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Low-thrust enabled highly non-Keplerian orbits in support of future Mars exploration

机译:低推力实现高度非克里普勒轨道,以支持未来的火星探索

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摘要

The technology of high specific impulse propulsion systems with low thrust is improving, opening up numerous possibilities for future missions applying continuous thrust to force a spacecraft out of a natural Keplerian orbit into a displaced non-Keplerian orbit. A systematic analysis is presented as to the applicability of highly non-Keplerian orbits throughout the Solar System. Thereafter, two applications of such orbits in support of future high-value asset exploration of Mars are detailed: a novel concept for an Earth-Mars interplanetary communications relay, on which the paper largely focuses, and a solar storm warning mission. In the former the relay makes use of artificial equilibrium points, allowing a spacecraft to hover above the orbital plane of Mars and thus ensuring communications when the planet is occulted by the Sun with respect to the Earth. The spacecraft’s power requirements and communications band utilized are taken into account to determine the relay architecture. A detailed contingency analysis is considered for recovering the relay after increasing periods of spacecraft propulsion failure, combined with a consideration of how to deploy the relay spacecraft to maximise propellant reserves and mission duration. For such a relay, a combination of solar sail and solar electric propulsion may prove advantageous, but only under specific circumstances of the relay architecture suggested. For highly non-Keplerian orbits the dynamics of the spacecraft is also briefly extended to consider the elliptic restricted three-body problem and the effects of orbit eccentricity.
机译:低推力的高比脉冲推进系统的技术正在改进,为未来的任务提供了许多可能性,这些任务使用连续推力将航天器从自然的开普勒轨道移出非开普勒的轨道。对整个太阳系中高度非Keplerian轨道的适用性进行了系统分析。此后,详细介绍了此类轨道在支持火星未来高价值资产勘探中的两种应用:本文主要关注的地球-火星行星际通信中继的新概念以及太阳风暴预警任务。在前者中,中继器利用人工平衡点,使航天器能够悬停在火星的轨道平面上方,从而在太阳相对于地球遮住行星时确保通信。在确定中继架构时,会考虑航天器的功率要求和所使用的通信频段。考虑了详细的应急分析,以便在增加航天器推进失效周期后恢复中继器,并考虑如何部署中继航天器以最大化推进剂储备和任务持续时间。对于这样的继电器,太阳帆和太阳能推进的结合可能被证明是有利的,但是仅在所建议的继​​电器架构的特定情况下。对于高度非Keplerian轨道,也将航天器的动力学简要扩展,以考虑椭圆约束三体问题和轨道偏心率的影响。

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