The Surface Compositions of Triton, Pluto, and Charon

Details The Surface Compositions of Triton, Pluto, and Charon The Surface Compositions of Triton, Pluto, and Charon

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ames.reptr....c&link_type=abstract

Technical Report, NASA Ames Research Center Moffett Field, CA United States

Other

Neptune (Planet), Binary Data, Charon, Pluto (Planet), Surface Properties, Natural Satellites, Planetary Surfaces, Planetary Composition, Spectroscopy, Nitrogen, Ice

Scientific paper

Neptune's satellite Triton, and the planet-satellite binary Pluto and Charon, are the most distant planetary bodies on which ices have been directly detected. Triton and Pluto have very similar dimensions and mean densities, suggesting a similar or common origin. Through earth-based spectroscopic observations in the near-infrared, solid N2, CH4, and CO have been found on both bodies, with the additional molecule C02 on Triton. N2 dominates both surfaces, although the coverage is not spatially uniform. On Triton, the CH4 and CO are mostly or entirely frozen in the N2 matrix, while CO2 may be spatially segregated. On Pluto, some CH4 and the CO are frozen in the N2 matrix, but there is evidence for additional CH4 in a pure state, perhaps lying as a lag deposit on a subsurface layer of N2. Despite their compositional and dimensional similarities, Pluto and Triton are quite different from one another in detail. Additional hydrocarbons and other volatile ices have been sought spectroscopically but not yet have been detected. The only molecule identified on Pluto's satellite Charon is solid H2O, but the spectroscopic data are of low precision and admit the presence of other ices such as CH4.

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