Research on Starlink Ephemeris Published by SpaceX

Q4 Physics and Astronomy
Liu Ai-rong , Xiong Yong-qing , Hui Jian-jiang , Xu Xiao-li , Gong Jun
{"title":"Research on Starlink Ephemeris Published by SpaceX","authors":"Liu Ai-rong ,&nbsp;Xiong Yong-qing ,&nbsp;Hui Jian-jiang ,&nbsp;Xu Xiao-li ,&nbsp;Gong Jun","doi":"10.1016/j.chinastron.2025.03.005","DOIUrl":null,"url":null,"abstract":"<div><div>Faced with the significant disruption of normal space activities caused by Starlink satellites, the Starlink ephemeris published by SpaceX provides an opportunity for relevant research on Starlink satellites. However, due to the lack of clear instructions, it is challenging to utilize the data further. Analysis of the ephemeris file reveals that it primarily represents the predicted orbit for the next 3 d. Research on mean orbital elements indicates that the front part of the ephemeris is an extrapolated orbit with perturbations up to at least the 20th order of Earth's gravitational field, while the latter part is a design orbit with <span><math><msub><mi>J</mi><mn>2</mn></msub></math></span> perturbation. The ephemeris includes covariance information, providing accuracy details. The covariance indicates that the accuracy of the ephemeris for satellites located in parking and working orbits is better than 2 km in the first day, while the accuracy of satellites in raising orbit increases rapidly to thousands of meters in less than half a day. Utilizing the designed orbit of the ephemeris enables a more accurate analysis of constellation configuration, especially the designated position of each satellite, thus facilitating the identification and tracking of Starlink satellites. The study provides valuable insights for the extensive application of Starlink ephemeris, serving as a beneficial reference for maneuver detection and collision warnings of Starlink satellites.</div></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"49 1","pages":"Pages 193-218"},"PeriodicalIF":0.0000,"publicationDate":"2025-01-01","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/S0275106225000050","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

Faced with the significant disruption of normal space activities caused by Starlink satellites, the Starlink ephemeris published by SpaceX provides an opportunity for relevant research on Starlink satellites. However, due to the lack of clear instructions, it is challenging to utilize the data further. Analysis of the ephemeris file reveals that it primarily represents the predicted orbit for the next 3 d. Research on mean orbital elements indicates that the front part of the ephemeris is an extrapolated orbit with perturbations up to at least the 20th order of Earth's gravitational field, while the latter part is a design orbit with J2 perturbation. The ephemeris includes covariance information, providing accuracy details. The covariance indicates that the accuracy of the ephemeris for satellites located in parking and working orbits is better than 2 km in the first day, while the accuracy of satellites in raising orbit increases rapidly to thousands of meters in less than half a day. Utilizing the designed orbit of the ephemeris enables a more accurate analysis of constellation configuration, especially the designated position of each satellite, thus facilitating the identification and tracking of Starlink satellites. The study provides valuable insights for the extensive application of Starlink ephemeris, serving as a beneficial reference for maneuver detection and collision warnings of Starlink satellites.
求助全文
约1分钟内获得全文 求助全文
来源期刊
Chinese Astronomy and Astrophysics
Chinese Astronomy and Astrophysics Physics and Astronomy-Astronomy and Astrophysics
CiteScore
0.70
自引率
0.00%
发文量
20
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信