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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/28610
Title: The geomorphology of Ceres
Authors: Buczkowski, D. L.
Schmidt, B. E.
Williams, D. A.
Mest, S. C.
Scully, J. E. C.
Ermakov, A. I.
Preusker, F.
Schenk, P.
Otto, K. A.
Hiesinger, H.
O'Brien, D.
Marchi, S.
Sizemore, H.
Hughson, K.
Chilton, H.
Bland, M.
Byrne, S.
Schorghofer, N.
Platz, T.
Jaumann, R.
Roatsch, T.
Sykes, M. V.
Nathues, A.
DE SANCTIS, MARIA CRISTINA 
Raymond, C. A.
Russell, C. T.
Issue Date: 2016
Journal: SCIENCE 
Number: 353
Issue: 6303
First Page: aaf4332
Abstract: Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomorphology of features on the surface of Ceres. The dwarf planet is dominated by numerous craters, but other features are also common. Linear structures include both those associated with impact craters and those that do not appear to have any correlation to an impact event. Abundant lobate flows are identified, and numerous domical features are found at a range of scales. Features suggestive of near-surface ice, cryomagmatism, and cryovolcanism have been identified. Although spectroscopic analysis has currently detected surface water ice at only one location on Ceres, the identification of these potentially ice-related features suggests that there may be at least some ice in localized regions in the crust.
URI: http://hdl.handle.net/20.500.12386/28610
URL: https://science.sciencemag.org/content/353/6303/aaf4332
ISSN: 0036-8075
DOI: 10.1126/science.aaf4332
Bibcode ADS: 2016Sci...353.4332B
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

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