24 Leonis Minoris

Author(s): Karistus

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24 Leonis Minoris, aka HD 88986, is a binary system comprised of a G-type main sequence star and a red dwarf located about 108.77 lightyears from the solar system. A single, potentially transiting sub-Neptune was found around the primary component of the binary on a mildly eccentric 146 day orbit.

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