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A low-thrust-enabled SmallSat heliophysics mission to Sun-Earth L5

机译:将一个低推力的小型光晕头晕物理学使命到Sun-earth L5

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We present an approach to enable SmallSat mission concepts to the Sun-Earth (SE) L5Lagrange point in support of advancing our understanding of solar processes and weather monitoring capabilities by addressing one of the primary challenges of such a mission: traveling to this distant region with limited propulsive capability. Heliophysicists have long been interested in missions to SE L5, which trails behind the Earth in its orbit, due to the capability for viewing solar and interplanetary phenomena. Consequently, a spacecraft orbiting in the vicinity of SE L5would observe the Sun before it rotates into Earth nadir and provide early warning of solar activity. Although SmallSats have emerged as an effective and low-cost platform for space-based science and exploration, operational and mission constraints create significant challenges during the trajectory design process. For instance, the miniaturization of electrospray and ion thrusters render low-thrust propulsion systems an enabling technology for upcoming small satellite missions. However, such systems supply only a low acceleration over limited time intervals. Furthermore, the deployment conditions associated with a SmallSat are typically determined by the primary mission and may evolve frequently throughout the lifecycle of the mission. These regular updates may result in deviations from an individual reference trajectory that are too large for a low-thrust propulsion system to overcome, thereby necessitating a complete trajectory redesign. Together, these operational and mission constraints severely impact the geometry and availability of feasible trajectories that deliver a low-thrust-enabled SmallSat from an uncertain deployment state to the vicinity of SE L5. In fact, these challenges necessitate a rapid and well-informed procedure that leverages dynamical systems techniques for trajectory design. We summarize and demonstrate such an approach within this paper.
机译:我们提出了一种向太阳地球(SE)L为Sun-Breations概念启用的方法 5 拉格朗日点支持推进我们对太阳能流程和天气监测能力的理解,通过解决此类任务的主要挑战之一:前往这个远处的区域,具有有限的推进能力。 Heliophysicists长期以来一直对任命的任务感兴趣 5 ,由于可观察太阳能和行星际现象的能力,在其轨道后面落后于地球。因此,在SE L附近的航天器轨道 5 将在旋转到地球Nadir之前观察太阳,并提供太阳能活动的预警。尽管Smallsats被出现为基于空间的科学和探索的有效和低成本平台,但在轨迹设计过程中运营和使命约束产生了重大挑战。例如,电喷雾和离子推进器的小型化使低推力推进系统成为即将到来的小型卫星任务的能力技术。然而,这种系统在有限的时间间隔内仅提供低加速度。此外,与小型组相关联的部署条件通常由主要任务确定,并且可以在任务的生命周期中经常演变。这些定期更新可能导致与单个参考轨迹的偏差太大,对于低推力推动系统来克服,从而需要完整的轨迹重新设计。这些操作和任务约束在一起严重影响了可行轨迹的几何形状和可用性,从不确定的部署状态到SE L的附近提供了低推力的小型。 5 。事实上,这些挑战需要一种快速且知情的程序,可以利用动态系统进行轨迹设计。我们概述并展示了本文中的这种方法。

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