Lessons learned from an NIAC Phase I study for the flat-fabrication of a Dark Ages observatory

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI:10.1117/1.jatis.10.2.024002
Manuel Indaco, Kanak Parmar, Ryan Long, James Whitehead, Russell W. Mailen, Davide Guzzetti
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Abstract

Flat-fabrication technology may enable the next generation of gigantic deployable architectures devoted to the detection of faint cosmological signals. We assess the applicability of a multifunctional roll-out structure based on shape memory polymer technology for the realization of a large space observatory to measure the cosmological Dark Ages radio signal. Roll-out solutions offer advantageous properties for probe class missions, such as the capability to morph the shape to achieve sufficient structural performance while ensuring high packaging efficiency. We characterize the feasibility of a roll-out observatory in the context of a 5 years-long heliocentric mission scenario. Our preliminary study demonstrates how a four-250 m-long arms architecture with 150 evenly spaced short dipole antennas potentially meets the basic mission requirements dictated by the Dark Ages science case. We conduct a quasi-static structural analysis considering axial and bending loads acting on the arms to assess the structural properties of the proposed architecture, identifying geometric ranges which enable the structure to withstand expected loads while satisfying mass and size constraints. Printable electronics are considered in the design due to the ease of integration with the polymer substrate. In this regard, we explore two distinct electronics configuration options—centralized and decentralized—discussing their benefits in terms of power demand and data management. If successful, such a design may set the stage for future technological development aiming to realize tomographic measurements of the cosmological Dark Ages.
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从 NIAC 关于黑暗时代天文台平面制造的第一阶段研究中汲取的经验教训
扁平制造技术可实现下一代巨型可部署结构,专门用于探测微弱的宇宙学信号。我们评估了基于形状记忆聚合物技术的多功能展开结构的适用性,以实现测量宇宙学黑暗时代无线电信号的大型空间观测站。滚动解决方案为探测类任务提供了有利的特性,例如能够改变形状以实现足够的结构性能,同时确保高封装效率。我们以为期 5 年的日心任务为背景,描述了滚动式观测台的可行性。我们的初步研究表明,带有 150 个均匀分布的短偶极子天线的 4-250 米长的臂架结构如何可能满足 "黑暗时代 "科学案例提出的基本任务要求。我们进行了准静态结构分析,考虑了作用在臂上的轴向和弯曲载荷,以评估拟议结构的结构特性,确定几何范围,使结构能够承受预期载荷,同时满足质量和尺寸限制。由于可印刷电子元件易于与聚合物基底集成,因此设计中考虑了可印刷电子元件。在这方面,我们探讨了两种不同的电子配置方案--集中式和分散式--讨论了它们在电力需求和数据管理方面的优势。这种设计如果成功,将为未来的技术发展奠定基础,从而实现对宇宙学黑暗时代的层析成像测量。
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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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