to take it. During the
Athenian expedition both Aetna and Hybla were allies of Syracuse. In 403
B.C. Aetna was taken by Dionysius, who placed in it a body of Campanian
mercenaries. Sixty-four years later (B.C. 339) the town was taken by
Timoleon. For many succeeding years we find no further mention of it.
Cicero speaks of it in his time as an important place, and the centre of
a very fertile district; it is also mentioned by Pliny and Ptolemy, and
Strabo says that it was usually the starting point for those who
ascended the mountain. Of its later history we know absolutely nothing.


Six miles to the north-west of St. Mariah di Licodia, the road passes
through Biancavilla--a town of 13,000 inhabitants, and the centre of a
cotton district.

The road continues in the same direction until the town of Aderno is
reached; and here we arrived late in the evening, and gained our first
experience of a Sicilian inn in an out-of-the-way town. After many
enquiries we were directed to the only inn which the place could boast,
kept by a doctor. No one appeared at or near the entrance, of course
there was no bell or knocker, and we made our way up a dark stone
staircase till we arrived at a dimly-lighted passage. A horrible old
Sicilian woman now appeared, and showed us with great incivility the
only room in the house, which its inmates were willing to place at our
disposal. It was a fairly large room, with a stone floor which
apparently had not been swept for weeks, and walls that had once been
whitewashed; the furniture consisted of three beds placed on tressels, a
plain deal table, and some primitive chairs. As to food they had neither
bread, meat, wine, eggs, macaroni, fruit, or butter in the house;
neither did they offer to procure anything. Even when some eggs had been
obtained, and (after an hour's delay) cooked, there was not a single
teaspoon to eat them with. The people of the town appear to subsist
chiefly on beans and a kind of dried fish. If our courier had not been a
very handy fellow and a tolerable cook, we should have been obliged
more than once to go to bed supperless. As it was, the best he could do
on this occasion was to get some bread, eggs, and wine, and--best of
all--some snow, for the heat was intolerable. In a town of the same
size--15,657 inhabitants--in England, we should have at least two really
comfortable inns ready at any moment to receive and entertain the weary
traveller.

[Illustration: View of Etna from Bronte]

Aderno stands on the site, and has preserved the name, of the ancient
Sikelian city of Adranum (~Adranon~). According to Diodorus there
existed here, from very early times, the temple of a local deity named
Adranus. The city was founded by the elder Dionysius in 400 B.C.; it
owed its importance to the renown of its temple, which was guarded by a
thousand dogs. In 345 B.C. the city fell into the hands of Timoleon, and
it was taken by the Romans at the commencement of the first Punic War.
After this we cease to hear of it. The modern town was founded by Roger
I. in the 12th century. The fine Norman tower--now used as a prison--and
the monastery, were both built by King Roger.

After leaving Aderno the base-road ascends, turns nearly due north, and
leads us past a number of lava streams, notably those of 1610, 1603, and
1651. A good view of Monte Minardo, and the minor cones in its more
immediate neighbourhood, is obtained on the left, while on the right we
see the Valley of the Simeto, and Centorbi high upon the hills.

Nearly due west of the great crater is the town of Bronte, which is
2,782 feet above the sea, and has a population of more than 15,000. It
is a very primitive place, and several centuries behind the age; it
reminded us forcibly, in one or two particulars, of Pompeii: the streets
are narrow and tortuous, and the roadway very uneven. Awnings are
sometimes hung across the street from side to side to provide shade. The
shops are exactly like those at Pompeii; and in the main street we
noticed an open-air kitchen, to which the would-be diner repairs,
purchases a plateful of food, and eats it standing in the public way.
The inn was even worse than that of Aderno, and apparently had never
before received guests. We were offered one miserable room, without a
lock to the door, and unprovided with either table or chair. Of course
the bare idea of offering to procure, or furnish, or cook, any kind of
food was too monstrous to be entertained for a moment. With difficulty
the courier obtained some eggs, macaroni, and fruit, on which we dined
in a small barn attached to a wine-shop.

At Bronte we are only nine miles from the crater, on the steepest side
of the mountain, and near the Tertiary sandstone which underlies this
portion of the mountain. A short distance outside the town we saw great
beds of the lava of 1832, piled up fantastically in all sorts of forms,
and excessively rugged and uneven. It is quite bare of vegetation, and
does not appear to have even commenced to be decomposed.

Bronte gave its name to Lord Nelson, who was created Duke of Bronte by
Ferdinand IV.:--an appropriate name for a great warrior ([Greek:
bronte], thunder). The Nelson estates are scattered around the town.

On leaving Bronte the road conducted us past several high hills of
sandstone and quartzite near Monte Rivoglia; then we passed near
Maletto, and, leaving the malarious lake Gurrita on our left, we soon
after arrived at Randazzo. Near Maletto the road reaches it highest
point--3,852 feet.

The town of Randazzo was founded by the Lombards in the 10th century;
during the Middle Ages it appears to have been a prosperous, populous,
place; at present it possesses more than 8,000 inhabitants. The Emperor
Frederick II. created his son Duke of Randazzo, and added to the name of
the town, _Etnea_. It contains several very interesting architectural
remains; a church of the 13th century, a mediaeval palace--the Palazzo
Finochiaro,--and a ducal palace now used as a prison. The houses are for
the most part built of lava, and some of the shops have massive lava
counters extending half across their open front, while the door occupies
the remainder, as at Pompeii. The view from Randazzo is very fine in
every direction; the crater of Etna appears near, and Monte
Spagnuolo--many hours distant--just outside the town. The town is 2,718
feet above the sea, just above the Valley of the Alcantara--of which it
commands a fine view, and also of the limestone hills on the other side.

We were obliged to pass the night in the town, in an inn scarcely
superior to that of Aderno, but distinctly better than the miserable
Albergo Collegio at Bronte. At least the people were civil, and did
their best. The one room of the inn had a bed in each corner, and a deal
table in the middle. Three of the beds were occupied by engineers who
were surveying in connection with a new line of railway; the fourth was
made over to the courier. I slept in a small kind of ante-room on a bed
chiefly composed of deal boards placed on tressels. Here again the
courier was invaluable, in fact it would be simply impossible to make
the circuit of Etna without a courier. He procured some eggs, macaroni,
fruit, snow, tomatoes, and even meat, and cooked everything well,
without a trace of garlic. He also took care that the linen was clean,
and the general arrangements as comfortable as they could be under the
circumstances. Let us also admit that neither at Aderno, Bronte, nor
Randazzo were we troubled with musquitoes or any worse species of
insect. These, we were assured, would appear in full force in the
following month (September). Our only inconvenience of this nature
arose from swarms of flies. The inns of these out-of-the-way towns
probably receive scarcely a dozen travellers in the year, and these are
Sicilians, who are not used to better accommodation. Evidently a
_forestiare_ is quite a novelty: the people of these small towns used to
look at us with great curiosity, and crowded round the carriage when we
started. At Bronte we had a good example of this curiosity: owing to the
hardness of the lava of 1832 the head had come off the handle of our
hammer, and we went into a carpenter's shop to have it put on again.
Presently we noticed that eleven people, including a priest, were
looking on, apparently with intense and absorbing interest.

From Randazzo the base-road descends, until at Giarre it is near the
sea-level. This road is one of the most beautiful in Sicily; it is part
of the old military route from Messina to Palermo, and it was traversed
by Himilco in 396 B.C.; by Timoleon in 344 B.C.; and by Charles V. in
1534. After leaving Randazzo the valley of the Alcantara becomes
visible, while beyond it rise the lofty mountains of the Nebrodes. The
road passes near Monte Dolce, and soon reaches Linguaglossa, a small
town from whence the craters of 1865 may be reached in about four hours.
The rapidly descending road passes through Piedemonte and Mascali, in
the heart of an extraordinarily fertile region. Mascali, a village of
3050 inhabitants, was considered by Cluverius to be the site of the
Greek town of Callipolis, founded by a colony from Naxos as early as the
fifth century, B.C. A full view of the coast line is obtained from the
Capo di Taormina on the north, to a point below Riposto on the south. We
descended through plantations of nuts, and groves of oranges and lemons,
to gentle <DW72>s covered with vineyards.

From the town of Giarre, (17,965 inhabitants), we get a view of the Val
del Bove, which, however, is almost always obscured by thin white
clouds, while the summit of the mountain is clear. We noticed, indeed,
every day that the summit, which had been absolutely clear all the day
and night, became covered with clouds shortly before sunset, while about
an hour later the clouds cleared off, and the mountain was sharply
defined against the sky during the starlit night. Some of the effects of
sunset behind clouds resting on the summit, while all the rest of the
sky was bright blue, were exceedingly beautiful, and were quite
untranslatable into any known language, save that of painting, and of
music. Perhaps Turner could have done justice to them.

After leaving Giarre we passed through a good deal of highly cultivated
land belonging to Baron Pennisi, the largest landholder and richest man
in Sicily. He makes good use of his wealth, and seems to be very
popular among all classes. He possesses three palaces in Aci Reale, and
has done a great deal to beautify the town. Archaeologists will remember
him as the possessor of the finest collection of Sicilian coins in the
world. Many of these have been found on his own estates, but he never
scruples to give large sums of money for any coin which he covets.

Aci Reale, one of the prettiest towns in Europe, is situated in the
midst of a very fertile region 550 feet above the sea. To the east it
faces the Ionian sea, while on the west towers Etna. The town is full of
wealthy inhabitants, and the houses are large, lofty, and well built. It
contains 24,151 inhabitants, and possesses celebrated sulphur baths, and
one of the best hotels in Sicily. The wealth of this small town is well
shown by the following fact: Since its foundation in the tenth century,
till within a year or two of the present time, the town had been under
the jurisdiction of the Archbishop of Catania. It happened, however, a
few years ago, on the occasion of a religious procession in Catania,
that the people of Aci considered that their patron Saint, S. Venera,
was slighted. In fact the image of S. Agata, the patron Saint of the
Catanese--whose veil has so often averted the lava-streams from the
city--was put in all the prominent parts of the procession, while the
image of S. Venera was comparatively neglected. The people of Aci at
once returned home, and sent a petition to the Pope, praying that they
might have a Bishop of their own directly subject to the Holy See, in
order that they might no longer be subjected to such slights. The
Vatican having duly considered the question consented to raise Aci to
the dignity of a Bishopric, and to pay the Bishop a yearly stipend of
10,000 lire, (about L400, but equal to L600 in Sicily), on condition
that 200,000 lire were paid at once into the coffers of the Vatican.
This was promptly done, and now Monsignore Gerlando Genuardi, Bishop of
Aci Reale, may snap his fingers in the face of Monsignore Giuseppe
Benedetto Dusmet, a Benedictine of the Congregation of Monte Cassino,
and Archbishop of Catania.

[Illustration: Island of Columnar Basalt off Trezza]

Six villages in the neighbourhood of Aci Reale bear the name of Aci: Aci
Castello, Aci Sant' Antonio, and so on, but Aci Reale claims to stand
upon the very site rendered memorable by the story of Acis and Galatea.
The river Acis (now called _Acque Grande_) rises from a bed of lava, and
falls into the sea a mile from its source. Aci Reale stands on seven
different beds of superposed lava, having layers of earth resulting from
decomposed lava between. The Canon Recupero calculated from observation,
that a lava requires at least 2000 years to form even a scanty layer of
earth, consequently he inferred that the lowest of the lava streams upon
which Aci rests must have been formed 14,000 years ago. These views he
stated to Brydone a hundred years ago; the latter says, "Recupero tells
me he is exceedingly embarrassed by these discoveries in writing the
history of the mountain. That Moses hangs like a dead weight upon him,
and blunts all his zeal for enquiry; for that really he has not the
conscience to make his mountain so young as that prophet makes the
world. What do you think of these sentiments from a Roman Catholic
Divine? The Bishop, who is strenuously orthodox--for it is an excellent
See--has already warned him to be upon his guard, and not to pretend to
be a better natural historian than Moses; not to presume to urge
anything that may, in the smallest degree, be deemed contradictory to
his sacred authority." The Canon Recupero lost his church preferment on
the publication of Brydone's book, and the whole body of clergy of
Girgenti received a reprimand on account of a capital story which
Brydone told of a dinner at which the Bishop presided, during which
several of the reverend Canons suffered severely from the effects of
English punch, which Brydone had brewed for them. We quite agree with
Admiral Smyth when he says, "It is a pity that Mr. Brydone laboured
under such a cacoethes, as to sacrifice a friend for the sake of a good
story." Of course we now know that Recupero's estimate of the age of
Etna was far within the true limits, but we derive this information
from other sources. No true estimate can be obtained from the
observation of the decomposition of lavas, for it has been often
observed that two lavas will decompose at very different rates.

