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

MPG-Autoren
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Rezac,  L.
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Hartogh,  P
Planetary Science Department, Max Planck Institute for Solar System Research, Max Planck Society;

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Cavalié, T., Rezac, L., Moreno, R., Lellouch, E., Fouchet, T., Benmahi, B., et al. (2023). Evidence for auroral influence on Jupiter's nitrogen and oxygen chemistry revealed by ALMA. Nature Astronomy, 7, 1048-1055. doi:10.1038/s41550-023-02016-7.


Zitierlink: https://hdl.handle.net/21.11116/0000-000D-7CA8-B
Zusammenfassung
The localized delivery of new long-lived species to Jupiter's stratosphere by comet Shoemaker-Levy 9 in 1994 opened a window to constrain Jovian chemistry and dynamics by monitoring the evolution of their vertical and horizontal distributions. However, the spatial distributions of CO and HCN, two of these long-lived species, had never been jointly observed at high latitudinal resolution. Atacama large millimeter/submillimeter array observations of HCN and CO in March 2017 show that CO was meridionally uniform and restricted to pressures lower than 3 ± 1 mbar. HCN shared a similar vertical distribution in the low- to mid-latitudes, but was depleted at pressures between 2−1+2 and 0.04−0.03+0.07 mbar in the aurora and surrounding regions, resulting in a drop by two orders of magnitude in column density. We propose that heterogeneous chemistry bonds HCN on large aurora-produced aerosols at these pressures in the Jovian auroral regions causing the observed depletion.