Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus

Context. The origin of water in the stratospheres of giant planets has been an outstanding question ever since its first detection by the Infrared Space Observatory some 20 years ago. Water can originate from interplanetary dust particles, icy rings and satellites, and large comet impacts. Analyses...

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Published in:Astronomy & Astrophysics
Main Authors: Cavalié, T., Hue, V., Hartogh, P., Moreno, R., Lellouch, E., Feuchtgruber, H., Jarchow, C., Cassidy, T., Fletcher, L., Billebaud, F., Dobrijevic, M., Rezac, L., Orton, G., Rengel, M., Fouchet, T., Guerlet, S.
Format: Article in Journal/Newspaper
Language:English
Published: 2019
Subjects:
Online Access:http://hdl.handle.net/21.11116/0000-0004-D0EA-9
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spelling ftpubman:oai:pure.mpg.de:item_3168582 2023-08-27T04:12:07+02:00 Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus Cavalié, T. Hue, V. Hartogh, P. Moreno, R. Lellouch, E. Feuchtgruber, H. Jarchow, C. Cassidy, T. Fletcher, L. Billebaud, F. Dobrijevic, M. Rezac, L. Orton, G. Rengel, M. Fouchet, T. Guerlet, S. 2019 http://hdl.handle.net/21.11116/0000-0004-D0EA-9 eng eng info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201935954 http://hdl.handle.net/21.11116/0000-0004-D0EA-9 Astronomy and Astrophysics Planetary Atmospheres HERSCHEL: HIFI info:eu-repo/semantics/article 2019 ftpubman https://doi.org/10.1051/0004-6361/201935954 2023-08-02T00:06:07Z Context. The origin of water in the stratospheres of giant planets has been an outstanding question ever since its first detection by the Infrared Space Observatory some 20 years ago. Water can originate from interplanetary dust particles, icy rings and satellites, and large comet impacts. Analyses of Herschel Space Observatory observations have proven that the bulk of Jupiter’s stratospheric water was delivered by the Shoemaker-Levy 9 impacts in 1994. In 2006, the Cassini mission detected water plumes at the South Pole of Enceladus, which made the moon a serious candidate for Saturn’s stratospheric water. Further evidence was found in 2011 when Herschel demonstrated the presence of a water torus at the orbital distance of Enceladus that was fed by the moon’s plumes. Finally, water falling from the rings onto Saturn’s uppermost atmospheric layers at low latitudes was detected during the final orbits of Cassini’s end-of-mission plunge into the atmosphere. Aims. In this paper, we use Herschel mapping observations of water in Saturn’s stratosphere to identify its source. Methods. We tested several empirical models against the Herschel-HIFI and -PACS observations, which were collected on December 30, 2010, and January 2, 2011, respectively. Results. We demonstrate that Saturn’s stratospheric water is not uniformly mixed as a function of latitude, but peaks at the equator and decreases poleward with a Gaussian distribution. We obtain our best fit with an equatorial mole fraction 1.1 ppb and a half width at half maximum of 25°, when accounting for a temperature increase in the two warm stratospheric vortices produced by Saturn’s Great Storm of 2010–2011. Conclusions. This work demonstrates that Enceladus is the main source of Saturn’s stratospheric water. Article in Journal/Newspaper South pole Max Planck Society: MPG.PuRe Levy ENVELOPE(-66.567,-66.567,-66.320,-66.320) South Pole Astronomy & Astrophysics 630 A87
institution Open Polar
collection Max Planck Society: MPG.PuRe
op_collection_id ftpubman
language English
topic Planetary Atmospheres
HERSCHEL: HIFI
spellingShingle Planetary Atmospheres
HERSCHEL: HIFI
Cavalié, T.
Hue, V.
Hartogh, P.
Moreno, R.
Lellouch, E.
Feuchtgruber, H.
Jarchow, C.
Cassidy, T.
Fletcher, L.
Billebaud, F.
Dobrijevic, M.
Rezac, L.
Orton, G.
Rengel, M.
Fouchet, T.
Guerlet, S.
Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
topic_facet Planetary Atmospheres
HERSCHEL: HIFI
description Context. The origin of water in the stratospheres of giant planets has been an outstanding question ever since its first detection by the Infrared Space Observatory some 20 years ago. Water can originate from interplanetary dust particles, icy rings and satellites, and large comet impacts. Analyses of Herschel Space Observatory observations have proven that the bulk of Jupiter’s stratospheric water was delivered by the Shoemaker-Levy 9 impacts in 1994. In 2006, the Cassini mission detected water plumes at the South Pole of Enceladus, which made the moon a serious candidate for Saturn’s stratospheric water. Further evidence was found in 2011 when Herschel demonstrated the presence of a water torus at the orbital distance of Enceladus that was fed by the moon’s plumes. Finally, water falling from the rings onto Saturn’s uppermost atmospheric layers at low latitudes was detected during the final orbits of Cassini’s end-of-mission plunge into the atmosphere. Aims. In this paper, we use Herschel mapping observations of water in Saturn’s stratosphere to identify its source. Methods. We tested several empirical models against the Herschel-HIFI and -PACS observations, which were collected on December 30, 2010, and January 2, 2011, respectively. Results. We demonstrate that Saturn’s stratospheric water is not uniformly mixed as a function of latitude, but peaks at the equator and decreases poleward with a Gaussian distribution. We obtain our best fit with an equatorial mole fraction 1.1 ppb and a half width at half maximum of 25°, when accounting for a temperature increase in the two warm stratospheric vortices produced by Saturn’s Great Storm of 2010–2011. Conclusions. This work demonstrates that Enceladus is the main source of Saturn’s stratospheric water.
format Article in Journal/Newspaper
author Cavalié, T.
Hue, V.
Hartogh, P.
Moreno, R.
Lellouch, E.
Feuchtgruber, H.
Jarchow, C.
Cassidy, T.
Fletcher, L.
Billebaud, F.
Dobrijevic, M.
Rezac, L.
Orton, G.
Rengel, M.
Fouchet, T.
Guerlet, S.
author_facet Cavalié, T.
Hue, V.
Hartogh, P.
Moreno, R.
Lellouch, E.
Feuchtgruber, H.
Jarchow, C.
Cassidy, T.
Fletcher, L.
Billebaud, F.
Dobrijevic, M.
Rezac, L.
Orton, G.
Rengel, M.
Fouchet, T.
Guerlet, S.
author_sort Cavalié, T.
title Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
title_short Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
title_full Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
title_fullStr Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
title_full_unstemmed Herschel map of Saturn’s stratospheric water, delivered by the plumes of Enceladus
title_sort herschel map of saturn’s stratospheric water, delivered by the plumes of enceladus
publishDate 2019
url http://hdl.handle.net/21.11116/0000-0004-D0EA-9
long_lat ENVELOPE(-66.567,-66.567,-66.320,-66.320)
geographic Levy
South Pole
geographic_facet Levy
South Pole
genre South pole
genre_facet South pole
op_source Astronomy and Astrophysics
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201935954
http://hdl.handle.net/21.11116/0000-0004-D0EA-9
op_doi https://doi.org/10.1051/0004-6361/201935954
container_title Astronomy & Astrophysics
container_volume 630
container_start_page A87
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