Evidence for Volcanic Support of Io's Jupiter-Facing Atmosphere from Constraints on Post-Eclipse Atmospheric Changes

Details Evidence for Volcanic Support of Io's Jupiter-Facing Atmosphere from Constraints on Post-Eclipse Atmospheric Changes Evidence for Volcanic Support of Io's Jupiter-Facing Atmosphere from Constraints on Post-Eclipse Atmospheric Changes

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2420s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2420

Physics

Scientific paper

New Hubble observations of Io's atmosphere show minimal changes in
atmospheric density as Io warms after Jupiter eclipse. The simplest
explanation of this surprising result is that the atmosphere on the this
side of Io is volcanically supported.

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