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Extensional and compressional instabilities in Icy satellite lithospheres

Herrick, David L. and Stevenson, David J. (1990) Extensional and compressional instabilities in Icy satellite lithospheres. Icarus, 85 (1). pp. 191-204. ISSN 0019-1035. https://resolver.caltech.edu/CaltechAUTHORS:20131025-154927964

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Abstract

A simple mechanical model of planetary lithospheres and asthenospheres is combined with the most recent experimental results concerning the brittle and ductile deformation of ice I_h to determine the plausibility of forming the grooved terrains on Ganymede, Enceladus, and Miranda by means of lithospheric instabilities. The model assumes a lithosphere of uniform strength atop a substrate whose strength decreases exponentially with depth. The thickness of the lithosphere is defined by the intersection of a near-surface Byerlee's law relationship for brittle failure with a standard exponential ductile flow law at depth. For Ganymede we find that the relatively high surface gravity warm temperatures render virtually unachievable an instability strong enough to account for the observed topographic relief. However, a sufficiently strong instability, capable of producing features with the proper spacing, could develop on a smaller, colder body such as Enceladus or Miranda. The requirements in this case would be a strain rate greater than about 10^(−14) sec^(−1) and a near-surface thermal gradient of a few tens of degrees Kelvin per kilometer. The most reasonable way to accomplish these requirements is by the intrusive emplacement of a thick layer of warm ice beneath a preexisting lithosphere of about a kilometer or so in thickness, accompanied almost contemporaneously by a strain event lasting on the order of 10^5 years for extension or 10^3 years for compression. However, observed properties of grooved terrains on Enceladus and Miranda, such as nonuniform feature spacing and low crater counts, force us to conclude that unstable deformation must be more complicated than this simple model would suggest if it is to explain these features.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/0019-1035(90)90110-UDOIArticle
http://www.sciencedirect.com/science/article/pii/001910359090110UPublisherArticle
ORCID:
AuthorORCID
Stevenson, David J.0000-0001-9432-7159
Additional Information:© 1990 by Academic Press, Inc. Received May 12, 1989; revised September 8, 1989. This work was supported by NASA Planetary Geophysics Grant NAGW-185. We thank the reviewers for helpful suggestions and R. C. Fletcher for discussions.
Funders:
Funding AgencyGrant Number
NASANAGW-185
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences4758
Issue or Number:1
Record Number:CaltechAUTHORS:20131025-154927964
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20131025-154927964
Official Citation:David L. Herrick, David J. Stevenson, Extensional and compressional instabilities in Icy satellite lithospheres, Icarus, Volume 85, Issue 1, May 1990, Pages 191-204, ISSN 0019-1035, http://dx.doi.org/10.1016/0019-1035(90)90110-U. (http://www.sciencedirect.com/science/article/pii/001910359090110U)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:42082
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Oct 2013 23:09
Last Modified:03 Oct 2019 05:55

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