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Energy Sources for Chemical Evolution

Chemical Evolution (Ferris and Hagan, 1984) in which he expressed the hope that the elucidation of the chemistry of HCN would make an extremely important contribution to the solution of the biogenesis problem. [Pg.105]

Type of energy Available today (J/cm2/year) Assumed values forr primeval Earth (J/cm2/year) [Pg.106]

Learning of chemical concepts is assessed through two tests and homework assignments. Many of the questions on the tests require students to connect chemical concepts to issues relevant to chemical evolution or chemical processes important for life. For example, questions look at the possibility of life on Titan and the potential for successful life on Titan. This requires students to address this possibility in terms of energy sources, temperature, chemical processes given Titan s atmosphere, and the differences in chemical and physical processes in a liquid methane environment versus water. [Pg.384]

See other pages where Energy Sources for Chemical Evolution is mentioned: [Pg.107]    [Pg.109]    [Pg.111]    [Pg.105]    [Pg.105]    [Pg.107]    [Pg.109]    [Pg.111]    [Pg.107]    [Pg.109]    [Pg.111]    [Pg.105]    [Pg.105]    [Pg.107]    [Pg.109]    [Pg.111]    [Pg.335]    [Pg.1373]    [Pg.310]    [Pg.77]    [Pg.92]    [Pg.98]    [Pg.211]    [Pg.233]    [Pg.240]    [Pg.311]    [Pg.312]    [Pg.395]    [Pg.402]    [Pg.413]    [Pg.420]    [Pg.421]    [Pg.428]    [Pg.445]    [Pg.450]    [Pg.452]    [Pg.388]    [Pg.393]    [Pg.2]    [Pg.327]    [Pg.365]    [Pg.3]    [Pg.199]    [Pg.79]    [Pg.80]    [Pg.179]    [Pg.1557]    [Pg.88]    [Pg.161]    [Pg.66]    [Pg.2546]    [Pg.251]    [Pg.287]    [Pg.478]    [Pg.479]    [Pg.51]   


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