Wagner Paul, Clausen Tim
DLR, Institute of Technical Physics, Pfaffenwaldring 38-40, 70569 Stuttgart, Germany.
CEAS Space J. 2022;14(2):303-326. doi: 10.1007/s12567-021-00380-6. Epub 2021 Jul 5.
For safe operation of active space crafts, the space debris population needs to be continuously scanned, to avoid collisions of active satellites with space debris. Especially the low Earth orbit (LEO) shows higher risks of collisions due to the highest density of orbital debris. Laser ranging stations can deliver highly accurate distance measurements of debris objects allowing precise orbit determination and more effective collision avoidance. However, a laser ranging station needs accurate a priori orbit information to track an orbital object. To detect and track unknown orbital objects in LEO, here, a passive optical staring system is developed for autonomous 24/7 operation. The system is weather-sealed and does not require any service to perform observations. To detect objects, a wide-angle imaging system with 10° field of view equipped with an astronomical CCD camera was designed and set up to continuously observe the sky for LEO objects. The system can monitor and process several passing objects simultaneously without limitations. It automatically starts an observation, processes the images and saves the 2D angular measurements of each object as equatorial coordinates in the TDM standard. This allows subsequent initial orbit determination and handover to a laser tracking system. During campaigns at twilight the system detected up to 36 objects per hour, with high detection efficiencies of LEO objects larger than 1 m. It is shown that objects as small as 0.1 m can be detected and that the estimated precision of the measurements is about 0.05° or 7 × the pixel scale.
为了使有源航天器安全运行,需要持续扫描空间碎片数量,以避免有源卫星与空间碎片发生碰撞。特别是近地轨道(LEO),由于轨道碎片密度最高,碰撞风险更高。激光测距站可以提供碎片物体的高精度距离测量,从而实现精确的轨道确定和更有效的碰撞避免。然而,激光测距站需要准确的先验轨道信息来跟踪轨道物体。为了探测和跟踪近地轨道中的未知轨道物体,本文开发了一种无源光学凝视系统,用于全天候自主运行。该系统密封防水,无需任何维护即可进行观测。为了探测物体,设计并搭建了一个配备天文CCD相机、视场为10°的广角成像系统,用于持续观测近地轨道物体的天空。该系统可以同时监测和处理多个经过的物体,没有任何限制。它会自动开始观测、处理图像,并将每个物体的二维角度测量值作为赤道坐标按照TDM标准保存下来。这使得后续能够进行初始轨道确定并移交给激光跟踪系统。在黄昏时分的观测活动中,该系统每小时最多可探测到36个物体,对大于1米的近地轨道物体具有很高的探测效率。结果表明,该系统能够探测到小至0.1米的物体,测量估计精度约为0.05°或7倍像素尺度。