The precession and long-term nutation of Venus

Details The precession and long-term nutation of Venus The precession and long-term nutation of Venus

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acasn..28..242z&link_type=abstract

(Acta Astronomica Sinica, vol. 28, no. 1-3, 1987, p. 242-249) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, Marc

Mathematics

Nutation, Planetary Rotation, Secular Variations, Venus (Planet), Equations Of Motion, Matrices (Mathematics), Oblate Spheroids

Scientific paper

A simple theory of the precession and nutation of Venus is constructed, referred to the inertial system defined by the ecliptic and dynamical equinox of J 2000.0. Using the recently published dynamical parameters, a precession rate of -7828.6144 arcsec/cy is found, corresponding to a period of 16,555 yr. Arguments, amplitudes, and periods of the long-term nutations; short-term nutations; the adopted value of the dynamical oblateness; and the mean obliquity are discussed and the results given in tables.

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