2023NatAs...7.1048C


Query : 2023NatAs...7.1048C

2023NatAs...7.1048C - Nature Astronomy, 7, 1048-1055 (2023/September-0)

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

CAVALIE T., REZAC L., MORENO R., LELLOUCH E., FOUCHET T., BENMAHI B., GREATHOUSE T.K., SINCLAIR J.A., HUE V., HARTOGH P., DOBRIJEVIC M., CARRASCO N. and PERRIN Z.

Abstract (from CDS):

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+2-12-1+2{2}_{-1}^{+2} and 0.04+0.07-0.030.04-0.03+0.07{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.


Abstract Copyright: 2023 The Author(s), under exclusive licence to Springer Nature Limited

Journal keyword(s):

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3205 2
2 [VV2006] J131250.9-042451 Bla 13 12 50.90123596 -04 24 49.8921276     18.7 19.29   ~ 86 1

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