Evolution of asteroidal orbits with high inclinations

Details Evolution of asteroidal orbits with high inclinations Evolution of asteroidal orbits with high inclinations

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..57..408s&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 57, no. 1-2, p. 408-409

Astronomy and Astrophysics

Astronomy

1

Asteroids, Evolution (Development), Inclination, Many Body Problem, Orbit Calculation, Orbit Perturbation, Orbital Elements, Solar Orbits, Computerized Simulation, Eccentric Orbits, Eccentricity, Numerical Integration, Temporal Distribution

Scientific paper

The 20,000 years orbital evolution of massless fictitious asteroid located at a border of the Hill's gravitational sphere has been investigated. The eleven orbits with the eccentricities from 0.0 to 0.4 in five groups of inclinations from 40 deg to 80 deg were numerically integrated with planetary perturbations of six major planets, using the numerical integration n-body program with the Everhart's integrator RA 15. For each group time evolution of orbital elements of the asteroids is presented.

Affiliated with

Also associated with

No associations

Rating

Evolution of asteroidal orbits with high inclinations 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 Evolution of asteroidal orbits with high inclinations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of asteroidal orbits with high inclinations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1325759