Photometrical observations and shape modeling of space debris in medium Earth orbits

I. Korobtsev, M. Mishina, Yurii Karavaev, Maxim Eselevich, V. Goryashin
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Abstract

The circular medium Earth orbits with a period of about half a day in the inclination range from 50° to 70° are used by various global navigation satellite systems (GNSS), such as GLONASS, GPS, Beidou, Galileo. GNSS operating orbits are one of the important areas in near-Earth space. The information about the space debris (SD) existing in this region and its characteristics is important for risk assessments and mitigation. We report the results of photometrical observations of SD objects in the vicinity of GNSS orbits obtained with the 1.6-meter AZT-33IK telescope of ISTP SB RAS Sayan Solar Observatory in 2018–2023. We show how SD objects existing in this region are distributed relative to GNSS objects. We derive time and phase dependences of the apparent brightness of all measured SD objects. Folded light curves are constructed, rotation periods and their dynamics are determined. The results of modeling the light curve inherent for several SD objects from the GNSS orbital are presented. We suggest a possible space object shape and parameters of proper rotation, which correspond to the observed light curve.
中地球轨道空间碎片的光度观测和形状建模
各种全球导航卫星系统(GNSS),如全球轨道导航卫星系统、全球定位系统、北斗、伽利略,都使用倾角范围在 50°至 70°之间、周期约为半天的圆形中地轨道。全球导航卫星系统的运行轨道是近地空间的重要领域之一。有关该区域存在的空间碎片(SD)及其特征的信息对于风险评估和减缓非常重要。我们报告了 2018-2023 年利用 ISTP SB RAS Sayan 太阳观测站的 1.6 米 AZT-33IK 望远镜对 GNSS 轨道附近的 SD 物体进行光度观测的结果。我们展示了该区域存在的自毁天体相对于全球导航卫星系统天体的分布情况。我们推导出所有测量到的自毁天体视亮度的时间和相位相关性。我们构建了折叠光曲线,确定了自转周期及其动态变化。介绍了对几个来自全球导航卫星系统轨道的自毁天体固有光曲线的建模结果。我们提出了与观测到的光曲线相对应的可能的空间物体形状和适当旋转参数。
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