HD 103197 b explained

HD 103197 b
Discoverer:Mordasini et al.
Discovery Site:La Silla Observatory
Discovered:October 19, 2009
Discovery Method:radial velocity (HARPS)
Apsis:astron
Semimajor:0.235AU
Eccentricity:0 (fixed)
Period:47.8 d
0.131 y

HD 103197 b (also known as HIP 57931 b) is an extrasolar planet which orbits the K-type main sequence star HD 103197, located approximately 170 light years away. It is outside of the habitable zone, and as such is unlikely to have liquid water on its moons, if there are any.