Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Delphinus |
Right ascension | 21h 00m 27.6883s[1] |
Declination | +19° 19′ 46.493″[1] |
Apparent magnitude (V) | 5.70±0.01[2] |
Characteristics | |
Evolutionary stage | AGB[3] |
Spectral type | M3 IIIab[4] |
B−V color index | +1.61[5] |
Variable type | suspected[6] |
Astrometry | |
Radial velocity (Rv) | −15.07±0.09[7] km/s |
Proper motion (μ) | RA: −15.483 mas/yr[1] Dec.: −59.705 mas/yr[1] |
Parallax (π) | 5.455 ± 0.0753 mas[1] |
Distance | 598 ± 8 ly (183 ± 3 pc) |
Absolute magnitude (MV) | −0.33[8] |
Details | |
Mass | 1.32[9] M☉ |
Radius | 58[10] R☉ |
Luminosity | 507[11] L☉ |
Surface gravity (log g) | 0.93[12] cgs |
Temperature | 3,707[10] K |
Other designations | |
Database references | |
SIMBAD | data |
HD 200044 (HR 8044) is a solitary[13] star in the equatorial constellation Delphinus. It has an apparent magnitude of 5.7,[2] allowing it to be faintly seen with the naked eye. The object is located 598 light years away,[1] but is approaching the Solar System with a heliocentric radial velocity of −15.07 km/s.[7]
HD 200044 has a spectral classification of M3 IIIab,[4] indicating that its an ageing red giant. It is currently on the asymptotic giant branch and is fusing hydrogen and helium in shells around an inert carbon core.[3] As a consequence, it has expanded to 58 times the radius of the Sun and is now radiating with a luminosity over 500 times greater than that of the Sun. HD 200044's large size and high luminosity yield an effective temperature of 3,707 K, giving it a red glow. HD 200044 is suspected to be a variable star with an amplitude of 0.05 magnitudes.[6]
There is a 10th magnitude optical companion separated 49.3″ away and at a position angle of 337° as of 2014. However, the separation is increasing due to HD 200044's high proper motion.[14]
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