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Multi-body trajectory design strategies based on periapsis Poincare maps.

机译:基于围手术期Poincare贴图的多体轨迹设计策略。

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摘要

Incorporating multi-body dynamics into preliminary spacecraft trajectory design expands the design space and provides trajectory options that may not otherwise be available. However, multi-body environments are not as well understood as those involving a single gravitational body, and preliminary design in these complicated scenarios is challenging. The current investigation focuses on preliminary design of orbits in the vicinity of the second primary in a 3- or 4-body model, for example, trajectories near a planet in a Sun-planet-moon system.;The tidal acceleration due to the distant larger primary (P1) has significant influence on large orbits about the second primary (P 2). The effects on individual orbits are explored before the investigation is expanded to include large groups of orbits. Periapsis Poincare maps are employed to simplify and organize the design space. By parameterizing trajectories in terms of periapse radius and orientation relative to the P 1-P2 line, the short- and long-term behaviors of many trajectories are predictable based on initial conditions. Trajectories that impact P 2 or escape its vicinity are easily identified. Initial conditions that lead to long-term orbits with particular characteristics, for example, periodic or quasi-periodic orbits, as well as quasi-frozen orbits, are selected from the maps. The existence of various types of trajectories at different spacecraft energy levels and in different P1-P2 systems is explored. The expanded knowledge of the design space in the vicinity of P2 is then applied to various mission design objectives. By employing periapsis Poincare maps, mission objectives are satisfied in a simple, methodical process.;In the same way, an examination of flybys from a multi-body perspective is insightful. Before adding the influence of a gravity assist body to the larger problem, the flyby itself is explored within the context of the 3-body problem. Then, the flyby design is combined with a tidally-influenced orbit to produce a trajectory that takes full advantage of its multi-body environment.
机译:将多体动力学纳入初始航天器的轨迹设计可扩展设计空间,并提供其他方式可能无法使用的轨迹选项。但是,对多体环境的了解不如涉及单个重力体的环境,因此在这些复杂场景中进行初步设计具有挑战性。当前的研究重点是在三体或四体模型中第二原初附近的轨道的初步设计,例如太阳-行星-月球系统中行星附近的轨迹;由于距离遥远而产生的潮汐加速度较大的原边(P1)对绕第二原边(P2)的大轨道有重大影响。在将调查范围扩大到包括大组轨道之前,先探讨对单个轨道的影响。 Periapsis Poincare地图用于简化和组织设计空间。通过根据轨迹半径和相对于P 1-P2线的方向对轨迹进行参数化,可以基于初始条件预测许多轨迹的短期和长期行为。很容易识别出影响P 2或逃脱P 2的轨迹。从地图中选择导致具有特定特征的长期轨道的初始条件,例如周期性或准周期性的轨道以及准冻结的轨道。探索了在不同的航天器能量水平和不同的P1-P2系统中存在各种类型的轨迹。然后将对P2附近的设计空间的扩展了解应用于各种任务设计目标。通过使用围手术期Poincare贴图,可以在一个简单,系统的过程中满足任务目标。以同样的方式,从多身体角度检查飞越是很有见地的。在将重力辅助物体的影响添加到更大的问题之前,先在3体问题的背景下探索飞越本身。然后,将飞越设计与潮汐影响的轨道相结合,以产生一条充分利用其多体环境的轨迹。

著录项

  • 作者单位

    Purdue University.;

  • 授予单位 Purdue University.;
  • 学科 Engineering Aerospace.
  • 学位 Ph.D.
  • 年度 2011
  • 页码 202 p.
  • 总页数 202
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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