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Compute the equation of time (#40)
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The equation of time is the difference of the real Sun time and the mean Sun time. This difference is due to the elliptical shape of the Earth's orbit, and the obliquity of the orbit.

`Sun` now has a `#equation_of_time` method that returns an integer: the time difference in seconds.

```rb
date = Date.new(2010, 7, 27)

Astronoby::Sun.equation_of_time(date: date)
# => -392
```
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rhannequin committed Mar 23, 2024
1 parent 09e3762 commit 5e3f122
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4 changes: 4 additions & 0 deletions UPGRADING.md
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Expand Up @@ -40,6 +40,10 @@ default vertical refraction angle or not.
With a default value of `true`, this new argument will make consider a
default vertical refraction angle or not.

### `Sun::equation_of_time` method added (#40)

Returns the equation of time for a given date.

### `Sun#distance` method added (#30)

Returns the approximate Earth-Sun distance in meters (`Numeric`).
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24 changes: 24 additions & 0 deletions lib/astronoby/bodies/sun.rb
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Expand Up @@ -6,6 +6,30 @@ class Sun
ANGULAR_DIAMETER = Angle.as_degrees(0.533128)
INTERPOLATION_FACTOR = BigDecimal("24.07")

# Source:
# Title: Practical Astronomy with your Calculator or Spreadsheet
# Authors: Peter Duffett-Smith and Jonathan Zwart
# Edition: Cambridge University Press
# Chapter: 51 - The equation of time

# @param date [Date] Requested date
# @return [Integer] Equation of time in seconds
def self.equation_of_time(date:)
noon = Time.utc(date.year, date.month, date.day, 12)
epoch_at_noon = Epoch.from_time(noon)
sun_at_noon = new(epoch: epoch_at_noon)
equatorial_hours = sun_at_noon
.ecliptic_coordinates
.to_equatorial(epoch: epoch_at_noon)
.right_ascension
.hours
gst = GreenwichSiderealTime
.new(date: date, time: equatorial_hours)
.to_utc

(noon - gst).to_i
end

# Source:
# Title: Celestial Calculations
# Author: J. L. Lawrence
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80 changes: 80 additions & 0 deletions spec/astronoby/bodies/sun_spec.rb
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Expand Up @@ -572,4 +572,84 @@
# Time from IMCCE: +266° 52′
end
end

describe "::equation_of_time" do
it "returns an Integer" do
date = Date.new

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to be_an Integer
end

# Source:
# Title: Practical Astronomy with your Calculator or Spreadsheet
# Authors: Peter Duffett-Smith and Jonathan Zwart
# Edition: Cambridge University Press
# Chapter: 51 - The equation of time
it "returns the right value of 2010-07-27" do
date = Date.new(2010, 7, 27)

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to eq(-392)
# Value from Practical Astronomy: 392
end

# Source:
# Title: Celestial Calculations
# Author: J. L. Lawrence
# Edition: MIT Press
# Chapter: 6 - The Sun
it "returns the right value of 2016-05-05" do
date = Date.new(2016, 5, 5)

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to eq(199)
# Value from Celestial Calculations: 199
end

# Source:
# Title: Celestial Calculations
# Author: J. L. Lawrence
# Edition: MIT Press
# Chapter: 6 - The Sun
it "returns the right value of 2015-08-09" do
date = Date.new(2015, 8, 9)

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to eq(-334)
# Value from Celestial Calculations: 337
end

# Source:
# Title: Celestial Calculations
# Author: J. L. Lawrence
# Edition: MIT Press
# Chapter: 6 - The Sun
it "returns the right value of 2010-05-06" do
date = Date.new(2010, 5, 6)

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to eq(201)
# Value from Celestial Calculations: 201
end

# Source:
# Title: Celestial Calculations
# Author: J. L. Lawrence
# Edition: MIT Press
# Chapter: 6 - The Sun
it "returns the right value of 2020-01-01" do
date = Date.new(2020, 1, 1)

equation_of_time = described_class.equation_of_time(date: date)

expect(equation_of_time).to eq(-200)
# Value from Celestial Calculations: 187
end
end
end

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