A form of the equation of rotational motion of planets

Details A form of the equation of rotational motion of planets A form of the equation of rotational motion of planets

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kosis..31..110d&link_type=abstract

Kosmicheskie Issledovaniya, vol. 31, p. 110

Physics

Planetary Rotation, Orbital Mechanics, Gravitational Fields, Numerical Integration, Circular Orbits, Center Of Mass

Scientific paper

The rotational motion of planets is examined using isometric
coordinates. The isometric coordinates are introduced for the case of
axial dynamic symmetry, assuming a nearly spherical central ellipsoid of
inertia for celestial bodies. Details of the derivation procedure are
presented.

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