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Trajectories for Europa Flyby Sample Return

机译:欧罗巴Flyby样品返回的轨迹

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Ballistic trajectories are computed which would enable a sample return mission to Europa without capturing, descending, or landing. The low-cost mission concept utilizes a free return trajectory that also involves a close flyby of Europa. Near Europa, a small impactor would kinetically impact the icy moon and generate a plume, subsequently sampled by the spacecraft. A broad search algorithm is developed to construct feasible itineraries, which considers Venus and Earth gravity assist sequences. High-quality solutions are then differentially corrected to be continuous using high-fidelity dynamics. The complete methodology is applicable to other outer-planet moons, notably Enceladus. The outbound VEEGA option is found to significantly reduce launch C_3 compared to alternate options. The characteristics and quality of the solutions exhibit substantial variation over the 12-year period of Jupiter. Nevertheless, a variety of optimized results are computed with C_3 as low as 16.0 km~2/sec~2, re-entry speed well below that of the Stardust capsule, and flight times of 9 to 15 years.
机译:计算出弹道,这将使样品能够返回欧罗巴,而无需捕获,下降或降落。低成本飞行任务的概念利用了自由返回轨迹,其中还涉及欧罗巴的近距离飞越。在欧罗巴附近,一个小型撞击器会动态撞击冰冷的月球并产生羽流,随后由航天器采样。开发了一种广泛的搜索算法来构造可行的路线,其中考虑了金星和地球重力辅助序列。然后,使用高保真动力学将高质量的解决方案进行差分校正以使其连续。完整的方法适用于其他外行星卫星,尤其是土卫二。与替代选项相比,发现出站VEEGA选项可大大减少启动C_3。在木星的12年期间,解决方案的特性和质量表现出很大的差异。尽管如此,在C_3低至16.0 km〜2 / sec〜2,重入速度远低于星尘太空舱,飞行时间为9至15年的情况下,仍可以计算出各种优化结果。

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