HD 17092

HD 17092 is a 355 light years from Earth distant K giant in the constellation Perseus. It is characterized by an apparent brightness of 7.7 may not be seen with the naked eye even under optimal viewing conditions. In 2007, Niedzielski et discovered. al. using the radial velocity method a planetary companion with an orbital period of around 360 days, which carries the systematic name HD 17092 b. The semi-major axis of its orbit measures 1.3 astronomical units, and its minimum mass is about 4.6 Jupiter masses.