The Inevitability of a Thick, Strongly Insulating Megaregolith on Bodies of Order 100-km to Moon-like in Size

Details The Inevitability of a Thick, Strongly Insulating Megaregolith on Bodies of Order 100-km to Moon-like in Size The Inevitability of a Thick, Strongly Insulating Megaregolith on Bodies of Order 100-km to Moon-like in Size

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2465w&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2465

Physics

Scientific paper

By modeling ejecta accumulation starting from assumed (a) largest
cratering event and (b) power-law size distribution, I show that
development of a km(+) thick insulating megaregolith is inevitable even
for planetesimals as small as 100 km in d.

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