Numerical model of the Solar System: Difference between revisions

Revision as of 05:47, 1 May 2006

Revision as of 19:11, 11 May 2006

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Readers may note that the code performs some complicated coordinate system conversion calculations, particularly in the calculation of the initial velocity components. These calculations are described in a separate article, on a [[transformation from spherical coordinates to rectangular coordinates]].

==References==

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==See also==