HAT-P-17

Author(s): Edasich

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HAT-P-17, also known as TOI-1283, is a binary star system consisting of a K-type main-sequence star and a red dwarf about 302.11 light-years away in the constellation Cygnus. Two super-Jovian planets orbit around the primary star, one of which complete an orbit once every 5.9 days

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