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Coupled atmosphere-ocean models of Titan's pastThe behavior and possible past evolution of fully coupled atmosphere and ocean model of Titan are investigated. It is found that Titan's surface temperature was about 20 K cooler at 4 Gyr ago and will be about 5 K warmer 0.5 Gyr in the future. The change in solar luminosity and the conversion of oceanic CH4 to C2H6 drive the evolution of the ocean and atmosphere over time. Titan appears to have experienced a frozen epoch about 3 Gyr ago independent of whether an ocean is present or not. This finding may have important implications for understanding the inventory of Titan's volatile compounds.
Document ID
19930049259
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mckay, Christopher P. (NASA Ames Research Center Moffett Field, CA, United States)
Pollack, James B. (NASA Ames Research Center Moffett Field, CA, United States)
Lunine, Jonathan I. (Arizona Univ. Tucson, United States)
Courtin, Regis (Paris Observatoire, Meudon, France)
Date Acquired
August 16, 2013
Publication Date
March 1, 1993
Publication Information
Publication: Icarus
Volume: 102
Issue: 1
ISSN: 0019-1035
Subject Category
LUNAR AND PLANETARY EXPLORATION
Distribution Limits
Public
Copyright
Other