Formation of Trans-Neptunian Objects

Details Formation of Trans-Neptunian Objects Formation of Trans-Neptunian Objects

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1165i&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1165

Computer Science

2

Scientific paper

It may be possible that some large trans-Neptunian objects, asteroids,
and planetesimals with diameter up to several hundreds kilometers were
formed by compression of rarefied dust condensations, but not by
accumulation of smaller planetesimals.

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