A Surface Dissolution/Precipitation Model for the Development of Lakes on Titan, Based on an Arid Terrestrial Analogue: The Pans and Calcretes of Etosha (Namibia)

Details A Surface Dissolution/Precipitation Model for the Development of Lakes on Titan, Based on an Arid Terrestrial Analogue: The Pans and Calcretes of Etosha (Namibia) A Surface Dissolution/Precipitation Model for the Development of Lakes on Titan, Based on an Arid Terrestrial Analogue: The Pans and Calcretes of Etosha (Namibia)

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1733b&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

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Scientific paper

Morphological comparisons between Titan, Namibia, and a geometrical
model suggest that the lakes of Titan develop by radial growth and
coalescence of circular seeds, controlled by dissolution of a
superficial porous layer in an arid environment.

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