On the ortho-para equilibrium of H2 in the atmospheres of the Jovian planets

  • William Hayden Smith

Research output: Contribution to journalArticlepeer-review

22 Scopus citations

Abstract

The ratio for the equivalent widths for the unsaturated H2 quadrupole transitions observed in the Jovian planets is calculated and compared with a large number of observations. The comparison indicates that equilibrium hydrogen may be present in Jupiter and Saturn, while Uranus and Nepture exhibit ratios not in accord with equilibrium hydrogen. Observations which can differentiate among the possible states of H2 are proposed.

Original languageEnglish
Pages (from-to)210-216
Number of pages7
JournalIcarus
Volume33
Issue number1
DOIs
StatePublished - Jan 1978

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