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  • 1
    Publication Date: 1995-03-03
    Description: Hubble Space Telescope (HST) images reveal major atmospheric changes created by the collision of comet Shoemaker-Levy 9 with Jupiter. Plumes rose to 3000 kilometers with ejection velocities on the order of 10 kilometers second-1; some plumes were visible in the shadow of Jupiter before rising into sunlight. During some impacts, the incoming bolide may have been detected. Impact times were on average about 8 minutes later than predicted. Atmospheric waves were seen with a wave front speed of 454 +/- 20 meters second-1. The HST images reveal impact site evolution and record the overall change in Jupiter's appearance as a result of the bombardment.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hammel, H B -- Beebe, R F -- Ingersoll, A P -- Orton, G S -- Mills, J R -- Simon, A A -- Chodas, P -- Clarke, J T -- De Jong, E -- Dowling, T E -- New York, N.Y. -- Science. 1995 Mar 3;267(5202):1288-96.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge 02139.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/7871425" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Extraterrestrial Environment ; *Jupiter ; *Solar System
    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: 1995-03-03
    Description: The National Aeronautics and Space Administration (NASA) Infrared Telescope Facility was used to investigate the collision of comet Shoemaker-Levy 9 with Jupiter from 12 July to 7 August 1994. Strong thermal infrared emission lasting several minutes was observed after the impacts of fragments C, G, and R. All impacts warmed the stratosphere and some the troposphere up to several degrees. The abundance of stratospheric ammonia increased by more than 50 times. Impact-related particles extended up to a level where the atmospheric pressure measured several millibars. The north polar near-infrared aurora brightened by nearly a factor of 5 a week after the impacts.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Orton, G -- A'Hearn, M -- Baines, K -- Deming, D -- Dowling, T -- Goguen, J -- Griffith, C -- Hammel, H -- Hoffmann, W -- Hunten, D -- New York, N.Y. -- Science. 1995 Mar 3;267(5202):1277-82.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91109.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/7871423" target="_blank"〉PubMed〈/a〉
    Keywords: Ammonia/analysis ; Atmosphere ; Carbon Monoxide/analysis ; *Extraterrestrial Environment ; *Jupiter ; *Solar System ; Temperature ; United States ; United States National Aeronautics and Space Administration
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
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