Stability of resonant planetary orbits in binary stars

Details Stability of resonant planetary orbits in binary stars Stability of resonant planetary orbits in binary stars

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989japa...10..347m&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 10, Dec. 1989, p. 347-365.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Orbital Resonances (Celestial Mechanics), Planetary Orbits, Planetary Systems, Dynamic Stability, Equations Of Motion, Four Body Problem, Jacobi Integral

Scientific paper

This paper contains a numerical study of the stability of resonant orbits in a planetary system consisting of two planets moving under the gravitational attraction of a binary star. The numerical results show that the main mechanism which generates instability is the destruction of the Jacobi integrals of the massless planets when their masses become nonzero. Considerable intervals of stable resonant orbits have been found.

Affiliated with

Also associated with

No associations

Rating

Stability of resonant planetary orbits in binary stars 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 resonant planetary orbits in binary stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of resonant planetary orbits in binary stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1571972