HAT-P-16, also known as TOI-1458, is a triple star system consisting of an F-type main-sequence star, a red dwarf, and a K-type main-sequence star about 743.65 light-years away in the constellation Andromeda. The primary star has a super-Jovian planet that completes an orbit once every days
Size comparison of Jupiter and HAT-P-16 b
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