Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability
Beneath the geologically complex ice shell of Europa, Jupiter’s innermost icy satellite, likely lies a vast, saline subsurface ocean that may hold conditions favorable for life. Key to that question is how processes in the ice shell, represented as a myriad of geologic features on the surface, facil...
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Georgia Institute of Technology
2022
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ftgeorgiatech:oai:smartech.gatech.edu:1853/66621 2023-05-15T18:18:48+02:00 Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability Chivers, Chase James Schmidt, Britney Earth and Atmospheric Sciences Robel, Alexander Wray, James Patterson, Wesley G. Hayne, Paul O. 2022-05-18T19:36:55Z application/pdf http://hdl.handle.net/1853/66621 en_US eng Georgia Institute of Technology http://hdl.handle.net/1853/66621 Planetary science Habitability Icy satellites Europa Ice dynamics Multiphase physics Numerical modeling Cryovolcanism Text Dissertation 2022 ftgeorgiatech 2023-04-03T17:55:42Z Beneath the geologically complex ice shell of Europa, Jupiter’s innermost icy satellite, likely lies a vast, saline subsurface ocean that may hold conditions favorable for life. Key to that question is how processes in the ice shell, represented as a myriad of geologic features on the surface, facilitate material transport between the surface and subsurface ocean. The formation of the young, elliptically shaped surface disruptions, lenticulae and chaotic (chaos) terrain that range from < 10 km to > 1000 km diameter, may represent one such process. Recent geologic analyses of the Galileo spacecraft observations suggests that both lenticulae and chaos terrain may form by reservoirs of saline liquid water emplaced as shallow as 1 km below the surface, or the so-called “shallow water” model. Lenticulae may form via the injection and freezing of liquid water sills < 10 km in diameter; Chaos terrain may form via local eutectic melting of the ice shell creating a “melt lens” > 50 km in diameter. In this thesis, I aim to link observations and formation hypotheses to theoretical numerical models that define hypothesis tests to motivate future observations for upcoming flyby mission NASA’s Europa Clipper. To that end, I developed a multiphase, two-dimensional, finite difference model that describes the thermal and chemical evolution of saline, shallow water reservoirs after they are emplaced in Europa’s ice shell. Built on the foundations of terrestrial sea ice formation by applying the microphysical process of mushy layer development, I can track the distribution of salts within the ice shell during and after the solidification of these saline reservoirs to predict both their longevity within the ice shell and how they may be detected by future missions. I show that while the liquid water within injected sills beneath lenticulae are shorter lived than previous estimates < 140,000 years, the interpretation of their geomorphology suggests liquid water is present within the ice shell. Similarly, I show that ... Doctoral or Postdoctoral Thesis Sea ice Georgia Institute of Technology: SMARTech - Scholarly Materials and Research at Georgia Tech |
institution |
Open Polar |
collection |
Georgia Institute of Technology: SMARTech - Scholarly Materials and Research at Georgia Tech |
op_collection_id |
ftgeorgiatech |
language |
English |
topic |
Planetary science Habitability Icy satellites Europa Ice dynamics Multiphase physics Numerical modeling Cryovolcanism |
spellingShingle |
Planetary science Habitability Icy satellites Europa Ice dynamics Multiphase physics Numerical modeling Cryovolcanism Chivers, Chase James Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
topic_facet |
Planetary science Habitability Icy satellites Europa Ice dynamics Multiphase physics Numerical modeling Cryovolcanism |
description |
Beneath the geologically complex ice shell of Europa, Jupiter’s innermost icy satellite, likely lies a vast, saline subsurface ocean that may hold conditions favorable for life. Key to that question is how processes in the ice shell, represented as a myriad of geologic features on the surface, facilitate material transport between the surface and subsurface ocean. The formation of the young, elliptically shaped surface disruptions, lenticulae and chaotic (chaos) terrain that range from < 10 km to > 1000 km diameter, may represent one such process. Recent geologic analyses of the Galileo spacecraft observations suggests that both lenticulae and chaos terrain may form by reservoirs of saline liquid water emplaced as shallow as 1 km below the surface, or the so-called “shallow water” model. Lenticulae may form via the injection and freezing of liquid water sills < 10 km in diameter; Chaos terrain may form via local eutectic melting of the ice shell creating a “melt lens” > 50 km in diameter. In this thesis, I aim to link observations and formation hypotheses to theoretical numerical models that define hypothesis tests to motivate future observations for upcoming flyby mission NASA’s Europa Clipper. To that end, I developed a multiphase, two-dimensional, finite difference model that describes the thermal and chemical evolution of saline, shallow water reservoirs after they are emplaced in Europa’s ice shell. Built on the foundations of terrestrial sea ice formation by applying the microphysical process of mushy layer development, I can track the distribution of salts within the ice shell during and after the solidification of these saline reservoirs to predict both their longevity within the ice shell and how they may be detected by future missions. I show that while the liquid water within injected sills beneath lenticulae are shorter lived than previous estimates < 140,000 years, the interpretation of their geomorphology suggests liquid water is present within the ice shell. Similarly, I show that ... |
author2 |
Schmidt, Britney Earth and Atmospheric Sciences Robel, Alexander Wray, James Patterson, Wesley G. Hayne, Paul O. |
format |
Doctoral or Postdoctoral Thesis |
author |
Chivers, Chase James |
author_facet |
Chivers, Chase James |
author_sort |
Chivers, Chase James |
title |
Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
title_short |
Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
title_full |
Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
title_fullStr |
Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
title_full_unstemmed |
Europa's Surface and Shallow Water: Ice Shell Activity and Implications for Habitability |
title_sort |
europa's surface and shallow water: ice shell activity and implications for habitability |
publisher |
Georgia Institute of Technology |
publishDate |
2022 |
url |
http://hdl.handle.net/1853/66621 |
genre |
Sea ice |
genre_facet |
Sea ice |
op_relation |
http://hdl.handle.net/1853/66621 |
_version_ |
1766195518623449088 |