Diurnal motion of the Sun as seen from Mercury

Physics

Scientific paper

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Celestial Mechanics, Mercury

Scientific paper

The quantitative description of the motion of the Sun as observed from Mercury is a problem suitable to a variety of classes. The only difficult aspect for introductory students is a determination of the position along the orbit for the planet. Two methods are described and a listing of a computer subroutine is included. The combination of slow rotation and high eccentricity of Mercury's orbit makes this problem an interesting one.

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