Evaluation of Mars probe positioning using X-ray pulsars, celestial, gravity-aided and ground-based measurements | |
Liu, Jiandong1,2; Jin, Shuanggen1,3 | |
刊名 | PLANETARY AND SPACE SCIENCE |
2018-11-15 | |
卷号 | 163页码:14-34 |
关键词 | Mars probe positioning X-ray pulsar Gravity-aided odometry Optical celestial techniques |
ISSN号 | 0032-0633 |
DOI | 10.1016/j.pss.2018.06.014 |
通讯作者 | Jin, Shuanggen(sgjin@shao.ac.cn) |
英文摘要 | Autonomous navigation of the Mars probe is a key step for the survivability of the space mission and the success of the scientific experiments. However, Mars probe positioning has large uncertainty due to imprecise techniques and limited observations. In this paper, several key factors of X-ray Pulsar, Optical Celestial, and Gravity-aided navigational system are investigated by the simulation in term of Nonlinear Kalman Filters. The navigational performances are evaluated to investigate the autonomy, accuracy, and stability of the systems. The numbers and the kinds of X-ray Pulsars detected by the antenna system have significant influence on the accuracy and stability of the X-ray Pulsars Navigation (XNAV) system. The XNAV achieves several hundreds of meters orbit accuracy by scanning PSR B1937 + 21, B1821-24 and B0531 + 21 in Earth-Mars cruise orbit. The improvement of pointing accuracy of the celestial sensor has less effect on increasing accuracy of the Optical Celestial Navigation (OCN) system. The OCN has relatively lower navigation accuracy with a few hundred kilometers but higher stability. For surface rover positioning, we introduce the Gravity-aided Odometry (GAO) and design two algorithms to verify its navigation ability. The accuracy of GAO approximately equals to the performance of the ground-based Radio Tracking (RT). The potential scientific perspectives of above methods are discussed, which could improve the astrophysical and planetary geodetic study. |
WOS关键词 | AUTONOMOUS NAVIGATION ; ORBIT DETERMINATION ; STAR TRACKERS ; PERFORMANCE ; SPACECRAFT ; FILTER |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | PERGAMON-ELSEVIER SCIENCE LTD |
WOS记录号 | WOS:000450381700003 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/20902] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Jin, Shuanggen |
作者单位 | 1.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Planetary Sci, Shanghai 200030, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Nanjing Univ Informat Sci & Technol, Sch Remote Sensing & Geomat Engn, Nanjing 210044, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Liu, Jiandong,Jin, Shuanggen. Evaluation of Mars probe positioning using X-ray pulsars, celestial, gravity-aided and ground-based measurements[J]. PLANETARY AND SPACE SCIENCE,2018,163:14-34. |
APA | Liu, Jiandong,&Jin, Shuanggen.(2018).Evaluation of Mars probe positioning using X-ray pulsars, celestial, gravity-aided and ground-based measurements.PLANETARY AND SPACE SCIENCE,163,14-34. |
MLA | Liu, Jiandong,et al."Evaluation of Mars probe positioning using X-ray pulsars, celestial, gravity-aided and ground-based measurements".PLANETARY AND SPACE SCIENCE 163(2018):14-34. |
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