Radar observations and the shape of near-Earth ASTEROID 2008 EV5

Michael W. Busch, Steven J. Ostro, Lance A.M. Benner, Marina Brozovic, Jon D. Giorgini, Joseph S. Jao, Daniel J. Scheeres, Christopher Magri, Michael C. Nolan, Ellen S. Howell, Patrick A. Taylor, Jean Luc Margot, Walter Brisken

Research output: Contribution to journalArticlepeer-review

78 Scopus citations


We observed the near-Earth ASTEROID 2008 EV5 with the Arecibo and Goldstone planetary radars and the Very Long Baseline Array during December 2008. EV5 rotates retrograde and its overall shape is a 400 ± 50 m oblate spheroid. The most prominent surface feature is a ridge parallel to the asteroid's equator that is broken by a concavity about 150. m in diameter. Otherwise the asteroid's surface is notably smooth on decameter scales. EV5's radar and optical albedos are consistent with either rocky or stony-iron composition. The equatorial ridge is similar to structure seen on the rubble-pile near-Earth asteroid (66391) 1999 KW4 and is consistent with YORP spin-up reconfiguring the asteroid in the past. We interpret the concavity as an impact crater. Shaking during the impact and later regolith redistribution may have erased smaller features, explaining the general lack of decameter-scale surface structure.

Original languageEnglish (US)
Pages (from-to)649-660
Number of pages12
Issue number2
StatePublished - Apr 2011
Externally publishedYes


  • Asteroids
  • Asteroids, Dynamics
  • Asteroids, Surfaces
  • Radar observations

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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