Goldstone Radar Observations of Horseshoe-orbiting Near-Earth Asteroid 2013 BS45, a Potential Mission Target

被引:0
作者
Brozovic, Marina [1 ]
Benner, Lance A. M. [1 ]
Giorgini, Jon D. [1 ]
Naidu, Shantanu P. [1 ]
Busch, Michael W. [2 ]
Lawrence, Kenneth J. [1 ]
Jao, Joseph S. [1 ]
Lee, Clement G. [1 ]
Snedeker, Lawrence G. [3 ]
Silva, Marc A. [3 ]
Slade, Martin A. [1 ]
Chodas, Paul W. [1 ]
机构
[1] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[2] SETI Inst, 189 North Bernardo Ave,Suite 200, Mountain View, CA 94043 USA
[3] SAITECH, Goldstone Deep Space Commun Complex, Ft Irwin, CA 92310 USA
基金
美国国家航空航天局;
关键词
minor planets; asteroids:; individual; (2013; B545); techniques: radar astronomy; SURFACE; COMPANION; REVISION; REGOLITH; BOULDERS; TOUTATIS; SHAPE; SIZE;
D O I
10.3847/1538-3881/aaf04f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report radar observations of near-Earth asteroid 2013 B545 obtained during the 2013 apparition. This object is in a resonant, Earth-like orbit, and it is a backup target for NASA's NEA Scout mission. 2013 B545 belongs to the Arjuna orbital domain, which currently has similar to 20 discovered representatives. These objects tend to be small and difficult to characterize, and 2013 B545 is only the third Aijuna object observed with radar to date. We observed 2013 B545 on three days at Goldstone (8560 MHz, 3.5 cm) between 2013 February 10 and 13. The closest approach occurred on February 12 at a distance of 0.0126 au. We obtained relatively weak echo power spectra and ranging data at resolutions up to 0.125 mu s (18.75 m px(-1)). The Doppler broadening of the echo power spectra strongly suggests an upper bound on the rotation period of 1.9 minutes. The radar data, in combination with an assumption that the asteroid's radar albedo is no higher than that of metallic NEA 1986 DA, constrain the equivalent diameter to 15 m <= D <= 38 m. The circular polarization ratio is 0.21 +/- 0.06, which implies a near-surface that is relatively smooth on decimeter spatial scales. We bounded the OC radar albedo to eta(OC) >= 0.09 and the optical albedo remains relatively unconstrained at 0.05 <= pv <= 0.35. The Yarkovsky acceleration has not been detected but, due to the object's rapid rotation, would be dominated by a seasonal component whose direction and magnitude depends on the currently unknown pole orientation and thermal inertia.
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页数:7
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