HD 85512

HD 85512 is a solitary K-type main-sequence star about 37 light-years away in the constellation Vela. It is about 1 billion years older than the Sun. It is extremely chromospherically inactive, only slightly more active than Tau Ceti. It exhibits a long-term variability and is known to host one low-mass planet.

HD 85512

HD 85512 is a solitary K-type main-sequence star about 37 light-years away in the constellation Vela. It is about 1 billion years older than the Sun. It is extremely chromospherically inactive, only slightly more active than Tau Ceti. It exhibits a long-term variability and is known to host one low-mass planet.