On the invariable plane of the solar system

Details On the invariable plane of the solar system On the invariable plane of the solar system

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...106..133b&link_type=abstract

Astronomy and Astrophysics, vol. 106, no. 1, Feb. 1982, p. 133-136.

Astronomy and Astrophysics

Astrophysics

1

Angular Momentum, Celestial Mechanics, Orbital Elements, Planetary Orbits, Solar System, Ecliptic, Equators, Equinoxes, Reference Systems, Stellar Evolution, Stellar Mass

Scientific paper

The position of the invariable plane of the solar system is determined using the development ephemeris number 102. The invariable plane is calculated with respect to the two coordinate systems ecliptic and equinox, and equator and equinox, as well as with respect to the reference systems of the new standard epoch J 2000.0. All the four DE-numbers 96, 102, 108, and 110 agree with respect to inclination and ascending node of the invariable plane up to about half a minute of arc and up to about three minutes of arc, respectively. The contribution of asteroids to the total angular momentum of the solar system is computed to be about 0.003%.

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