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  • *Extraterrestrial Environment  (3)
  • Lunar and Planetary Science and Exploration
  • American Association for the Advancement of Science (AAAS)  (3)
Sammlung
Verlag/Herausgeber
  • American Association for the Advancement of Science (AAAS)  (3)
Erscheinungszeitraum
  • 1
    Publikationsdatum: 2000-05-20
    Beschreibung: 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〉
    Schlagwort(e): *Extraterrestrial Environment ; Geological Phenomena ; Geology ; Image Enhancement ; *Jupiter ; *Space Flight ; Spectrophotometry, Infrared ; *Volcanic Eruptions
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
    Publikationsdatum: 1999-08-07
    Beschreibung: 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〉
    Schlagwort(e): Atmosphere ; *Extraterrestrial Environment ; *Jupiter ; *Oxygen ; Sodium ; *Sulfur Dioxide
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
    Publikationsdatum: 1998-07-04
    Beschreibung: 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〉
    Schlagwort(e): *Extraterrestrial Environment ; Hot Temperature ; *Jupiter ; Minerals ; *Silicates ; Spectrophotometry, Infrared ; Volcanic Eruptions
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
    BibTip Andere fanden auch interessant ...
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