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Latitudinal distribution of carbon monoxide in the deep atmosphere of Venus

✍ Scribed by A.D. Collard; F.W. Taylor; S.B. Calcutt; R.W. Carlson; L.W. Kamp; K.H. Baines; Th. Encrenaz; P. Drossart; E. Lellouch; B. Bézard


Publisher
Elsevier Science
Year
1993
Tongue
English
Weight
959 KB
Volume
41
Category
Article
ISSN
0032-0633

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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