Based upon stellar parallax measurements by the Hipparcos spacecraft, HD 147513 lies some 42 light years from the Sun.
[3] It has about 11% greater mass than the Sun, and is considered young with an estimated age of 400 million years.
[14] HD 147513 is a member of the Ursa Major moving group that share a common proper motion through space.
The progenitor of the white dwarf may have been a closer companion, and while passing through the asymptotic giant branch stage of its evolution, could have transferred matter onto HD 147513 and contaminated this star's photosphere.
As such, it is unlikely that a terrestrial planet could have a stable orbit within the HZ unless it moves in a synchronized fashion with the gas giant.