A little to the north of the village of La Scaletta, at the base of the
rocks upon which Aci Reale stands, there are two small caverns in the
abrupt face of the basalt, which can only be approached in a boat. They
consist of columnar basalt bent very curiously, and capped by amorphous
basalt.

A drive of a few miles to the South of Aci Reale brings us to Trezza, a
small village built of lava. A short distance from the shore are the
celebrated _Scogli di Ciclopi_, or rocks of the Cyclops, said to be
those which Polyphemus hurled at Ulysses after his escape from the cave.
The rocks, seven in number, form small islets, the largest of which, the
Isola d'Aci, is about 3000 feet in circumference, and 150 feet high. It
consists of crudely columnar basalt capped by a kind of marl. Near the
top of the island there is a cave called the "Grotto of Polyphemus,"
also a cistern of water. To the south of this island a very picturesque
rock rises from the sea. It is 2000 feet in circumference and about 200
feet in height, and consists of columnar basalt in four and eight-sided
prisms, but not very regular; a hard calcareous substance is found in
their interstices. Fine crystals of analcime are sometimes met with in
the basalts of the Cyclops Islands. Lyell considers these basalts "the
most ancient monuments of volcanic action within the region of Etna."

A few miles south of the Isole di Ciclopi are the bay and city of
Catania. We started from the latter when we commenced our ascent of
Etna, and now on returning to it, we completed the circuit of the
mountain by its base-road of 87 miles.

Katana (~Katane~) is believed to have been founded about 730 B.C.
by a Greek colony of Naxos, which had originally come from Chalcis. The
city maintained its independence till the time of Hieron, who expelled
the original inhabitants in 476 B.C., and peopled the city with
Syracusans and inhabitants of the Peloponnesus to the number of 10,000.
At the same time the name of the city was changed to Aetna ([Greek:
Aitne]). In 461 B.C., however, the old inhabitants retook their city,
and drove out the newly-settled strangers, who betook themselves to
Inessa, occupied it, and changed its name to _Aetna_. At a later period
the Katanians sided with the Athenians against the Syracusans. But in
403 B.C. Dionysius of Syracuse took and plundered the city, sold the
inhabitants as slaves, and established in it a body of Campanian
mercenaries. The latter quitted it and retired to Aetna in 396 B.C.,
when the city was taken by the Carthaginians after a battle off the
rocks of the Cyclops. Katana submitted to the Romans in 263 B.C.,
during the first Punic War, and it soon became a very populous city.
Cicero mentions it as a wealthy city and important seaport. During the
Middle Ages it underwent many changes both at the hands of nature and of
man; it belonged in succession to the Goths, Saracens, and Normans; and
in 1169 was destroyed by an earthquake, during which 15,000 of its
inhabitants perished. Again in 1669, and 1693, it was almost destroyed
by earthquakes. The present town is comparatively new, many of its more
ancient remains are covered with lava, among them the remains of a fine
Greco-Roman theatre, in which it is probable that Alcibiades addressed
the Catanians in 415 B.C. There are also remains of a Roman
amphitheatre, bath, and tombs. Of more modern structures, the cathedral
is the first to claim our notice. It was commenced by Roger I. in 1091,
but in less than a century was almost entirely destroyed by an
earthquake. At one corner of the building you descend through a narrow
passage cut in the lava, to a crypt in which some ancient Roman arches
are shown, partly filled up with lava. Here also is seen a small stream
of very clear water flowing through the lava. The cathedral contains
several interesting tombs, and in the chapel of S. Agata, her body is
preserved in a silver sarcophagus, which during certain fetes is carried
through the town in procession, attended by all the authorities. S.
Agata was martyred by the Praetor Quintianus in the reign of Decius, and
is the patron saint of the city. Whenever Catania has been in trouble
from the approach of lava streams, or from earthquakes, the veil of S.
Agata has been used as a charm to avert the evil.

The University of Catania is the most celebrated in Sicily. It was
founded in 1445 by Alfonso of Arragon, and has produced several men of
eminence. The city also possesses one of the finest monasteries in the
world, now converted into schools and barracks. Formerly the monastery
of S. Nicola was occupied by 40 monks, all members of noble families; it
is sufficiently large to hold 400.




CHAPTER V.

ERUPTIONS OF THE MOUNTAIN.

    Their frequency within the historical period.--525 B.C.--477 B.C.--
    426 B.C.--396 B.C.--140 B.C.--134 B.C.--126 B.C.--122 B.C.--49 B.C.
    --43 B.C.--38 B.C.--32 B.C.--40 A.D.--72.--253.--420.--812.--1169.
    --1181.--1285.--1329.--1333.--1371.--1408.--1444.--1446.--1447.--
    Close of the Fifteenth Century.--1536.--1537--1566.--1579.--1603.--
    1607.--1610.--1614.--1619.--1633.--1646.--1651.--1669.--1682.--1688.
    --1689.--1693.--1694.--1702.--1723.--1732.--1735.--1744.--1747.--
    1755.--Flood of 1755.--1759.--1763.--1766.--1780.--1781.--1787.--
    1792.--1797.--1798.--1799.--1800.--1802.--1805.--1808.--1809.--1811.
    --1819.--1831.--1832.--1838.--1842.--1843.--1852.--1865.--1874.--
    General character of the Eruptions.


A list of all the eruptions of Etna from the earliest times has been
given by several writers, notably by Ferrara in his _Descrizione
dell' Etna_, and by Gemellaro. The latter places the first eruption in
1226 B.C. in the time of the Sicani; the second in 1170 B.C.; and of the
third he says, "In 1149 B.C. there was an eruption, and Hercules in
consequence fled from the island." Of course these dates are worthless,
and the statements are no doubt based upon the assertion of Diodorus,
that before the Trojan war the Sicani were driven from the east side of
Sicily by the eruptions of the volcano.

1. The first eruption appears to have occurred in the time of
Pythagoras; we have no details as to its nature.

2. The second eruption occurred in 477 B.C. It is mentioned by
Thucydides, and it must be the eruption to which Pindar and AEschylus
allude. The former visited the tomb of Hiero I. of Syracuse in 473 B.C.,
and the latter was in Sicily in 471 B.C. On the occasion of this
eruption, two heroic youths named Anapias and Amphinomus,
performed a deed to which Seneca and other writers allude with
enthusiasm. While the lava was rapidly overwhelming the city of Katana,
they placed their aged parents on their shoulders, and, at the risk of
their lives, bore them through the flaming streets, and succeeded in
placing them in safety. It was said that the fiery stream of lava parted
to make way for them. Statues were raised to the honour of the _Pii
Fratres_, and their burial place was long known as the _Campus Piorum_.
Even a temple was erected to commemorate the deed.

Lucilius Junior devotes the concluding lines of his poem on Etna to the
glory of the brothers: "The flames blushed to touch the filial youths,
and wherever they plant their footsteps, they retire. That day is a day
of fortune; harmless that land. On their right hand fierce dangers
prevail; on their left are burning fires. Athwart the flames they pass
in triumph, his brother and he, each safe beneath his filial burden.
There the devouring fire flees backward, and checks itself round the
twin pair. At length they issue forth unharmed, and bear with them their
deities in safety. Songs of poets honour and admire them; them has Pluto
placed apart beneath a glorious name, nor can the mean Fates reach the
holy youths, but have truly granted them the homes and dominion of the
blessed."[18]

[18] Translated by L. E. Upcott, M.A.

3. The third eruption occurred in the year 426 B.C. It is mentioned by
Thucydides as having commenced in the sixth year of the Peloponnesian
War. It destroyed a portion of the territory of the inhabitants of
Katana.

4. An important eruption occurred in the year 396 B.C. It broke out from
Monte di Mojo, the most northerly of the minor cones of Etna, and
following the course of the river Acesines, (now the Alcantara) entered
the sea at the site of the ancient Greek colony of Naxos. Himilco the
Carthaginian general, was at this time on his way from Messana to
Syracuse, and he was compelled to march his troops round the west side
of the mountain in order to avoid the stream of lava.

5. We hear of no further eruption for 256 years, when in the year 140
B.C., in the consulship of C. Laelius Sapiens and Q. Servilius Caepio,
there was an outburst from the volcano which destroyed 40 people.

6. Six years later an eruption occurred according to Orosius and Julius
Obsequens, in the consulship of Sergius Fulvius Flaccus, and Quintus
Calpurnius Piso. We have no details concerning its nature or extent.

7. The same authorities state that in the year 126 B.C. in the
consulship of L. OEmilius Lepidus, and L. Aurelius Orestes, Sicily
suffered from a very severe earthquake, and a deluge of fiery matter
poured from Etna, overwhelming large tracts of country, and rendering
the waters of the adjacent Ionian sea positively hot. It is said that
the sea near the island of Lipari boiled, and that the inhabitants ate
so large a number of the fishes which were cast, already cooked, upon
their shores, that a distemper appeared which destroyed a large number
of people.

8. Four years later Katana was nearly destroyed by a new eruption. The
roofs of many of the houses were broken in by the weight of hot ashes
which fell upon them; but the lava stream turned aside near the city and
flowed into the sea. The lava is believed to have issued from a small
crater near Gravina, about 2-1/2 miles from Katana. The city was so much
injured by this eruption that the Romans granted the inhabitants an
immunity from all taxes for a space of ten years.

9. An eruption, of which we have no details, occurred during the civil
war between Caesar and Pompey.

10. Livy speaks of an eruption and earthquake which took place shortly
before the death of Caesar, which it was believed to portend.

11. In 38 B.C., during the civil war between Octavianus and Sextus
Pompeius, a violent eruption occurred on the east side of the mountain,
accompanied by fearful noises and outbursts of flame.

12. Six years afterwards an eruption of a less violent character took
place.

13. The next eruption of which we hear is that mentioned by Suetonius in
his Life of Caligula. The Emperor happened to be at Messina at the time,
and he fled from the town through fear of the eruption. This was in 40
A.D.

14. An eruption is said to have occurred in 72, in the second year after
the capture of Jerusalem by Titus.

15. Etna was now quiescent for nearly two centuries, but in the year
253, in the reign of the Emperor Decius, a violent eruption lasting nine
days occurred. The lava flowed in the direction of Catania, and the
inhabitants for the first time tested the efficacy of the veil of S.
Agatha, which afterwards stood them in such good stead on more than one
occasion. The Saint had been martyred the year before, and when the
frightened inhabitants saw the stream of lava approaching the city,
they rushed to the tomb, and removed the veil which covered her body.
This was carried to the edge of the descending torrent of lava, and is
asserted to have at once arrested its progress.

16. According to Carrera and Photius an eruption occurred in the year
420.

17. We now find no record of any volcanic action for nearly four hundred
years. Geoffrey of Viterbo states that an eruption occurred in 812, when
Charlemagne was in Messina.

18. After another long interval of more than three centuries and a half,
the mountain again entered into eruption. In February, 1169, occurred
one of the most disastrous eruptions on record. A violent earthquake,
which was felt as far as Reggio, occurred about dawn, and in a few
minutes Catania was a heap of ruins. It is estimated that 15,000 persons
were buried beneath the ruins. It was the vigil of the feast of S.
Agatha, and the Cathedral of Catania was crowded with people, who were
all buried beneath the ruins, together with the Bishop and forty-four
Benedictine monks. The side of the cone of the great crater towards
Taormina fell into the crater. At Messina the sea retired to some
distance from the shore, and then suddenly returned, overwhelming a
portion of the city, and sweeping away a number of persons who had fled
to the shore for safety. The clear and pure fountain of Arethusa at
Syracuse became muddy and brackish; while the fountain of Ajo, near the
village of Saraceni, ceased to flow for two hours, and then emitted
water of the colour of blood. Ludovico Aurelio states that the vines,
corn, and trees were burnt up over large districts.

19. According to Nicolo Speziale, there was a great eruption from the
eastern side of the mountain in 1181.

20. A stream of lava is said to have burst from the eastern side of the
mountain in 1285, when Charles of Anjou was on his death-bed, and to
have flowed fifteen miles.

