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In-situ detection of Europa's water plumes is harder than previously thought

In-situ detection of Europa's water plumes is harder than previously thought
In-situ detection of Europa's water plumes is harder than previously thought

Europa's subsurface ocean is a potential candidate for life in the outer solar system. It is thought that plumes may exist which eject ocean material out into space, which may be detected by a spacecraft flyby. Previous work on the feasibility of these detections has assumed a collisionless model of the plume particles. New models of the plumes including particle collisions have shown that a shock can develop in the plume interior as rising particles collide with particles falling back to the moon's surface, limiting the plume's altitude. These models also assume a Laval nozzle-like vent which results in a colder plume source temperature than in previous studies, further limiting the plume's extent. We investigate to what degree the limited extent of the shocked plumes reduces the ability of the JUICE spacecraft to detect plume H 2O molecules. Results show that the region over Europa's surface within which plumes would be separable from the H 2O atmosphere by JUICE (the region of separability) is reduced by up to a half with the collisional model compared to the collisionless model. Putative plume sources which are on the border of the region of separability for the collisionless model cannot be separated from the atmosphere when the shock is considered for a mass flux case of 100 kgs −1. Increasing the flyby altitude by 100 km such that the spacecraft passes above the shock canopy results in a reduction in region of separability by a third, whilst decreasing the flyby altitude by 100 km increases the region of separability by the same amount. We recommend flybys pass through or as close to the shock as possible to sample the most high-density region. If the spacecraft flies close to the shock, the structure of the plume could be resolvable using the neutral mass spectrometer on JUICE, allowing us to test models of the plume physics and understand the underlying physics of Europa's plumes. As the altitude of the shock is uncertain and dependent on unpredictable plume parameters, we recommend flybys be lowered where possible to reduce the risk of passing above the shock and losing detection coverage, density and duration.

Atmospheres, dynamics, Europa, Jupiter, Satellites, Satellites, atmospheres, Satellites, composition, Volcanism, Jupiter, satellites
0019-1035
Dayton-Oxland, Rowan
96dd567a-6644-4207-a112-8023c4f18d8a
Huybrights, Hans L.F.
7928b4a8-0055-4d65-85fc-96cbd268a3d7
Winterhalder, Thomas O.
9f06e33e-1bf5-44b4-ba18-a50d759bcd00
Mahieux, Arnaud
ef5af8a2-2805-4f3f-9748-cf914f0f96d7
Goldstein, David
a400cd04-7a3b-419a-85d9-ca77eeabb08c
Dayton-Oxland, Rowan
96dd567a-6644-4207-a112-8023c4f18d8a
Huybrights, Hans L.F.
7928b4a8-0055-4d65-85fc-96cbd268a3d7
Winterhalder, Thomas O.
9f06e33e-1bf5-44b4-ba18-a50d759bcd00
Mahieux, Arnaud
ef5af8a2-2805-4f3f-9748-cf914f0f96d7
Goldstein, David
a400cd04-7a3b-419a-85d9-ca77eeabb08c

Dayton-Oxland, Rowan, Huybrights, Hans L.F., Winterhalder, Thomas O., Mahieux, Arnaud and Goldstein, David (2023) In-situ detection of Europa's water plumes is harder than previously thought. Icarus, 395, [115488]. (doi:10.1016/j.icarus.2023.115488).

