The thermal conditions of a protoplanetary disk

Details The thermal conditions of a protoplanetary disk The thermal conditions of a protoplanetary disk

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987avest..21..324m&link_type=abstract

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

Astronomy and Astrophysics

Astronomy

2

Accretion Disks, Planetary Evolution, Protoplanets, Thermodynamic Properties, Agglomeration, Chemical Reactions, Cosmic Dust, Density Distribution, Temperature Dependence

Scientific paper

The physical and chemical evolution of protoplanetary matter can be understood through the study of the thermal conditions in a protoplanetary gas-disk dust. The kinetics of chemical reactions, the condensation and evaporation of matter, the efficiency of dust particle amalgamation during collisions, and the thermal conditions inside planetesimals are all strongly dependent on temperature. Thermal models of a disk are constructed on the basis of dynamic models in which the surface density distribution is found.

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