21. In the year 1329 Niccolo Speziale was in Catania, and witnessed the
eruption of which he has left us an account. On the evening of June
28th, about the hour of vespers, Etna was strongly convulsed, terrible
noises were emitted, and flames issued from the south side of the
mountain. A new crater--Monte Lepre--opened in the Val del Bove above
the rock of Musarra, and emitted large quantities of dense black smoke.
Soon afterwards a torrent of lava poured from the crater, and red-hot
masses of rock were projected into the air. These effects continued till
the 15th of July, when a second crater opened ten miles to the S.E. of
Montelepre, and near the Church of S. Giovanni Paparometto. Soon after
four other craters opened around it, and emitted smoke and lava. The
sun was obscured from morning till evening by the smoke and ashes, and
the adjacent fields were burnt up by the hot sand and ashes. Multitudes
of birds and animals perished, and many persons are said to have died
from terror. The lava streams were divided into three portions, two of
which flowed towards Aci, and the third towards Catania. The ashes were
carried as far as Malta, a distance of 130 miles.

22. Four years afterwards an eruption is recorded by Silvaggio.

23. A manuscript preserved in the archives of the Cathedral of Catania
mentions an eruption which occurred on the 6th of August, 1371, which
caused the destruction of numerous olive groves near the city.

24. An eruption which lasted for twelve days commenced on the 9th of
November, 1408; it originated in the great crater, but several mouths
subsequently opened near the base of the mountain. Large quantities of
red-hot ashes were emitted, some of which fell in Calabria. The villages
of Pedara and Tre Castagne suffered severely from this eruption.

25. A violent earthquake in 1444 caused the upper cone of the mountain
to fall into the crater. A torrent of lava also issued from the
mountain, and moved for a space of twenty days towards Catania, but it
did not reach the city.

26. Two years later lava issued from the Val del Bove near the Rock of
Musarra; the crater then formed was perhaps the present Monte Finocchio.

27. A short eruption, of which we have no details, occurred in 1447:
after which Etna was quiescent for 89 years.

28. Bembo and Fazzello mention an eruption which occurred towards the
close of the 15th century, during which a current of lava flowed from
the great crater, and destroyed a portion of Catania. In 1533 Filoteo,
of whom we have before spoken as one of the earliest historians of Etna,
descended into the crater, which possessed its present funnel-like form.
He found at the bottom a hole, not larger than a man's head, from which
issued a thin moist sulphurous vapour.

29. In March, 1536, a quantity of lava issued from the great crater, and
several new apertures opened near the summit of the mountain and emitted
lava. It divided into several streams, flowing in different directions,
one towards Randazzo, a second towards Aderno, and a third towards
Bronte. The lava swept everything before it; at the same time quantities
of smoke and ashes were ejected, the mountain was convulsed, and fearful
noises were heard. Three new craters were formed on the south and west
sides of the mountain, and on the 26th of March twelve new craters, or
_bocche_, opened between Monte Manfre and Monte Vituri. A physician of
Lentini, named <DW64> di Piazza, having approached too near to the scene
of the eruption, was destroyed by a volley of red-hot stones. Several
rifts were formed in the sides of the mountain from which issued flames
and hot cinders.

30. A year later, in May, 1537, a fresh outburst occurred; a number of
new mouths were opened on the south <DW72> of the mountain near La
Fontanelle, and a quantity of lava was emitted, which flowed in the
direction of Catania, destroying a part of Nicolosi, and S. Antonio. In
four days the lava had run fifteen miles. At the same time violent
shocks of earthquake occurred all over Sicily, the inhabitants thought
that the last day had come, and many prepared for their end by receiving
Extreme Unction. According to Filoteo the noises were so violent that
many persons were struck deaf. The sun was obscured by smoke and dust,
ashes fell in sufficient quantities to destroy the olive plantations of
Messina, and were even carried 300 miles out to sea. The great crater
suddenly fell in, so as to become level with the Piano del Lago. The
height of the mountain was thus diminished by 320 feet.

31. Three new craters opened in November, 1566, on the north-east <DW72>
of the mountain. Quantities of lava were emitted, which flowed towards
Linguaglossa and Randazzo.

32. A slight eruption, of which we have no details, occurred in 1579.

33. According to Carrera, an eruption occurred in June, 1603. The
mountain was shaken with earthquakes, and great volumes of smoke and
flame were emitted.

34. A stream of lava issued from the great crater four years later, and
filled up the lake which had previously existed in the Piano del Lago.

35. In February, 1610, lava was emitted from the great crater. It flowed
towards Aderno, and filled up the bed of the Simeto, a little above the
Ponte di Carcaci. A few months later a second stream destroyed a large
portion of the forest Del Pino.

36. In 1614 several new craters were opened between Randazzo and the
great crater on the north side of the mountain. A quantity of lava
issued from them, which united into one stream, and ran for ten miles,
destroying a great deal of wooded country.

37. A slight eruption occurred in 1619.

38. In February, 1633, Nicolosi was partially destroyed by a violent
earthquake; and in the following December earthquakes became frequent on
the mountain. A new crater opened above the cone called Serrapizzuta,
five miles from the great crater, and emitted a good deal of lava. A
second crater afterwards opened about two miles to the east of the
former. The eruption lasted off and on for four years: the ejected lava
then covered a tract eighteen miles in length by two miles in width,
the thickness sometimes attaining 42 feet. In 1643 a severe earthquake
occurred, which was mainly felt on the west side of the mountain.

39. In 1646 a new mouth opened on the north-north-east side of the
mountain, five miles from the great crater. The lava flowed towards
Castiglione.

40. In February, 1651, several new mouths opened on the west side of the
mountain, and poured out vast volumes of lava which threatened to
overwhelm Bronte. In twenty-four hours the lava ran sixteen miles with a
breadth of four miles.

41. We have a more detailed account of the eruption of 1669 than of any
previous outburst. It was observed by many men of different nations; and
we find accounts of it in our own _Philosophical Transactions_, in
French, and of course in Italian. Perhaps the most accurate and complete
description is that given by Alfonso Borelli, Professor of Mathematics
in Catania. The eruption was, in every respect, one of the most terrible
on record. On the 8th of March the sun was obscured, and a whirlwind
blew over the face of the mountain; at the same time earthquakes
commenced, and continued to increase in violence for three days, when
Nicolosi was converted into a heap of ruins. On the morning of the 11th
a fissure nearly twelve miles in length opened in the side of the
mountain, and extended from the Piano di S. Leo to Monte Frumento, a
mile from the summit. The fissure was only six feet wide, but it seemed
to be of unknown depth, and a bright light proceeded from it. Six mouths
opened in a line with the principal fissure; they emitted vast columns
of smoke, accompanied by loud bellowings which could be heard 40 miles
off. Towards the close of the day, a crater opened about a mile below
the others, and it ejected red hot stones to a considerable distance,
and afterwards sand and ashes which covered the country for a distance
of 60 miles. The new crater soon vomited forth a torrent of lava which
presented a front of two miles, it encircled Monpilieri, and afterwards
flowed towards Belpasso, a town of 8000 inhabitants, which was speedily
destroyed. Seven mouths of fire opened around the new crater, and in
three days united with it, forming one large crater 800 feet in
diameter. The torrent of lava all this time continued to descend, and it
destroyed the town of Mascalucia on the 23rd of March. On the same day
the crater cast up great quantities of sand, ashes, and scoriae, and
formed above itself the great double-coned hill now called Monti Rossi
from the red colour of the ashes of which it is mainly composed. On the
25th very violent earthquakes occurred, and the cone of the great
central crater was shaken down into the crater for the fifth time since
the first century A.D. The original current of lava had divided into
three streams, one of which destroyed S. Pietro, the second
Camporotondo, and the third the lands about Mascalucia, and afterwards
the village of Misterbianco. Fourteen villages were altogether
destroyed, and the lava was on its way to Catania. At Albanelli, two
miles from the city, it undermined a hill covered with cornfields, and
carried it forward a considerable distance; a vineyard was also seen to
be floating on its fiery surface. When the lava reached the walls of
Catania it accumulated without progression until it rose to the top of
the wall, 60 feet in height, and it then fell over in a fiery cascade,
and overwhelmed a part of the city. Another portion of the same stream
threw down 120 feet of the wall, and flowed into the city. On the 23rd
of April the lava reached the sea, which it entered as a stream 600
yards broad and 40 feet deep. The stream had moved at the rate of
thirteen miles in twenty days, but as it cooled it moved less quickly,
and during the last twenty-three days of its course it only moved two
miles. On reaching the sea the water of course began to boil violently,
and clouds of steam arose, carrying with them particles of scoriae.
Towards the end of April the stream on the west side of Catania, which
had appeared to be consolidated, again burst forth, and flowed into the
garden of the Benedictine Monastery of S. Niccola, and then branched
off into the city. Attempts were made to build walls to arrest its
progress. An attempt of another kind was made by a gentleman of Catania,
named Pappalardo, who took fifty men with him, having previously
provided them with skins for protection from the intense heat, and with
crowbars to effect an opening in the lava. They pierced the solid outer
crust of solidified lava, and a rivulet of the molten interior
immediately gushed out, and flowed in the direction of Paterno;
whereupon 500 men of that town, alarmed for its safety, took up arms,
and caused Pappalardo and his men to desist. The lava did not altogether
stop for four months; and two years after it had ceased to flow it was
found to be red hot beneath the surface. Even eight years after the
eruption quantities of steam escaped from the lava after a shower of
rain. The stones which were ejected from the crater during this eruption
were often of considerable magnitude, and Borelli calculated that the
diameter of one which he saw was 50 feet; it was thrown to a distance of
a mile, and as it fell it penetrated the earth to a depth of 23 feet.
The volume of lava emitted during this eruption amounted to many
millions of cubic feet: Ferrara considers that the length of the stream
was at least fifteen miles, while its average width was between two and
three miles, so that it covered at least forty square miles of surface.

In a somewhat rare tract,[19] Lord Winchelsea, who was returning to
England from Constantinople, and who landed at Catania, gives an account
of what he saw of the eruption. He appears to have been frightened at
the sight, and took good care to keep in a safe place; hence his letter,
which is a short one, is mainly founded on hearsay. However, he says, "I
could discern the river of fire to descend the mountain, of a terrible
fiery or red colour, and stones of a paler red to swim thereon, and to
be as big as an ordinary table.... Of 20,000 persons which inhabited
Catania, 3000 did only remain; all their goods are carried away, the
cannon of brass are removed out of the castle, some great bells taken
down, the city gates walled up next the fire, and preparations made by
all to abandon the city." The noble earl is less happy in his scientific
ideas than in his general statement of the facts of which he was an
eye-witness; we can only hope that he joined the recently-formed Royal
Society on his return to England, and listened to Robert Hooke's
discourse on fire. In describing the lava, Lord Winchelsea says, "The
composition of this fire, stones, and cinders, are sulphur, nitre,
quicksilver, sal-ammoniac, lead, iron, brass, and all other mettals!"
Two other accounts are appended to the above letter; in one of these we
are told that as the lava approached Catania, the various religious
bodies carried their relics in procession, "followed by great multitudes
of people, some of them mortifying themselves with whips, and other
signs of penance, with great complaints and cries, expressing their
dreadful expectation of the events of those prodigious fiery
inundations." In the midst of all this, news was brought that a large
band of robbers had taken advantage of the general distress, and were
robbing right and left, and murdering the people: whereupon a troop of
Spanish horse was sent out to protect the city and country, three pair
of gallows were set up, and such as were found robbing were executed
without trial by martial law.

[19] "A true and exact relation of the late prodigious earthquake and
eruption of Mount AEtna or Monte Gibello; as it came in a letter written
to his Majesty from Naples by the Rt. Honble. the Earl of Winchelsea
late Ambassadour at Constantinople, who in his return from thence
visiting Catania in the Island of Sicily, was an eye-witness of that
dreadful spectacle." Published by Authority. Printed by T. Newcomb in
the Savoy. 1669.

As the lava streams approached the city, the Senate, accompanied by the
Bishop and all the clergy, secular and regular, went in procession out
of the city to Monte di S. Sofia with all their relics, etc. There they
erected an altar in view of the burning mountain, and celebrated mass,
"and used the exorcismes accustomed upon such extraordinary occasions,
all which time the mountain ceased not as before with excessive roaring
to throw up its smoak and flames with extraordinary violence, and
abundance of great stones, which were carried through the air."

42. For a few years after this terrible eruption Etna was quiescent, but
in 1682 a new mouth opened on the east side of the mountain, a little
below the summit, and above the Val del Bove. Lava issued from it, and
rushed down the precipices of the Val del Bove as far as the rock of
Musarra.

