Titan and habitable planets around M-dwarfs
Abstract
The Cassini–Huygens mission discovered an active “hydrologic cycle” on Saturn's giant moon Titan, in which
- This article is part of the themed collection: Chemistry of the Planets
a Dipartimento di Fisica, University of Rome “Tor Vergata”, Rome, Italy
b
Istituto di Fisica dello Spazio Interplanetario, Istituto Nazionale di Astrofisica, Rome, Italy
E-mail:
jlunine@roma2.infn.it
The Cassini–Huygens mission discovered an active “hydrologic cycle” on Saturn's giant moon Titan, in which
J. I. Lunine, Faraday Discuss., 2010, 147, 405 DOI: 10.1039/C004788K
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