论文标题
在月球南极的高积极紫外线望远镜套件
A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole
论文作者
论文摘要
我们建议将一组望远镜部署为Artemis III人类训练的探险队的一部分，向Lunar South Pole进行，能够以快速节奏（10秒）的单个天空连续几个小时的快速节奏（10秒）来收集宽阔的远场（UV），近紫外线和光带图像。光学制度中的宽阔场，高环境监测为系外行星，恒星天体物理学和天文瞬态提供了新的科学突破。类似的观察结果不能从地球内部的紫外线中进行，而是从月球的表面进行的。提出的观察结果将使大气从近距离的巨大系外星球，系外球星，恒星耀斑形成的物理学，恒星耀斑对系外球星的居住能力的影响，热，紧凑型星的内部恒星结构以及超级nevae and Novae to to to to to to to to to to to to to to to to to to to to to and spromist and Nogientors and Nogity and Nogity and Nogity and Nogity and Nogity and Nogity and Nogientors和Notation机构。
We propose a suite of telescopes be deployed as part of the Artemis III human-crewed expedition to the lunar south pole, able to collect wide-field simultaneous far-ultraviolet (UV), near-UV, and optical band images with a fast cadence (10 seconds) of a single part of the sky for several hours continuously. Wide-field, high-cadence monitoring in the optical regime has provided new scientific breakthroughs in the fields of exoplanets, stellar astrophysics, and astronomical transients. Similar observations cannot be made in the UV from within Earth's atmosphere, but are possible from the Moon's surface. The proposed observations will enable studies of atmospheric escape from close-in giant exoplanets, exoplanet magnetospheres, the physics of stellar flare formation, the impact of stellar flares on exoplanet habitability, the internal stellar structure of hot, compact stars, and the early-time evolution of supernovae and novae to better understand their progenitors and formation mechanisms.
