Author(s): Gurren Lagann
XO-3, also known as TOI-1676, is a binary star system of an F-type and a K-type main sequence stars about 699 light-years away in the constellation Camelopardalis. The larger star of the two (component A) has a massive superjovian or low-end brown dwarf that completes a 2.26-day orbit around its star
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