The Ginger-shaped Asteroid 4179 Toutatis: New Observations from a Successful Flyby of Chang’e-2

Jiangchuan Huang(China Academy of Space Technology), Jianghui Ji(Purple Mountain Observatory), Peijian Ye(China Academy of Space Technology), Xiaolei Wang, Jun Yan(Chinese Academy of Sciences), Linzhi Meng, Su Wang(Purple Mountain Observatory), Chunlai Li(Chinese Academy of Sciences), Yuan Li(Macau University of Science and Technology), Dong Qiao(Beijing Institute of Technology), Wei Zhao(Harbin Institute of Technology), Yuhui Zhao(Purple Mountain Observatory), Tingxin Zhang(China Academy of Space Technology), Peng Liu(Harbin Institute of Technology), Yun Jiang(Purple Mountain Observatory), Wei Rao, Sheng Li(Peking University), Changning Huang, Wing‐Huen Ip(Macau University of Science and Technology), Shoucun Hu(Purple Mountain Observatory), Meng‐Hua Zhu(Macau University of Science and Technology), Liangliang Yu(Purple Mountain Observatory), Yongliao Zou(Chinese Academy of Sciences), Xianglong Tang(Harbin Institute of Technology), Jian‐Yang Li(Planetary Science Institute), Haibin Zhao(Purple Mountain Observatory), Hao Huang, Xiaojun Jiang(Chinese Academy of Sciences), Jinming Bai(Yunnan Observatories)
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August 15, 2016
Cited by 75

Abstract

On 13 December 2012, Chang'e-2 conducted a successful flyby of the near-Earth asteroid 4179 Toutatis at a closest distance of 770 ± 120 meters from the asteroid's surface. The highest-resolution image, with a resolution of better than 3 meters, reveals new discoveries on the asteroid, e.g., a giant basin at the big end, a sharply perpendicular silhouette near the neck region, and direct evidence of boulders and regolith, which suggests that Toutatis may bear a rubble-pile structure. Toutatis' maximum physical length and width are (4.75 × 1.95 km) ±10%, respectively, and the direction of the +z axis is estimated to be (250 ± 5°, 63 ± 5°) with respect to the J2000 ecliptic coordinate system. The bifurcated configuration is indicative of a contact binary origin for Toutatis, which is composed of two lobes (head and body). Chang'e-2 observations have significantly improved our understanding of the characteristics, formation, and evolution of asteroids in general.


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