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Distribution of phyllosilicates on the surface of Ceres

Ammannito, E. and Ehlmann, Bethany L. (2016) Distribution of phyllosilicates on the surface of Ceres. Science, 353 (6303). p. 1006. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20160528-213740751

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Abstract

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 5.0 micrometers). 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.aaf4279DOIArticle
http://sbn.psi.edu/pds/resource/dwncvir.htmlRelated ItemVIR spectral data
ORCID:
AuthorORCID
Ehlmann, Bethany L.0000-0002-2745-3240
Additional Information:© 2016 American Association for the Advancement of Science. 5 February 2016; accepted 29 July 2016. We thank the Italian Space Agency (ASI), NASA, and the Deutsches Zentrum für Luft- und Raumfahrt for supporting this work. The VIR instrument was funded and coordinated by the ASI and built by Selex ES, with the scientific leadership of the Institute for Space Astrophysics and Planetology, Italian National Institute for Astrophysics, Italy, and it is operated by the Institute for Space Astrophysics and Planetology, Rome, Italy. A portion of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, USA, under contract to NASA. Dawn data are archived in NASA's Planetary Data System; VIR spectral data may be obtained at http://sbn.psi.edu/pds/resource/dwncvir.html.
Funders:
Funding AgencyGrant Number
Agenzia Spaziale Italiana (ASI)UNSPECIFIED
NASAUNSPECIFIED
Deutsches Zentrum für Luft- und Raumfahrt (DLR)UNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Issue or Number:6303
Record Number:CaltechAUTHORS:20160528-213740751
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160528-213740751
Official Citation:Distribution of phyllosilicates on the surface of Ceres BY E. AMMANNITO, M. C. DESANCTIS, M. CIARNIELLO, A. FRIGERI, F. G. CARROZZO, J.-PH. COMBE, B. L. EHLMANN, S. MARCHI, H. Y. MCSWEEN, A. RAPONI, M. J. TOPLIS, F. TOSI, J. C. CASTILLO-ROGEZ, F. CAPACCIONI, M. T. CAPRIA, S. FONTE, M. GIARDINO, R. JAUMANN, A. LONGOBARDO, S. P. JOY, G. MAGNI, T. B. MCCORD, L. A. MCFADDEN, E. PALOMBA, C. M. PIETERS, C. A. POLANSKEY, M. D. RAYMAN, C. A. RAYMOND, P. M. SCHENK, F. ZAMBON, C. T. RUSSELL Science 02 Sep 2016: Vol. 353, Issue 6303, pp. 1006 DOI: 10.1126/science.aaf4279
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:67465
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:01 Sep 2016 19:54
Last Modified:06 Nov 2020 17:05

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