HD 141937 b

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HD 141937 b is a brown dwarf or exoplanet orbiting the yellow dwarf HD 141937 with an orbital period of approximately 653  days . The object orbits its star at a distance of about 1.5  astronomical units and has a minimum mass of about 9 to 10 Jupiter's masses. It was discovered using the radial velocity method; its discovery was made in 2002 by Udry  et al. published.

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