Evolution of dust condensations in the preplanetary disk

Details Evolution of dust condensations in the preplanetary disk Evolution of dust condensations in the preplanetary disk

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65...58p&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 58-72. In Russian.

Astronomy and Astrophysics

Astronomy

2

Interplanetary Dust, Planetary Evolution, Planetary Mass, Protoplanets, Astronomical Models, Gravitational Effects, Rotating Matter

Scientific paper

It is proposed that dust condensations were formed in the circumsolar preplanetry disk after dust sedimentation in the disk and gravitational instability in the dust subdisk. Relationships betwen the radius, mass, density, and spin of rotating condensations are examined. The time of their growth and transformation into solid bodies is estimated. It is hypothesized that the largest of them could have evolved into protoplanets.

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