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Update 05-outer_solar_system.jmd
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tutorials/models/05-outer_solar_system.jmd

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@@ -5,6 +5,7 @@ author: Yingbo Ma, Chris Rackauckas
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## Data
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The chosen units are: masses relative to the sun, so that the sun has mass $1$. We have taken $m_0 = 1.00000597682$ to take account of the inner planets. Distances are in astronomical units , times in earth days, and the gravitational constant is thus $G = 2.95912208286 \cdot 10^{-4}$.
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| planet | mass | initial position | initial velocity |

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