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首页> 外文期刊>Acta astronautica >High-fidelity trajectory design to flyby near-Earth asteroids using CubeSats
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High-fidelity trajectory design to flyby near-Earth asteroids using CubeSats

机译:使用CubeSats的高保真轨迹设计,飞越近地小行星

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摘要

Fast development of CubeSat technology now enables the first interplanetary missions. The potential application of CubeSats to flyby near-Earth asteroids is explored in this paper in consideration of CubeSats' limited propulsive capabilities and systems constraints. Low-energy asteroid flyby trajectories are designed assuming a CubeSat is initially parked around to the Sun-Earth Lagrange points. High-impulse and low-thrust trajectories with realistic thrusting models are computed first in the Circular Restricted Three-Body Problem (CR3BP), and then in a high-fidelity ephemeris model. Analysis in the ephemeris model is used to confirm that trajectories computed in the CR3BP model also exist in a more realistic dynamical model, and to verify the validity of the results obtained in CR3BP analysis. A catalogue of asteroid flyby opportunities between years 2019 and 2030 is provided, with 80 m/s of available Delta V and departure from halo orbits around the first and second Sun-Earth Lagrange points (of similar size to those typically used by scientific missions). Results show that the CR3BP model can serve as an effective tool to identify reachable asteroids and can provide an initial estimation of the Delta V cost in the ephemeris model (with +/- 15 m/s accuracy). An impulsive maneuver model can also provide an accurate estimation of the Delta V requirement for a CubeSat equipped with a high-impulse thruster (with 4 m/s accuracy), even if its thrust magnitude is small and requires duty cycling; low-thrust Delta V requirements, however, may differ significantly from the impulsive results (+/- 15 m/s).
机译:现在,CubeSat技术的快速发展使首次行星际飞行成为可能。考虑到CubeSats有限的推进能力和系统限制,本文探讨了CubeSats在飞越近地小行星上的潜在应用。低能小行星飞越轨迹的设计是假设CubeSat最初停放在太阳地球Lagrange点附近。首先在圆形限制三体问题(CR3BP)中计算具有逼真的推力模型的高冲力和低推力轨迹,然后在高保真星历模型中进行计算。星历模型中的分析用于确认CR3BP模型中计算出的轨迹也存在于更现实的动力学模型中,并验证CR3BP分析中获得的结果的有效性。提供了2019年至2030年之间的小行星飞越机会目录,其中有80 m / s的可用Delta V和从第一和第二太阳地球拉格朗日点附近的晕圈轨道偏离(大小与科学飞行任务通常使用的类似) 。结果表明,CR3BP模型可以作为识别可到达小行星的有效工具,并且可以对星历模型中的Delta V成本进行初步估算(精度为+/- 15 m / s)。脉冲机动模型还可以提供对配备高脉冲推进器(精度为4 m / s)的CubeSat的Delta V要求的准确估算,即使其推力大小较小且需要占空比也是如此;但是,低推力Delta V的要求可能与脉冲结果(+/- 15 m / s)明显不同。

著录项

  • 来源
    《Acta astronautica》 |2020年第2期|146-163|共18页
  • 作者

  • 作者单位

    Cranfield Univ Space Res Grp Cranfield Beds England;

    Univ Politecn Cataluna IEEC Barcelona Spain|Univ Politecn Cataluna Dept Matemat Barcelona Spain;

    Univ Barcelona IEEC Barcelona Spain|Univ Barcelona Dept Matemat & Informat Barcelona Spain;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Trajectory design; Interplanetary CubeSats; Near-Earth asteroids; Low-thrust trajectories; Sun-Earth Lagrange points;

    机译:弹道设计;行星际立方体卫星;近地小行星;低推力轨迹;日地拉格朗日积分;

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