It can be viewed with binoculars or a small telescope but is too faint to be seen with the naked eye, having an apparent visual magnitude of 7.60.
[2] This object is located at a distance of 154 light years from the Sun, as determined from its parallax, and is drifting further away with a radial velocity of +31 km/s.
[1] This is an ordinary G-type main-sequence star with a stellar classification of G0V,[3] which indicates it, like the Sun, is generating energy through core hydrogen fusion.
The metal content is about 8% greater than the Sun, and it has a quiet (magnetically inactive) chromosphere.
This planet takes 11.55 years to orbit the star at the typical distance of 5.15 AU (770 Gm).