The Ancient Heat Flow and Elastic Thickness on Enceladus: Constraints from Photoclinometry and Numerical Modeling

Details The Ancient Heat Flow and Elastic Thickness on Enceladus: Constraints from Photoclinometry and Numerical Modeling The Ancient Heat Flow and Elastic Thickness on Enceladus: Constraints from Photoclinometry and Numerical Modeling

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1653b&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

Scientific paper

Comparison of photoclinometry with numerical modeling suggests that the
heat flow in Diyar/Sarandib Planitia was 30-60 mW/m^2 at the time of
their formation. These high heat flows are consistent with the former
existence of a now-inactive diapir.

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