NASA NTRS · 19900041678
Nonisothermal Pluto atmosphere models
Abstract
The present thermal profile calculation for a Pluto atmosphere model characterized by a high number fraction of CH4 molecules encompasses atmospheric heating by solar UV flux absorption and conductive transport cooling to the surface of Pluto. The stellar occultation curve predicted for an atmosphere of several-microbar surface pressures (which entail the existence of a substantial temperature gradient close to the surface) agrees with observations and implies that the normal and tangential optical depth of the atmosphere is almost negligible. The minimum period for atmospheric methane depletion is calculated to be 30 years.
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Hubbard, W. B., Yelle, Roger V., Lunine, Jonathan I.. 1990-03-01. Nonisothermal Pluto atmosphere models. https://ntrs.nasa.gov/citations/19900041678
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