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Carbon monoxide in the deep atmosphere of Venus

✍ Scribed by F.W. Taylor


Publisher
Elsevier Science
Year
1995
Tongue
English
Weight
614 KB
Volume
16
Category
Article
ISSN
0273-1177

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The Origin of Carbon Monoxide in Neptune
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The \(\mathrm{CO}\) abundance in the observable atmosphere of Neptune can be plausibly explained by rapid vertical mixing from the deeper atmosphere if Neptune has a greater complement of water than Uranus. Thermochemical equilibrium and kinetic calculations reveal that Neptune must and Uranus may h