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A subsolar oxygen abundance or a radiative region deep in Jupiter revealed by thermochemical modelling

A diffusion model of Jupiter’s troposphere with updated thermochemistry can explain the upper tropospheric CO observations if the deep oxygen abundance is subsolar. Alternatively, to reproduce Juno’s supersolar deep oxygen abundances, a deep layer of reduced vertical mixing is necessary.

T. Cavalié
J. Lunine
O. Mousis
Research30 Mar 2023
Nature Astronomy

Volume: 7, P: 678-683
Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA

Trace gases CO and HCN are detected by ALMA in various locations of Jupiter’s disc. Contrary to CO, HCN is depleted in the auroral regions, indicative of the action of heterogeneous chemistry that bonds HCN to organic aerosol particles produced in the aurorae.

T. Cavalié
L. Rezac
Z. Perrin
Research06 Jul 2023
Nature Astronomy

Volume: 7, P: 1048-1055
Author Correction: Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA

T. Cavalié
L. Rezac
Z. Perrin
Amendments and Corrections02 Aug 2024
Nature Astronomy

Volume: 8, P: 1206

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A subsolar oxygen abundance or a radiative region deep in Jupiter revealed by thermochemical modelling

Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA

Author Correction: Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA

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