Double star in the constellation Delphinus.
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! style="text-align: center; background-color: #FFFFC0;" colspan="2" | Observation dataEpoch J2000      Equinox J2000
! style="text-align:left" | Apparent magnitude (V)
! style="text-align:left" | Apparent magnitude (V)
! style="background-color: #FFFFC0; text-align: center;" colspan="2"| Characteristics
! style="text-align:center" colspan="2" | A
! style="text-align:left" | Spectral type
! style="text-align:left" | U−B 
! style="text-align:left" | B−V 
! style="text-align:center" colspan="2" | B
! style="text-align:left" | Spectral type
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HD 199223 (HR 8010) 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 125% of the mass of the Sun and an enlarged radius of . It shines at 37.1 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 146% of the mass of the Sun and 2.1 times its radius. It radiates with a luminosity of from its photosphere at an effective temperature of , giving it a yellow white glow.
References.
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