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The ginger-shaped asteroid 4179 Toutatis: new observations from a successful flyby of Chang'e-2.
Huang, Jiangchuan; Ji, Jianghui; Ye, Peijian; Wang, Xiaolei; Yan, Jun; Meng, Linzhi; Wang, Su; Li, Chunlai; Li, Yuan; Qiao, Dong; Zhao, Wei; Zhao, Yuhui; Zhang, Tingxin; Liu, Peng; Jiang, Yun; Rao, Wei; Li, Sheng; Huang, Changning; Ip, Wing-Huen; Hu, Shoucun; Zhu, Menghua; Yu, Liangliang; Zou, Yongliao; Tang, Xianglong; Li, Jianyang; Zhao, Haibin; Huang, Hao; Jiang, Xiaojun; Bai, Jinming.
Afiliación
  • Huang J; 1] China Academy of Space Technology, Beijing 100094, China [2] Institute of Space System Engineering, Beijing 100094, China [3].
  • Ji J; 1] Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China [2].
  • Ye P; China Academy of Space Technology, Beijing 100094, China.
  • Wang X; Beijing Institute of Control Engineering, Beijing 100190, China.
  • Yan J; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China.
  • Meng L; Institute of Space System Engineering, Beijing 100094, China.
  • Wang S; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Li C; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China.
  • Li Y; Space Science Institute, Macau University of Science and Technology, Taipa, Macau.
  • Qiao D; Beijing Institute of Technology, Beijing 100081, China.
  • Zhao W; Harbin Institute of Technology, Harbin 150001, China.
  • Zhao Y; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Zhang T; China Academy of Space Technology, Beijing 100094, China.
  • Liu P; Harbin Institute of Technology, Harbin 150001, China.
  • Jiang Y; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Rao W; Institute of Space System Engineering, Beijing 100094, China.
  • Li S; School of Electronic Engineering and Computer Science, Peking University, Beijing 100871, China.
  • Huang C; Beijing Institute of Space Mechanics and Electricity, Beijing 100076, China.
  • Ip WH; 1] Space Science Institute, Macau University of Science and Technology, Taipa, Macau [2] Institute of Astronomy, National Central University, Taoyuan, Taiwan.
  • Hu S; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Zhu M; Space Science Institute, Macau University of Science and Technology, Taipa, Macau.
  • Yu L; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Zou Y; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China.
  • Tang X; Harbin Institute of Technology, Harbin 150001, China.
  • Li J; Planetary Science Institute, AZ 85719, USA.
  • Zhao H; Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China.
  • Huang H; Institute of Space System Engineering, Beijing 100094, China.
  • Jiang X; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China.
  • Bai J; Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China.
Sci Rep ; 3: 3411, 2013 Dec 12.
Article en En | MEDLINE | ID: mdl-24336501
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.

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Sci Rep Año: 2013 Tipo del documento: Article Pais de publicación: ENGLAND / ESCOCIA / GB / GREAT BRITAIN / INGLATERRA / REINO UNIDO / SCOTLAND / UK / UNITED KINGDOM

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Sci Rep Año: 2013 Tipo del documento: Article Pais de publicación: ENGLAND / ESCOCIA / GB / GREAT BRITAIN / INGLATERRA / REINO UNIDO / SCOTLAND / UK / UNITED KINGDOM