43. Six years later a torrent of lava burst from an opening in the great
cone, and flowed into the Val del Bove for a distance of three miles.

44. In the following year lava was emitted from a mouth in the Val del
Bove, and it descended for about ten miles, destroying everything in its
course, until it reached a little valley near Macchia.

45. Early in January 1693, clouds of black smoke were poured from the
great crater, and loud noises resembling the discharge of artillery were
heard. A violent earthquake succeeded, and Catania was shaken to the
ground, burying 18,000 of its inhabitants in the ruins. It is said that
in all fifty towns were destroyed in Sicily, together with from 60,000
to 100,000 inhabitants. Lava was emitted from the crater, which was
lowered by the eruption.

46. In the following year Etna again entered into eruption, ejecting
large quantities of ashes, some of which were carried as far as Malta.

47. In March 1702, three mouths opened in the Contrada del Trifoglietto,
near the head of the Val del Bove. Lava was emitted from them, which
flowed into the Valley of Calanna.

48. Towards the end of 1723 loud bellowings issued from the mountain;
earthquakes occurred, and a torrent of lava issued from the crater,
which flowed towards Bronte, through the Bosco di Bronte.

49. A small lava stream issued from the crater in 1732, and descended
the western <DW72> of the mountain, but without producing any damage.

50. In October 1735, the usual noises which presage an eruption were
heard, earthquakes followed, and a little later the crater emitted
flames and red-hot stones. Lava also issued from it, and the stream
divided into three branches, one of which flowed towards Bronte, a
second towards Linguaglossa, and a third towards Mascali; but they did
not get beyond the upper regions of the mountain.

51. In 1744 the mountain threw out great quantities of ashes, but no
lava.

52. In 1747 a quantity of lava flowed from the great crater into the Val
del Bove, and the height of the cone was considerably increased during
the eruption.

53. Early in the year 1755, Etna began to show signs of disturbance; a
great column of black smoke issued from the crater, from which forked
lightning was frequently emitted. Loud detonations were heard, and two
streams of lava issued from the crater. A new mouth opened near the
Rocca di Musarra in the Val del Bove, four miles from the summit, and a
quantity of lava was ejected from it. An extraordinary flood of water
descended from the Val del Bove, carrying all before it, and strewing
its path, with huge blocks. Recupero estimated the volume of water as
16,000,000 cubic feet, probably a greater amount than could be furnished
by the melting of all the winter's snow on the mountain. It formed a
channel two miles broad, and, in some places, thirty-four feet deep, and
it flowed at the rate of a mile in a minute and a half during the first
twelve miles of its course. Lyell considers the flood was probably
produced by the melting, not only of the winter's snow, but also of
older layers of ice, which were suddenly melted by the permeation of hot
steam and lava, and which had been previously preserved from melting by
a deposit of sand and ashes, as in the case of the ancient glacier found
near the summit of the mountain in 1828. In November 1758, a smart shock
of earthquake caused the cone of the great crater to fall in, but no
eruption occurred at the time.

54. Great quantities of ashes, and some small streams of lava, were
emitted from the crater in 1759, a little later the cone, which had been
again raised by the eruption, gave way, and the greater part of it fell
into the crater. Two parts of it however were left standing.

55. Severe shocks of earthquakes were felt on the east side of the
mountain in 1763, and a new mouth opened in the Bosco di Bronte, ten
miles from the town, between Monte Rosso and Monte Lepre. Four other
mouths were afterwards opened in a line; they threw up quantities of
scoriae and ashes, and afterwards lava. In the middle of June several
mouths opened on the south side of the mountain, and a fissure 2000 feet
long opened downwards in a southerly direction. The lava divided into
two branches, the larger of which was ten miles long and 250 feet wide,
with a depth of 25 feet.

56. Several new mouths opened in the spring of 1766, and ejected large
volumes of ashes, also streams of lava, which flowed in the direction of
Nicolosi and Pedara. The Canon Recupero, one of the historians of Etna,
witnessed this eruption, and narrowly escaped being destroyed. He had
ascended a small hill 50 feet high, of ancient volcanic matter, in order
to witness the approach of the lava stream which was slowly advancing
with a front of two miles and a half. Suddenly two small streams
detached themselves from the main stream, and ran rapidly towards the
hill. Recupero and his guide at once hastened to descend, and had
barely escaped when they saw the hill surrounded by lava, and in a few
minutes it was melted down and sank into the molten mass.

57. In the early part of 1780, earthquakes were felt all over Sicily,
and on the 18th of May a fissure opened on the south-west side of the
mountain, and extended from the base of the great crater for seven
miles, terminating in a new mouth from which a stream of lava emanated.
This encountered the cone of Palmintelli in its course, and separated
into two branches, each of which was 400 feet wide. Other mouths opened
later in the year, and emitted large quantities of lava, which
devastated the country of Montemazzo.

58. In 1781 the volcano emitted a quantity of lava which flowed into the
Val del Bove. Clouds of grey ashes were also ejected. At the
commencement of the great Calabrian earthquake of 1783, Etna ejected
large quantities of smoke, but it was otherwise quiescent.

59. In the middle of 1787 lava burst from the great crater, which also
discharged quantities of sand, scoriae, and red-hot ashes. Large heated
masses of rock were ejected to a great height, and subterranean
bellowings were heard by the dwellers on the mountain.

60. Five years afterwards a fresh outburst occurred, earthquakes were
prevalent, and vast volumes of smoke bore to seaward, and seemed to
bridge the sea between Sicily and Africa. A torrent of lava flowed
towards Aderno, and a second flowed into the Val del Bove as far as
Zoccolaro. A pit called _La Cisterna_, 40 feet in diameter, opened in
the Piano del Lago, near the great cone, and ejected smoke and masses of
old lava saturated with water. Several mouths opened below the crater,
and the country round about Zaffarana was desolated. The Abate Ferrara,
the author of the _Descrizione dell' Etna_, witnessed this eruption: "I
shall never forget," he writes, "that this last mouth opened precisely
on the spot where, the day before, I had made my meal with a shepherd.
On my return next day he related how, after a stunning explosion, the
rocks on which we had sat together were blown into the air, and a mouth
opened, discharging a flood of fire, which, rushing down with the
rapidity of water, hardly gave him time to make his escape."

61. In 1797 a slight eruption occurred, and the great crater threw out
ashes and sand, but no lava. Earthquakes were frequent.

62. In the following year lava was emitted, and severe earthquakes
occurred.

63. The eruptions continued during 1799.

64. In February 1800 loud explosions were heard by the dwellers on the
mountain, and columns of fire issued from the crater, accompanied by
forked lightning. This was succeeded by a discharge of hot ashes and
scoriae, which, falling on the snows accumulated near the summit of the
mountain, produced devastating floods of water.

65. In November 1802 a new mouth opened near the Rocca di Musarra in the
Val del Bove, which emitted a copious stream of lava. In a day and a
half the lava had run twelve miles.

66. In 1805 the great crater was in a state of eruption, and a cone was
thrown up within it to a height of 1,050 feet.

67. In 1808 the mountain again became active, and fire and smoke were
emitted from the crater.

68. In March 1809, no less than twenty-one mouths of fire opened in the
direction of Castiglione. They ejected volumes of smoke, large
quantities of scoriae and ashes, and afterwards lava, which, uniting into
one torrent, flowed with a front of 450 feet for 8 miles. Fissures were
formed in the earth, and loud explosions constantly occurred within the
great crater; a small cone was thrown up.

69. Two years afterwards more than thirty mouths opened in a line
running eastwards for five miles. They ejected jets of fire accompanied
by much smoke. The eruptions soon diminished in the higher mouths, and
became more and more violent in the lower mouths, until the eruption
centred in the lowest one called S. Simone, near the head of the Val del
Bove. From this, great black clouds, having a lustre like that of black
wool, issued, and afterwards quantities of lava, which formed a stream
a mile wide, and eight miles long. It flowed nearly as far as the
village of Milo. Frequent earthquakes accompanied this outburst, and
they continued in various parts of the island for the following five
years.

70. In 1819 five new mouths of fire opened near the scene of the
eruption of 1811; three of these united into one large crater, and
poured forth a quantity of lava into the Val del Bove. The lava flowed
until it reached a nearly perpendicular precipice at the bend of the
valley of Calanna, over which it fell in a cascade, and, being hardened
by its descent, it was forced against the sides of the tufaceous rock at
the bottom, so as to produce an extraordinary amount of abrasion,
accompanied by clouds of dust, worn off by the friction. Mr. Scrope
observed that the lava flowed at the rate of about a yard an hour, nine
months after its emission.

71. A slight eruption occurred in 1831 from the great crater, which
threw out lava on its northern side.

72. In October of the following year a violent eruption occurred. A new
crater was formed in the Val del Serbo, above Bronte and three miles
from the summit. Seven mouths afterwards opened, three miles below the
first. From one of these lava was emitted, which flowed to within a mile
and a half of Bronte. The stream was a mile and a half broad, and 40
feet deep.

73. A slight eruption occurred in 1838, when a small quantity of lava
was poured from the great crater into the Val del Bove.

74. Four years later the crater discharged ashes and scoriae, and lava
burst from the cone 300 feet from the summit. It flowed into the Val del
Bove, in a stream 600 feet wide, and it came to a standstill ten miles
from the summit.

75. Near the end of the following year, fifteen mouths of fire opened
near the crater of 1832, at a height of 7000 feet above the sea. They
began by discharging scoriae and sand, and afterwards lava, which divided
into three streams, the two outer ones soon came to a standstill, while
the central stream continued to flow at the rapid rate of 180 feet a
minute, the descent being an angle of 25 deg.. The heat at a distance of 120
feet from the current was 90 deg. F. A new crater opened just above Bronte,
and discharged lava which threatened the town, but it fortunately
encountered Monte Vittoria and was diverted into another course. While a
number of the inhabitants of Bronte were watching the progress of the
lava, the front of the stream was suddenly blown out as by an explosion
of gunpowder; in an instant red-hot masses were hurled in every
direction; and a cloud of vapour enveloped everything. Thirty-six
persons were killed on the spot, and twenty survived but a few hours.
The great crater showed signs of disturbance, by emitting dense volumes
of smoke, and loud bellowings, also quantities of volcanic dust
saturated with hydrochloric acid, which destroyed the vegetation
wherever it fell.

76. A very violent eruption which lasted more than nine months,
commenced on the 21st of August, 1852. It was first witnessed by a party
of six English tourists, who were ascending the mountain from Nicolosi
in order to see the sunrise from the summit. As they approached the Casa
Inglesi the crater commenced to give forth ashes and flames of fire. In
a narrow defile they were met by a violent hurricane, which overthrew
both the mules and their riders, and urged them towards the precipices
of the Val del Bove. They sheltered themselves beneath some masses of
lava, when suddenly an earthquake shook the mountain, and their mules in
terror fled away. They returned on foot towards daylight to Nicolosi,
fortunately without having sustained injury. In the course of the night
many _bocche del fuoco_ opened in that part of the Val del Bove called
the Balzo di Trifoglietto, and a great fissure opened at the base of the
Giannicola Grande, and a crater was thrown up from which for seventeen
days showers of sand and scoriae were ejected. During the next day a
quantity of lava flowed down the Val del Bove, branching off so that one
stream advanced to the foot of Monte Finocchio, and the other to Monte
Calanna. Afterwards it flowed towards Zaffarana, and devastated a large
tract of woody region. Four days later a second crater was formed near
the first, from which lava was emitted together with sand and scoriae,
which caused cones to rise around the craters. The lava moved but
slowly, and towards the end of August it came to a stand, only a quarter
of a mile from Zaffarana: on the second of September, Gemellaro ascended
Monte Finocchio in the Val del Bove in order to witness the outburst. He
states that the hill was violently agitated, like a ship at sea. The
surface of the Val del Bove appeared like a molten lake; scoriae were
thrown up from the craters to a great height, and loud explosions were
heard at frequent intervals. The eruption continued to increase in
violence. On October 6th two new mouths opened in the Val del Bove,
emitting lava which flowed towards the Valley of Calanna, and fell over
the Salto della Giumenta, a precipice nearly 200 feet deep. The noise
which it produced was like that of the clash of metallic masses. The
eruption continued with abated violence during the early months of 1853,
and it did not finally cease till May 27. The entire mass of lava
ejected is estimated to be equal to an area six miles long by two miles
broad, with an average depth of about twelve feet.

