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Triton's geyser-like plumes - Discovery and basic characterizationOne model for the mechanism driving the plumes of the four active geyser-like eruptions observed by Voyager 2 on Triton is a heating up of nitrogen ice in a subsurface greenhouse environment, where nitrogen gas pressurized by solar heating explosively vents to the surface carrying clouds of ice and dark particles into the atmosphere. A temperature increase of less than 4 K above the ambient surface value of 38 + or - 3 K suffices to drive the plumes to 8-km altitude. Each eruption may last a year or more, over the course of which 0.1 cu km of ice is sublimed.
Document ID
19910027591
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Soderblom, L. A.
(Geological Survey Flagstaff, AZ, United States)
Becker, T. L.
(USGS Flagstaff, AZ, United States)
Kieffer, S. W.
(Arizona State University Tempe, United States)
Brown, R. H.
(Geological Survey Flagstaff, AZ, United States)
Hansen, C. J.
(Geological Survey Flagstaff, AZ, United States)
Johnson, T. V.
(JPL Pasadena, CA, United States)
Date Acquired
August 14, 2013
Publication Date
October 19, 1990
Publication Information
Publication: Science
Volume: 250
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
91A12214
Distribution Limits
Public
Copyright
Other

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