Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar..100..221l&link_type=abstract
Icarus (ISSN 0019-1035), vol. 100, no. 1, p. 221-234.
Astronomy and Astrophysics
Astronomy
11
Astronomical Models, Atmospheric Models, Satellite Atmospheres, Triton, Abundance, Cratering, Heat Flux, Photochemical Reactions, Radiative Lifetime, Surface Temperature, Temperature Profiles, Volatility
Scientific paper
The idea of an early greenhouse atmosphere for Triton is presented and the conditions under which it may have been sustained are quantified. The volatile content of primordial Triton is modeled, and tidal heating rates are assessed to set bounds on the available energy. The atmospheric model formalism is presented, and it is shown how a massive atmosphere could have been raised by modest tidal heating fluxes. The implications of the model atmospheres for the atmospheric escape rates, the chemical evolution, and the cratering record are addressed.
Lunine Jonathan I.
Nolan Michael C.
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