Physics
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338...77m&link_type=abstract
In ESA, Symposium on Titan p 77-80 (SEE N92-32348 23-91)
Physics
Atmospheric Temperature, Satellite Atmospheres, Titan, Greenhouse Effect, Haze, Oceans
Scientific paper
The contribution of various factors to the thermal structure of Titan's past and present atmosphere are discussed. A one dimensional model of Titan's thermal structure is summarized. The greenhouse effect of Titan's atmosphere, caused primarily by pressure induced opacity of N2, CH4, and H2, is discussed together with the antigreenhouse effect dominated by the haze which absorbs incident sunlight. The implications for the atmosphere of the presence of an ocean on Titan are also discussed.
Courtin Regis
Lunine Jonathan I.
McKay Christopher P.
Pollack James B.
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