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Vital Signs: Seismology of Icy Ocean Worlds

Vance, Steven D. and Kedar, Sharon and Panning, Mark P. and Stähler, Simon C. and Bills, Bruce G. and Lorenz, Ralph D. and Huang, Hsin-Hua and Pike, W. T. and Castillo, Julie C. and Lognonné, Philippe and Tsai, Victor C. and Rhoden, Alyssa R. (2018) Vital Signs: Seismology of Icy Ocean Worlds. Astrobiology, 18 (1). pp. 37-53. ISSN 1531-1074. https://resolver.caltech.edu/CaltechAUTHORS:20180122-074827302

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Abstract

Ice-covered ocean worlds possess diverse energy sources and associated mechanisms that are capable of driving significant seismic activity, but to date no measurements of their seismic activity have been obtained. Such investigations could reveal the transport properties and radial structures, with possibilities for locating and characterizing trapped liquids that may host life and yielding critical constraints on redox fluxes and thus on habitability. Modeling efforts have examined seismic sources from tectonic fracturing and impacts. Here, we describe other possible seismic sources, their associations with science questions constraining habitability, and the feasibility of implementing such investigations. We argue, by analogy with the Moon, that detectable seismic activity should occur frequently on tidally flexed ocean worlds. Their ices fracture more easily than rocks and dissipate more tidal energy than the <1 GW of the Moon and Mars. Icy ocean worlds also should create less thermal noise due to their greater distance and consequently smaller diurnal temperature variations. They also lack substantial atmospheres (except in the case of Titan) that would create additional noise. Thus, seismic experiments could be less complex and less susceptible to noise than prior or planned planetary seismology investigations of the Moon or Mars.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1089/ast.2016.1612DOIArticle
http://online.liebertpub.com/doi/abs/10.1089/ast.2016.1612PublisherArticle
ORCID:
AuthorORCID
Vance, Steven D.0000-0002-4242-3293
Panning, Mark P.0000-0002-2041-3190
Stähler, Simon C.0000-0002-0783-2489
Lorenz, Ralph D.0000-0001-8528-4644
Huang, Hsin-Hua0000-0002-1115-2427
Pike, W. T.0000-0002-7660-6231
Tsai, Victor C.0000-0003-1809-6672
Additional Information:© 2018 Mary Ann Liebert, Inc. Submitted 27 October 2016; Accepted 7 June 2017. We thank for their helpful input Sridhar Anandakrishnan, Bruce Banerdt, Jason Goodman, and Jennifer Jackson. This work was partially supported by strategic research and technology funds from the Jet Propulsion Laboratory, Caltech, and by the Icy Worlds node of NASA's Astrobiology Institute (13-13NAI7_2-0024). The research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. No competing financial interests exist.
Group:Seismological Laboratory
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
NASA13-13NAI7_2-0024
Subject Keywords:Seismology—Redox—Ocean worlds—Europa—Ice—Hydrothermal
Issue or Number:1
Record Number:CaltechAUTHORS:20180122-074827302
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180122-074827302
Official Citation:Vance Steven D., Kedar Sharon, Panning Mark P., Stähler Simon C., Bills Bruce G., Lorenz Ralph D., Huang Hsin-Hua, Pike W.T., Castillo Julie C., Lognonné Philippe, Tsai Victor C., and Rhoden Alyssa R.. Astrobiology. January 2018, 18(1): 37-53. https://doi.org/10.1089/ast.2016.1612
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84437
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:23 Jan 2018 13:07
Last Modified:09 Mar 2020 13:19

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