Dynamics of binary asteroids. II - Jovian perturbations

Details Dynamics of binary asteroids. II - Jovian perturbations Dynamics of binary asteroids. II - Jovian perturbations

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...87..377c&link_type=abstract

Icarus (ISSN 0019-1035), vol. 87, Oct. 1990, p. 377-390.

Computer Science

15

Asteroids, Computerized Simulation, Jupiter (Planet), Orbit Perturbation, Secular Variations, Hill Method, Perturbation Theory, Solar Planetary Interactions, Solar System

Scientific paper

The stability conditions over the age of the solar system of an asteroid circled by a satellite are determined as a function of the system separation and mass. It is found that Jupiter drives systematically binary asteroids toward the instability region of Hill's problem, thus causing a disruption of the binary system. Actual asteroids suspected of having a binary nature are treated via this approach.

Affiliated with

Also associated with

No associations

Rating

Dynamics of binary asteroids. II - Jovian perturbations 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 Dynamics of binary asteroids. II - Jovian perturbations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of binary asteroids. II - Jovian perturbations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1304265