Resurfacing of Ganymede by Liquid-Water Volcanism

Details Resurfacing of Ganymede by Liquid-Water Volcanism Resurfacing of Ganymede by Liquid-Water Volcanism

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1490s&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1490

Physics

Scientific paper

Topography, such as a global set of graben, causes subsurface pressure
gradients that can drive pore-space liquid water (produced by tidal
heating) onto graben floors despite the negative buoyancy of the liquid.
This mechanism helps explain Ganymede's bright terrain.

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