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  • 1
    Publication Date: 1999-03-26
    Description: Spatially resolved infrared and ultraviolet wavelength spectra of Europa's leading, anti-jovian quadrant observed from the Galileo spacecraft show absorption features resulting from hydrogen peroxide. Comparisons with laboratory measurements indicate surface hydrogen peroxide concentrations of about 0.13 percent, by number, relative to water ice. The inferred abundance is consistent with radiolytic production of hydrogen peroxide by intense energetic particle bombardment and demonstrates that Europa's surface chemistry is dominated by radiolysis.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Carlson, R W -- Anderson, M S -- Johnson, R E -- Smythe, W D -- Hendrix, A R -- Barth, C A -- Soderblom, L A -- Hansen, G B -- McCord, T B -- Dalton, J B -- Clark, R N -- Shirley, J H -- Ocampo, A C -- Matson, D L -- New York, N.Y. -- Science. 1999 Mar 26;283(5410):2062-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. rcarlson@lively.jpl.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10092224" target="_blank"〉PubMed〈/a〉
    Keywords: *Extraterrestrial Environment ; Hydrogen Peroxide/*analysis/chemistry ; Ice ; *Jupiter ; Spectrophotometry, Infrared ; Spectrophotometry, Ultraviolet ; Water/chemistry
    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: 1998-06-20
    Description: Reflectance spectra in the 1- to 2.5-micrometer wavelength region of the surface of Europa obtained by Galileo's Near Infrared Mapping Spectrometer exhibit distorted water absorption bands that indicate the presence of hydrated minerals. The laboratory spectra of hydrated salt minerals such as magnesium sulfates and sodium carbonates and mixtures of these minerals provide a close match to the Europa spectra. The distorted bands are only observed in the optically darker areas of Europa, including the lineaments, and may represent evaporite deposits formed by water, rich in dissolved salts, reaching the surface from a water-rich layer underlying an ice crust.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉McCord, T B -- Hansen, G B -- Fanale, F P -- Carlson, R W -- Matson, D L -- Johnson, T V -- Smythe, W D -- Crowley, J K -- Martin, P D -- Ocampo, A -- Hibbitts, C A -- Granahan, J C -- New York, N.Y. -- Science. 1998 May 22;280(5367):1242-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9596573" target="_blank"〉PubMed〈/a〉
    Keywords: Carbonates ; Evolution, Planetary ; Ice ; *Jupiter ; Magnesium Sulfate ; Oceans and Seas ; *Salts ; Spectrophotometry, Infrared ; Temperature ; *Water
    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: 1997-10-10
    Description: Five absorption features are reported at wavelengths of 3.4, 3.88, 4. 05, 4.25, and 4.57 micrometers in the surface materials of the Galilean satellites Callisto and Ganymede from analysis of reflectance spectra returned by the Galileo mission near-infrared mapping spectrometer. Candidate materials include CO2, organic materials (such as tholins containing C(triple bond)N and C-H), SO2, and compounds containing an SH-functional group; CO2, SO2, and perhaps cyanogen [(CN)2] may be present within the surface material itself as collections of a few molecules each. The spectra indicate that the primary surface constituents are water ice and hydrated minerals.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉McCord, T B -- Carlson, R W -- Smythe, W D -- Hansen, G B -- Clark, R N -- Hibbitts, C A -- Fanale, F P -- Granahan, J C -- Segura, M -- Matson, D L -- Johnson, T V -- Martin, P D -- New York, N.Y. -- Science. 1997 Oct 10;278(5336):271-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, USA. tom@kahana.pgd.hawaii.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9323203" target="_blank"〉PubMed〈/a〉
    Keywords: Carbon Dioxide/*analysis ; Hydrocarbons/analysis ; Ice ; *Jupiter ; Nitriles/*analysis ; Spectrum Analysis ; Sulfur/*analysis ; Sulfur Dioxide/analysis ; Water
    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: 1996-10-18
    Description: The Near Infrared Mapping Spectrometer performed spectral studies of Jupiter and the Galilean satellites during the June 1996 perijove pass of the Galileo spacecraft. Spectra for a 5-micrometer hot spot on Jupiter are consistent with the absence of a significant water cloud above 8 bars and with a depletion of water compared to that predicted for solar composition, corroborating results from the Galileo probe. Great Red Spot (GRS) spectral images show that parts of this feature extend upward to 240 millibars, although considerable altitude-dependent structure is found within it. A ring of dense clouds surrounds the GRS and is lower than it by 3 to 7 kilometers. Spectra of Callisto and Ganymede reveal a feature at 4. 25 micrometers, attributed to the presence of hydrated minerals or possibly carbon dioxide on their surfaces. Spectra of Europa's high latitudes imply that fine-grained water frost overlies larger grains. Several active volcanic regions were found on Io, with temperatures of 420 to 620 kelvin and projected areas of 5 to 70 square kilometers.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Carlson, R -- Smythe, W -- Baines, K -- Barbinis, E -- Becker, K -- Burns, R -- Calcutt, S -- Calvin, W -- Clark, R -- Danielson, G -- Davies, A -- Drossart, P -- Encrenaz, T -- Fanale, F -- Granahan, J -- Hansen, G -- Herrera, P -- Hibbitts, C -- Hui, J -- Irwin, P -- Johnson, T -- Kamp, L -- Kieffer, H -- Leader, F -- Weissman, P -- New York, N.Y. -- Science. 1996 Oct 18;274(5286):385-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91109, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/8832878" target="_blank"〉PubMed〈/a〉
    Keywords: Ammonia/analysis ; Carbon Dioxide/analysis ; Extraterrestrial Environment ; Hydroxides/analysis ; *Jupiter ; Methane/analysis ; Phosphines/analysis ; Spectroscopy, Near-Infrared ; Water/analysis
    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
    Publication Date: 1996-10-04
    Description: Patients with human severe combined immunodeficiency (SCID) can be divided into those with B lymphocytes (B+ SCID) and those without (B- SCID). Although several genetic causes are known for B+ SCID, the etiology of B- SCID has not been defined. Six of 14 B- SCID patients tested were found to carry a mutation of the recombinase activating gene 1 (RAG-1), RAG-2, or both. This mutation resulted in a functional inability to form antigen receptors through genetic recombination and links a defect in one of the site-specific recombination systems to a human disease.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Schwarz, K -- Gauss, G H -- Ludwig, L -- Pannicke, U -- Li, Z -- Lindner, D -- Friedrich, W -- Seger, R A -- Hansen-Hagge, T E -- Desiderio, S -- Lieber, M R -- Bartram, C R -- New York, N.Y. -- Science. 1996 Oct 4;274(5284):97-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Section of Molecular Biology, University of Ulm, D-89070 Ulm, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/8810255" target="_blank"〉PubMed〈/a〉
    Keywords: B-Lymphocytes/immunology ; Cell Line ; Consanguinity ; *DNA-Binding Proteins ; Female ; Genes, Immunoglobulin ; Genes, Recessive ; *Homeodomain Proteins ; Humans ; Immunophenotyping ; Male ; Mutation ; Nuclear Proteins ; Polymorphism, Single-Stranded Conformational ; Proteins/*genetics ; Receptors, Antigen, T-Cell/genetics ; Recombination, Genetic ; Sequence Deletion ; Severe Combined Immunodeficiency/*genetics/immunology ; Transfection
    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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