๐”– Bobbio Scriptorium
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The rotation period of Neptune's upper atmosphere

โœ Scribed by R.Hamilton Brown; Dale P. Cruikshank; Alan T. Tokunaga


Publisher
Elsevier Science
Year
1981
Tongue
English
Weight
450 KB
Volume
47
Category
Article
ISSN
0019-1035

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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