Research ArticlePLANETARY SCIENCE

Hypervelocity impacts as a source of deceiving surface signatures on iron-rich asteroids

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Science Advances  28 Aug 2019:
Vol. 5, no. 8, eaav3971
DOI: 10.1126/sciadv.aav3971

Article Information

vol. 5 no. 8

Online ISSN: 
History: 
  • Received for publication September 12, 2018
  • Accepted for publication July 19, 2019
  • .

Author Information

  1. Guy Libourel1,2,*,
  2. Akiko M. Nakamura3,
  3. Pierre Beck4,
  4. Sandra Potin4,
  5. Clément Ganino5,
  6. Suzanne Jacomet6,
  7. Ryo Ogawa3,
  8. Sunao Hasegawa7 and
  9. Patrick Michel1
  1. 1Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Boulevard de l’Observatoire, CS 34229, 06304 Nice Cedex 4, France.
  2. 2Hawai‘i Institute of Geophysics and Planetology, School of Ocean, Earth Science and Technology, University of Hawai‘i at Mānoa, Honolulu, HI 96821, USA.
  3. 3Graduate School of Science, Kobe University, 1-1 Rokkoudai-cho, Nada-ku, Kobe 657-8501, Japan.
  4. 4UJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble F-38041, France.
  5. 5Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Géoazur, 250 rue Albert Einstein, Sophia-Antipolis, 06560 Valbonne, France.
  6. 6MINES Paristech, PSL-Research University, CEMEF-Centre de Mise en Forme des Matériaux/Centre for Material Forming, CNRS UMR 7635, CS 10207, 1 rue Claude Daunesse, 06904 Sophia-Antipolis Cedex, France.
  7. 7Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara 252-5210, Japan.
  1. *Corresponding author. Email: libou{at}oca.eu

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Aug 20193739135
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Oct 20192518259
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Dec 2019615228
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Mar 202097815
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