hd 101930

HD 101930 is a dim 8th magnitude star in the constellation of Centaurus. It is an orange dwarf (spectral class K1 V), somewhat dimmer and cooler than our Sun. In 2005 it was announced that a planet orbits the star.

HD 101930 b

HD 101830 b is an extrasolar planet orbiting the star. It has a minimum mass a third of Jupiters, nearly the same as Saturns so it must be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric.

External links

101930 57172

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