The Mystery of Io's Warm Polar Regions: Implications for Heat Flow

Details The Mystery of Io's Warm Polar Regions: Implications for Heat Flow The Mystery of Io's Warm Polar Regions: Implications for Heat Flow

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1413m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1413

Computer Science

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Scientific paper

Unexpectedly warm polar temperatures further support the idea that Io is
covered virtually everywhere by cooling lava flows. This implies a new
heat flow component. Io's heat flow remains constrained between a lower
bound of ~2.5 W m^{-2} and an upper bound of ~13 W m^{-2}.

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