Yi-Xing Li , Kai Tang , Fan Min , Yao-Bin Qu , Yong Huang
{"title":"Orbit Accuracy Simulation Analysis of Asteroid (469219) Kamoòalewa by Optical Observation of Tianwen-2","authors":"Yi-Xing Li , Kai Tang , Fan Min , Yao-Bin Qu , Yong Huang","doi":"10.1016/j.chinastron.2025.05.007","DOIUrl":null,"url":null,"abstract":"<div><div>China’s asteroid exploration mission, Tianwen-2, is scheduled to launch in 2025. Its first target, asteroid (469219) Kamoòalewa (also known as 2016 HO3), is a near-Earth object in co-orbit with Earth, with significant research value in terms of its motion evolution. Currently, there are limited ground observation data available for asteroid (469219) Kamoòalewa, which restricts its orbit accuracy. Tianwen-2, equipped with an optical payload, is expected to acquire a large amount of onboard optical observation data during its approach to Kamoòalewa. This will greatly improve the study situation of asteroid (469219) Kamoòalewa, which currently has only ground-based optical observation data and lacks publicly available observation data after 2021. By simulating the optical observation data of Tianwen-2 with a spacecraft orbit error of 2 km, the pre-mission evaluation of the orbit prediction accuracy of asteroid (469219) Kamoòalewa has been completed. The precision evaluation was performed using covariance analysis and numerical comparison methods. Within the possible range of observation precision considered in this study, it is estimated that the optical observation data from Tianwen-2 can improve the overall orbit accuracy of asteroid (469219) Kamoòalewa to better than 15 km. Additionally, an analysis was conducted to examine the differences and characteristics of the results obtained from the two precision evaluation methods.</div></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"49 2","pages":"Pages 376-393"},"PeriodicalIF":0.0000,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0275106225000487","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
Abstract
China’s asteroid exploration mission, Tianwen-2, is scheduled to launch in 2025. Its first target, asteroid (469219) Kamoòalewa (also known as 2016 HO3), is a near-Earth object in co-orbit with Earth, with significant research value in terms of its motion evolution. Currently, there are limited ground observation data available for asteroid (469219) Kamoòalewa, which restricts its orbit accuracy. Tianwen-2, equipped with an optical payload, is expected to acquire a large amount of onboard optical observation data during its approach to Kamoòalewa. This will greatly improve the study situation of asteroid (469219) Kamoòalewa, which currently has only ground-based optical observation data and lacks publicly available observation data after 2021. By simulating the optical observation data of Tianwen-2 with a spacecraft orbit error of 2 km, the pre-mission evaluation of the orbit prediction accuracy of asteroid (469219) Kamoòalewa has been completed. The precision evaluation was performed using covariance analysis and numerical comparison methods. Within the possible range of observation precision considered in this study, it is estimated that the optical observation data from Tianwen-2 can improve the overall orbit accuracy of asteroid (469219) Kamoòalewa to better than 15 km. Additionally, an analysis was conducted to examine the differences and characteristics of the results obtained from the two precision evaluation methods.
期刊介绍:
The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.