小行星着陆柔性网航天器动力学特性研究

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Yu Zhang, Yang Yu, Hexi Baoyin
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引用次数: 15

摘要

21世纪,近距离小行星探测进入了一个新时代。然而,小行星广泛崎岖的地形和微重力场仍然对航天器的稳定着陆构成重大挑战,甚至可能直接导致探索者逃跑。由于多个物体之间的相互作用会产生大量的能量耗散,柔性网作为一种典型的多体系统,可能能够克服上述问题。本研究建立了一个动力学模型,全面分析了柔性网航天器在小行星附近和小行星上的运动。首先,我们将多面体方法和球谐参数曲面建模方法相结合,研究了目标小行星的动力学环境。之后,我们使用线性Kelvin–Voigt方法构建了探索者的多体动力学模型。随后,我们基于弹簧-阻尼器接触动力学模型研究了FNS与小行星之间的碰撞过程。FNS的轨迹和速度可以通过并行求解系统动力学方程来推导。最后,我们分析了FNS在运动过程中的变形、下降、跳跃和表面运动过程。因此,为未来的小行星探测任务提供了一个有前景的方案。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dynamical behavior of flexible net spacecraft for landing on asteroid

A new era of up-close asteroid exploration has been entered in the 21st century. However, the widely rugged terrain and microgravity field of asteroids still pose significant challenges to the stable landing of spacecraft and may even directly lead to the escape of the explorer. Owing to the substantial energy dissipation arising from the interaction among multiple bodies, the flexible net, which is a typical multibody system, may be capable of overcoming the above problems. In this study, a dynamical model was established to analyze the movement of the flexible net spacecraft (FNS) near and on the asteroid comprehensively. First, we investigated the dynamical environment of the target asteroid by combining the polyhedron method and spherical harmonics parametric surface modeling approach. Thereafter, we constructed the multibody dynamics model of the explorer using the linear Kelvin–Voigt method. Subsequently, we studied the collision process between the FNS and asteroid based on the spring–damper contact dynamics model. The trajectory and speed of the FNS could be derived by solving the system dynamic equations in parallel. Finally, we analyzed the deformation, descent, jumping motion, and surface movement process of the FNS during the movement. Consequently, a promising scheme is provided for asteroid exploration missions in the future.

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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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