The obliquity of Titan as evidence for the presence of a liquid ocean beneath the surface and perspectives for the determination of the ice shell thickness of Europa

Details The obliquity of Titan as evidence for the presence of a liquid ocean beneath the surface and perspectives for the determination of the ice shell thickness of Europa The obliquity of Titan as evidence for the presence of a liquid ocean beneath the surface and perspectives for the determination of the ice shell thickness of Europa

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010epsc.conf..203b&link_type=article

"European Planetary Science Congress 2010, held 20-24 September in Rome, Italy. http://meetings.copernicus.org/epsc2010, p.203"

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