Modeling the Thermal State of Titan Volatiles and Shallow Melting Involving Hydrocarbons, Organics and Ice

Details Modeling the Thermal State of Titan Volatiles and Shallow Melting Involving Hydrocarbons, Organics and Ice Modeling the Thermal State of Titan Volatiles and Shallow Melting Involving Hydrocarbons, Organics and Ice

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1828f&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

This paper is about modeling the thermal environment within, beneath and
adjacent to hydrocarbon sand dunes overlying a water-ice crust on Titan.
Finite element modeling provides a key basis for the analysis.

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