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ORBIT ESTIMATION OF LUNAR SPACECRAFT USING EARTH-BASED OPTICAL SENSORS

机译:基于地球光学传感器的月牙太空船轨道估计

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The feasibility of using angles-only measurements from passive, Earth-based optical sensors is explored for the orbit estimation of lunar spacecraft. Such a capability may serve as a backup to active tracking methods or extend space situational awareness. Historical examples from real-world spacecraft dating back to the 1960s and mathematical models for predicting the brightness of objects in space show that the reflected sunlight from a lunar spacecraft may be detectable from the ground. A test scenario is developed where an actively tracked lunar spacecraft loses contact with the ground and must be tracked with angles-only measurements from an optical system. An extended Kalman filter is used for the orbit estimation, and historical ephemerides of the Lunar Prospector and SMART-1 spacecraft are used as truth models. The Monte Carlo simulations show that the orbit state does not diverge after over 24 hours of sequential visibilities. However, the current filter implementation suffers divergence as the orbit is viewed edge-on, and requires additional tuning before being useful as an operational system.
机译:探索了使用来自被动的,基于地球的光学传感器的仅角度测量来进行月球航天器轨道估计的可行性。这样的功能可以用作主动跟踪方法的备用或扩展空间状况感知。可以追溯到1960年代的现实宇宙飞船的历史示例以及用于预测太空中物体​​亮度的数学模型表明,从月球飞船反射的阳光可以从地面上检测到。开发了一种测试方案,其中主动跟踪的月球飞船失去与地面的接触,必须使用光学系统的仅角度测量值进行跟踪。扩展的卡尔曼滤波器用于轨道估计,月球探测仪和SMART-1航天器的历史星历表用作真实模型。蒙特卡洛模拟显示,经过24小时的连续可见性后,轨道状态不会发散。但是,当前的滤波器实现方式在沿轨道边缘观察时会出现发散,并且在用作操作系统之前需要进行额外的调整。

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