HD 202206

Autor(es): SolHorizon

Data de publicación:

HD 202206, also known as HIP 104903, is a binary star system consisting of a G-type main-sequence star and a red dwarf. The two orbit each other once approximately every 256 days and are about 150.12 light-years away from the Solar System. This system has a Jupiter-like planet or a brown dwarf, which orbits around these two stars once every 3.45 years.

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