HIP 14810 is a star with three exoplanetary companions in the northern constellation of Aries.
It positioned about 1.3° to the north of Delta Arietis,[7] but is too faint to be visible to the naked eye with an apparent visual magnitude of 8.6.
[2] The system is located at a distance of 165 light-years from the Sun based on parallax measurements,[1] but is drifting closer with a radial velocity of −5 km/s.
[2] This is an ordinary G-type main-sequence star with a stellar classification of G6V.
[5] The star has a high metallicity with a mass and luminosity about the same as the Sun.