首页> 外文会议>ESA SP-587; European Conference on Space Debris; 20050418-20; Darmstadt(DE) >ASTROPHOTOMETRICAL OBSERVATION OF ARTIFICIAL SATELLITES AND STUDY OF THE TECHNICAL STATUS OF PARENTAL BODIES OF SPACE DEBRIS AT GEOSTATIONARY RING
【24h】

ASTROPHOTOMETRICAL OBSERVATION OF ARTIFICIAL SATELLITES AND STUDY OF THE TECHNICAL STATUS OF PARENTAL BODIES OF SPACE DEBRIS AT GEOSTATIONARY RING

机译:人造卫星天体光谱的观测及空间碎屑母体的技术状况研究

获取原文
获取原文并翻译 | 示例

摘要

The amount of faint objects has been observed form a significant portion of all population of a GEO orbit objects. According to statistical observation the magnitudes of those faint objects are in a range from 16 up to 19 (V). These mean that debris have the sizes less than one meter. It is accepted to count, that these debris were formed as a result of explosions and destructions of several space vehicles and means of their mulflucatins or dead such as the Soviet satellites the Ekran 2 and 4 and the last stage American buster Transtage. In the literature some documentary certificates of the explosion and destructions also are resulted. But on the other hand, almost all SC from the list of the objects which are suspected of destruction had observed too enough a long time and in detail and their observably magnitudes does not differ from average magnitudes which we are considered as the intact. They also are registered in a range of the magnitudes from 11 up to 14, which does not allow us speaking about their full destruction. There is one of the basic questions concerning nature small sized debris on GEO. Basically conclusions about destructions and collisions are based on the analysis of the ballistic information. This analysis has its own restrictions. Other in formations does need which has not been connected to measurement of orbits of satellites. In the report we shall show that the photometric information received on these objects is not allowed to draw conclusions on that, these objects in partly or completely destroyed. Thus we in any degree do not call in question about existence small sized faint debris on GEO. The first that we want is to establish their nature and origin. Further it is necessary to remove the contradiction between amount of fragments which observed and on the average by normal photometrical observed behaviors of those space vehicles. In connection with the received results on spacecraft "Ekran 2", that was published early we carried out additional observations of geostationary objects which were considered to be destroyed by different reasons. The objects of observation were chosen from the lists published in the works. We shall try to establish nature of the "faint population" GEO debris with use of methods of precision multi-color astrophotometrical observations of GEO satellites.
机译:观测到的微弱物体数量占整个GEO轨道物体总数的很大一部分。根据统计观察,这些微弱物体的大小在16到19(V)之间。这意味着碎片的大小小于一米。可以认为,这些碎片是由于数种航天器的爆炸和破坏以及其多氟卡汀或死者的手段而形成的,例如苏联卫星Ekran 2和4和最后阶段的美国克星Transtage。在文献中还获得了有关爆炸和破坏的一些证明文件。但是,另一方面,怀疑被破坏的物体列表中的几乎所有SC都已经长时间,详细地观察到了足够多的时间,它们的可观察幅度与我们认为是完整的平均幅度没有差异。它们的登记数量级也从11到14,这不允许我们谈论它们的完全销毁。关于地球静止轨道上自然界小碎片的基本问题之一。关于破坏和碰撞的基本结论是基于对弹道信息的分析。这种分析有其自身的局限性。确实需要与卫星轨道的测量无关的其他编队。在报告中,我们将表明,不允许对这些物体接收的光度信息得出结论,即这些物体被部分或完全破坏。因此,我们无论如何都不会在GEO上引起关于存在小型微弱碎片的质疑。我们首先要确定它们的性质和起源。此外,有必要消除那些被观测的碎片数量与那些航天器的正常光度观测行为所得出的平均值之间的矛盾。关于在早期发布的“ Ekran 2”号航天器上收到的结果,我们对地球静止物体进行了另外的观测,这些地球静止物体被认为是由于各种原因而被破坏的。从作品发表的清单中选择观察对象。我们将尝试使用GEO卫星的精密多色天文光度观测方法来确定“微弱人口” GEO碎片的性质。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号