HENON立方体卫星任务的任务分析到一个大的太阳-地球遥远的逆行轨道

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Stefano Cicalò, Elisa Maria Alessi, Lorenzo Provinciali, Paride Amabili, Giorgio Saita, Davide Calcagno, Maria Federica Marcucci, Monica Laurenza, Gaetano Zimbardo, Simone Landi, Roger Walker, Michael Khan
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引用次数: 0

摘要

太阳和行星际威胁防御(HENON)任务是一项立方体卫星空间天气任务,旨在在距离地球超过1000万公里的日地远逆行轨道(DRO)上运行。HENON将搭载为空间天气(SWE)观测量身定制的有效载荷,即高分辨率高能粒子辐射监测器、法拉第杯和磁力计,使其能够提供深空行星际条件的准实时监测。HENON有许多重要的目标,比如展示立方体卫星在深空的能力,包括长时间的电力推进,定期遥测和指挥,以及对深空操作的强大姿态控制。它将为未来在ro上的航天器舰队铺平道路,为SWE预测提供连续的近实时测量。本文重点介绍了A/B阶段的任务分析,主要目标是确定与地球共轨道运动的日心DRO的基线转移轨迹。拟议中的转移利用了逃离地球重力场的乘车机会,最有可能是前往太阳-地球L2区域的任务,并且完全依靠机载电力推进到达深空,使其成为这种方法和技术的开创性演示。在对电力推进系统性能、s/c质量和推进剂预算的适当假设下,将显示HENON目标DRO可以在大约1年内达到,同时考虑到周期性的推力中断,以允许遥测、跟踪和指挥。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Mission analysis for the HENON CubeSat mission to a large Sun-Earth distant retrograde orbit

Mission analysis for the HENON CubeSat mission to a large Sun-Earth distant retrograde orbit

The HEliospheric pioNeer for sOlar and interplanetary threats defeNce (HENON) mission is a CubeSat Space Weather mission, designed to operate in a Sun-Earth Distant Retrograde Orbit (DRO) at more than 10 million km from the Earth. HENON will embark payloads tailored for Space Weather (SWE) observations, i.e., a high-resolution energetic particle radiation monitor, a Faraday cup, and a magnetometer enabling it to provide quasi-real-time monitoring of the interplanetary conditions in deep space. HENON has many important goals, such as demonstrating CubeSat capabilities in deep space, including long-duration electric propulsion with periodic telemetry and command, and robust attitude control for deep-space operations. It will pave the way for a future fleet of spacecraft on DROs, providing continuous near real-time measurements for SWE forecasting. This paper focuses on the mission analysis performed for phase A/B, with the main goal of defining a baseline transfer trajectory to a heliocentric DRO in co-orbital motion with the Earth. The proposed transfer leverages a rideshare opportunity on a mission escaping Earth’s gravity field, most likely one headed toward the Sun–Earth L2 region, and relies exclusively on on-board electric propulsion to reach deep space, making it a pioneering demonstration of this approach and the technology. Under appropriate assumptions on the electric propulsion system performances, s/c mass and propellant budget, it will be shown that the HENON target DRO can be reached in about 1 year, taking into account also periodic interruptions of thrusting to allow for Telemetry, Tracking and Command.

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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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