It has a yellow hue and is too dim to be readily visible to the average sight, having an apparent visual magnitude of 6.86.
[2] The distance to this star is 513 light years based on parallax, and it is drifting further away from the Sun with a radial velocity of 73 km/s.
[3] It is cooling and expanding along the red giant branch,[5] having evolved off the main sequence after exhausting its core supply of hydrogen fuel.
The star has a lower metallicity the Sun – what astronomers term the abundance of elements with more mass than helium – and it is spinning with a projected rotational velocity of 3.3 km/s.
[4] It is radiating 50.5[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,793 K.[4] HD 112410 has a substellar companion calculated to have a mass at least 9.2 times that of Jupiter and an orbital period of 124.6 days at a typical separation of approximately 0.57 astronomical units (AU).