On the dynamics of the relativistic restricted three-body problem.

Details On the dynamics of the relativistic restricted three-body problem. On the dynamics of the relativistic restricted three-body problem.

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...290..335m&link_type=abstract

Astronomy and Astrophysics 290, 335-339 (1994)

Astronomy and Astrophysics

Astrophysics

5

Celestial Mechanics, Relativity

Scientific paper

The equations of motion for the relativistic restricted three-body problem are derived using the post-Newtonian approximation of relativity. It turns out that they obey the same symmetry relations as the classical eqations and that they depend - as second parameter besides the mass ratio μ - on (M)/(R), on the ratio of the total mass of the system and the separation of the primaries. This parameter (M)/(R) is thus a kind of measure for the role of relativistic effects in the system (the classical case is (M)/(R)=0). Finally, the model is applied to the computation of the advance of Mercury's perihelion in the Solar system and leads to results compatible with published data.

Affiliated with

Also associated with

No associations

Rating

On the dynamics of the relativistic restricted three-body problem. 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 On the dynamics of the relativistic restricted three-body problem., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the dynamics of the relativistic restricted three-body problem. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1067372