Growth of planetesimals in the transneptunian zone.

Details Growth of planetesimals in the transneptunian zone. Growth of planetesimals in the transneptunian zone.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994avest..28r...3s&link_type=abstract

Astronomicheskii Vestnik, Tom 28, No. 6, p. 3 - 9

Astronomy and Astrophysics

Astronomy

1

Solar Nebula: Condensation, Solar Nebula: Planetesimals, Solar Nebula: Comets, Formation: Comets

Scientific paper

The formation of two-hundred km bodies in situ in the transneptunian zone is considered. The direct growth of particles with account for their radial and vertical migration in the gaseous solar nebula is not effective even for the origin of bodies of cometary sizes. The combined process of gravitational instability in the dust subdisk followed by subsequent growth of primary condensations may result in formation of more sizeable bodies.

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