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DOI | 10.1126/science.aaf4279 |
Distribution of phyllosilicates on the surface of Ceres | |
Ammannito E.; Desanctis M.C.; Ciarniello M.; Frigeri A.; Carrozzo F.G.; Combe J.-Ph.; Ehlmann B.L.; Marchi S.; McSween H.Y.; Raponi A.; Toplis M.J.; Tosi F.; Castillo-Rogez J.C.; Capaccioni F.; Capria M.T.; Fonte S.; Giardino M.; Jaumann R.; Longobardo A.; Joy S.P.; Magni G.; McCord T.B.; McFadden L.A.; Palomba E.; Pieters C.M.; Polanskey C.A.; Rayman M.D.; Raymond C.A.; Schenk P.M.; Zambon F.; Russell C.T. | |
发表日期 | 2016 |
ISSN | 0036-8075 |
卷号 | 353期号:6303 |
英文摘要 | The dwarf planet Ceres is known to host phyllosilicate minerals at its surface, but their distribution and origin have not previously been determined.We used the spectrometer onboard the Dawn spacecraft to map their spatial distribution on the basis of diagnostic absorption features in the visible and near-infrared spectral range (0.25 to 5.0micrometers).We found that magnesium- and ammonium-bearing minerals are ubiquitous across the surface.Variations in the strength of the absorption features are spatially correlated and indicate considerable variability in the relative abundance of the phyllosilicates, although their composition is fairly uniform.These data, along with the distinctive spectral properties of Ceres relative to other asteroids and carbonaceous meteorites, indicate that the phyllosilicates were formed endogenously by a globally widespread and extensive alteration process. |
英文关键词 | ammonia; magnesium; mineral; silicate; absorption; ammonium; asteroid; magnesium; meteorite; near infrared; phyllosilicate; spacecraft; spatial distribution; spectrometer; visible spectrum; Article; astronomy; chemical composition; near infrared spectroscopy; photometry; priority journal; Ceres |
语种 | 英语 |
来源期刊 | Science
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/242827 |
作者单位 | Earth Planetary and Space Sciences, University of California-Los Angeles, 603 Charles Young Drive, Los Angeles, CA 90095-1567, United States; Istituto di Astrofisica e Planetologia Spaziali, Istituto Nazionale di Astrofisica, Roma, 00133, Italy; Bear Fight Institute, Winthrop, WA 98862, United States; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, United States; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, United States; Southwest Research Institute, Boulder, CO 80302, United States; Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1410, United States; Institut de Recherche en Astrophysique et Planétologie (UMR 5277), Université de Toulouse, Toulouse, F-31400, France; Institute of Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt, Berlin, 12489, Germany; NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States; Department of Earth, Environment... |
推荐引用方式 GB/T 7714 | Ammannito E.,Desanctis M.C.,Ciarniello M.,et al. Distribution of phyllosilicates on the surface of Ceres[J],2016,353(6303). |
APA | Ammannito E..,Desanctis M.C..,Ciarniello M..,Frigeri A..,Carrozzo F.G..,...&Russell C.T..(2016).Distribution of phyllosilicates on the surface of Ceres.Science,353(6303). |
MLA | Ammannito E.,et al."Distribution of phyllosilicates on the surface of Ceres".Science 353.6303(2016). |
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