Radar Imaging of Binary Near-Earth Asteroid (66391) 1999 KW4
Steven. J. Ostro,1*
Jean-Luc Margot,2
Lance A. M. Benner,1
Jon D. Giorgini,1
Daniel J. Scheeres,3
Eugene G. Fahnestock,3
Stephen B. Broschart,3
Julie Bellerose,3
Michael C. Nolan,4
Christopher Magri,5
Petr Pravec,6
Petr Scheirich,6
Randy Rose,1
Raymond F. Jurgens,1
Eric M. De Jong,1
Shigeru Suzuki1
High-resolution radar images reveal near-Earth asteroid (66391) 1999 KW4 to be a binary system. The
1.5-kilometer-diameter primary (Alpha) is an unconsolidated gravitational aggregate with a spin period
2.8 hours, bulk density
2 grams per cubic centimeter, porosity
50%, and an oblate shape dominated by an equatorial ridge at the object's potential-energy minimum. The
0.5-kilometer secondary (Beta) is elongated and probably is denser than Alpha. Its average orbit about Alpha is circular with a radius
2.5 kilometers and period
17.4 hours, and its average rotation is synchronous with the long axis pointed toward Alpha, but librational departures from that orientation are evident. Exotic physical and dynamical properties may be common among near-Earth binaries.
1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 911098099, USA.
2 Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 148536801, USA.
3 Department of Aerospace Engineering, University of Michigan, 1320 Beal Avenue, Ann Arbor, MI 481092140, USA.
4 Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612, USA.
5 University of Maine at Farmington, 173 High StreetPreble Hall, Farmington, ME 04938, USA.
6 Astronomical Institute, Academy of Sciences of the Czech Republic, Fri
ova 1, CZ-25165 Ond
ejov, Czech Republic.
* To whom correspondence should be addressed. E-mail: ostro{at}reason.jpl.nasa.gov