Modeling the Early Thermal Evolution of Meteorite Parent Bodies Based on New Thermal Conductivity Measurements of Highly Porous Aggregates

Details Modeling the Early Thermal Evolution of Meteorite Parent Bodies Based on New Thermal Conductivity Measurements of Highly Porous Aggregates Modeling the Early Thermal Evolution of Meteorite Parent Bodies Based on New Thermal Conductivity Measurements of Highly Porous Aggregates

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2696k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2696

Physics

1

Scientific paper

Peak central temperatures in initially highly porous planetesimals
heated by short-lived nuclide decay energy are significantly higher
particularly for small km sized planetesimals.

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