Aerogel-based collection of ejecta material from asteroids from libration point orbits: Dynamics and capture design

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Carlo Burattini, Camilla Colombo, Mirko Trisolini
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Abstract

Scientific interest in asteroids and their physical characteristics is growing. These bodies provide insights into the primordial solar system and represent a valuable source of metals, silicates, and water. Several missions over the past few years have aimed to improve and better identify the main properties of these poorly known celestial bodies. However, these missions relied on touchdown(s) on the target asteroid to gather samples, which is complicated owing to the difficulty of accurately reaching and rendezvousing with the body. This study aims to assess the feasibility of an in-orbit asteroid sample collection mission. Such a strategy could prevent complex operations related to landing and touchdown maneuvers and avoid the dead times present in a mission requiring several landings. The presented collection scenario, which focuses on the asteroid Ryugu, proposes gathering samples using a spacecraft injected into a halo orbit around the second libration point, L2. For this purpose, the orbits in the neck region of the zero velocity curves are analyzed. A novel methodology to characterize bouncing behavior is introduced. An interpolation-based approach was used to recover the appropriate restitution coefficients for each collision occurring at a specific impact angle. This was applied to both the rigid body model and the point mass approximation studied for two different sites on the asteroid. Furthermore, the study enlarged the region of interest from only L2 to its neighboring zones to return a more global and realistic point of view. Considering the solar radiation pressure and asteroid aspherical potential, particles of different sizes ejected from different longitudes and with different ejection angles were classified according to their trajectories to finally build a database. Based on this analysis, an aerogel-based collection strategy inspired by that used in the Stardust-NExT (NASA) mission was investigated to assess its possible applicability to the analyzed scenario.

以气凝胶为基础收集来自天平点轨道的小行星喷出物质:动力学和捕获设计
科学界对小行星及其物理特性的兴趣与日俱增。这些天体提供了对原始太阳系的了解,是金属、硅酸盐和水的宝贵来源。过去几年中的几次飞行任务旨在改进和更好地确定这些鲜为人知的天体的主要特性。然而,这些任务都依赖于在目标小行星上的着陆来采集样本,由于难以准确到达目标小行星并与之会合,因此采集工作十分复杂。本研究旨在评估在轨小行星样本采集任务的可行性。这种策略可以避免与着陆和着陆机动有关的复杂操作,并避免需要多次着陆的任务中出现的死机时间。所提出的收集方案以小行星龙宫为重点,建议使用一个航天器,将其注入围绕第二个天平点 L2 的光环轨道,以收集样本。为此,对零速度曲线颈部区域的轨道进行了分析。介绍了一种描述弹跳行为特征的新方法。采用基于插值的方法,为在特定撞击角度发生的每次碰撞恢复适当的恢复系数。该方法同时适用于刚体模型和点质量近似模型,对小行星上的两个不同位置进行了研究。此外,该研究还将关注区域从 L2 扩大到其邻近区域,以返回一个更全面和更现实的视角。考虑到太阳辐射压力和小行星非球面势能,从不同经度和不同抛射角度抛射出的不同大小的粒子根据其轨迹进行了分类,最终建立了一个数据库。在这一分析的基础上,受星尘-NExT(美国航天局)飞行任务的启发,对基于气凝胶的收集战略进行了研究,以评估其是否适用于所分析的情况。
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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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