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MICROSATELLITES FORMATION FLYING FOR OPTICAL SPACE DEBRIS IN-ORBIT OBSERVATION

机译:光学卫星碎片在轨观测的微卫星形成飞行

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For fifteen years, GAUSS (Group of Astrodynamics of the "Sapienza" University of Roma) has been designing, manufacturing and launching four University Satellites (UNISAT) at the School of Aerospace Engineering of Roma. In recent years, GAUSS has also been involved in optical space debris observation, through the creation of the first Italian observatory, completely dedicated to space debris monitoring. In this context, GAUSS students have been analysing the feasibility of a formation flight mission in order to detect space debris, taking advantage of an observation above Earth's atmosphere. This paper will focus particularly on the detection of objects along MEO orbits. The concept is to use optical devices to make observation and orbit determination with the use of a formation of two or more microsatel-lites (depending on the error constraints) taking pictures of the same area from different locations and making a reconstruction of the position of the object using angular measurements. These are obtained through a comparison of the images taken from multiple points of observation by the satellites. Two different strategies of orbit reconstruction are analysed: the first one consists of taking different pictures in order to estimate the position at distinct instants of time; the second one involves capturing a single picture from each satellite, with a higher shutter time so that the position and velocity can be estimated analysing the trail of the object's stripe in the picture. Particularly in this case an accurate attitude control is needed; in fact, to avoid stars generating excessive stripes on the pictures, spacecraft attitude must be kept as fixed as possible, with respect to an inertial reference frame. The paper also describes the choice of the optical configuration and CCD sensors needed in order to obtain an optimal image acquisition, taking into account the weight and the dimensions of the microsatellites. In order to avoid eclipses, the satellites will be placed in a formation along a Sun-synchronous dawn-dusk orbit.The satellite's attitude control will be attained with the use of eight pulsed plasma thrusters.
机译:十五年来,GAUSS(“萨皮恩扎”罗马大学的天体动力学小组)一直在罗马航空工程学院设计,制造和发射四枚大学卫星(UNISAT)。近年来,GAUSS还通过创建首家完全致力于空间碎片监测的意大利天文台,参与了光学空间碎片观察。在这种情况下,GAUSS的学生一直在利用编队飞行任务的可行性进行分析,以便利用对地球大气层的观测来探测太空碎片。本文将特别关注沿MEO轨道的物体的检测。概念是使用光学设备通过形成两个或多个微卫星(根据误差约束)来进行观察和确定轨道,这些微卫星从不同的位置拍摄同一区域的图像,并重新构造卫星的位置。使用角度测量的对象。这些是通过比较从多个观测点拍摄的卫星图像获得的。分析了两种不同的轨道重建策略:第一种策略是拍摄不同的照片,以估计不同时刻的位置;第二种方法是从每颗卫星捕获单个图像,快门时间更长,以便可以通过分析图像中物体条纹的轨迹来估计位置和速度。特别是在这种情况下,需要精确的姿态控制。实际上,为了避免恒星在图片上产生过多的条纹,相对于惯性参考系,航天器的姿态必须保持尽可能固定。本文还介绍了为了获得最佳图像采集所需的光学配置和CCD传感器的选择,同时考虑了微卫星的重量和尺寸。为了避免日食,卫星将沿着太阳同步黎明-黄昏轨道的编队放置。 卫星的姿态控制将通过使用八个脉冲等离子推进器来实现。

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