Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Delphinus |
A | |
Right ascension | 20h 55m 40.6778s[1] |
Declination | +04° 31′ 57.7994″[1] |
Apparent magnitude (V) | 6.34±0.01[2] |
B | |
Right ascension | 20h 55m 40.5439s[3] |
Declination | +04° 31′ 58.2271″[3] |
Apparent magnitude (V) | 7.49±0.01[2] |
Characteristics | |
A | |
Spectral type | G8 III/IV[4] |
U−B color index | +0.49[5] |
B−V color index | +0.82[5] |
B | |
Spectral type | F/G[6] |
Astrometry | |
Radial velocity (Rv) | −32.6±0.4[7] km/s |
Absolute magnitude (MV) | +0.33[8] |
A | |
Proper motion (μ) | RA: +60.413[1] mas/yr Dec.: +10.949[1] mas/yr |
Parallax (π) | 9.2067 ± 0.0354 mas[1] |
Distance | 354 ± 1 ly (108.6 ± 0.4 pc) |
B | |
Proper motion (μ) | RA: +60.315[3] mas/yr Dec.: +9.758[3] mas/yr |
Parallax (π) | 9.0757 ± 0.0758 mas[3] |
Distance | 359 ± 3 ly (110.2 ± 0.9 pc) |
Details | |
A | |
Mass | 1.25[9] M☉ |
Radius | 8.26+0.65 −0.22[10] R☉ |
Luminosity | 37.1±0.4[10] L☉ |
Surface gravity (log g) | 2.60±0.25[11] cgs |
Temperature | 4,956+68 −185[10] K |
Metallicity [Fe/H] | 0.13±0.09[11] dex |
Rotational velocity (v sin i) | <1[12] km/s |
B | |
Mass | 1.46[9] M☉ |
Radius | 2.10+0.16 −0.27[13] R☉ |
Luminosity | 8.82±0.23[13] L☉ |
Surface gravity (log g) | 3.85[9] cgs |
Temperature | 6,865+494 −251[13] K |
Metallicity [Fe/H] | −0.2[9] dex |
Other designations | |
Database references | |
SIMBAD | The system |
A | |
B |
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.[15] The components have a separation of 2″ at a position angle of 282° as of 2016.[16] 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 −33 km/s.
The brighter component has a stellar classification of G8 III/IV,[4] 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[9] and an enlarged radius of 8.26 R☉.[10] It shines at 37.1 times the luminosity of the Sun[10] from its photosphere at an effective temperature of 4,956 K,[10] giving it a yellow glow. HD 199223A's iron abundance is 135% that of the Sun[11] and it spins modestly with a projected rotational velocity less than 1 km/s.[12]
As for the dimmer one, it is classified as an F/G star,[6] and is calculated to be an F-type subgiant. It has 146% of the mass of the Sun[9] and 2.1 times its radius.[13] It radiates with a luminosity of 8.82 L☉[13] from its photosphere at an effective temperature of 6,865 K,[13] giving it a yellow white glow.
EDR3A
was invoked but never defined (see the help page).Fabricius2002
was invoked but never defined (see the help page).EDR3B
was invoked but never defined (see the help page).Harlan1974
was invoked but never defined (see the help page).Johnson1966
was invoked but never defined (see the help page).Houk1999
was invoked but never defined (see the help page).Gontcharov2006
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Anders2019
was invoked but never defined (see the help page).DR2A
was invoked but never defined (see the help page).Randich1999
was invoked but never defined (see the help page).deMed1999
was invoked but never defined (see the help page).DR2B
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was invoked but never defined (see the help page).Davenhall1997
was invoked but never defined (see the help page).Mason2001
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