中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Surface Thermal Inertia of Near-Earth Asteroid (469219) Kamo`oalewa: Statistical Estimation and Implications

文献类型:期刊论文

作者Liu, Lu5; Chen, Qiao5; Yan, Jianguo2,4; Yu, Liangliang1; Fenucci, Marco6; Ye, Mao4; Zhong, Zhen3; Qiu, Denggao4; Barriot, Jean-Pierre4,7
刊名SOLAR SYSTEM RESEARCH
出版日期2024-08-01
卷号58期号:4页码:469-479
关键词Thermal inertia Kamo`oalewa Yarkovsky effect Chinese Small Body Exploration Mission
ISSN号0038-0946
DOI10.1134/S0038094624700321
产权排序3
英文摘要The Chinese small body exploration mission Tianwen-2 is aimed at sampling the near-Earth, fast-rotating asteroid (469219) Kamo`oalewa and returning the samples to Earth. Characterisation of the currently unknown physical properties of Kamo`oalewa in the pre-mission phase would support mission implementation. In this study, we preliminarily estimate the surface thermal inertia of Kamo`oalewa using a statistical method, based on the Yarkovsky-related orbital drift of (-6.155 +/- 1.758) x 10(-3) au/Myr for Kamo`oalewa obtained in our previous work. A reasonable estimate of the surface thermal inertia obtained is 402.05(- 194.37)(+ 376.29)J K-1 m(-2) s(-1/2). This low value suggests the presence of coarse regolith on the surface of Kamo`oalewa or its nature as a porous rock. The regolith potentially present on the surface of Kamo`oalewa may have millimetre- to decimetre-sized grains with cohesive strengths varying from similar to 0.76 to similar to 0.045 Pa. If Kamo'oalewa is a porous rock, its porosity is expected to range from similar to 20 to 50%, corresponding to tensile strengths of similar to 1.3 to 11.5 MPa. This study provides preliminary insights into the surface thermal inertia of Kamo`oalewa from a statistical viewpoint, which may facilitate the Tianwen-2 mission.
WOS关键词THERMOPHYSICAL PROPERTIES ; GRAIN-SIZE ; YARKOVSKY ; MAGNITUDE ; STRENGTH ; DENSITY ; ORBIT
资助项目National Natural Science Foundation of China[42241116] ; National Natural Science Foundation of China[42030110] ; National Key Research and Development Program of China[2022YFF0503202] ; The 2022 Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; Macau University of Science and Technology[SKL-LPS(MUST)-2021-2023] ; Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan University[21-01-01] ; French Space Agency (CNES)
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001270369800007
出版者PLEIADES PUBLISHING INC
资助机构National Natural Science Foundation of China ; National Key Research and Development Program of China ; The 2022 Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; Macau University of Science and Technology ; Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan University ; French Space Agency (CNES)
源URL[http://ir.xao.ac.cn/handle/45760611-7/6858]  
专题研究单元未命名
通讯作者Yan, Jianguo
作者单位1.Macau Univ Sci & Technol, State Key Lab Lunar & Planetary Sci, Macau, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550025, Peoples R China
4.Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & Re, Wuhan 430070, Peoples R China
5.Chongqing Satellite Network Syst Co Ltd, Chongqing 401135, Peoples R China
6.ESA NEO Coordinat Ctr, Largo Galileo Galilei 1, I-00044 Frascati, RM, Italy
7.Univ French Polynesia, Geodesy Observ Tahiti, BP 6570, F-98702 Faaa Tahiti, France
推荐引用方式
GB/T 7714
Liu, Lu,Chen, Qiao,Yan, Jianguo,et al. Surface Thermal Inertia of Near-Earth Asteroid (469219) Kamo`oalewa: Statistical Estimation and Implications[J]. SOLAR SYSTEM RESEARCH,2024,58(4):469-479.
APA Liu, Lu.,Chen, Qiao.,Yan, Jianguo.,Yu, Liangliang.,Fenucci, Marco.,...&Barriot, Jean-Pierre.(2024).Surface Thermal Inertia of Near-Earth Asteroid (469219) Kamo`oalewa: Statistical Estimation and Implications.SOLAR SYSTEM RESEARCH,58(4),469-479.
MLA Liu, Lu,et al."Surface Thermal Inertia of Near-Earth Asteroid (469219) Kamo`oalewa: Statistical Estimation and Implications".SOLAR SYSTEM RESEARCH 58.4(2024):469-479.

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