Ices on the surface of Triton

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Atmospheric Chemistry, Carbon Dioxide, Ice, Satellite Atmospheres, Triton, Astronomical Spectroscopy, Infrared Spectra, Photochemical Reactions, Satellite Surfaces, Neptune, Triton, Satellites, Ice, Surface, Spectroscopy, Wavelengths, Near-Infrared, Composition, Nitrogen, Methane, Carbon Monoxide, Spectra, Carbon Dioxide, Atmosphere, Earth-Based Observations, Reflectance, Model, Procedure, Parameters, Abundance, Volatility, Hypotheses, Hydrocarbons

Scientific paper

The near-infrared spectrum of Triton reveals ices of nitrogen, methane, carbon monoxide, and carbon dioxide, of which nitrogen is the dominant component. Carbon dioxide ice may be spatially segregated from the other more volatile ices, covering about 10 percent of Triton's surface. The absence of ices of other hydrocarbons and nitriles challenges existing models of methane and nitrogen photochemistry on Triton.

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