Radar detection of asteroid 2002 AA29

被引:9
作者
Ostro, SJ [1 ]
Giorgini, JD
Benner, LAM
Hine, AA
Nolan, MC
Margot, JL
Chodas, PW
Veillet, C
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Arecibo Observ, Natl Astron & Ionosphere Ctr, Arecibo, PR 00612 USA
[3] CALTECH, Pasadena, CA 91125 USA
[4] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
关键词
asteroids; radar; photometry;
D O I
10.1016/j.icarus.2003.09.001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Radar echoes from Earth co-orbital Asteroid 2002 AA29 yield a total-power radar cross section of 2.9 x 10(-5) km(2) +/-25%, a circular polarization ratio of SC/OC = 0.26 +/- 0.07, and an echo bandwidth of at least 1.5 Hz. Combining these results with the estimate of its visual absolute magnitude, H-V = 25.23 +/- 0.24, from reported Spacewatch photometry indicates an effective diameter of 25 +/- 5 m, a rotation period no longer than 33 min, and an average surface bulk density no larger than 2.0 g cm(-3); the asteroid is radar dark and optically bright, and its statistically most likely spectral class is S. The Hv estimate from LINEAR photometry (23.58 +/- 0.38) is not compatible with either Spacewatch's H-V or our radar results. If a bias this large were generally present in LINEAR's estimates of Hv for asteroids it has discovered or observed, then estimates of the current completeness of the Spaceguard Survey would have to be revised downward. (C) 2003 Elsevier Inc. All rights reserved.
引用
收藏
页码:271 / 275
页数:5
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