HD 100777 b

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

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