Planet formation process as a phase transition. I - Elementary model

Details Planet formation process as a phase transition. I - Elementary model Planet formation process as a phase transition. I - Elementary model

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....19..327f&link_type=abstract

Moon and the Planets, vol. 19, Nov. 1978, p. 327-339. Research sponsored by the Consiglio Nazionale delle Ricerche.

Other

3

Astronomical Models, Interplanetary Medium, Phase Transformations, Planetary Evolution, Temperature Effects, Condensing, Graphs (Charts), Isothermal Processes, Kepler Laws, Mass Distribution, Ring Structures, Thermalization (Energy Absorption)

Scientific paper

A model for the condensation of ring-shaped nebular matter into a protoplanet is described. The condensation is considered as a phase transition between a ring phase and a planetary phase. A constant nonzero temperature is assumed. The model is used to study the effect of physical parameters on the critical ring width permitting transition. The parameters considered are mass and temperature of the nebular matter.

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