The Emissivity of Mars and Callisto in the Far Infrared

Details The Emissivity of Mars and Callisto in the Far Infrared The Emissivity of Mars and Callisto in the Far Infrared

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456....9b&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

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Iso, Planets And Satellites: Individual: Callisto And Mars

Scientific paper

Infrared spectra of Mars were taken with the two complementary spectrometers onboard the European Space Agency's Infrared Space Observatory, ISO, both in moder- ate- and high-resolution mode. From the strengths of the observed water lines we derived information about the vertical distribution of water vapor and on the emissivity of the dust/surface system in the far infrared. The emissivity values obtained with this method were then compared with laboratory spectra of several minerals. A complete spectrum of Callisto from 50 to 180 μm is presented. It shows very good overall agreement with a model originally developed to match the far-infrared spectra of asteroids. Slight discrepancies between observation and model at certain wavelengths are discussed.

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