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Simulated Gravity Field Estimation for the Main Belt Comet 133P/Elst-Pizarro Based on a Satellite-to-satellite Tracking Mode
Sun, Shang-Biao1; Yan, Jian-Guo1,2; Gao, Wu-Tong1; Wang, Bo1; Wang, Zhen2; Ye, Mao1; Barriot, Jean-Pierre1,3
2023-09-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume23Issue:9Pages:095012
Contribution Rank2
AbstractMost asteroids and comets are formed in the early stages of the solar system and therefore contain a wealth of information about their birth. The asteroid exploration mission planned in the coming years by China will likely target the celestial body named 133P/Elst-Pizarro (estimated diameter of about 4 km). The orbit of this asteroid stays within the asteroid belt, but nevertheless, it displays a comet-like dust tail. In this study, we used differential tracking data between two simulated probes and the data from an Earth station to estimate 133P gravity field model. This observation mode is similar to how the gravity field was estimated for large celestial objects in the GRAIL and GRACE missions, but here the object is the very small 133P asteroid. We compared the estimated gravity fields obtained for 133P from the satellite-to-satellite combined with the Earth-based two-way range-rate observation mode, with only the Earth-based two-way range rate mode. The results show that the accuracy of the low-degree (4 degree and order) estimate of the gravity field is improved by one order of magnitude by using the satellite-to-satellite combined with the Earth-based two-way range-rate observation mode with respect to the Earth-only tracking. Furthermore, another order of magnitude improvement in the gravity field solution is gained by decreasing the orbit altitude from 12 to 8 km.
Keywordgravitation methods: data analysis celestial mechanics comets: general
DOI10.1088/1674-4527/acdc89
Indexed BySCI
Language英语
WOS KeywordRADIO SCIENCE EXPERIMENT ; ROTATION PERIOD ; SPIN POLE ; MISSION ; NAVIGATION ; ORBIT ; 67P/CHURYUMOV-GERASIMENKO ; RECOVERY
Funding ProjectNational Natural Science Foundation of China[42241116] ; National Natural Science Foundation of China[U1831132] ; Macau Science and Technology Development Fund ; 2022 Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; Chinese Academy of Sciences Foundation of the young scholars of western[SKL-LPS(MUST)-2021-2023] ; French Space Agency (CNES) ; [2020-XBQNXZ-019]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001040045200001
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Funding OrganizationNational Natural Science Foundation of China ; Macau Science and Technology Development Fund ; 2022 Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; Chinese Academy of Sciences Foundation of the young scholars of western ; French Space Agency (CNES)
Citation statistics
Cited Times:5[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5350
Collection中国科学院新疆天文台
Corresponding AuthorYan, Jian-Guo
Affiliation1.Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & Re, Wuhan 430079, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Univ French Polynesia, Geodesy Observ Tahiti, BP 6570, F-98702 Tahiti, French Polynesi, France
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Sun, Shang-Biao,Yan, Jian-Guo,Gao, Wu-Tong,et al. Simulated Gravity Field Estimation for the Main Belt Comet 133P/Elst-Pizarro Based on a Satellite-to-satellite Tracking Mode[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(9):095012.
APA Sun, Shang-Biao.,Yan, Jian-Guo.,Gao, Wu-Tong.,Wang, Bo.,Wang, Zhen.,...&Barriot, Jean-Pierre.(2023).Simulated Gravity Field Estimation for the Main Belt Comet 133P/Elst-Pizarro Based on a Satellite-to-satellite Tracking Mode.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(9),095012.
MLA Sun, Shang-Biao,et al."Simulated Gravity Field Estimation for the Main Belt Comet 133P/Elst-Pizarro Based on a Satellite-to-satellite Tracking Mode".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.9(2023):095012.
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