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Description

As Earth cools, water in the atmosphere condenses: torrential rains fall on, and on, and on. Great seas form. Exuberant volcanoes expel hotly agitated deep earth to the surface.

The hot, early atmosphere dances with an abundance of carbon dioxide, nitrogen, and water, and lesser amounts of methane and ammonia. Intense energy sources available on the primitive Earth form biologically important molecules from these gases. Candidate sources include solar UV-radiation (there is as yet no UV-protective ozone shield), radioactivity, and hot oceanic vents.

Date Created

1997

Holding Institution

University of Montana--Missoula. Environmental Studies Program

Rights Statement

In Copyright

Rights Holder

© 1997 Stiftung Drittes Millennium

Item Type

Exhibit

Digital File Format

image/jpeg

Media Type

Text; Image

Digital Image Number

08_wtt_file01_1-19.jpg

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