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  • 1
    Publication Date: 2000-05-20
    Description: Galileo's photopolarimeter-radiometer instrument mapped Io's thermal emission during the I24, I25, and I27 flybys with a spatial resolution of 2.2 to 300 kilometers. Mapping of Loki in I24 shows uniform temperatures for most of Loki Patera and high temperatures in the southwest corner, probably resulting from an eruption that began 1 month before the observation. Most of Loki Patera was resurfaced before I27. Pele's caldera floor has a low temperature of 160 kelvin, whereas flows at Pillan and Zamama have temperatures of up to 200 kelvin. Global maps of nighttime temperatures provide a means for estimating global heat flow.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Spencer, J R -- Rathbun, J A -- Travis, L D -- Tamppari, L K -- Barnard, L -- Martin, T Z -- McEwen, A S -- New York, N.Y. -- Science. 2000 May 19;288(5469):1198-201.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10817987" target="_blank"〉PubMed〈/a〉
    Keywords: Darkness ; Extraterrestrial Environment ; Filtration ; *Hot Temperature ; *Jupiter ; Photometry ; *Space Flight ; Sunlight ; *Volcanic Eruptions
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2000-05-20
    Description: During late 1999/early 2000, the solid state imaging experiment on the Galileo spacecraft returned more than 100 high-resolution (5 to 500 meters per pixel) images of volcanically active Io. We observed an active lava lake, an active curtain of lava, active lava flows, calderas, mountains, plateaus, and plains. Several of the sulfur dioxide-rich plumes are erupting from distal flows, rather than from the source of silicate lava (caldera or fissure, often with red pyroclastic deposits). Most of the active flows in equatorial regions are being emplaced slowly beneath insulated crust, but rapidly emplaced channelized flows are also found at all latitudes. There is no evidence for high-viscosity lava, but some bright flows may consist of sulfur rather than mafic silicates. The mountains, plateaus, and calderas are strongly influenced by tectonics and gravitational collapse. Sapping channels and scarps suggest that many portions of the upper approximately 1 kilometer are rich in volatiles.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉McEwen, A S -- Belton, M J -- Breneman, H H -- Fagents, S A -- Geissler, P -- Greeley, R -- Head, J W -- Hoppa, G -- Jaeger, W L -- Johnson, T V -- Keszthelyi, L -- Klaasen, K P -- Lopes-Gautier, R -- Magee, K P -- Milazzo, M P -- Moore, J M -- Pappalardo, R T -- Phillips, C B -- Radebaugh, J -- Schubert, G -- Schuster, P -- Simonelli, D P -- Sullivan, R -- Thomas, P C -- Turtle, E P -- Williams, D A -- New York, N.Y. -- Science. 2000 May 19;288(5469):1193-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10817986" target="_blank"〉PubMed〈/a〉
    Keywords: *Extraterrestrial Environment ; Geological Phenomena ; Geology ; Image Enhancement ; *Jupiter ; *Space Flight ; Spectrophotometry, Infrared ; *Volcanic Eruptions
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 3
    Publication Date: 1999-08-07
    Description: The Galileo spacecraft has detected diffuse optical emissions from Io in high-resolution images acquired while the satellite was eclipsed by Jupiter. Three distinct components make up Io's visible emissions. Bright blue glows of more than 300 kilorayleighs emanate from volcanic plumes, probably due to electron impact on molecular sulfur dioxide. Weaker red emissions, possibly due to atomic oxygen, are seen along the limbs, brighter on the pole closest to the plasma torus. A faint green glow appears concentrated on the night side of Io, possibly produced by atomic sodium. Io's disk-averaged emission diminishes with time after entering eclipse, whereas the localized blue glows brighten instead.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Geissler, P E -- McEwen, A S -- Ip, W -- Belton, M J -- Johnson, T V -- Smyth, W H -- Ingersoll, A P -- New York, N.Y. -- Science. 1999 Aug 6;285(5429):870-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85711, USA. geissler@lpl.arizona.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10436151" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Extraterrestrial Environment ; *Jupiter ; *Oxygen ; Sodium ; *Sulfur Dioxide
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 2000-05-20
    Description: Infrared 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.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Lopes-Gautier, R -- 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 -- New York, N.Y. -- Science. 2000 May 19;288(5469):1201-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10817988" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Hot Temperature ; *Jupiter ; *Spacecraft ; Spectroscopy, Near-Infrared/methods ; Sunlight ; Temperature ; *Volcanic Eruptions
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 5
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2000-05-20
    Description: Unlike any volcanic behavior ever observed on Earth, the plume from Prometheus on Io has wandered 75 to 95 kilometers west over the last 20 years since it was first discovered by Voyager and more recently observed by Galileo. Despite the source motion, the geometric and optical properties of the plume have remained constant. We propose that this can be explained by vaporization of a sulfur dioxide and/or sulfur "snowfield" over which a lava flow is moving. Eruption of a boundary-layer slurry through a rootless conduit with sonic conditions at the intake of the melted snow can account for the constancy of plume properties.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kieffer, S W -- Lopes-Gautier, R -- McEwen, A -- Smythe, W -- Keszthelyi, L -- Carlson, R -- New York, N.Y. -- Science. 2000 May 19;288(5469):1204-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉S. W. Kieffer Science Consulting, Inc., 6 Queen Street, Suite 206, Post Office Box 520, Bolton, ON L7E 5T4, Canada. skieffer@geyser.com〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10817989" target="_blank"〉PubMed〈/a〉
    Keywords: Cold Temperature ; Entropy ; Extraterrestrial Environment ; Hot Temperature ; Ice ; *Jupiter ; Models, Chemical ; Snow ; Spacecraft ; *Volcanic Eruptions
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 6
    Publication Date: 1998-07-04
    Description: Infrared wavelength observations of Io by the Galileo spacecraft show that at least 12 different vents are erupting lavas that are probably hotter than the highest temperature basaltic eruptions on Earth today. In at least one case, the eruption near Pillan Patera, two independent instruments on Galileo show that the lava temperature must have exceeded 1700 kelvin and may have reached 2000 kelvin. The most likely explanation is that these lavas are ultramafic (magnesium-rich) silicates, and this idea is supported by the tentative identification of magnesium-rich orthopyroxene in lava flows associated with these high-temperature hot spots.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉McEwen, A S -- Keszthelyi, L -- Spencer, J R -- Schubert, G -- Matson, D L -- Lopes-Gautier, R -- Klaasen, K P -- Johnson, T V -- Head, J W -- Geissler, P -- Fagents, S -- Davies, A G -- Carr, M H -- Breneman, H H -- Belton, M J -- New York, N.Y. -- Science. 1998 Jul 3;281(5373):87-90.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lunar and Planetary Lab, University of Arizona, Tucson, AZ 85711, USA. mcewen@lpl.arizona.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9651251" target="_blank"〉PubMed〈/a〉
    Keywords: *Extraterrestrial Environment ; Hot Temperature ; *Jupiter ; Minerals ; *Silicates ; Spectrophotometry, Infrared ; Volcanic Eruptions
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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