The Fate of Water in Early-Accreting Internally Heated Planetesimals

Details The Fate of Water in Early-Accreting Internally Heated Planetesimals The Fate of Water in Early-Accreting Internally Heated Planetesimals

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1582e&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1582

Computer Science

Scientific paper

Partial differentiation in early-forming planetesimals results in bulk
densities and water compositions that vary by total mass, time of
accretion, and bulk radiogenic content. Crusts will be heterogeneous in
density and water content.

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