Spectral and spin measurement of two small and fast-rotating near-Earth asteroids

被引:8
|
作者
Polishook, D. [1 ]
Binzel, R. P. [1 ]
Lockhart, M. [1 ]
DeMeo, F. E. [1 ]
Golisch, W. [2 ]
Bus, S. J. [2 ]
Gulbis, A. A. S. [1 ,3 ,4 ]
机构
[1] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[2] Inst Astron, Hilo, HI 96720 USA
[3] S African Astron Observ, ZA-7935 Cape Town, South Africa
[4] So African Large Telescope, ZA-7935 Cape Town, South Africa
基金
美国国家航空航天局;
关键词
Asteroids; Near-Earth objects; Surfaces; Rotation; Spectroscopy; INFRARED SPECTROSCOPY; MAGNITUDE; SURFACES; ALBEDO;
D O I
10.1016/j.icarus.2012.08.013
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In May 2012 two asteroids made near-miss "grazing" passes at distances of a few Earth -radii: 2012 KP24 passed at 9 Earth-radii and 2012 KT42 at only 3 Earth-radii. The latter passed inside the orbital distance of geosynchronous satellites. From spectral and imaging measurements using NASA's 3-m Infrared Telescope facility (IRTF), we deduce taxonomic, rotational, and physical properties. Their spectral characteristics are somewhat atypical among near-Earth asteroids: C-complex for 2012 KP24 and B-type for 2012 KT42, from which we interpret the albedos of both asteroids to be between 0.10 and 0.15 and maximum effective diameters of 20 +/- 6 and 6 +/- 1 m, respectively. Among B-type asteroids, the spectrum of 2012 KT42 is most similar to 3200 Phaethon and 4015 Wilson-Harrington. Not only are these among the smallest asteroids spectrally measured, we also find they are among the fastest-spinning: 2012 KP24 completes a rotation in 2.5008 +/- 0.0006 min and 2012 KT42 rotates in 3.634 +/- 0.001 min. (C) 2012 Elsevier Inc. All rights reserved.
引用
收藏
页码:1187 / 1189
页数:3
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