Solar system planetary motion to third order of the masses

Details Solar system planetary motion to third order of the masses Solar system planetary motion to third order of the masses

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...341..318m&link_type=abstract

Astronomy and Astrophysics, v.341, p.318-327 (1999)

Astronomy and Astrophysics

Astrophysics

4

Celestial Mechanics, Stellar Dynamics, Ephemerides, Solar System: General

Scientific paper

We present in this paper a new solution for planetary motion. It consists in developing the perturbations up to the third order of the planetary masses and uses the IERS92 masses set. The relativistic perturbations expressed in isotropic coordinates and the perturbations of the Moon on the inner planets are also included. Effects of asteroids on Earth-Moon barycenter, Mars and Jupiter have been taken into account. We used adjustments to numerical DE403 and DE405 integrations of the Jet Propulsion Laboratory (JPL) to obtain the theory's integration constants.

Affiliated with

Also associated with

No associations

Rating

Solar system planetary motion to third order of the masses does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Solar system planetary motion to third order of the masses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar system planetary motion to third order of the masses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1183799