Refining a model for the formation of solid matter in a protoplanetary disk

Details Refining a model for the formation of solid matter in a protoplanetary disk Refining a model for the formation of solid matter in a protoplanetary disk

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987avest..21..327i&link_type=abstract

(AN SSSR, Seminar po Astrofizicheskim Problemam Planetnoi Kosmogonii, Moscow, USSR, Apr. 1, 1987) Astronomicheskii Vestnik (ISSN

Astronomy and Astrophysics

Astronomy

Accretion Disks, Astronomical Models, Chondrites, Protoplanets, Pressure Distribution, Radial Distribution, Temperature Dependence

Scientific paper

A model describing the formation of solid matter in a protoplanetary disk (PD) during disk formation which incorporates data on the properties of chondrites and the theory of PD formation is described. It can be used to describe a number of basic properties of chondrites and presents agruments in favor of a PD model with low mass and momentum values. In the present paper, this model is refined on the basis of a numerical model for PD formation. The surface density, pressure, and temperature in the PD at the end of protosun accretion and disk formation are investigated as a function of distance from the protosun.

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