Fluvial Erosion on Titan

Details Fluvial Erosion on Titan Fluvial Erosion on Titan

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..508l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.508

Physics

Scientific paper

Titan's surface is shaped by a rich abundance of fluvial valleys, which is an indication for the activity of a volatile cycle even in current times (e.g. [1, 2]). In contrast to the water cycle on terrestrial planets such as Earth and Mars, Titan's volatile cycle is based on liquid methane, which is in liquid and gaseous aggregate state within the atmosphere and near the surface, given Titan's environmental conditions (e.g. [3, 4, 5]). This study aims to investigate the entirety of fluvial channels identifiable by the current Cassini-image data inventory.

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