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THE ORBIT DESIGN FOR MARS DETECTOR WITH THE MINIMUM ENERGY

机译:最低能量的火星探测器的轨道设计

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The deep space exploration to Mars has been a hotspot and the detectors' orbits are the primary concern. The key factors are to realize the flight with the minimum energy consumption and fulfill some constraints. In this paper, the transfer orbit is constructed with Patched Conic Method (PCM) and revalued in the whole mechanical model integrated Sun, Earth and Mars for further performance analysis. The constraint is focused on the visibility limitation that the orbit key point could be locked by the ground station in China. This means that the important orbit maneuver, such as captured by Mars, should be carried out over China to sure the available orbit operation. The main research works are followed. Firstly, based on the idealized two-body model and sphere of influence model, the mechanical model for flight is established. And the flight can be divided into three stages which consist of the Earth escape stage, the Sun transfer stage and the Mars capture stage; Secondly, the orbits corresponding to the different stages are designed separately, and connected together with PCM principle. The concrete realization process contains four steps: 1. Under the visibility limitation, listing all the orbital energy parameters in period of time to launching and arrival with the exhaust algorithm, picking the minimum energy from the energy contour figures, the minimum energy orbit's transfer date to launching and arrival could be determined. 2. The velocity and the position vectors of the Earth and Mars on the launching and arrival date could be gotten with the arithmetic of planetary ephemeris, and then the Lambert theory is used to get the detector's velocity in the launching and arrival point. 3. The reverse calculation method is used to calculate the azimuth angle and velocity increment of the detector in the process of the Earth escape stage. 4. The minimum velocity increment in the Mars capture stage could be calculated based on the known orbit period which the detector would runs around Mars. Finally, the whole mechanical model which includes Earth、Mars、Sun and detector is established. The real energy consumption and the captured position error in Mars are selected as the assessment index to analyze the performance of orbit constructed by PCM. The simulation shows that under the visibility limitation, the transfer orbit is reliable and could be as a design reference.
机译:火星的深空探测一直是一个热点,探测器的轨道是主要问题。关键因素是要以最小的能耗实现飞行并满足一些约束条件。在本文中,转移轨道是用修正圆锥法(PCM)构建的,并在集成了太阳,地球和火星的整个力学模型中进行了重新估值,以进行进一步的性能分析。该约束集中在可见性限制上,即中国的地面站可能会锁定轨道关键点。这意味着重要的机动动作,如火星捕获的,应在中国进行,以确保可用的轨道运行。主要研究工作如下。首先,基于理想化的二体模型和影响范围模型,建立了飞行力学模型。飞行分为三个阶段,分别是地球逃逸阶段,太阳转移阶段和火星捕获阶段。其次,分别设计不同阶段的轨道,并用PCM原理连接在一起。具体的实现过程包括四个步骤:1.在能见度限制下,用排气算法列出发射和到达前一段时间内的所有轨道能量参数,从能量轮廓图中选取最小能量,最小能量轨道的转移日期发射和到达的时间可以确定。 2.利用行星星历法可以得到地球和火星在发射和到达日期的速度和位置矢量,然后利用Lambert理论获得探测器在发射和到达点的速度。 3.逆向计算方法用于计算地球逃逸阶段过程中探测器的方位角和速度增量。 4.火星捕获阶段的最小速度增量可以根据探测器绕火星运行的已知轨道周期来计算。最后,建立了包括地球,火星,太阳和探测器在内的整个力学模型。选择火星中的实际能量消耗和捕获的位置误差作为评估指标,以分析PCM构造的轨道的性能。仿真表明,在能见度的限制下,转移轨道是可靠的,可以作为设计参考。

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