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Ices on Io — Composition and Texture

  • Douglas B. Nash
  • Bruce H. Betts
Part of the Astrophysics and Space Science Library book series (ASSL, volume 227)

Abstract

Io is the innermost (nearest to Jupiter) of the four Galilean satellites. We know from their infrared radiometric and spectral signatures that the outer three satellites, Europa, Ganymede, and Callisto, have cold surfaces (~ 120 K or less) containing abundant H2O ice, with Europa’s surface being nearly pure water ice and that of the others showing water ice with dark, presumably non-ice (perhaps rocky) components [Clark et al., 1986].

Keywords

Volcanic Plume Galilean Satellite Jovian System Cold Trapping Frost Deposit 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1998

Authors and Affiliations

  • Douglas B. Nash
    • 1
  • Bruce H. Betts
    • 1
  1. 1.San Juan Capistrano Research InstituteSan Juan CapistranoUSA

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