OPTICAL OBSERVATIONS OF SMALL SPACECRAFT AND SPACE DEBRIS AT ISTP SB RAS SAYAN OBSERVATORY

Ivan Korobcev, M. Mishina
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Abstract

Launch of several thousands of small spacecraft as part of satellite groups of various companies (OneWeb, SpaceX, etc.) is expected in the coming years. They will significantly increase the “population” in the low-orbit region. The spacecraft are designed mainly to provide telecommunications and remote sensing of Earth from space. They have a short lifetime. The use of high-speed sCMOS (scientific complementary metal-oxide-semiconductor) detectors in combination with medium diameter optical telescopes provides high temporal resolution, which allows us to get detailed brightness light curves and to estimate the state of small spacecraft. We present the technique and results of photometric measurements of small spacecraft obtained with the 1.6-meter AZT-33IK telescope of ISTP SB RAS Sayan Solar Observatory. Photometric measurements are shown to be an important source of information at various operational stages of satellites.
小型航天器和空间碎片的光学观测
预计未来几年将发射数千艘小型航天器,这些航天器是各公司(OneWeb、SpaceX等)卫星组的一部分。它们将显著增加低轨道区域的“人口”。这些航天器的设计主要是为了从太空提供对地球的电信和遥感。它们的寿命很短。高速sCMOS(科学互补金属氧化物半导体)探测器与中直径光学望远镜相结合,提供了高时间分辨率,使我们能够获得详细的亮度光曲线并估计小型航天器的状态。本文介绍了isp SB RAS Sayan太阳天文台的1.6 m AZT-33IK望远镜对小型航天器的光度测量技术和结果。光度测量显示是卫星各运行阶段的重要信息来源。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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