I am indebted to M. Antonin Moris of Palermo for the following account
of the eruption of 1852:

The eruption of 1852 commenced on the 21st of August. The earthquakes,
the jets of flame from the great crater, and the subterranean rumblings
which usually precede an eruption, did not herald the approach of this
one. An English family, who were then making the ascent of the mountain,
together with a poor shepherd of Riposto, were the only witnesses of the
first outburst. The latter was asleep in the midst of his flocks, and
was awakened by violent shakings of the ground; he fled in haste, and
some seconds afterwards the earth opened with a loud noise, vomiting a
terrible column of fire, at the very spot which he had just abandoned.
An enormous crevasse opened on the north side of Trifoglietto in the
direction of the great crater. On its summit near the opening called the
Piccolo Teatro, several openings were produced at the very first, but
they only emitted feeble currents of lava. All the force of the eruption
was concentrated at the foot of the escarpment of the Serra di
Giannicola, 4 kilometres, (2-1/2 miles) from the summit of Etna. To the
west of, and somewhat above the principal crater, a second one was
formed, but its activity was of short duration. The liquid lava issued
with such violence that in 24 hours it had reached the base of Monte
Calanna, a distance of 3 kilometres, (nearly 2 miles). After surrounding
this hill, it divided into two currents, one of which ran towards
Zaffarana, and the other towards Milo. At a distance they seemed to
present a united front of 2 kilometres, (1-1/4 mile), which threatened
to destroy all the villages below. The Val del Bove was already
entirely overrun; Isoletta dei Zappinelli in the midst of the lavas of
1811 and 1819 was overwhelmed; the valley of Calanna was buried under
the fire with lava, when on the 28th of August the lava hurled itself
into the narrow passage of the Portella di Calanna. A frightful cascade
of lava was then seen to precipitate itself from a height of 60 metres,
with a harsh metallic noise, accompanied by loud cracking. Zaffarana was
on the eve of total ruin; the fire had taken the direction of the ravine
which terminates there, when suddenly, in the beginning of September,
the devastating stream stayed its march against the ill-fated district.

On the contrary that which had taken the direction of Milo, reinforced
by a new current on the 10th of September, destroyed the hamlet of
Caselle del Milo; and afterwards divided itself into two branches, which
left the village of Caselle in safety between them.

The inhabitants of La Macchia and Giarre gave themselves up for lost;
for it seemed that the lava would be obliged to follow the valley of
Santa Maria della Strada; happily, however, from the 20th of September
onward, it ceased to advance perceptibly. The eruption did not totally
subside till March 1853; but the lava-flows did no more than travel by
the side, or on the top of the older, without extending beyond them.

The crater of 1852 was called the Centenario, from its having been
formed at the time of the centenary of the fete of S. Agatha. Santiago,
in the island of Cuba, was destroyed by an earthquake on the very day of
the eruption.

During the whole period of the eruption, only one explosion proceeded
from the great crater of Etna. By it an enormous column of ashes and
scoriae was cast into the air.

On the 9th of September white ashes were seen on the summit, which at a
distance appeared like snow. When pressed together by the hand they took
the consistence of clay, but they hardened in the fire, and could then
be reduced to powder. They have been considered to be the _debris_ of
felspathic rocks, disintegrated by the heat of the lava, and blown out
by the expansive power of disengaged gas.

The eruption of 1852 was one of the grandest of the recorded eruptions
of Etna. More than 2,000,000,000 cubic feet of red hot lava was spread
over three square miles. This eruption was minutely described by Carlo
Gemellaro, in a memoir entitled, "_Breve ragguaglio della eruzione
dell' Etna del 21 Agosto, 1852_."

77. In October 1864, frequent shocks of earthquakes were felt by the
dwellers on Etna. In January clouds of smoke were emitted by the great
crater, and roaring sounds were heard. On the night of the 30th a
violent shock was felt on the north-east side of the mountain, and a
mouth opened below Monte Frumento, from which lava was ejected. It
flowed at a rate of about a mile a day, and ultimately divided into two
streams. By March 10th the new mouths of fire had increased to seven in
number, and they were all situated along a line stretching down from the
summit. The three upper craters gave forth loud detonations three or
four times a minute. Professor Orazio Silvestri has devoted a quarto of
267 pages to an account of _I Fenomeni Vulcanici presentati dall'Etna
nel 1863-64-65-66_.

78. In August 1874 the inhabitants of the towns situated on the north,
west, and east sides of the mountain, were awakened by loud subterranean
rumblings. Soon afterwards a formidable column of black smoke issued
from the crater, accompanied by sand, scoriae, and ignited matter
(_infuocata materia_). Severe shocks of earthquake were felt, the centre
of impulsion being apparently situated on the northern flank of the
mountain, at a height of 2450 metres above the level of the sea. Some
small _bocche eruttive_ opened near the great crater, and ejected lava,
but the quantity was comparatively small, and but little damage was
done. An account of this eruption was given by Silvestri in 1874, in a
small pamphlet entitled, _Notizie sulla eruzione dell' Etna del 29
Agosto, 1874_. Since 1874 the mountain has been in a quiescent state.
The centre of disturbance was at an elevation of 2450 metres (7600 feet)
above the sea, on the north side of the crater, and between the minor
cones known as the _Fratelli Pii_ and _Monte Grigio_. A new crater,
having an elliptical contour, and a diameter of about 100 metres, was
formed at this point. It is composed of a prehistoric grey labradorite,
and of doleritic lava. Downwards from the main crater, in the direction
of Monte di Mojo, a long fissure extended for 400 metres, and along the
line of this fissure no less than _thirty-five_ minor cones opened, with
craters of from thirty to three metres in diameter. The stream of lava
ejected from the various _boccarelle_ was 400 metres long, 80 wide, and
2 metres in thickness, and the bulk of volcanic material brought to the
surface, including the principal cone and its thirty-five subordinates
and their ejectamenta, was calculated to amount to 1,351,000 cubic
metres. The lava is of an augitic character, and magnetic; it possesses
a specific gravity of 2.3636 at 25 deg. C.

It will be seen from the account of the foregoing eruptions that there
is a great similarity in the character of the eruptions of Etna.
Earthquakes presage the outburst; loud explosions follow, rifts and
_bocche del fuoco_ open in the sides of the mountain; smoke, sand,
ashes, and scoriae are discharged, the action localises itself in one or
more craters, cinders are thrown up, and accumulate around the crater
and cone, ultimately lava rises, and frequently breaks down one side of
the cone, where the resistance is least. Then the eruption is at an
end.

Smyth says, "The symptoms which precede an eruption are generally
irregular clouds of smoke, ferilli, or volcanic lightnings, hollow
intonations, and local earthquakes that often alarm the surrounding
country as far as Messina, and have given the whole province the name of
Val Demone, as being the abode of infernal spirits. These agitations
increase until the vast cauldron becomes surcharged with the fused
minerals, when, if the convulsion is not sufficiently powerful to force
them from the great crater (which, from its great altitude and the
weight of the candent matter, requires an uncommon effort), they explode
through that part of the side which offers the least resistance with a
grand and terrific effect, throwing red-hot stones and flakes of fire to
an incredible height, and spreading ignited cinders and ashes in every
direction." After the eruption of ashes, lava frequently follows,
sometimes rising to the top of the cone of cinders, at others breaching
it on the least resisting side. When the lava has reached the base of
the cone, it begins to flow down the mountain, and being then in a very
fluid state, it moves with great velocity. As it cools the sides and
surface begin to harden, its velocity decreases, and in the course of a
few days it only moves a few yards in an hour. The internal portions,
however, part slowly with their heat, and months after the eruption,
clouds of steam arise from the black and externally cold lava beds after
rain, which, having penetrated through the cracks, has found its way to
the heated mass within.

Of the seventy-eight eruptions described above, it will be noticed that
not more than nineteen have been of extreme violence, while the majority
have been of a slight and comparatively harmless character.

[Illustration: Geological Map of Etna]




CHAPTER VI.

GEOLOGY AND MINERALOGY OF THE MOUNTAIN.

    Elie de Beaumont's classification of rocks of Etna.--Hoffman's
    geological map.--Lyell's researches.--The period of earliest
    eruption.--The Val del Bove.--Two craters of eruption.--Antiquity of
    Etna.--The lavas of Etna.--Labradorite.--Augite.--Olivine.--
    Analcime.--Titaniferous iron.--Mr. Rutley's examination of Etna
    lavas under the microscope.


The opinion of geologists is divided as to the manner in which a volcano
is first formed. Some hold that the volcanic forces have upraised the
rocks from beneath, and at last finding vent have scattered the lighter
portions of such rocks into the air, and have poured out lava through
the rent masses, thus forming a _crater of elevation_. Others maintain
that the volcanic products are ejected from an aperture or fissure
already existing in rocks previously formed, and that the accumulation
of these products around the vent forms the mass of the volcano and the
_crater of eruption_. Lyell favours the latter view; Von Buch, Dufrenoy,
and Elie de Beaumont the former.

According to M. Elie de Beaumont, Etna is an irregular crater of
elevation. The original deposits were nearly horizontal, and lavas were
poured through fissures in these, and accumulated at first in layers;
afterwards the whole mass was upheaved and a crater formed.[20] The
upheaving force does not appear to have acted at one point, but along a
line traversing the Val del Bove. The latter he refers to a subsidence
of a portion of the mountain. He divides the rocks of Etna into six
orders: 1. The lowest basis of the mountain would appear to consist of
granite, because masses of that rock have from time to time been
ejected. 2. Calcareous and arenaceous rocks, of which the mountains
surrounding Etna are composed, and which appear capped with lava near
Bronte and elsewhere. 3. Basaltic rocks, which are met with near Motta
S. Anastasia, Paterno, Licodia, and Aderno, and in the Isole de'Ciclopi.
4. Rolled pebbles, which form a range of slightly rising ground between
the first <DW72>s of Etna on the southern side and the plain of Catania.
(Lyell speaks of this rising ground as consisting of "argillaceous and
sandy beds with marine shells, nearly all of living Mediterranean
species, and with associated and contemporaneous volcanic rocks.") 5.
Ancient lavas forming the escarpments around the Val del Bove; and 6th,
Modern lavas. He considers that the fissures which abound on Etna are
shifts or faults produced by dislocation, and that the minor cones are
points along such fissures from which ashes and lava have been ejected.
He admits the existence of two cones. The geological map of Etna
prepared by M. Elie de Beaumont to accompany his memoir can scarcely be
regarded as a great addition to our knowledge of the mountain. For
although in the main points it is correct, so many details have been
omitted that the map must be considered to have now been quite
superseded by those of Von Waltershausen and Friedrich Hoffmann.

[20] "Recherches sur la structure et sur l'origine du Mont Etna." 1836.

The most convenient geological map of the mountain is without doubt that
of Hoffmann, given in the _Vulkanen Atlas_ of Dr. Von Leonhard; and here
reproduced. Von Waltershausen's geological map has been the foundation
of all others which have subsequently appeared. It is a marvel of
accurate work, and patient industry. The form however is inconvenient,
as it nowhere appears as a whole, but in separate portions, which are
scattered through the folio sheets of the very expensive _Atlas des
Aetna_. It is accurate, and at the same time very clear and
intelligible. By reference to the map it will be seen that from Capo di
Schiso westward, to near Paterno, Etna is surrounded by sandstone hills;
at the south we have recent clays, and, at intervals, chalk. A large
triangular space having the two angles at its base, respectively near
Maletto and Aderno, and its apex at the great crater, is covered with
new lava; while around Nicolosi there is volcanic sand. At the Isole
de'Ciclopi, Motta S. Anastasia, and a few other places, basalt is seen;
on each side of the Val del Bove, dolerite; and near Misterbianco and
Piedemonte, small deposits of clay slate. The great mass of the surface
of the mountain, not specially mentioned above, is volcanic tuff.

[Illustration: Map of the Val del Bove, to illustrate the theory of a
double axis of eruption. (_Lyell_).]

Among the more important and recent additions to our knowledge of the
geology of Etna may be mentioned Lyell's paper on the subject,
communicated to the Royal Society in 1858, the matter of which is
incorporated in a lengthy chapter on Etna in the "Principles of
Geology." Lyell visited the mountain in 1828, 1857, and 1858, and he
then collected together a great number of personal observations; he also
made use of the maps and plans of Von Waltershausen, and he has analysed
the views of Elie de Beaumont and other writers. He alludes at the
outset to the numerous minor cones of Etna produced by lateral eruption,
and points out the fact that they are gradually obliterated by the lava
descending from the upper part of the mountain, which flows around them
and heightens the ground on which they stand. In this way the crater of
Monte Nocilla is now level with the plain, and the crater of Monte
Capreolo was nearly filled by a lava stream in 1669. Thus without
doubt beneath the sloping sides of Etna a multitude of obliterated
monticules exist.

