The Origin of Carbon Monoxide in Neptune's Atmosphere

K. Lodders, B. Fegley

Research output: Contribution to journalArticlepeer-review

68 Scopus citations

Abstract

The 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 have about 10 times more oxygen than carbon, whereas for Jupiter and Saturn equal enrichments of carbon and oxygen are satisfactory to explain the observed CO abundances by deep vertical mixing. Relative to hydrogen and solar composition, the respective enrichment factors for carbon and oxygen are 41, 440 (Neptune); 32, ≤260 (Uranus); 6.6, 6.6 (Saturn); and 2.8, 2.8 (Jupiter). Because water ice is the most refractory ice among the ices assumed to be present in the outer solar nebula, the most massive H2O enrichment is expected for the outermost planet of this group. Thus, Neptune can indeed be regarded as the "god of the seas".

Original languageEnglish
Pages (from-to)368-375
Number of pages8
JournalIcarus
Volume112
Issue number2
DOIs
StatePublished - Dec 1994

Fingerprint

Dive into the research topics of 'The Origin of Carbon Monoxide in Neptune's Atmosphere'. Together they form a unique fingerprint.

Cite this