Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation
The thickness of the outer ice shell plays an important role in several geodynamical processes at ocean worlds. Here, we show that observations of tidally driven diurnal surface displacements can constrain the mean ice shell thickness, dᵢ꜀ₑ. Such estimates are sensitive to any significant stru...
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2023
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ftcaltechauth:oai:authors.library.caltech.edu:wsgsq-5tv25 2024-09-15T18:36:55+00:00 Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation Berne, Alexander Simons, Mark Keane, James Tuttle Park, Ryan S. 2023-06 https://doi.org/10.1029/2022je007712 unknown American Geophysical Union https://doi.org/10.1029/2022je007712 oai:authors.library.caltech.edu:wsgsq-5tv25 eprintid:122538 resolverid:CaltechAUTHORS:20230725-447695700.1 info:eu-repo/semantics/openAccess Other Journal of Geophysical Research. Planets, 128(6), Art. No. e2022JE007712, (2023-06) Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Geochemistry and Petrology Geophysics info:eu-repo/semantics/article 2023 ftcaltechauth https://doi.org/10.1029/2022je007712 2024-08-06T15:35:04Z The thickness of the outer ice shell plays an important role in several geodynamical processes at ocean worlds. Here, we show that observations of tidally driven diurnal surface displacements can constrain the mean ice shell thickness, dᵢ꜀ₑ. Such estimates are sensitive to any significant structural features that break spherical symmetry such as faults and lateral variation in ice shell thickness and structure. We develop a finite-element model of Enceladus to calculate diurnal tidal displacements for a range of dᵢ꜀ₑ values in the presence of such structural heterogeneities. Consistent with results from prior studies, we find that the presence of variations in ice shell thickness can significantly amplify deformation in thinned regions. If major faults are also activated by tidal forcing—such as Tiger Stripes on Enceladus—their characteristic surface displacement patterns could easily be measured using modern geodetic methods. Within the family of Enceladus models explored, estimates of dᵢ꜀ₑ that assume spherical symmetry a priori can deviate from the true value by as much as ∼41% when structural heterogeneities are present. Additionally, we show that crustal heterogeneities near the South Pole produce differences of up to 35% between Love numbers evaluated at different spherical harmonic orders. A ∼41% range in estimates of dᵢ꜀ₑ from Love numbers is smaller than that found with approaches relying on static gravity and topography (∼250%) or analyzing diurnal libration amplitudes (∼85%) to infer dᵢ꜀ₑ at Enceladus. As such, we find that analysis of diurnal tidal deformation is a relatively robust approach to inferring mean crustal thickness. © 2023 American Geophysical Union. We would like to express our gratitude to the reviewers and editors for their valuable contributions in improving the clarity and content of this manuscript. This research was supported by the Future Investigators in NASA Earth and Space Science and Technology (FINESST) Program (80NSSC22K1318). We ... Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) Journal of Geophysical Research: Planets 128 6 |
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Open Polar |
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Caltech Authors (California Institute of Technology) |
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ftcaltechauth |
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unknown |
topic |
Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Geochemistry and Petrology Geophysics |
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Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Geochemistry and Petrology Geophysics Berne, Alexander Simons, Mark Keane, James Tuttle Park, Ryan S. Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
topic_facet |
Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Geochemistry and Petrology Geophysics |
description |
The thickness of the outer ice shell plays an important role in several geodynamical processes at ocean worlds. Here, we show that observations of tidally driven diurnal surface displacements can constrain the mean ice shell thickness, dᵢ꜀ₑ. Such estimates are sensitive to any significant structural features that break spherical symmetry such as faults and lateral variation in ice shell thickness and structure. We develop a finite-element model of Enceladus to calculate diurnal tidal displacements for a range of dᵢ꜀ₑ values in the presence of such structural heterogeneities. Consistent with results from prior studies, we find that the presence of variations in ice shell thickness can significantly amplify deformation in thinned regions. If major faults are also activated by tidal forcing—such as Tiger Stripes on Enceladus—their characteristic surface displacement patterns could easily be measured using modern geodetic methods. Within the family of Enceladus models explored, estimates of dᵢ꜀ₑ that assume spherical symmetry a priori can deviate from the true value by as much as ∼41% when structural heterogeneities are present. Additionally, we show that crustal heterogeneities near the South Pole produce differences of up to 35% between Love numbers evaluated at different spherical harmonic orders. A ∼41% range in estimates of dᵢ꜀ₑ from Love numbers is smaller than that found with approaches relying on static gravity and topography (∼250%) or analyzing diurnal libration amplitudes (∼85%) to infer dᵢ꜀ₑ at Enceladus. As such, we find that analysis of diurnal tidal deformation is a relatively robust approach to inferring mean crustal thickness. © 2023 American Geophysical Union. We would like to express our gratitude to the reviewers and editors for their valuable contributions in improving the clarity and content of this manuscript. This research was supported by the Future Investigators in NASA Earth and Space Science and Technology (FINESST) Program (80NSSC22K1318). We ... |
format |
Article in Journal/Newspaper |
author |
Berne, Alexander Simons, Mark Keane, James Tuttle Park, Ryan S. |
author_facet |
Berne, Alexander Simons, Mark Keane, James Tuttle Park, Ryan S. |
author_sort |
Berne, Alexander |
title |
Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
title_short |
Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
title_full |
Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
title_fullStr |
Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
title_full_unstemmed |
Inferring the Mean Thickness of the Outer Ice Shell of Enceladus From Diurnal Crustal Deformation |
title_sort |
inferring the mean thickness of the outer ice shell of enceladus from diurnal crustal deformation |
publisher |
American Geophysical Union |
publishDate |
2023 |
url |
https://doi.org/10.1029/2022je007712 |
genre |
South pole |
genre_facet |
South pole |
op_source |
Journal of Geophysical Research. Planets, 128(6), Art. No. e2022JE007712, (2023-06) |
op_relation |
https://doi.org/10.1029/2022je007712 oai:authors.library.caltech.edu:wsgsq-5tv25 eprintid:122538 resolverid:CaltechAUTHORS:20230725-447695700.1 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1029/2022je007712 |
container_title |
Journal of Geophysical Research: Planets |
container_volume |
128 |
container_issue |
6 |
_version_ |
1810480659506921472 |