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An inversion in the atmosphere of TitanA very detailed greenhouse model derives a methane to hydrogen ratio of unity and a minimum surface pressure of 0.4 atm. Based on a surface gravity g = 140 cm sec/2, the minimum CH4 abundance is 30-40 km-A and the minimum H2 abundance varies from 15 to 85 km-A. A model of the atmosphere of Titan is proposed which seems to be consistent with observations and requires a much smaller CH4 abundance (of the order or 2 km-atm). Although no H2 is required, the presence of some H2 is readily accommodated. In this model, a temperature inversion exists in the atmosphere due to absorption of blue and ultraviolet solar radiation by small particles. The absorbed radiation is re-radiated by the dust and by molecules having long wavelength bands such as CH4 7.7 micrometer and ethane at 12.2 micrometer. The brightness temperature at 20 micrometer is primarily due to re-radiation by the dust.
Document ID
19740012375
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Danielson, R. E.
(Princeton Univ. NJ, United States)
Caldwell, J. J.
(Princeton Univ. NJ, United States)
Larach, D. R.
(Princeton Univ. NJ, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Publication Information
Publication: NASA. Ames Res. Center The Atmos. of Titan
Subject Category
Space Sciences
Accession Number
74N20488
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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