GR Andromedae

From Wikipedia, the free encyclopedia

Right ascension00h 28m 28.5694s[2]
Declination+32° 26 15.876[2]
Apparentmagnitude(V)6.87 6.95 variable[3]
GR Andromedae

The visual band light curve of GR Andromedae, showing variation about the mean brightness. Adapted from Pyper et al. (2017)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 00h 28m 28.5694s[2]
Declination +32° 26 15.876[2]
Apparent magnitude (V) 6.87 6.95 variable[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A2pSrCrEu[3]
Apparent magnitude (B) 6.99[4]
Apparent magnitude (V) 6.91[4]
Apparent magnitude (G) 6.8449[2]
Apparent magnitude (J) 6.708[5]
Apparent magnitude (H) 6.765[5]
Apparent magnitude (K) 6.739[5]
Variable type α2 CVn[3]
Astrometry
Radial velocity (Rv)−18.2±0.7[6] km/s
Proper motion (μ) RA: −28.947±0.032 [2] mas/yr
Dec.: −20.114±0.026[2] mas/yr
Parallax (π)5.7439±0.0306 mas[2]
Distance568 ± 3 ly
(174.1 ± 0.9 pc)
Absolute magnitude (MV)+0.88[7]
Details
Mass2.24[7] M
Radius2.24[8] R
Luminosity37[7] L
Surface gravity (log g)3[9] cgs
Temperature8,542[9] K
Metallicity [Fe/H]1[9] dex
Rotation518.2 days[1]
Rotational velocity (v sin i)< 6[8] km/s
Age525[7] Myr
Other designations
2MASS J00282858+3226159, BD+31 59, HD 2453, HIP 2243, SAO 53921, TYC 2266-725-1
Database references
SIMBADdata

GR Andromedae (often abbreviated to GR And) is a variable star in the constellation Andromeda. Its apparent visual magnitude varies between 6.87 and 6.95 in a cycle of 518.2 days.[1] It is classified as an α2 Canum Venaticorum variable.[3]

Variability

References

Related Articles

Wikiwand AI