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  • 1
    Publikationsdatum: 2011-06-09
    Beschreibung: The Cassini Ultraviolet Imaging Spectrograph (UVIS) observed an occultation of the Sun by the water vapor plume at the south polar region of Saturn's moon Enceladus. The Extreme Ultraviolet (EUV) spectrum is dominated by the spectral signature of H2O gas, with a nominal line-of-sight column density of 0.90 ± 0.23 × 1016 cm−2 (upper limit of 1.0 × 1016 cm−2). The upper limit for N2 is 5 × 1013 cm−2, or
    Print ISSN: 0094-8276
    Digitale ISSN: 1944-8007
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
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    American Association for the Advancement of Science (AAAS)
    Publikationsdatum: 1998-04-29
    Beschreibung: Interplanetary and interstellar dust grains entering Jupiter's magnetosphere form a detectable diffuse faint ring of exogenic material. This ring is composed of particles in the size range of 0. 5 to 1.5 micrometers on retrograde and prograde orbits in a 4:1 ratio, with semimajor axes 3 〈 a 〈 20 jovian radii, eccentricities 0. 1 〈 e 〈 0.3, and inclinations i less, similar 20 degrees or i greater, similar 160 degrees. The size range and the orbital characteristics are consistent with in situ detections of micrometer-sized grains by the Galileo dust detector, and the measured rates match the number densities predicted from numerical trajectory integrations.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Colwell, J E -- Horanyi, M -- Grun, E -- New York, N.Y. -- Science. 1998 Apr 3;280(5360):88-91.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309-0392, USA. colwell@casper.colorado.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9525863" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): *Cosmic Dust ; *Jupiter
    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: 1989-12-15
    Beschreibung: The Voyager photopolarimeter successfully accomplished its objectives for the Neptune encounter, performing measurements on the planet, several of its satellites, and its ring system. A photometric map of Neptune at 0.26 micrometer (microm) shows the planet to be bland, with no obvious contrast features. No polar haze was observed. At 0.75 microm, contrast features are observed, with the Great Dark Spot appearing as a low-albedo region and the bright companion as being substantially brighter than its surroundings, implying it to be at a higher altitude than the Great Dark Spot. Triton's linear phase coefficients of 0.011 magnitudes per degree at 0.26 microm and 0.013 magnitudes per degree at 0.75 microm are consistent with a solid-surface object possessing high reflectivity. Preliminary geometric albedos for Triton, Nereid, and 1989N2 were obtained at 0.26 and 0.75 microm. Triton's rotational phase curve shows evidence of two major compositional units on its surface. A single stellar occultation of the Neptune ring system elucidated an internal structure in 1989N1R, in the approximately 50-kilometer region of modest optical depth. 1989N2R may have been detected. The deficiency of material in the Neptune ring system, when compared to Uranus', may imply the lack of a "recent" moon-shattering event.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Lane, A L -- West, R A -- Hord, C W -- Nelson, R M -- Simmons, K E -- Pryor, W R -- Eposito, L W -- Horn, L J -- Wallis, B D -- Buratti, B J -- Brophy, T G -- Yanamandra-Fisher, P -- Colwell, J E -- Bliss, D A -- Mayo, M J -- Smythe, W D -- New York, N.Y. -- Science. 1989 Dec 15;246(4936):1450-4.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17755998" target="_blank"〉PubMed〈/a〉
    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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  • 4
    Publikationsdatum: 2008-11-28
    Beschreibung: A plume of water vapour escapes from fissures crossing the south polar region of the Saturnian moon Enceladus. Tidal deformation of a thin surface crust above an internal ocean could result in tensile and compressive stresses that would affect the width of the fissures; therefore, the quantity of water vapour released at different locations in Enceladus' eccentric orbit is a crucial measurement of tidal control of venting. Here we report observations of an occultation of a star by the plume on 24 October 2007 that revealed four high-density gas jets superimposed on the background plume. The gas jet positions coincide with those of dust jets reported elsewhere inside the plume. The maximum water column density in the plume is about twice the density reported earlier. The density ratio does not agree with predictions-we should have seen less water than was observed in 2005. The ratio of the jets' bulk vertical velocities to their thermal velocities is 1.5 +/- 0.2, which supports the hypothesis that the source of the plume is liquid water, with gas accelerated to supersonic velocity in nozzle-like channels.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hansen, C J -- Esposito, L W -- Stewart, A I F -- Meinke, B -- Wallis, B -- Colwell, J E -- Hendrix, A R -- Larsen, K -- Pryor, W -- Tian, F -- England -- Nature. 2008 Nov 27;456(7221):477-9. doi: 10.1038/nature07542.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory/California Institute of Technology, Pasadena, California 91109, USA. candice.j.hansen@jpl.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19037310" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Digitale ISSN: 1476-4687
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 5
    Publikationsdatum: 2004-12-18
