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Precession and Nutations of Mars calculated with Kinoshita’s Model

Published online by Cambridge University Press:  12 April 2016

S. Bouquillon  and
J. Souchay
S. Bouquillon
Affiliation:
Observatoire de Paris Paris, France
J. Souchay
Affiliation:
Observatoire de Paris Paris, France

Abstract

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This paper presents the theoretical study of precession and nutation of Mars in a rigourous way. For this work we choose a natural reference system, based on the concept of non-rotating origin, and the appropriate canonical variables. Then, we solve the equations of the problem by taking into account the effects of the Sun, the Earth, Jupiter, and satellites of Mars, Phobos and Deimos.

Type
Rotation of Solar System Objects
Information
International Astronomical Union Colloquium , Volume 165: Dynamics and Astrometry of Natural and Artificial Celestial Bodies , 1997 , pp. 325 - 330
Copyright
Copyright © Kluwer 1997

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