On Low-Mass Planetary Migration in an Optically Thick Disk

Details On Low-Mass Planetary Migration in an Optically Thick Disk On Low-Mass Planetary Migration in an Optically Thick Disk

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1126y&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1126

Physics

Scientific paper

A protoplanet embedded in a gas disk experiences a torque from the disk
that generally changes its orbit elements. We numerically examine the
torque exerted on a planet by an optically thick accretion disk for
various values of the opacity and the accretion rate.

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