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We propose a suite of telescopes be deployed as part of the Artemis IIIhuman-crewed expedition to the lunar south pole, able to collect wide-fieldsimultaneous far-ultraviolet (UV), near-UV, and optical band images with a fastcadence (10 seconds) of a single part of the sky for several hourscontinuously. Wide-field, high-cadence monitoring in the optical regime hasprovided new scientific breakthroughs in the fields of exoplanets, stellarastrophysics, and astronomical transients. Similar observations cannot be madein the UV from within Earth's atmosphere, but are possible from the Moon'ssurface. The proposed observations will enable studies of atmospheric escapefrom close-in giant exoplanets, exoplanet magnetospheres, the physics ofstellar flare formation, the impact of stellar flares on exoplanethabitability, the internal stellar structure of hot, compact stars, and theearly-time evolution of supernovae and novae to better understand theirprogenitors and formation mechanisms.

A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole