Low Hadean Heat Flow and Heat Transport by Melt Segregation in the Early Earth and Io

Details Low Hadean Heat Flow and Heat Transport by Melt Segregation in the Early Earth and Io Low Hadean Heat Flow and Heat Transport by Melt Segregation in the Early Earth and Io

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpico1538.5598m&link_type=abstract

Astrobiology Science Conference 2010: Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond, held April 2

Biology

Scientific paper

An alternative explanation for the low thermal gradients recently
observed in Hadean zircons is that melt segregation dominated the
surface heat transport in the Hadean as is observed today on Jupiter's
moon Io.

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