HD 100777 b

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HD 100777 b is an exoplanet orbiting the star HD 100777 with an orbital period of around 384 days . The major semiaxis of the orbit measures approx. 1.0 astronomical units , the minimum mass is 1.2 Jupiter masses (approx. 370 earth masses ). The discovery of the object using the radial velocity method was made by Naef et al. published in 2007.

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