PMO OpenIR
Tiangong-1’s accelerated self-spin before reentry
Lin,Hou-Yuan1,6; Zhu,Ting-Lei1,6; Liang,Zhi-Peng2,6; Zhao,Chang-Yin1,6; Wei,Dong1,6; Zhang,Wei1,6; Han,Xing-Wei2,6; Zhang,Hai-Feng3,6; Wei,Zhi-Bin4; Li,Yu-Qiang5,6; Xiong,Jian-Ning1,6; Zhan,Jin-Wei1,6; Zhang,Chen1,6; Ping,Yi-Ding1,6; Song,Qing-Li2,6; Zhang,Hai-Tao2,6; Deng,Hua-Rong3,6
2019-02-12
Source PublicationEarth, Planets and Space
ISSN1880-5981
Volume71Issue:1
Corresponding AuthorZhao,Chang-Yin(cyzhao@pmo.ac.cn)
AbstractAbstractThe detection and study of the rotational motion of space debris, which is affected by environmental factors, is a popular topic. However, relevant research in extremely low-orbit regions cannot be conducted due to a lack of observational data. Here, we fill in the gaps to present the rotational evolution of Tiangong-1 in the 5?months prior to reentry. Derived from the changes in the relative distance of its two corner cube reflectors from satellite laser ranging data, the angular momentum of Tiangong-1, which is relatively stable during observation, deviates from its maximum principal axis of inertia and precesses around the normal direction of the orbital plane due to gravity gradient torque at an angle of 23.1°±2.5°\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$23.1^\circ \pm\,2.5^\circ$$\end{document}. Requiring consistency with the relationship between the angular momentum and precession rate leads to a solution for the rotation rate, which is thus found to increase. This result cannot be explained by any previously developed torque models. Hence, an atmospheric density gradient torque (ADGT) model that considers the torque generated by the change in atmospheric density with orbital altitude at the satellite scale is proposed to explain the rotational acceleration mechanism of extremely low-orbit objects. The numerical results show that the ADGT model provides a non-negligible ability to explain, but cannot fully describe, the acceleration effect. The data on the rotational evolution of Tiangong-1 can provide an important basis for aerodynamic model improvement by addressing minor factors omitted in previous models.
KeywordTiangong-1 Rotational state estimation Space debris SLR
DOI10.1186/s40623-019-0996-8
Language英语
WOS IDBMC:10.1186/s40623-019-0996-8
PublisherSpringer Berlin Heidelberg
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/23735
Collection中国科学院紫金山天文台
Corresponding AuthorZhao,Chang-Yin
Affiliation1.
2.
3.
4.
5.
6.
Recommended Citation
GB/T 7714
Lin,Hou-Yuan,Zhu,Ting-Lei,Liang,Zhi-Peng,等. Tiangong-1’s accelerated self-spin before reentry[J]. Earth, Planets and Space,2019,71(1).
APA Lin,Hou-Yuan.,Zhu,Ting-Lei.,Liang,Zhi-Peng.,Zhao,Chang-Yin.,Wei,Dong.,...&Deng,Hua-Rong.(2019).Tiangong-1’s accelerated self-spin before reentry.Earth, Planets and Space,71(1).
MLA Lin,Hou-Yuan,et al."Tiangong-1’s accelerated self-spin before reentry".Earth, Planets and Space 71.1(2019).
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Lin,Hou-Yuan]'s Articles
[Zhu,Ting-Lei]'s Articles
[Liang,Zhi-Peng]'s Articles
Baidu academic
Similar articles in Baidu academic
[Lin,Hou-Yuan]'s Articles
[Zhu,Ting-Lei]'s Articles
[Liang,Zhi-Peng]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Lin,Hou-Yuan]'s Articles
[Zhu,Ting-Lei]'s Articles
[Liang,Zhi-Peng]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.