Shell Thickness Variations and the Long Wavelength Topography of Titan

Details Shell Thickness Variations and the Long Wavelength Topography of Titan Shell Thickness Variations and the Long Wavelength Topography of Titan

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1068n&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1068

Physics

Scientific paper

Titan's global shape and gravity can be explained by shell thickness
variations arising from tidal heating in a conductive ice shell.

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