Physical characteristics of Hayabusa target Asteroid 25143 Itokawa

被引:32
作者
Lederer, SM
Domingue, DL
Vilas, F
Abe, M
Farnham, TL
Jarvis, KS
Lowry, SC
Ohba, Y
Weissman, PR
French, LM
Fukai, H
Hasegawa, S
Ishiguro, M
Larson, SM
Takagi, Y
机构
[1] NASA, Lyndon B Johnson Space Ctr, Planetary Astron Grp, Houston, TX 77058 USA
[2] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[3] Inst Space & Astronaut Sci, Japanese Aerosp Explorat Agcy, Sagamihara, Kanagawa 2298510, Japan
[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[5] Lockheed Martin Space Operat, Houston, TX 77058 USA
[6] CALTECH, Jet Prop Lab, Div Earth & Space Sci, Pasadena, CA 91109 USA
[7] Illinois Wesleyan Univ, Dept Phys, Bloomington, IL 61701 USA
[8] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[9] Tohoku Gakuin Univ, Meito Ku, Nagoya, Aichi 4658515, Japan
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
surfaces; asteroids; photometry; regoliths; composition;
D O I
10.1016/j.icarus.2004.07.022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In March 2001, the Hayabusa spacecraft target, Asteroid 25143 Itokawa, made its final close approach to Earth prior to the spacecraft's launch. We carried out an extensive observing campaign from January to September 2001 to better characterize this near-Earth asteroid. Global physical properties of the surface of Itokawa were characterized by analyzing its photometric properties and behavior. Results included here capitalize on analysis of broadband photometric observations taken with a number of telescopes, instruments, and observers. We employed a Hapke model to estimate the surface roughness, single particle scattering albedo, single particle scattering characteristics, phase integral, and geometric and bond albedo. We find that this asteroid has a higher geometric albedo than average main belt S-class asteroids; this is consistent with results from other observers. The broadband colors of Itokawa further support evidence that this is an atypical S-class asteroid. Broadband colors show spectral characteristics more typically found on large-diameter main-belt asteroids believed to be space-weathered, suggesting the surface of this small diameter, near-Earth asteroid could likewise be space-weathered. (C) 2004 Elsevier Inc. All rights reserved.
引用
收藏
页码:153 / 165
页数:13
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