[Illustration: Ideal section of Mount Etna]

The strata which surround Mount Etna on the south are of Newer Pliocene
date, and contain shells which are nearly all of species still living in
the Mediterranean. Out of sixty-five species collected by Lyell in 1828,
sixty-one were found to belong to species still common in the
Mediterranean. These strata are about the age of the Norwich crag; and
the oldest eruptions of Etna must have taken place during the glacial
period, but before the period of greatest cold in Northern Europe.

Before visiting Etna, Lyell had been told by Dr. Buckland that in his
opinion the Val del Bove was the most interesting part of Etna,
accordingly he specially and minutely examined that part of the
mountain. This vast valley is situated on the eastern flanks of the
mountain, and it commences near the base of the cone, stretching for
nearly five miles downwards. It is a large oval basin formed in the side
of the mountain, and surrounded by vast precipices, some of which at the
head of the valley are between three and four thousand feet in height.
The surface is covered with lava of various dates, and several minor
cones, notably those of 1852, are within its boundaries. The abrupt
precipices reveal the presence of a large number of vertical dikes,
radiating from a point within the valley, some of them, according to Von
Waltershausen, being of ancient greenstone. Other dikes of more modern
doleritic lava radiate from the present crater. From the <DW72> of the
beds in the Val del Bove, Lyell and Von Waltershausen have independently
inferred that there was once a second great centre of eruption in the
Val del Bove between the Sierra Giannicola, and Zoccolaro (_vide_ the
Figure on p. 117). The axis of eruption passing through this point Lyell
calls the _Axis of Trifoglietto_; while he distinguishes the present
centre of eruption as the _Axis of Mongibello_. These centres probably
existed simultaneously, but were unequal as regards eruptive violence;
the crater of Mongibello was the more active of the two, and eventually
overwhelmed the crater of Trifoglietto with its products, by which means
the whole mountain became a fairly symmetrical cone, having the crater
of Mongibello at its apex (_vide_ the Figures on pp. 119 and 121).
Subsequently the Val del Bove was formed, probably by some paroxysmal
explosion, caused by pent-up gases escaping from fissures. Possibly also
subsidence may have occurred.

[Illustration: Profile of Etna]

We must then in the first place think of Etna as a submarine volcano
of the Newer Pliocene age; when it reached the surface it increased
rapidly in bulk by pouring out scoriae and lava from its two centres
of eruption--the centre of Mongibello, and the centre of
Trifoglietto,--general upheaval of the surrounding district followed,
and ultimately the crater of Trifoglietto was obliterated by the
discharges from the crater of Mongibello. Afterwards the Val del Bove
was blown out by sudden eruptive force from beneath, and the mountain
assumed its present aspect. Then the historical eruptions commenced,
and of these we have given an account in the preceding chapter.

The most obvious method of obtaining some idea as to the age of Etna, is
to ascertain the thickness of matter added during the historical period
to the sides of the mountain, and to compare this with the thickness of
the beds of ancient lava and scoriae exposed at the abrupt precipices of
the Val del Bove. There is reason for believing, however, that none of
the ancient lavas equalled in volume the lava streams of 1809 and 1852,
and the question is much complicated by other considerations. Lyell
compares the growth of a volcano to that of an exogenous tree, which
increases both in bulk and height by the external application of
ligneous matter. Branches which shoot out from the trunk, first pierce
the bark and proceed outwards, but if they die or are broken off they
become inclosed in the body of the tree, forming knots in the wood.
Similarly the volcano consists of a series of conical masses placed one
above the other, while the minor cones, corresponding to the branches of
the tree, first project, and then become buried again, as successive
layers of lava flow around them. But volcanic action is very
intermittent, the layers of lava and scoriae do not accumulate evenly and
regularly like the layers of a tree. A violent paroxysmal outbreak may
be succeeded by centuries of quiescence, or by a number of ordinary
eruptions; or, again, several paroxysmal outbreaks may occur in
succession. Moreover, each conical envelope of the mountain is made up
of a number of distinct currents of lava, and showers of scoriae. "Yet we
cannot fail to form the most exalted conception of the antiquity of this
mountain, when we consider that its base is about 90 miles in
circumference; so that it would require ninety flows of lava, each a
mile in breadth at their termination, to raise the present foot of the
volcano as much as the average height of one lava current." If all the
minor cones now visible on Etna could be removed, with all the lava and
scoriae which have ever proceeded from them, the mountain would appear
scarcely perceptibly smaller. Other cones would reveal themselves
beneath those now existing. Since the time when, in the Newer Pliocene
period, the foundations of Etna were laid in the sea, it is quite
impossible even to hint at the number of hundreds of thousands of years
which have elapsed.

We collected specimens of lava from various points around and upon the
mountain. They presented a wonderful similarity of structure, and a
mineralogist to whom they were shown remarked that they might almost
all have come from the same crater, at the same time. A specimen of the
lava of 1535 found near Borello, was ground by a lapidary until it was
sufficiently transparent to be examined under the microscope by
polarised light. It was found to contain good crystals of augite and
olivine, well striated labradorite, and titaniferous iron ore.

Elie de Beaumont affirms that the lavas of Etna consist of labradorite,
pyroxene (augite), peridot (olivine), and titaniferous iron. Rose was
the first to prove that the lavas of Etna do not contain ordinary
felspar (or potash felspar), but labradorite (or lime felspar.)
(_Annales des Mines_, 3 serie, t. viii., p. 3.) Elie de Beaumont
detached a quantity of white crystals from the interior of a lava found
between Giarre and Aci Reale; these were analysed by M. Auguste Laurent
with the following results in 100 parts:--

    Silica            47.9
    Alumina           34.0
    Oxide of Iron      2.4
    Soda (Na{2}O)      5.1
    Potash (K{2}O)      .9
    Lime               9.5
    Magnesia            .2
                     -----
                     100.0

Von Waltershausen gives the following as the composition of two
specimens of Labradorite from Etna:--

                            I.               II.

    Silica                53.56             55.83
    Alumina               25.82             25.31
    Sesquioxide of Iron    3.41              3.64
    Magnesia                .52               .74
    Lime                  11.69             10.49
    Soda                   4.09              3.52
    Potash                  .54               .83
    Water                   .95                --
                         ------            ------
                         100.58            100.36

Specimens of Augite from Etna have been examined by Von Waltershausen
and Rammelsberg, with the following results:--

                                   _Greenish_   _From_       _From_
                         _Black._   _Black._   _Mascali._ _Monti Rossi._

  Silica                  47.63      51.70       49.69       47.38
  Alumina                  6.74       4.38        5.22        5.52
  Protoxide of Iron       11.39       4.24       10.75        7.89
      "        Manganese    .21         --          --         .10
  Magnesia                12.90      21.11       14.74       15.29
  Lime                    20.87      18.02       18.44       19.10
  Sesquioxide of Iron        --         --          --        3.85
  Water                     .28        .49         .51         .43
                         ------      -----       -----       -----
                         100.02      99.94       99.35       99.56

Olivine is generally met with in the lavas of Etna. It has an olive, or
bottle-glass green colour, and is disseminated through the lavas in the
form of small crystalline grains, sometimes of some magnitude. Specific
gravity 3.334. A specimen from Etna gave the following results on
analysis:--

    Silica              41.01
    Protoxide of Iron   10.06
    Magnesia            47.27
    Alumina               .64
    Oxide of Nickel       .20
    Water                1.04
                       ------
                       100.22

The titaniferous iron of Etna is found disseminated through the mass of
the lavas, and is plainly distinguished when a thin section is examined
under the microscope. It is sometimes met with in masses. A specimen
from Etna, analysed by Von Waltershausen, was found to contain:--

    Titanic Acid          11.14
    Sesquioxide of Iron   58.86
    Protoxide of Iron     30.00
                         ------
                         100.00

The basalts of the Isole de'Ciclopi enclose beautiful transparent
crystals of Analcime, the _zeolite dure_ of Dolomieu. The word is
derived from ~analkis~ weak, in allusion to the weak electric
power which the mineral acquires when heated or rubbed. Dana prefers the
term _analcite_. Specimens from the Cyclops Islands have been analysed
by Von Waltershausen and Rammelsberg, with the following results:--

                             I.        II.       III.

    Silica                 53.72      55.22      54.34
    Alumina                24.03      23.14      23.61
    Lime                    1.23        .25        .21
    Soda (Na{2}O)           7.92      12.19      12.95
    Potash (K{2}O)          4.46       1.52        .66
    Water                   8.50       7.68       8.11
    Magnesia                 .05         --         --
    Sesquioxide of Iron       --         --        .12
                           -----     ------     ------
                           99.91     100.00     100.00

The minerals of Etna are not nearly as numerous as those of Vesuvius. It
has been remarked that no area of equal size on the face of the globe
furnishes so many different species of minerals as Vesuvius and its
immediate neighbourhood. Out of the 380 species of simple minerals
enumerated by Hauy, no less than 82 had been found on and around
Vesuvius, as long ago as 1828, and many have been since found.

Of other common products of Etna, there are sulphur in various forms,
sulphurous acid gas, ammonia salts, hydrochloric acid gas, and steam. A
curious white mass, which we found near the summit, proved to be the
result of the decomposition of lava by hot acid vapours. In the
different lavas, the crystals of labradorite, and of olivine, vary in
size considerably. Magnetic oxide of iron is very visible in thin
slices of the lavas when placed under the microscope; and iron appears
to be a constant constituent in nearly all the products of the mountain.

Within the last few months Prof. Silvestri has detected a mineral oil in
the cavities of a prehistoric doleritic lava found near Paterno.[21] The
lava is in close contiguity to the clay deposits of a mud volcano, and
when examined under the microscope is seen to consist mainly of augite,
together with olivine and transparent crystals of labradorite. It
contains numerous cavities coated with arragonite, and filled with a
mineral oil which constitutes about one per cent of the whole weight of
the lava. It was taken from the lava at a temperature of 24 deg. C., (75.2 deg.
F.), and solidified at 17 deg. C. (62.6 deg. F.) to a yellowish green mass,
which on analysis gave the following percentage composition:--

    Liquid hydrocarbons boiling at 79 deg. C.            = 17.97
    Hydrocarbons solidifying below 0 deg. C., boiling }
      between 280 deg. and 400 deg. C.                    }  = 31.95
    Paraffine melting between 52 deg. and 57 deg. C.         = 42.79
    Asphalt containing 12 per cent of ash            =  2.90
    Sulphur                                          =  4.32
                                                      ------
                                                       99.93

[21] "Atti Accademia Gioenia," serie iii., vol. xii.

Prof. Silvestri has recently made some interesting determinations of the
specific gravity and chemical composition of the different products of
Etna. They are given in full in his work entitled, "_I Fenomeni
Vulcanici presentati dall'Etna, nel 1863, 1864, 1865, 1866_," which was
published in Catania in 1867. The following table gives the specific
gravity of various ancient and modern forms of lava, ashes, etc. of
Etna:--

                                               _Sp. Gr._

    Ashes ejected in 1865                        2.644
    Sand     "     "   "                         2.715
    Scoriae   "     "   "                         2.633
    Compact lava   "   "                         2.771
    Scoriae ejected in 1669                       2.622
    Compact lava   "   "                         2.697
    Lapilli ejected in 1444                      2.420
    Compact lava ejected in prehistoric times    2.854

A very decided change in the specific gravity was found to take place
after fusion. This can only be accounted for on the supposition that a
chemical change is effected during the fusion:--

                                _Sp. Gr._               _Sp. Gr._
                             _before fusion._        _after fusion._

    Pyroxene of Etna              3.453                  2.148
    Felspar   "   "               2.925                  1.361
    Olivine   "   "               3.410                  2.290
    Lava of 1865                  2.771                  1.972
    Ancient basaltic lava from }  2.854                  2.000
      the Scogli de'Ciclopi    }
    Ancient basaltic lava from }  2.795                  1.947
      Aci Reale                }

It will be seen from the following analyses that the sand, ashes,
scoriae, and compact lava have virtually the same composition--indeed
they consist of the same substance in different states of aggregation.

