Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids

Details Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1359g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1359

Physics

Scientific paper

We have adapted the planet building code, a multizone code, to study the
collisional evolution of asteroids in the main belt. In this way the
effects of resonances and Yarkowski's drift are statistically included
and we can estimate the flux of bodies into NEO orbits.

Affiliated with

Also associated with

No associations

Rating

Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids 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 Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multi-Zone Simulations of the Collisional Evolution of Main Belt Asteroids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-867164