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REVIEWS OF GEOPHYSICS,
VOL. 31, NO. 2,
PAGES 133–149,
1993
Does Titan Have an Ocean? A Review of Current Understanding of Titan's Surface
Jonathan I. Lunine
Lunar and Planetary Laboratory, University of Arizona, Tucson
Abstract
The nature of Titan’s surface has been a fascinating puzzle since the first definitive detection of an atmosphere in 1944.
Pre-Voyager models of the surface based largely on cosmochemistry and the detection of atmospheric methane permitted a range
of possibilities from clathrate hydrate to pure methane snow. The Voyager 1 flyby ruled out this last possibility but pointed
to a mixed ocean of methane, higher hydrocarbons, and nitrogen about a kilometer in thickness. Subsequent ground-based radar
observations reveal a reflective surface, inconsistent with pure light hydrocarbons. The variation in radar reflectivity from
night to night is surprisingly high. Passive radiometry at centimeter wavelengths indicates a surface emissivity distinct
from that of the icier Galilean satellites, suggesting that water ice does not dominate the surface either. Observations in
the near-infrared region are consistent with dirty water ice as well as a suite of other materials, including areas of hydrocarbon
seas. Reconciling the Voyager, radar and near-infrared data continue to be a challenge. Possibilities include the following:
a hydrocarbon ocean, which is frothy or contains a significant amount of aerosol contaminants, maintained near the surface
by stirring; an ocean stored in pore spaces of the ice regolith or in an aquiferlike system; an ocean that is somewhat smaller
than estimated from the methane photolysis rate because of impact-driven chemistry. Models involving significant amounts of
dry land exposed above a shallow ocean potentially run afoul of tidal constraints imposed by Titan’s nonzero free orbital
eccentricity. The Cassini/Huygens mission will investigate the nature of the surface through a variety of techniques and hopefully
solve this long-standing planetary puzzle.
Free Access to Full Article
Citation: Lunine, J. I.
(1993),
Does Titan Have an Ocean? A Review of Current Understanding of Titan's Surface,
Rev. Geophys.,
31(2),
133–149.
Copyright 1993 by the American Geophysical Union.
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