WASP-167

Autor(es): Trappist-1F_Ce

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WASP-167, also known as KELT-13 and TOI-748, is a binary star system consisting of an F-type main sequence star and a G-type star, located approximately 1,345.64 light-years from the Solar System in the constellation Centaurus. In 2017, a hot Jupiter orbiting component A with an orbital period of only 2 days was discovered via the transit method.

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