Accumulation and migration of the bodies from the zones of giant planets

Details Accumulation and migration of the bodies from the zones of giant planets Accumulation and migration of the bodies from the zones of giant planets

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987em%26p...39..101i&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 39, Oct. 1987, p. 101-128.

Astronomy and Astrophysics

Astronomy

19

Astronomical Models, Gas Giant Planets, Planetary Evolution, Asteroids, Celestial Mechanics, Computerized Simulation, Planetary Mass, Planetary Orbits, Solar System

Scientific paper

Within the model of solid-body accumulation of planets (or their nuclei) the accumulation and migration of bodies from the feeding zones of the giant planets are investigated. The investigation is based on results of computer simulation of evolving disks which initially consisted of hundreds of particles moving about the Sun and coagulating under collisions. In this paper the characteristics of an initial protoplanetary circumsolar cloud, the body migration in the forming solar system, the planet orbit evolution, the formation of the beyond-Neptune belt and asteroid belts between the giant planet orbits are considered. The results obtained confirm many analytical estimates earlier made by V. S. Safronov and his colleagues.

Affiliated with

Also associated with

No associations

Rating

Accumulation and migration of the bodies from the zones of giant planets 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 Accumulation and migration of the bodies from the zones of giant planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accumulation and migration of the bodies from the zones of giant planets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1774186