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Widespread carbon-bearing materials on near-Earth asteroid (101955) Bennu.
Simon, Amy A; Kaplan, Hannah H; Hamilton, Victoria E; Lauretta, Dante S; Campins, Humberto; Emery, Joshua P; Barucci, M Antonietta; DellaGiustina, Daniella N; Reuter, Dennis C; Sandford, Scott A; Golish, Dathon R; Lim, Lucy F; Ryan, Andrew; Rozitis, Benjamin; Bennett, Carina A.
Afiliação
  • Simon AA; Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA. amy.simon@nasa.gov.
  • Kaplan HH; Southwest Research Institute, Boulder, CO, USA.
  • Hamilton VE; Southwest Research Institute, Boulder, CO, USA.
  • Lauretta DS; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Campins H; Department of Physics, University of Central Florida, Orlando, FL, USA.
  • Emery JP; Department of Astronomy and Planetary Sciences, Northern Arizona University, Flagstaff, AZ, USA.
  • Barucci MA; Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Université Paris Sciences et Lettres, Centre National de la Recherche Scientifique, Université de Paris, Sorbonne Université, Meudon, France.
  • DellaGiustina DN; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Reuter DC; Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
  • Sandford SA; NASA Ames Research Center, Moffett Field, CA, USA.
  • Golish DR; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Lim LF; Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
  • Ryan A; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
  • Rozitis B; School of Physical Sciences, The Open University, Milton Keynes, UK.
  • Bennett CA; Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.
Science ; 370(6517)2020 11 06.
Article em En | MEDLINE | ID: mdl-33033153
ABSTRACT
Asteroid (101955) Bennu is a dark asteroid on an Earth-crossing orbit that is thought to have assembled from the fragments of an ancient collision. We use spatially resolved visible and near-infrared spectra of Bennu to investigate its surface properties and composition. In addition to a hydrated phyllosilicate band, we detect a ubiquitous 3.4-micrometer absorption feature, which we attribute to a mix of organic and carbonate materials. The shape and depth of this absorption feature vary across Bennu's surface, spanning the range seen among similar main-belt asteroids. The distribution of the absorption feature does not correlate with temperature, reflectance, spectral slope, or hydrated minerals, although some of those characteristics correlate with each other. The deepest 3.4-micrometer absorptions occur on individual boulders. The variations may be due to differences in abundance, recent exposure, or space weathering.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article