Estimating erosional exhumation on Titan from drainage network morphology

Estimating erosional exhumation on Titan from drainage network morphology

Drainage networks on Titan, Earth, and Mars provide the only known examples of non-volcanic fluvial activity in our solar system. The drainage networks on Titan are apparently the result of a methane-ethane cycle similar to Earth's water cycle. The scarcity of impact craters and the uneven dist...

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Bibliographic Details
Main Authors: Perron, J. Taylor, Burr, Devon M., Drummond, Sarah A., Black, Benjamin Alexander
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: American Geophysical Union (AGU) 2014
Online Access:http://hdl.handle.net/1721.1/85624
https://orcid.org/0000-0002-0404-8701

Internet

http://hdl.handle.net/1721.1/85624
https://orcid.org/0000-0002-0404-8701

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