HD 80869

Yazar(lar): Trappist-1F_Ce

Yayın tarihi:

HD 80869, also known as HIP 46022, is a binary star system consisting of a G-type main-sequence star and a K-type main-sequence star, located about 276.118 light-years from the Solar System. Component A has a gas giant planet with a mass approximately 5.67 times that of Jupiter, orbiting once every 4.684 years.

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