Numerical Simulations of Sub-Catastrophic Porous Planetesimal Collisions

Details Numerical Simulations of Sub-Catastrophic Porous Planetesimal Collisions Numerical Simulations of Sub-Catastrophic Porous Planetesimal Collisions

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1933c&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1933

Astronomy and Astrophysics

Astrophysics

Scientific paper

Numerical simulations show that large sub-catastrophic collisions
between porous planetesimals at speeds greater than 4 km/s can generate
significant volumes of heated material that is retained on the surviving
planetesimal.

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