Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Delphinus |
Right ascension | 20h 19m 29.2960s[1] |
Declination | +13° 13′ 00.3571″[1] |
Apparent magnitude (V) | 6.21[2] |
Characteristics | |
Evolutionary stage | AGB[3] |
Spectral type | M1 III[4] |
B−V color index | +1.63[2] |
Astrometry | |
Radial velocity (Rv) | 22.68±0.13[5] km/s |
Proper motion (μ) | RA: −15.865 mas/yr[1] Dec.: −18.581 mas/yr[1] |
Parallax (π) | 3.8556 ± 0.0442 mas[1] |
Distance | 846 ± 10 ly (259 ± 3 pc) |
Absolute magnitude (MV) | −0.46[6] |
Details | |
Mass | 1.77[7] M☉ |
Radius | 57.5[8] R☉ |
Luminosity | 592±16[9] L☉ |
Surface gravity (log g) | 0.89[10] cgs |
Temperature | 3,884±122[8] K |
Metallicity [Fe/H] | +0.08[10] dex |
Other designations | |
Database references | |
SIMBAD | data |
HD 193373 (HR 7771) is a solitary red hued star located in the equatorial constellation Delphinus. It has an apparent magnitude of 6.21,[2] placing it near the limit for naked eye visibility. Parallax measurements place it 846 light years distant[1] and it is currently receding with a heliocentric radial velocity of 22.7 km/s.[5]
This is an asymptotic giant branch star[3] with a stellar classification of M1 III.[4] In its current state, the object is fusing hydrogen and helium shells around an inert carbon core. HR 7771 has 177% the mass of the Sun[7] but has expanded to an enlarged radius of 57.5 R☉.[8] It radiates at 592 times the luminosity of the Sun[9] from its photosphere at an effective temperature of 3,884 K,[8] giving a red hue. HD 193373 has an iron abundance 120% that of the Sun, making it slightly metal enriched.[10]
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