Venus, the second planet from the Sun, is perpetually veiled behind
opaque clouds of sulfuric acid droplets atop a hot, heavy, mostly carbon
dioxide atmosphere. In size and apparent composition, however, it is a
near twin-sister of the Earth. Why is it do different? This lecture
reviews the basic properties of Venus, and examines the similarties and
differences with the Earth. Recorded 2006 Nov 9 in 100 Stillman Hall on
the Columbus campus of The Ohio State University.
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