                           _Ashes._  _Sand._  _Scoriae._  _Compact lava._

    Silica                  50.00     49.80     50.00        49.95
    Alumina                 19.08     18.20     19.00        18.75
    Protoxide of iron       12.16     12.42     11.70        11.21
    Protoxide of Manganese    .40       .45       .50          .49
    Lime                     9.98     11.00     10.28        11.10
    Magnesia                 4.12      4.00      4.20         4.05
    Potash                    .60       .49       .69          .70
    Soda                     3.72      3.60      3.40         3.71
    Water                     .36       .29       .33          .23
    Phosphoric acid      }
    Titanic acid         } traces    traces    traces       traces
    Vanadic acid         }
    Sesquioxide of iron  }
                           ------    ------    ------       ------
                           100.42    100.25    100.10       100.19

With these we may compare the composition of the lava which issued from
Monti Rossi in 1669, and was analysed by Lowe, and of an ancient lava of
Etna ejected during an unknown eruption, and analysed by Hesser.

                            _Ancient lava._     _Lava of 1669._

    Silica                      49.63                48.83
    Alumina                     22.47                16.15
    Protoxide of Iron           10.80                16.32
    Protoxide of Manganese        .63                  .54
    Lime                         9.05                 9.31
    Magnesia                     2.68                 4.58
    Soda                         3.07                 3.45
    Potash                        .98                  .77
                                -----                -----
                                99.31                99.95

The sublimations from the fumaroles are chiefly chloride of ammonium,
perchloride of iron, and sulphur. An analysis of the gases of the
fumaroles of 1865 gave the following results:--

    Carbonic acid                 50.5
    Hydrosulphuric acid           11.9
    Oxygen                         7.1
    Nitrogen                      30.5
                                 -----
                                 100.0

An account of microscopic analysis of some of the lavas of Etna, for
which I am indebted to Mr. Frank Rutley, will be found appended to this
chapter. He considers that they are Plagioclase-basalts, and
occasionally Olivine-basalts; and that they consist of Plagioclase,
Augite, Olivine, Magnetite, Titaniferous iron, and a residuum of glass.

Near the summit of the great crater I found a mass of perfectly white,
vesicular, and very friable substance, somewhat pumiceous in appearance.
It proved to be a decomposed lava, and was found elsewhere on the sides
of the crater. Mr. Rutley examined a section of it, and reports: "Under
the microscope a tolerably thin section shows the outlines of felspar
crystals, lying in a hazy milk-white semi-opaque granular matrix. The
felspar crystals are lighter and more translucent than the matrix, but
are of much the same character, having a granulated or flocculent
appearance, somewhat like that of the decomposed felspars in diabase.
There are numerous roundish cavities in the section which may once have
contained olivine, or some other mineral, or they may be merely
vesicles."

A qualitative analysis of this substance, made by Mr. H. M. Elder, has
proved that it contains a large quantity of Silica (about 70 per cent.),
and smaller proportions of Alumina, Iron, Magnesium, Calcium, and
Potash; together with very small amounts of Sulphuric Acid and a trace
of Ammonia. Lithium is absent, and Sodium is only present in very minute
quantity. Water is present to the extent of nearly 20 per cent.

During the eruption of Etna in 1869 Von Waltershausen noticed on some of
the lava blocks which were still hot and smoking, silver-
particles, which rapidly underwent change. An insufficient quantity for
analysis was collected, but during the eruption of 1874, Silvestri found
a quantity of the substance and analysed it. (_Poggendorff's Annalen_,
CLVII. 165, 1876.) It possesses a specific gravity of 3.147, and shows a
metallic lustre similar to that of steel. On analysis it was found to
consist of:--

    Iron        90.86
    Nitrogen     9.14
               ------
               100.00

which corresponds with the formula Fe{5}N{2},--a formula assigned by
Fremy to Nitride of iron. It has been named _Siderazote_. This new
mineral species appears to be formed by the action of hydrochloric acid,
and of ammonia on red-hot lava containing a large percentage of iron. It
was formed artificially by exposing fragments of lava alternately to the
action of hydrochloric acid and ammonia in a red-hot tube. At a high
temperature Siderazote undergoes decomposition, nitrogen being evolved.
In contact with steam at a red heat it forms magnetite and ammonia.




_The Mineral Constitution and Microscopic Characters of some of the
Lavas of Etna._

By Frank Rutley, F.R.G.S., of H.M. GEOLOGICAL SURVEY.


A cursory examination of the series of specimens collected by Mr.
Rodwell, seemed to show that all the lavas of Etna, irrespective of
their differences in age, exhibit a remarkable similarity in
mineralogical constitution. Occasionally, however, there appears to have
been a little difference in their respective viscidity at the time of
the eruption, the crystals in some of them lying in all directions,
while in others there appears to be a more or less definite arrangement
of the felspar crystals, as seen in the lava of A.D. 1689.

Although the specimens which I have examined microscopically do not
appear to differ in the nature of their constituents, yet in some of
them certain minerals fluctuate in quantity, some containing a
comparatively large amount of olivine and well-developed crystals of
augite, while, in others, these minerals, although one or other is
always present, are but poorly represented by minute and
sparsely-disseminated grains. It seems probable that all the Etna lavas
contain traces of a vitreous residuum, since, when sections are
examined under the microscope, a more or less general darkness pervades
their ground mass as soon as the Nicols are crossed, and this general
darkness does not appear to be dissipated during the horizontal
revolution of the sections themselves. The translucent minerals in these
sections are all doubly refracting, and as I have not been able to
detect the presence of hauyne, noseau, sodalite, analcime, or any other
cubic mineral in them, the natural inference is that the obscurity
between crossed Nicols is due to amorphous matter. I have only been able
to ascertain the presence of glass distinctly in a microscopic section
of the lava of Salto di Pulichello. In the other sections which I have
examined there appears to be a small quantity of interstitial glass, but
it is so finely disseminated between the microliths of felspar and
granules of olivine, augite and magnetite, which constitute the
ground-mass of these rocks, that it is most difficult to determine the
single refraction of such minute specks during revolution between
crossed Nicols, and I therefore merely express a belief, which, in some
instances, I cannot demonstrate with any certainty.

[Illustration: Sections of Etna Lavas seen under the Microscope]

Plagioclastic felspars are unquestionably the dominant constituents of
these lavas. Lyell, in his "Principles of Geology," (9th Edition, p.
411), states that the felspar is Labradorite. He does not, however, give
the grounds for this conclusion, and, as microscopic examination alone
merely indicates the crystalline system and not the species of felspar,
it is unsafe to speculate upon this point in the absence of chemical
investigation. In some of these lavas Sanidine is also present, but it
is always subordinate to the plagioclase, and does not, as a rule,
appear to play a part sufficiently prominent to entitle the rock to the
appellation Trachy-dolerite.

Augite and olivine are generally present in the Etna lavas, especially
the latter mineral.

Magnetite appears to occur in all of them. Titaniferous iron may also be
represented, but I have failed to detect any well-defined crystals, or
any traces of the characteristic white decomposition product which would
justify me in citing the presence of this mineral, although it is stated
by Lyell to occur in these rocks.

The constituent minerals of the Etna lavas now to be described, namely,
those of B.C. 396 and A.D. 1535, 1603 and 1689, are:--

Plagioclase, augite, olivine, magnetite, and, in some cases,
sanidine--possibly titaniferous iron--and in some, if not in all, a
slight residuum of glass. These lavas must therefore be regarded as
plagioclase-basalts, or occasionally as olivine-basalts. The plagioclase
crystals vary greatly in size, some being mere microliths while others
are over the eighth of an inch in length. They show the characteristic
twin lamellation by polarized light, but the lamellae are often very
irregular as regards their boundaries. The sections of the crystals
themselves are also frequently bounded by irregular outlines, but they
often show internally delicate zonal markings, as indicated in Fig.
1,[22] which correspond with the outlines of perfectly developed
crystals. The inclosures in the larger plagioclastic felspars consist
for the most part either of brownish glass, containing fine dark
granular matter--probably magnetite, which often renders them
opaque,--or of matter similar to that which constitutes the groundmass
of the surrounding rock. These stone and glass cavities are very
numerous and most irregular in outline, as shown in Figs. 1 and 2. They
appear, however, to be elongated generally in the direction of the
planes of composition of the twin lamellae. Zirkel has noted the
plentiful occurrence of these glass inclosures in the felspar crystals
and fragments of crystals which partly constitute the volcanic sands of
Etna, in which he has also detected the presence of numerous isolated
particles of brownish glass.[23] The felspar microliths, which
constitute so large a proportion of the ground-mass in the Etna lavas,
are in most instances probably triclinic. Monoclinic felspar does,
however, occur in some of these rocks; but the difficulty of
ascertaining the precise character of microliths renders it unsafe to
speculate on the amount of sanidine which may be present. Some crystals,
such as that shown in the centre of Fig. 2, appear at first sight to be
sanidine, twinned on the Carlsbad type, but closer inspection often
demonstrates the presence of other and very delicate twin lamellae.

[22] _The figures in this plate are magnified 35 diameters._ Fig. 1.
Lava of B.C. 396. The upper half of the drawing is occupied by a crystal
of plagioclastic felspar showing twin lamellation and faint zonal
markings, and with numerous irregular dark-brown inclosures of glass,
probably containing magnetite dust and matter similar to that of the
groundmass of the rock which consists of felspar microliths, granules of
olivine, and augite crystals, grains of magnetite, and apparently a
little interstitial glass. A crystal of augite is shown near the bottom
of the drawing.

Fig. 2. Lava of A.D. 1689. On the right hand side part of a plagioclase
crystal with inclosures similar to that in the preceding figure. In the
centre a small crystal of plagioclase. Groundmass similar to that of
Fig. 1, but showing a somewhat definite arrangement of the small felspar
crystals, indicative of fluxion.

[23] "Mikroskopische Beschaffenheit der Mineralien und Gesteine."
Leipzig, 1873; p. 480.

The augite in these lavas sometimes occurs in well-formed crystals of a
green or brown colour, and often shows the characteristic cleavage very
well, especially in the augite crystals of the lava of the Boccarelle
del Fuoco, erupted in 1535. A small crystal of green augite is
represented at the bottom of Fig. 1. Augite, however, appears to be more
plentiful in the rocks in the form of small roundish grains.

Olivine is of very common occurrence in the Etna lavas, mostly in round
or irregularly shaped grains, but also in crystals which usually exhibit
rounded angles.

A specimen of lava from Salto di Pulichello, erupted in 1603, gave
well-developed examples of the presence of olivine, and also of
plagioclase. The ground mass was found to consist of felspar microliths,
and grains of olivine, augite, and magnetite, with some interstitial
glass.

Magnetite is present in all of the lavas here described. It occurs both
in octahedral crystals and in the form of irregular grains and fine
dust. To the presence of this substance much of the opacity of thin
sections of the Etna lavas is due.

Titaniferous iron may also be present. One small crystal in the lava of
1535 appeared to show a somewhat characteristic form, but although much
of the black opaque matter has undergone decomposition, I have failed to
detect any of the white or greyish alteration product which
characterises titaniferous iron, and in the absence of this, of definite
crystalline form, and of chemical analysis, it seems better to speak of
this mineral with reserve, although titanium is very probably present,
since much magnetite is known to be titaniferous.

The vitreous matter which occurs in these lavas is principally present
in the form of inclosures in the felspar, and, sometimes, the augite and
olivine crystals previously described. Its occurrence in the groundmass
of these rocks has also been alluded to. In this interstitial condition
its amount is usually very small--a fact already pointed out by Zirkel.

I have unfortunately had no opportunity of examining the volcanic sands
and ashes of Etna, but Zirkel's description of them seems to indicate
their close mineralogical relation to lavas erupted in this district,
with one exception, as pointed out by Rosenbusch,[24] namely, that he
makes no mention of the occurrence of olivine in these ejectamenta.

[24] "Mikroskopische Physiographie der Massigen Gesteine. Stuttgart,
1877; p. 547.

Reference to the Figures 1 and 2 will suffice to show how close a
relationship in mineral constitution exists between these two lavas,
separated in the dates of their eruption by an interval of over two
thousand years.

