HAT-P-33

Author(s): SolHorizon

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HAT-P-33, also known as TOI-1714 and Gaia-TROI-212, is a binary star system comprising of an F-type giant star and a red dwarf about 1,306 light-years away in the constellation Cygnus. The larger star has an enormous gas giant planet almost twice the size, but only 3/4 the mass of Jupiter, which completes an orbit once every 3.07 days

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