Radar Imaging of binary near-Earth asteroid (66391) 1999 KW4

被引:254
|
作者
Ostro, Steven. J.
Margot, Jean-Luc
Benner, Lance A. M.
Giorgini, Jon D.
Scheeres, Daniel J.
Fahnestock, Eugene G.
Broschart, Stephen B.
Bellerose, Julie
Nolan, Michael C.
Magri, Christopher
Pravec, Petr
Scheirich, Petr
Rose, Randy
Jurgens, Raymond F.
De Jong, Eric M.
Suzuki, Shigeru
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[3] Univ Michigan, Dept Aerosp Engn, Ann Arbor, MI 48109 USA
[4] Arecibo Observ, Arecibo, PR 00612 USA
[5] Univ Maine, Farmington, ME 04938 USA
[6] Acad Sci Czech Republ, Astron Inst, CZ-25165 Ondrejov, Czech Republic
关键词
D O I
10.1126/science.1133622
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
High-resolution radar images reveal near-Earth asteroid ( 66391) 1999 KW4 to be a binary system. The similar to 1.5-kilometer-diameter primary ( Alpha) is an unconsolidated gravitational aggregate with a spin period similar to 2.8 hours, bulk density similar to 2 grams per cubic centimeter, porosity similar to 50%, and an oblate shape dominated by an equatorial ridge at the object's potential-energy minimum. The similar to 0.5-kilometer secondary ( Beta) is elongated and probably is denser than Alpha. Its average orbit about Alpha is circular with a radius similar to 2.5 kilometers and period similar to 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.
引用
收藏
页码:1276 / 1280
页数:5
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