Distributions of H2O and CO2 ices on Ariel, Umbriel, Titania, and Oberon from IRTF/SpeX observations

@article{Grundy2006DistributionsOH,
  title={Distributions of H2O and CO2 ices on Ariel, Umbriel, Titania, and Oberon from IRTF/SpeX observations},
  author={William M. Grundy and Leslie A. Young and John R. Spencer and R. E. Johnson and Eliot F. Young and Marc W. Buie},
  journal={Icarus},
  year={2006},
  volume={184},
  pages={543-555}
}

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References

SHOWING 1-10 OF 98 REFERENCES

The Distribution and Physical State of H2O on Charon

We present new 1.4- to 2.5-μm geometric albedo spectra of Charon taken with HST/NICMOS in 1998. These new data provide global coverage of the surface with four spectra at evenly spaced longitudes.

Distributions of CO2 and SO2 on the surface of Callisto

Absorption bands in the infrared reflectance spectra from the Galileo Near-Infrared Mapping Spectrometer (NIMS) which are attributed to the presence of CO2 and SO2 on the surface of Callisto have

Cassini Visual and Infrared Mapping Spectrometer Observations of Iapetus: Detection of CO2

The Visual and Infrared Mapping Spectrometer (VIMS) instrument aboard the Cassini spacecraft obtained its first spectral map of the satellite Iapetus in which new absorption bands are seen in the

Cratering history of the Uranian satellites: Umbriel, Titania, and Oberon

Crater size-frequency data for Umbriel, Titania, and Oberon are presented, and the implications of those data are discussed in terms of the geologic histories of these bodies and the populations of

Ice chemistry on the Galilean satellites

Jupiter's icy satellites Europa, Ganymede, and Callisto are subject to energy fluxes from electrons, photons, and magnetospheric plasma ion bombardment. As water ice and CO2 ice are thought to be

The Strengths of Near-Infrared Absorption Features Relevant to Interstellar and Planetary Ices

The abundances of ices in planetary environments have historically been obtained through measurements of near-infrared absorption features (λ = 1.0-2.5 μm), and near-IR transmission measurements of

Photolysis and radiolysis of water ice on outer solar system bodies

In this paper the available laboratory data on photolysis and radiolysis of water ice are summarized for the purpose of interpreting remote sensing data for the icy satellites. The relevance of these
...