HD 17926

作者：Karistus

发布日期：

HD 17926, aka TOI-396 and HR 858, is a binary system comprised of an F-type main sequence star and a red dwarf located about 104.35 lightyears from the solar system. The primary component of the pair is known to have three transiting, hot mini-Neptunes orbiting around it in a near-resonant structure

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