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November 03, 2009

Lecture 28: The Galilean Moons of Jupiter

44 minutes

The four large Galilean Moons of Jupiter seem unlikely places to look

for life; at first glance they should be cold, dead, icy worlds.

Instead we find tremendous geological diversity, and two big surprises:

volcanically-active Io, and icy Europa. Io is the most volcanically

active world in the Solar System, heated by tides from Jupiter. Europa

is even more surprising: its icy surface is young, with few impact

craters and extensive signs of recent repaving by liquid water. Even

more surprising is the distinct possibility that underneath Europa's ice

is a deep liquid water ocean, heated by tides from Jupiter. We will

review the evidence for Europa's liquid sub-ice ocean and look at its

potential as an abode of life. If there is life to be found anywhere in

the Solar System beyond Earth, beneath the ice of Europa may be the best

place to look. Recorded live on 2009 Nov 3 in Room 1005 Smith

Laboratory on the Columbus campus of The Ohio State University.

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By Richard Pogge