       *       *       *       *       *

_New Maps of Etna._--After these pages had received their final revision
in type, I met with two new maps of Etna in the Paris Exhibition. The
literature of our subject will obviously be incomplete without some
notice of them, although this belongs properly to the first chapter
rather than to the last. The one is a map in relief constructed by
Captain Francesco Pistoja for the _Istituto Topografico Militare_ of
Florence. The vertical scale is 1/25,000 and the horizontal is 1/50,000.
The surface is  geologically: the lavas erupted during each
century being differently , while the course of each stream is
traced. This map, although by no means free from errors, is a vast
improvement on the relief map of M. Elie de Beaumont. One defect, which
might be easily remedied, is due to the fact that the lavas of three
consecutive centuries are  so much alike, that it is almost
impossible to distinguish them. The minor cones are well shown, the Val
del Bove fairly well, and the map is altogether a valuable addition to
our knowledge of the mountain.

The other map is a _Carta Agronomica dell' Etna_, showing the surface
cultivation. Different colours denote different plants, pistachio nuts,
vines, olives, chestnuts, etc. It is beautifully drawn and  by
hand, and is the work of Signor L. Ardini, of Catania.




INDEX.


    Abich, 22
    Acesines, River, 81
    Aci Reale, 72, 73
    Acis, River, 73
    Acque Grande, 73
    Aderno, 65
    Adranum, City of, 66
    AEschylus, 4
    Aetna, Town of, 64
    Ajo, Fountain of, 85
    Alcantara, Valley of, 69
    Amphinomus, 80
    Analcime, Analysis of, 128
    Analcite, 127
    Analysis of Augite, 126
        "    "  Labradorite, 125, 126
        "    "  Olivine, 127
        "    "  Titaniferous Iron, 127
        "    "  Analcime, 128
        "    "  Mineral Oil, 129
        "    "  Volcanic Ashes, 131
        "    "  Lava, 131, 132
        "    "  Sand, 131
        "    "  Scoriae, 131
        "       Microscopic, of Lavas, 135-141
        "    "  Siderazote, 133, 134
        "    "  Sublimations, 132
        "    "  white friable substance, 133
    Anapias, 80
    Arethusa, Fountain of, 85
    Ascent, Fatigue of, 60
    Ashes, Volcanic, Analysis of, 131
      "        "   Specific Gravity of, 130
    Atlas des Aetna, 23
    Augite, Analysis of, 126
    Axis of Mongibello, 119, 122
      "   " Trifoglietto, 119, 122

    Baltzer, 24
    Basalt, Columnar, 75
    Base, Circumference of, 30
    Belpasso, 63
    Bembo, Cardinal, 10
    Biancavilla, 65
    Boccarelle del Fuoco, 36
    Bocche eruttive, 110
       "   del Fuoco, 36
    Borelli, 90
    Bosco di Bronte, 99
    Botanical Regions, 40-42
    Boundaries of Etna, 29
    Brilliancy of Stars, 48, 49
    Bronte, 67, 68
    Brydone, 15

    Campi Phlegraei, 14
    Campus Piorum, 80
    Cardinal Bembo, 10
    Carpinetto, Forest of, 39
    Carrera, 12
    Casa del Bosco, 48
      "  Inglesi, 51, 52
    Castagno di Cento Cavalli, 39
        "    della Galea, 39
    Catania, 76-78
       "  Destruction of, 94-96
    Caverns of Etna, 37
    Cavern of Thalia, 37
    Centenario, 108
    Chestnuts, 39
    Circumference of base, 30
    Cisterna, 101
    Coltivata, Regione, 37, 38
    Cones, Minor, 34-36
    Crater of Elevation, 114
       "   of Eruption, 114
       "   The Great, 56-58
    Craters, Minor, 34-36
    Cultivated Region, 38
    Cyclops, Rocks of, 75

    Decomposed Lava, Analysis of, 133
    Desert Region, 39, 40

    Effects of Refraction, 59, 60
    Elevation, Crater of, 114
    Elie de Beaumont, 21
    Elie de Beaumont's Classification, 115, 116
    Empedokles, 10
    Errors in Maps, 24
    Eruption, Crater of, 114
    Eruptions, General Character of, 112
        "      Number of, 113
    Etna, the Home of Early Myths, 9
      "   a Submarine Volcano, 122
    Enceladus, 4

    Fatigue of Ascent, 60
    Fazzello, 11
    Ferrara, 15, 16
    Filoteo, 11
    Flood of 1755, 98
    Forest of Carpinetto, 39
    Fratelli Pii, Cone of, 111
    Fumaroles, Sublimations of, 132
    Fuoco, Regione del, 37

    Gemellaro, Giuseppe, 18
        "      Mario, 19
        "      Carlo, 19, 20
    General aspect of Etna, 34
    _Genista Etnensis_, 45
    Geological Maps of Etna, 117-18
    Gibel Uttamat, 3
    Gladstone's Account of Eruption, 58
    Gravity, Specific, of Ejectamenta, 130
    Great Crater, 57, 58
    Grotto of Polyphemus, 75
       "  delle Palombe, 37
    Growth of a Volcano, 123
    Gurrita, Lake, 68

    Hamilton, 14
    Height of Etna, 26, 27
    Hephaistos, Forge of, 4
    Himilco, 81
    Hoffmann, 22
    Homer, 4
    Houel, 14
    Hybla Major, 63

    Increase of Population, 33
    Inessa, City of, 64
    Inglesi, Casa, 51, 52
    Inns, Sicilian, 65, 67, 69
    Iron, Nitride of, 134
      "   Perchloride of, 132
    Iron, Titaniferous, 127
    Isola d'Aci, 75

    Katana, 76, 77
    Kircher, 12

    Labradorite, Analysis of, 125, 126
    La Cisterna, 101
    Latitude of Crater, 2
    La Scaletta, 75
    Lava, Analysis of, 131, 132
      "   Specific Gravity of, 130
      "   Decomposed, Analysis of, 133
    Lavas, Microscopic Analysis of, 135-141
    Lavas of Etna, 125-141
    Linguaglossa, 70
    Longitude of Crater, 2
    Lucilius Junior, 7-9
    Lucretius, 6
    Lyell, 23
    Lyell's Researches, 118-122

    Magnetite, 139
    Maletto, 68
    Maps, Geological, of Etna, 117, 118
      "   of Etna, 13, 16, 21-24
    Mascali, 71
    Microscopic Analysis of Lavas, 135-141
    Milo, 108
    Mineral Oil in Lava, 129
    Minor Cones, 34-36
    Mongibello, 3
        "      Axis of, 122
    Monte Calanna, 107
       "  Capreolo, 118
       "  di Mojo, 36,81
       "  Minardo, 34
       "  Ste. Sofia, 36
       "  Fusara, 37
       "  Grigio, 111
       "  Lepre, 85
       "  Nocilla, 118
       "  Rosso, 99
       "  Spagnuolo, 69
       "  Ste. Sofia, 95
    Monti Rossi, 35, 91
    Mules, 47

    Name of Etna, 3
    Natural Boundaries of Etna, 30
    Naxos, 81
    Newer Pliocene Strata, 120
    Nicolosi, 46
    Nitride of Iron, 134

    Observatory on Etna, 50
    Oil, Mineral, in Lava, 129
    Olivine, 139
        "   Analysis of, 127

    Palombe, Grotto delle, 37
    Paterno, 63
    Pennisi, Baron, 71, 72
    Piano del Lago, 51
       "  di S. Leo, 90
    Piedimontana, Regione, 37, 38
    Pii Fratres, 80, 81
    Pindar, 4
    Polarized Light, applied to Analysis of Lavas, 136-139
    Polyphemus, Grotto of, 75
    Population, 31-33
    Position of Etna, 2
    Presl's _Flora Sicula_, 41, 42

    Radius of Vision, 28
    Randazzo, 68, 69
    Recupero, 17
    Recupero's Account of Eruption, 99
    Refraction, Effects of, 59, 60
    Regions of Etna, 37-42
    Regione del Fuoco, 37
    River, Acis, 73
    Road around Etna, 29
    Rocca di Musarra, 98
    Rocks of Cyclops, 75
    Rutley's, Mr. Frank, Analysis of Lavas, 135-141

    St. Agatha, Veil of, 83
     "  Maria di Licodia, 64
    S. Niccola, Monastery of, 92
    S. Simone, 102
    Salto della Guimenta, 106
    Sand, Volcanic, Analysis of, 131
      "   Specific Gravity of, 130
    Scogli di Ciclopi, 75
    Scoriae, Volcanic, Analysis of, 131
       "    Specific Gravity of, 130
    Serra delle Concazze, 59
      "   del Solfizio, 59
      "   di Giannicola, 107
    Serrapizzuta, 89
    Sicilian Inns, 65, 67, 69
    Siderazote, 133, 134
    Silvestri, Researches of, 25
    Simeto, Valley of, 67
    Smyth, 18
    Smyth's Observations, 2
    Snow of Etna, 59
    Specific Gravity, Alteration of, 130
        "       "     of  Ejectamenta, 130
    Strabo, 6
    Stars, Brilliancy of, 48, 49
    Stato Maggiore, Map of, 24
    Sulphur in Sublimations, 132
    Sublimations from Fumaroles, 132
    Summit of Cone, 53, 54
    Sunrise seen from Summit, 54, 55

    Tacchini, 50
    Taormina, 71
    Tertiary Sandstone of Bronte, 67
    Thucydides, 5
    Titaniferous Iron, 127
    Torre del Filosofo, 10, 59
    Towns on Etna, 31
    Trezza, 75
    Trifoglietto, Axis of, 121
    Trunks of Large Chestnuts, 39

    Val del Bove, 34, 71, 98, 100, 119-121
     "  Serbo, 103
    Valley of Alcantara, 69
    Virgil, 5
    Vision, Radius of, 28
    Volcano, Growth of, 123
    Von Waltershausen, 23, 120
    Vulkanen Atlas, 116

    Winchelsea, Lord, 12, 94, 95
    Woody Region, 38

    _Zeolite dure_, 127
    Zones of Temperature, 38

       *       *       *       *       *

Transcribers Notes:

OE ligatures have been written as two letters. The chemical formulae
in this text have subscripts written in curly brackets. For example,
water appears as H{2}O.

Passages in italics indicated by _underscores_. Passages in Greek
indicated by ~tildes~.

Printer's errors corrected and other transcription points as follows:

 Page    Correction
 ---------------------------------------------------------------------
   -     Some arcane spellings retained where verified as correct for
         the time of publication or quote, such as 'musquitoes',
         'plaintain', 'mettals', 'felspar', etc.
   -     Italian quotations sometimes include phrases such as "sull'
         Etna" or "dell' Asia". There should be no space after the
         apostrophes but spaces are often present. This may have been
         done to better space the text during justification. Such errors
         have not been corrected.
   -     The document is inconsistent in the use of commas where quoting
         numbers of over 1,000; sometimes they are used and sometimes
         they are not used. These inconsistencies remain.
  ix     Added '.' at end of 'Silvestri' in text block to maintain
         style of other entries.
   x     Added '.' at end of 'Eruptions' in text block to maintain
         style of other entries.
   x     Added '.' after '1408' in text block to maintain style of
         other entries.
  xi     Added '.' after 'microscope' in text block to maintain style
         of other entries.
   4     Corrected 'ength' to 'length'.
  12     Corrected 't'jncedie' to 't'incedie'. 't'jncedie' and
         'treblement' both printed with tildes over the first
         occurrence of e in each word. Tildes omitted in this version.
  17     Corrected 'Guiseppe' to 'Giuseppe'.
  27     Added end quotes after final word on page.
  29     Inserted full-stop after '(S.W.)', to end sentence.
  33     Corrected 'f' to 'of'.
  42     'of-course' corrected to 'of course'.
  44     Corrected 'unusally' to 'unusually'.
  59     Corrected 'subsequenly' to 'subsequently'.
  64     Corrected 'athough' to 'although'.
  79     Added '.' after '812' in text block to maintain style of
         other entries.
  80     Anapias and Amphinomus printed with diacritic marks omitted
         in this text (breves over first 'a' in 'anapias' and 'i' in
         'Amphinomus').
  82     Numbered list runs 1, 2, 3, 4, 5, 5, 7, 8... Second occurrence
         of 5 amended to 6.
  85     'In the 1329' corrected to 'In the year 1329'.
 127     'the time analcite' corrected to 'the term analcite'.
 144     Corrected 'Guiseppe' to 'Giuseppe'.
 145     Corrected 'Miscroscope' to 'Microscope'.
 152     Corrected 'magnitite' to 'magnetite'.





End of the Project Gutenberg EBook of Etna, by G. F. Rodwell

*** 