Infrared reflectance spectra of Hyperion, Titania, and Triton

Details Infrared reflectance spectra of Hyperion, Titania, and Triton Infrared reflectance spectra of Hyperion, Titania, and Triton

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...46..169l&link_type=abstract

Icarus, vol. 46, May 1981, p. 169-174.

Computer Science

11

Hyperion, Infrared Reflection, Satellite Surfaces, Titania, Triton, Uranus (Planet), Frost, Infrared Spectra, Natural Satellites, Satellite Atmospheres, Spectral Reflectance, Spectrophotometry, Spectrum Analysis, Planets, Uranus, Neptune, Saturn, Satellites, Triton, Titania, Frost, Hyperion, Spectrum, Reflectance, Infrared, Spectroscopy, Data, Methane, Comparisons, Surface, Observations, Wavelengths, Magnitude, Photometry

Scientific paper

Medium-resolution infrared (1-2.5 microns; Delta-lambda/lambda = 0.05) photometry of Triton, Titania, and Hyperion and medium-resolution (1.5-2.4 microns; Delta-lambda/lambda not greater than 0.01) spectroscopy of Triton are presented. Hyperion and Titania have spectra roughly similar to the laboratory spectrum of water frost, while the spectrum of Triton is inconsistent with the spectra of frosts likely to be major surface constituents.

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