{"title":"Precise Orbit Determination for Cislunar Space Targets Based on Ground/Space/Lunar Based Integrated Optical Observation Model","authors":"Zhenqi Wang, Zhongmiao Sun, Bin Guan, Jianguo Yan, Shangbiao Sun, Wanling Yang, Jean-Pierre Barriot","doi":"10.1134/S0038094625600313","DOIUrl":null,"url":null,"abstract":"<p>Cislunar space, as a strategically significant domain for humanity’s future survival and development, has become a new battleground for deep space exploration activities among leading spacefaring nations. Driven by the growing demands for deep space exploration missions, the monitoring and early warning of cislunar space debris have increasingly become a priority. Precise orbit determination (POD) of cislunar space targets provides essential support for debris surveillance. Against this backdrop, this study proposes a ground/space/lunar integrated optical observation model, implemented through SPOT (Small Body and Planets Precise Orbit Determination Toolkit)—a software platform independently developed by Wuhan University’s Planetary Geodesy Team. We conducted numerical simulations for POD of targets at Earth–Moon libration points L1, L4, and L5. The results demonstrate that the orbit determination accuracy using only ground-based observations is on the order of several hundred meters. Space-based observations can serve as a valuable supplement to ground-based data, providing a modest improvement in accuracy. However, the addition of lunar-based observations significantly enhances the orbit determination accuracy, reducing position errors and uncertainties to the order of tens of meters. Furthermore, variations in the noise level of lunar-based observations have a stronger impact on orbit determination accuracy than space-based observations. Finally, comparative experiments verify the necessity of solving the solar radiation pressure coefficient Cr for improving orbit determination accuracy. These findings highlight the tremendous potential of lunar-based optical observations in achieving high-precision orbit determination for cislunar space targets and provide valuable insights for future advancements in deep-space situational awareness and autonomous navigation.</p>","PeriodicalId":778,"journal":{"name":"Solar System Research","volume":"59 7","pages":""},"PeriodicalIF":0.8000,"publicationDate":"2025-08-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar System Research","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0038094625600313","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Cislunar space, as a strategically significant domain for humanity’s future survival and development, has become a new battleground for deep space exploration activities among leading spacefaring nations. Driven by the growing demands for deep space exploration missions, the monitoring and early warning of cislunar space debris have increasingly become a priority. Precise orbit determination (POD) of cislunar space targets provides essential support for debris surveillance. Against this backdrop, this study proposes a ground/space/lunar integrated optical observation model, implemented through SPOT (Small Body and Planets Precise Orbit Determination Toolkit)—a software platform independently developed by Wuhan University’s Planetary Geodesy Team. We conducted numerical simulations for POD of targets at Earth–Moon libration points L1, L4, and L5. The results demonstrate that the orbit determination accuracy using only ground-based observations is on the order of several hundred meters. Space-based observations can serve as a valuable supplement to ground-based data, providing a modest improvement in accuracy. However, the addition of lunar-based observations significantly enhances the orbit determination accuracy, reducing position errors and uncertainties to the order of tens of meters. Furthermore, variations in the noise level of lunar-based observations have a stronger impact on orbit determination accuracy than space-based observations. Finally, comparative experiments verify the necessity of solving the solar radiation pressure coefficient Cr for improving orbit determination accuracy. These findings highlight the tremendous potential of lunar-based optical observations in achieving high-precision orbit determination for cislunar space targets and provide valuable insights for future advancements in deep-space situational awareness and autonomous navigation.
期刊介绍:
Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.