HD 199223

HD 199223 is a double star in the equatorial constellation Delphinus. However, the system was originally in Equuleus prior to the creation of official IAU constellation borders. The components have a separation of at a position angle of as of 2016. They have apparent magnitudes of 6.34 and 7.49 and distances of 354 and 359 light years respectively. The system is drifting closer with a radial velocity of.
The brighter component has a stellar classification of G8 III/IV, indicating that it is a G-type star with the blended luminosity class of a giant star and a subgiant. It has 163% of the mass of the Sun and an enlarged radius of. It shines at 36.5 times the luminosity of the Sun from its photosphere at an effective temperature of, giving it a yellow glow. HD 199223A's iron abundance is 135% that of the Sun and it spins modestly with a projected rotational velocity less than.
As for the dimmer one, it is classified as an F/G star, and is calculated to be an F-type subgiant. It has 136% of the mass of the Sun and 2.3 times its radius. It radiates with a luminosity of from its photosphere at an effective temperature of, giving it a yellow white glow.