    Beschreibung: Neutral oxygen in the saturnian system shows variability, and the total number of oxygen atoms peaks at 4 x 10(34). Saturn's aurora brightens in response to solar-wind forcing, and the auroral spectrum resembles Jupiter's. Phoebe's surface shows variable water-ice content, and the data indicate it originated in the outer solar system. Saturn's rings also show variable water abundance, with the purest ice in the outermost A ring. This radial variation is consistent with initially pure water ice bombarded by meteors, but smaller radial structures may indicate collisional transport and recent renewal events in the past 10(7) to 10(8) years.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Esposito, Larry W -- Colwell, Joshua E -- Larsen, Kristopher -- McClintock, William E -- Stewart, A Ian F -- Hallett, Janet Tew -- Shemansky, Donald E -- Ajello, Joseph M -- Hansen, Candice J -- Hendrix, Amanda R -- West, Robert A -- Keller, H Uwe -- Korth, Axel -- Pryor, Wayne R -- Reulke, Ralf -- Yung, Yuk L -- New York, N.Y. -- Science. 2005 Feb 25;307(5713):1251-5. Epub 2004 Dec 16.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉University of Colorado, Laboratory for Atmospheric and Space Physics, 234 Innovation Drive, Boulder, CO 80303-7814, USA. larry.esposito@lasp.colorado.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15604361" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): Extraterrestrial Environment ; *Hydrogen ; *Ice ; *Oxygen ; *Saturn ; Spacecraft ; Spectrum Analysis ; Ultraviolet Rays ; Water
    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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  • 6
    Publikationsdatum: 2011-04-23
    Beschreibung: Although there are substantial differences between the magnetospheres of Jupiter and Saturn, it has been suggested that cryovolcanic activity at Enceladus could lead to electrodynamic coupling between Enceladus and Saturn like that which links Jupiter with Io, Europa and Ganymede. Powerful field-aligned electron beams associated with the Io-Jupiter coupling, for example, create an auroral footprint in Jupiter's ionosphere. Auroral ultraviolet emission associated with Enceladus-Saturn coupling is anticipated to be just a few tenths of a kilorayleigh (ref. 12), about an order of magnitude dimmer than Io's footprint and below the observable threshold, consistent with its non-detection. Here we report the detection of magnetic-field-aligned ion and electron beams (offset several moon radii downstream from Enceladus) with sufficient power to stimulate detectable aurora, and the subsequent discovery of Enceladus-associated aurora in a few per cent of the scans of the moon's footprint. The footprint varies in emission magnitude more than can plausibly be explained by changes in magnetospheric parameters--and as such is probably indicative of variable plume activity.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Pryor, Wayne R -- Rymer, Abigail M -- Mitchell, Donald G -- Hill, Thomas W -- Young, David T -- Saur, Joachim -- Jones, Geraint H -- Jacobsen, Sven -- Cowley, Stan W H -- Mauk, Barry H -- Coates, Andrew J -- Gustin, Jacques -- Grodent, Denis -- Gerard, Jean-Claude -- Lamy, Laurent -- Nichols, Jonathan D -- Krimigis, Stamatios M -- Esposito, Larry W -- Dougherty, Michele K -- Jouchoux, Alain J -- Stewart, A Ian F -- McClintock, William E -- Holsclaw, Gregory M -- Ajello, Joseph M -- Colwell, Joshua E -- Hendrix, Amanda R -- Crary, Frank J -- Clarke, John T -- Zhou, Xiaoyan -- England -- Nature. 2011 Apr 21;472(7343):331-3. doi: 10.1038/nature09928.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Science Department, Central Arizona College, Coolidge, Arizona 85128, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21512570" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Digitale ISSN: 1476-4687
    Thema: Biologie , Chemie und Pharmazie , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 7
    Publikationsdatum: 2010-03-20
    Beschreibung: We review our understanding of Saturn's rings after nearly 6 years of observations by the Cassini spacecraft. Saturn's rings are composed mostly of water ice but also contain an undetermined reddish contaminant. The rings exhibit a range of structure across many spatial scales; some of this involves the interplay of the fluid nature and the self-gravity of innumerable orbiting centimeter- to meter-sized particles, and the effects of several peripheral and embedded moonlets, but much remains unexplained. A few aspects of ring structure change on time scales as short as days. It remains unclear whether the vigorous evolutionary processes to which the rings are subject imply a much younger age than that of the solar system. Processes on view at Saturn have parallels in circumstellar disks.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Cuzzi, J N -- Burns, J A -- Charnoz, S -- Clark, R N -- Colwell, J E -- Dones, L -- Esposito, L W -- Filacchione, G -- French, R G -- Hedman, M M -- Kempf, S -- Marouf, E A -- Murray, C D -- Nicholson, P D -- Porco, C C -- Schmidt, J -- Showalter, M R -- Spilker, L J -- Spitale, J N -- Srama, R -- Sremcevic, M -- Tiscareno, M S -- Weiss, J -- New York, N.Y. -- Science. 2010 Mar 19;327(5972):1470-5. doi: 10.1126/science.1179118.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Ames Research Center, NASA, Mail Stop 245-3, Moffett Field, CA 94035-1000, USA. jeffrey.cuzzi@nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20299586" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): Evolution, Planetary ; *Ice ; *Saturn ; Spacecraft ; Water
    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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  • 8
    Publikationsdatum: 2017-01-06
    Beschreibung: An occultation of ε Orionis by Enceladus’ plume was observed with Enceladus at an orbital longitude near apoapsis in order to investigate whether water vapor flow is modulated diurnally, similarly to ice particles. The occultation showed that the bulk water vapor emanating from Enceladus changes little with orbital position. The amount of gas in at least one supersonic jet increased significantly, implying that the increase in the number of particles lofted at apoapsis could be due to more gas coming from the supersonic jets, and not the overall gas flux from the tiger stripe fissures that cross Enceladus’ south polar region.
    Print ISSN: 0094-8276
    Digitale ISSN: 1944-8007
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 9
    Publikationsdatum: 2000-06-26
    Print ISSN: 0031-9007
    Digitale ISSN: 1079-7114
    Thema: Physik
    Publiziert von American Physical Society
    Standort Signatur Erwartet Verfügbarkeit
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  • 10
    Publikationsdatum: 2007-06-26
    Print ISSN: 8755-1209
    Thema: Geologie und Paläontologie
    Standort Signatur Erwartet Verfügbarkeit
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