HD 106270

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HD 106270, also known as HIP 59625, is a single G5 subgiant star about 306 light-years away in the constellation Virgo. A super-Jupiter with a mass of approximately 11 times that of Jupiter was discovered orbiting this star via the radial velocity method in 2011, with an orbital period of about 1,890 days at a semi-major axis of 3.347 AU.

Note: This add-on also includes four fictional moons.

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