Precession-nutation torque due to planets exerted on the sun

Details Precession-nutation torque due to planets exerted on the sun Precession-nutation torque due to planets exerted on the sun

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35...87b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, March 1984, p. 87-91.

Astronomy and Astrophysics

Astronomy

Nutation, Solar Oscillations, Solar Planetary Interactions, Solar Rotation, Stellar Models, Torque, Astrodynamics, Euler Equations Of Motion, Precession, Rigid Structures, Solar System, Stellar Structure

Scientific paper

The precession-nutation torque due to planets, exerted on the Sun, is treated for a model of the Sun with a core which is capable of precession-nutation motion as a rigid body. The period of the precession motion computed is ≡1.2×109 years and the amplitude of the nutation motion has been found to be negligibly small, so that the angle between the plane of the heliocentric equator and the plane of the fixed ecliptic may be assumed to be constant in all actual problems of dynamics of the Solar System.

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