Hydrodynamic Escape from Disks Formed by Giant Impacts

Details Hydrodynamic Escape from Disks Formed by Giant Impacts Hydrodynamic Escape from Disks Formed by Giant Impacts

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1452g&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1452

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Scientific paper

Circumterrestrial disk formed by a giant impact can escape from the
Earth, because the disk is likely close to isothermal. A criterion for
the escape and its dependence on the physical parameters was estimated
from the hydrostatic equation.

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