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 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cha%26a..12...38z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 12, Issue 1, p. 38-42.

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We construct a simple theory of precession and nutation of Venus, referred to the inertial system defined by the ecliptic and dynamical equinox of J 2000.0. Using the recenly published dynamical parameters, we find a precession rate of -7828.6144 arcsec/cy, corresponding to a period of 16 555 yr. Arguments, amplitudes and periods of the long-term nutations are given in TABLE 1. The short-term nutations, the adopted value of the dynamical oblateness and the mean obliquity are discussed and the results given in TABLEs 2-4.

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