M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak
{"title":"考虑光压力的人造地球卫星轨道运动持续时间的近似计算","authors":"M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak","doi":"10.30970/JPS.25.1901","DOIUrl":null,"url":null,"abstract":"A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords:","PeriodicalId":43482,"journal":{"name":"Journal of Physical Studies","volume":"20 1","pages":""},"PeriodicalIF":0.7000,"publicationDate":"2021-01-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Approximate evaluation of the duration of the orbital motion of artificial Earth satellites taking into account light pressure\",\"authors\":\"M. M. Koval'chuk, Y. Vovchyk, O. Baran, A. Bilinsky, I. P. Laushnyk, M. Stodilka, M. Hirnyak\",\"doi\":\"10.30970/JPS.25.1901\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords:\",\"PeriodicalId\":43482,\"journal\":{\"name\":\"Journal of Physical Studies\",\"volume\":\"20 1\",\"pages\":\"\"},\"PeriodicalIF\":0.7000,\"publicationDate\":\"2021-01-29\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Physical Studies\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.30970/JPS.25.1901\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Physical Studies","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.30970/JPS.25.1901","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
引用次数: 0
摘要
为了确定太阳压力对人造地球卫星在轨存在的影响,进行了全面的研究。选取2001(cid:21)2020年在轨运行的6颗低轨道卫星和1颗高椭圆轨道卫星作为研究对象。我们使用了USSTRATCOM卫星轨道要素数据库(http://www.space-track.org/),其他数据来自CalSky (https://www.calsky.com)和TLEtools (https://tletools.readthedocs.io)。考虑到光的压力,我们(cid:28)需要计算卫星轨道运动的持续时间,我们之前已经做过了。科瓦尔丘克先生,布尔。国家的。大学,基辅。天文学,55,39(2017)],而克拉丽(cid:28)则记录了它毁灭的时刻。采用该方法可以减小卫星计算寿命与实际寿命之间的差值(cid:27):对于低轨道卫星,其计算寿命与实际在轨生存时间的差值不超过±1天,对于高椭圆轨道卫星,其差值为+2天。这样的精确度对于做出正确的预测是非常重要的。因此,在低轨道卫星的情况下,考虑光压的计算误差很小,但对于在中、高(地球静止)轨道上运行的低质量和大表面物体,这种误差可能很大(cid:28) [Ch. Lucking, C. Colombo, C. R. McInnes,《宇航员学报》,77,197(2012)]。关键词:
Approximate evaluation of the duration of the orbital motion of artificial Earth satellites taking into account light pressure
A comprehensive research was conducted to establish the in(cid:29)uence of solar pressure on the existence of arti(cid:28)cial Earth satellites in their orbit. Six low-orbit satellites and one satellite with a high-elliptical orbit moving in orbit during 2001(cid:21)2020 were selected for the study. We used the USSTRATCOM database of the satellites’ orbital elements (http://www.space-track.org/), additional data were taken from CalSky (https://www.calsky.com) and TLEtools (https://tletools.readthedocs.io). Taking into account light pressure, we re(cid:28)ned the calculation of the duration of a satellite’s orbital motion, which we had performed earlier [M. M. Koval’chuk, Bull. Natl. Univ. Kyiv. Astron. 55, 39 (2017)], and clari(cid:28)ed the moment of its destruction. Using the proposed method allowed us to reduce the di(cid:27)erence between the calculated and the real lifetime of satellites: for low-orbit satellites, the di(cid:27)erence between the calculated and the real time of their existence in orbit does not exceed ± 1 day, for a satellite with a highly elliptical orbit it is +2 days. Such accuracy is su(cid:30)cient to produce proper forecasts. Thus, consideration of light pressure gives a small correction in the calculations in the case of low-orbit satellites, but this correction can be signi(cid:28)cant for low-mass and large-surface objects moving in medium and high (geostationary) orbits [Ch. Lucking, C. Colombo, C. R. McInnes, Acta Astronaut. 77, 197 (2012)].Keywords: