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Formation and Migration of Trans-Neptunian Objects - Proceedings of the conference "Scientific Frontiers in Research of Extrasolar Planets"

 
STATUS REPORT
Date Released: Saturday, January 4, 2003
Source: arXiv.org e-Print archive


Astrophysics, abstract
astro-ph/0210131

From: Sergei Ipatov <ipatov@stars.gsfc.nasa.gov>
Date: Sat, 5 Oct 2002 15:48:47 GMT   (116kb)

Formation and Migration of Trans-Neptunian Objects - Proceedings of the conference "Scientific Frontiers in Research of Extrasolar Planets"

Authors: S.I. Ipatov
Comments: Proc. of conf. "Scientific Frontiers in Research of Extrasolar Planets" (18-21 June 2002, Washington, DC). 4 pages, 3 fig., submitted
Some large trans-Neptunian objects could be formed by the compression of rarefied dust condensations, but not by the accumulation of smaller planetesimals. A considerable portion of near-Earth objects could have come from the trans-Neptunian region. Our runs of the evolution of thousands orbits of Jupiter-family comets under the gravitational influence of planets showed that former Jupiter-family comets collide with the terrestrial planets mostly from orbits with aphelia located deep inside Jupiter's orbit.

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References and citations for this submission:
SLAC-SPIRES HEP (refers to , cited by, arXiv reformatted)


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