Convective Cooling of Protoplanetary Disks and Rapid Giant Planet Formation

Details Convective Cooling of Protoplanetary Disks and Rapid Giant Planet Formation Convective Cooling of Protoplanetary Disks and Rapid Giant Planet Formation

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1124b&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1124

Physics

3

Scientific paper

Convective cooling is shown to be a self-consistent mechanism for
cooling the midplanes of protoplanetary disks, thereby allowing disk
instabilities in marginally gravitationally unstable disks to form dense
clumps that could become giant planets.

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