Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 01h 30m 06.10154s[1] |
Declination | +47° 00′ 26.1860″[1] |
Apparent magnitude (V) | 5.269[2] |
Characteristics | |
Spectral type | K0 III[3] |
B−V color index | 0.993[2] |
Astrometry | |
Radial velocity (Rv) | −11.48[2] km/s |
Proper motion (μ) | RA: −0.939[1] mas/yr Dec.: −42.969[1] mas/yr |
Parallax (π) | 10.3989 ± 0.1605 mas[1] |
Distance | 314 ± 5 ly (96 ± 1 pc) |
Absolute magnitude (MV) | 0.50[4] |
Details | |
Mass | 2.07[2] M☉ |
Radius | 11[5] R☉ |
Luminosity | 70.8[2] L☉ |
Surface gravity (log g) | 2.30[6] cgs |
Temperature | 4,879±106[2] K |
Metallicity [Fe/H] | +0.020±0.04[6] dex |
Rotational velocity (v sin i) | 2.0[7] km/s |
Age | 1.75[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
49 Andromedae (abbreviated 49 And) is a star in the constellation Andromeda. 49 Andromedae is the Flamsteed designation though it also bears the Bayer designation A Andromedae. It is visible to the naked eye under good viewing conditions with an apparent visual magnitude of 5.269.[2] The distance to 49 Andromedae, as determined from its annual parallax shift of 10.4 mas,[1] is around 314 light-years. It is moving closer to the Sun with a heliocentric radial velocity of −11.5 km/s.[2]
With an estimated age of 1.75 Gyr[2] years, this is an aging red-clump[6] giant star with a stellar classification of K0 III,[3] indicating it is generating energy by helium fusion at its core. The spectrum displays "slightly strong" absorption lines of cyanogen (CN).[3] It has 2.07[2] times the mass of the Sun and has expanded to 11[5] times the Sun's radius. The star is radiating 71[2] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,879 K.[2]
GaiaDR2
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was invoked but never defined (see the help page).uranometria1987
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).