MoonLITE:CLPS交付的美国宇航局天体物理学先锋月球光学干涉仪,用于敏感的毫微秒观测

Gerard T. van Belle, David Ciardi, Daniel Hillsberry, Anders Jorgensen, John Monnier, Krista Lynne Smith, Tabetha Boyajian, Kenneth Carpenter, Catherine Clark, Gioia Rau, Gail Schaefer
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引用次数: 0

摘要

MoonLITE(月球干涉测量探测器)是天体物理学先锋计划的一项提案,旨在开发、建造、飞行和运行第一台空间分离孔径光学干涉仪,提供亚玛斯科学成果。MoonLITE将利用先驱者计划的机会,利用NASA的商业月球有效载荷服务(CLPS)将光学干涉仪运送到月球表面,通过结合光学干涉测量的高空间分辨率和月球表面稳定性的高灵敏度,实现前所未有的发现能力。着陆后,CLPS 提供的漫游车将在距离着陆器板载望远镜 100 米处部署预先装载的 MoonLITE 板载光学望远镜,通过一次部署建立一个双元素干涉测量天文台。MoonLITE 将观测可见光中暗至 17 等的目标,其灵敏度比地面干涉测量仪高出许多个量级,比空间光学系统的分辨率高出 50 倍。MoonLITE 的能力开辟了一个独特的发现空间,包括直接测量最小、最冷恒星和亚恒星褐矮星的大小;寻找环绕外行星寄主恒星的近距离恒星伴星,这些伴星可能会混淆我们对类地行星频率的理解和描述;直接测量年轻恒星天体的大小,描述这些年轻恒星的陆地行星形成区域;测量活动星系核的内部区域和双星部分;以及探测时空泡沫本身的性质。部分观测时间还将通过客座观察员计划提供给更广泛的群体。MoonLITE利用了CLPS的机会,以 "先驱者 "的极低成本提供了前所未有的灵敏度和角分辨率组合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
MoonLITE: a CLPS-delivered NASA Astrophysics Pioneers lunar optical interferometer for sensitive, milliarcsecond observing
MoonLITE (Lunar InTerferometry Explorer) is an Astrophysics Pioneers proposal to develop, build, fly, and operate the first separated-aperture optical interferometer in space, delivering sub-mas science results. MoonLITE will leverage the Pioneers opportunity for utilizing NASA's Commercial Lunar Payload Services (CLPS) to deliver an optical interferometer to the lunar surface, enabling unprecedented discovery power by combining high spatial resolution from optical interferometry with deep sensitivity from the stability of the lunar surface. Following landing, the CLPS-provided rover will deploy the pre-loaded MoonLITE outboard optical telescope 100 meters from the lander's inboard telescope, establishing a two-element interferometric observatory with a single deployment. MoonLITE will observe targets as faint as 17th magnitude in the visible, exceeding ground-based interferometric sensitivity by many magnitudes, and surpassing space-based optical systems resolution by a factor of 50 times. The capabilities of MoonLITE open a unique discovery space that includes direct size measurements of the smallest, coolest stars and substellar brown dwarfs; searches for close-in stellar companions orbiting exoplanet-hosting stars that could confound our understanding and characterization of the frequency of Earth-like planets; direct size measurements of young stellar objects and characterization of the terrestrial planet-forming regions of these young stars; measurements of the inner regions and binary fraction of active galactic nuclei; and a probe of the very nature of spacetime foam itself. A portion of the observing time will also be made available to the broader community via a guest observer program. MoonLITE takes advantage of the CLPS opportunity and delivers an unprecedented combination of sensitivity and angular resolution at the remarkably affordable cost point of Pioneers.
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