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Coupled orbit and attitude dynamics of a reconfigurable spacecraft with solar radiation pressure

机译:具有太阳辐射压力的可重构航天器的轨道和姿态耦合动力学

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摘要

This work investigates the orbital and attitude dynamics of future reconfigurable multi-panel solar sails able to change their shape during a mission. This can be enabled either by changing the relative position of the individual panels, or by using articulated mechanisms and deployable, retractable and/or inflatable structures. Such a model introduces the concept of modular spacecraft of variable morphology to large gossamer spacecraft. However, this joint concept is complex in nature and requires equations for coupled orbit/attitude dynamics. Therefore, as a starting point, the system is modelled as a rigid-body dumbbell consisting of two tip masses connected by a rigid, massless panel. The system is subjected to a central gravitational force field under consideration of solar radiation pressure forces. Therefore, we assign reflectivity coefficients to the tip masses and a high area-to-mass ratio. An analytical Hamiltonian approach is used to describe the planar motion of the system in Sun-centred Keplerian and non-Keplerian circular orbits. The stability and controllability of the system is enabled through changing the reflectivity coefficients, for example through the use of electro-chromic coating on its surface. The creation of artificial unstable equilibria of the system due to the presence of solar radiation pressure and heteroclinic connections between the equilibria are investigated. We further derive a constraint for the solar radiation pressure forces to maintain the system on a circular Sun-centred orbit. It is planned that the structure is eventually capable of reconfiguring between the equilibria by a minimum actuation effort.
机译:这项工作研究了未来可重新配置的多面板太阳帆在任务期间可以改变形状的轨道和姿态动力学。这可以通过改变各个面板的相对位置,或者通过使用铰接机构和可展开,可伸缩和/或可充气结构来实现。这种模型将可变形态的模块化航天器的概念引入了大型蛛形航天器。但是,这种联合概念本质上是复杂的,需要方程式来求解轨道/姿态动力学耦合问题。因此,作为一个起点,系统被建模为一个刚体哑铃,该哑铃由通过刚性无质量面板连接的两个尖端质量组成。该系统在考虑太阳辐射压力的作用下受到中央重力场的作用。因此,我们将反射率系数分配给尖端质量,并赋予较高的面积质量比。哈密​​顿分析方法用于描述系统在以太阳为中心的开普勒和非开普勒圆形轨道上的平面运动。通过改变反射系数,例如通过在其表面上使用电致变色涂层,可以实现系统的稳定性和可控制性。研究了由于太阳辐射压力的存在而造成的系统的人工不稳定平衡和平衡之间的异质连接。我们进一步推导出太阳辐射压力的约束条件,以将系统维持在圆形的以太阳为中心的轨道上。计划通过最小的驱动力最终使结构能够在平衡之间重新配置。

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