Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria.

Details Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria. Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria.

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.223..191s&link_type=openurl

Astrophysics and Space Science, Vol. 223, No. 1 - 2, p. 191

Astronomy and Astrophysics

Astrophysics

Three-Body Problem: Stability, Binaries: Planetary Systems

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria. 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 Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of planetary orbits around binary stars: a comparison of Hill's and Laplace's stability criteria. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1818672