Is Enceladus' plume tidally controlled?

Explanations for the plume of gas, water vapor and ice particles jetting from rifts in Enceladus' south polar region include boiling of liquid water and dissociation of clathrate hydrates. In either case, production of the plume may be quasi‐static or tidally controlled, with implications for t...

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Main Authors: I. Halevy, S. T. Stewart
Format: Article
Language:English
Published: Wiley 2008-06-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1029/2008GL034349
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author I. Halevy
S. T. Stewart
author_facet I. Halevy
S. T. Stewart
author_sort I. Halevy
collection DOAJ
description Explanations for the plume of gas, water vapor and ice particles jetting from rifts in Enceladus' south polar region include boiling of liquid water and dissociation of clathrate hydrates. In either case, production of the plume may be quasi‐static or tidally controlled, with implications for the interior structure and composition of Enceladus. Previous quantification of the clathrate explanation assumed equilibrium dissociation and cannot be used to simulate a tidally generated plume. We present a non‐equilibrium clathrate dissociation model, which we use to reproduce past observations and predict the plume's properties during upcoming close encounters. The total mass flux and water to gas mass ratio of a tidally generated plume are predicted to be lower than previous measurements. In comparison, for a quasi‐static plume these properties should have values close to previous measurements. This provides an observational means of distinguishing quasi‐static from dynamic processes as the plume's source.
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spelling doaj-art-8c6478793edc4f9a8dc2ea3e6ce0ccb42025-08-20T01:52:19ZengWileyGeophysical Research Letters0094-82761944-80072008-06-013512n/an/a10.1029/2008GL034349Is Enceladus' plume tidally controlled?I. Halevy0S. T. Stewart1Department of Earth and Planetary Sciences Harvard University Cambridge Massachusetts USADepartment of Earth and Planetary Sciences Harvard University Cambridge Massachusetts USAExplanations for the plume of gas, water vapor and ice particles jetting from rifts in Enceladus' south polar region include boiling of liquid water and dissociation of clathrate hydrates. In either case, production of the plume may be quasi‐static or tidally controlled, with implications for the interior structure and composition of Enceladus. Previous quantification of the clathrate explanation assumed equilibrium dissociation and cannot be used to simulate a tidally generated plume. We present a non‐equilibrium clathrate dissociation model, which we use to reproduce past observations and predict the plume's properties during upcoming close encounters. The total mass flux and water to gas mass ratio of a tidally generated plume are predicted to be lower than previous measurements. In comparison, for a quasi‐static plume these properties should have values close to previous measurements. This provides an observational means of distinguishing quasi‐static from dynamic processes as the plume's source.https://doi.org/10.1029/2008GL034349Enceladusplumeclathrate
spellingShingle I. Halevy
S. T. Stewart
Is Enceladus' plume tidally controlled?
Geophysical Research Letters
Enceladus
plume
clathrate
title Is Enceladus' plume tidally controlled?
title_full Is Enceladus' plume tidally controlled?
title_fullStr Is Enceladus' plume tidally controlled?
title_full_unstemmed Is Enceladus' plume tidally controlled?
title_short Is Enceladus' plume tidally controlled?
title_sort is enceladus plume tidally controlled
topic Enceladus
plume
clathrate
url https://doi.org/10.1029/2008GL034349
work_keys_str_mv AT ihalevy isenceladusplumetidallycontrolled
AT ststewart isenceladusplumetidallycontrolled