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A close-up look at Io from Galileo's near-infrared mapping spectrometerInfrared spectral images of Jupiter's volcanic moon Io, acquired during the October and November 1999 and February 2000 flybys of the Galileo spacecraft, were used to study the thermal structure and sulfur dioxide distribution of active volcanoes. Loki Patera, the solar system's most powerful known volcano, exhibits large expanses of dark, cooling lava on its caldera floor. Prometheus, the site of long-lived plume activity, has two major areas of thermal emission, which support ideas of plume migration. Sulfur dioxide deposits were mapped at local scales and show a more complex relationship to surface colors than previously thought, indicating the presence of other sulfur compounds.
Document ID
20040141561
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lopes-Gautier, R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena CA United States)
Doute, S.
Smythe, W. D.
Kamp, L. W.
Carlson, R. W.
Davies, A. G.
Leader, F. E.
McEwen, A. S.
Geissler, P. E.
Kieffer, S. W.
Keszthelyi, L.
Barbinis, E.
Mehlman, R.
Segura, M.
Shirley, J.
Soderblom, L. A.
Date Acquired
August 22, 2013
Publication Date
May 19, 2000
Publication Information
Publication: Science
Volume: 288
Issue: 5469
ISSN: 0036-8075
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ISSN: 0036-8075
Distribution Limits
Public
Copyright
Other
Keywords
long duration
Galileo Project
Flight Experiment
unmanned
Spacecraft
Volcanic Eruption
Jupiter
Temperature
Heat
Spectroscopy, Near-Infrared/methods
Support, U.S. Gov't, Non-P.H.S
Extraterrestrial Environment
Support, Non-U.S. Gov't
Sunlight

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