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Diapirism on Triton - A record of crustal layering and instabilityCantaloupe terrain on Neptune's large, icy satellite Triton comprises an organized cellular pattern of noncircular dimples that structurally and geologically most closely resemble salt diapirs exposed on Earth. The mean separation of these cells is 47 km. Modeling of the cells as compositionally driven diapirs suggests that cantaloupe terrain forms by gravity-driven overturn within an ice crust about 20 km thick with a maximum viscosity of 10 exp 22 Pa s. These diapirs probably formed as a result of a density inversion in a layered crust composed partly of ice phases other than water ice.
Document ID
19930068198
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schenk, Paul
(Lunar and Planetary Inst. Houston, TX, United States)
Jackson, M. P. A.
(Texas Univ. Austin, United States)
Date Acquired
August 16, 2013
Publication Date
April 1, 1993
Publication Information
Publication: Geology
ISSN: 0091-7613
Subject Category
Lunar And Planetary Exploration
Accession Number
93A52195
Funding Number(s)
CONTRACT_GRANT: NASW-4574
Distribution Limits
Public
Copyright
Other

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