HD 169904

HD 169904 (HR 6912; 35 G. Octantis) is a solitary star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 6.26, placing it near the limit for naked eye visibility, even under ideal conditions. Gaia DR3 parallax measurements imply a distance of 482 light-years and it is currently drifting closer with a somewhat constrained radial velocity of $$. At its current distance, HD 169904's brightness is diminished by 0.24 magnitudes due to interstellar extinction and it has an absolute magnitude of +0.19.

HD 169904 has a stellar classification of B8 V, indicating that it is an ordinary B-type main-sequence star that is generating energy via hydrogen fusion at its core. It has 3.25 times the mass of the Sun and 2.42 times the radius of the Sun. It radiates 141 times the luminosity of the Sun from its photosphere at an effective temperature of $$, giving it a blue-white hue when viewed in the night sky. HD 169904 is metal deficient with an iron abundance of [Fe/H] = −0.18 or 66.1% of the Sun's, and it spins rapidly with a projected rotational velocity of $$. HD 169904 is estimated to have completed 47.5% of its main sequence lifetime.

The object was listed as a suspected variable star based on photometric observations, but subsequent observations have not confirmed this.