Record type: Article

Abstract

Europa's subsurface ocean is a potential candidate for life in the outer solar system. It is thought that plumes may exist which eject ocean material out into space, which may be detected by a spacecraft flyby. Previous work on the feasibility of these detections has assumed a collisionless model of the plume particles. New models of the plumes including particle collisions have shown that a shock can develop in the plume interior as rising particles collide with particles falling back to the moon's surface, limiting the plume's altitude. These models also assume a Laval nozzle-like vent which results in a colder plume source temperature than in previous studies, further limiting the plume's extent. We investigate to what degree the limited extent of the shocked plumes reduces the ability of the JUICE spacecraft to detect plume H 2O molecules. Results show that the region over Europa's surface within which plumes would be separable from the H 2O atmosphere by JUICE (the region of separability) is reduced by up to a half with the collisional model compared to the collisionless model. Putative plume sources which are on the border of the region of separability for the collisionless model cannot be separated from the atmosphere when the shock is considered for a mass flux case of 100 kgs −1. Increasing the flyby altitude by 100 km such that the spacecraft passes above the shock canopy results in a reduction in region of separability by a third, whilst decreasing the flyby altitude by 100 km increases the region of separability by the same amount. We recommend flybys pass through or as close to the shock as possible to sample the most high-density region. If the spacecraft flies close to the shock, the structure of the plume could be resolvable using the neutral mass spectrometer on JUICE, allowing us to test models of the plume physics and understand the underlying physics of Europa's plumes. As the altitude of the shock is uncertain and dependent on unpredictable plume parameters, we recommend flybys be lowered where possible to reduce the risk of passing above the shock and losing detection coverage, density and duration.

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Accepted/In Press date: 13 February 2023
e-pub ahead of print date: 15 February 2023
Published date: 1 May 2023
Additional Information: Funding Information: We thank the reviewers for their effort in providing their useful and insightful comments on the manuscript. This work was carried out during the Leiden/ESA Astrophysics Program for Summer students (LEAPS) 2020 hosted by the European Space Research and Technology Centre (ESTEC) - European Space Agency (ESA) and Leiden Observatory. R. Dayton-Oxland is supported by the University of Southampton and INSPIRE Doctoral Training Program; this work was supported by the Natural Environmental Research Council [grant number NE/S007210/1]. H. Huybrighs gratefully acknowledges the support from Khalifa University's Space and Planetary Science Center under grant N. KU-SPSC-8474000336, the ESA research fellowship and the International Space Science Institute (ISSI) visiting scientist program. T. O. Winterhalder was supported by the University of Heidelberg and the European Southern Observatory. D. B. Goldstein and A. Mahieux were supported by the SSW NASA grant with award number 80NSSC21K016. Plume computations were done at the Texas Advanced Computing Center. Funding Information: We thank the reviewers for their effort in providing their useful and insightful comments on the manuscript. This work was carried out during the Leiden/ESA Astrophysics Program for Summer students (LEAPS) 2020 hosted by the European Space Research and Technology Centre (ESTEC) - European Space Agency (ESA) and Leiden Observatory. R. Dayton-Oxland is supported by the University of Southampton and INSPIRE Doctoral Training Program ; this work was supported by the Natural Environmental Research Council [grant number NE/S007210/1 ]. H. Huybrighs gratefully acknowledges the support from Khalifa University’s Space and Planetary Science Center under grant N. KU-SPSC-8474000336 , the ESA research fellowship and the International Space Science Institute (ISSI) visiting scientist program . T. O. Winterhalder was supported by the University of Heidelberg and the European Southern Observatory . D. B. Goldstein and A. Mahieux were supported by the SSW NASA grant with award number 80NSSC21K016 . Plume computations were done at the Texas Advanced Computing Center. Publisher Copyright: © 2023 The Author(s)
Keywords: Atmospheres, dynamics, Europa, Jupiter, Satellites, Satellites, atmospheres, Satellites, composition, Volcanism, Jupiter, satellites

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Local EPrints ID: 475592
URI: http://eprints.soton.ac.uk/id/eprint/475592
ISSN: 0019-1035
PURE UUID: 151fd4f9-8ec8-4e8a-bc2e-644abd1b0d08

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Date deposited: 22 Mar 2023 17:31
Last modified: 17 Mar 2024 00:49

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Contributors

Author: Hans L.F. Huybrights
Author: Thomas O. Winterhalder
Author: Arnaud Mahieux
Author: David Goldstein

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