A light curve for V439 Andromedae, plotted from TESS data,[1] with the 6.23 day rotation period shown in red, | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 06m 36.7841s[2] |
Declination | +29° 01′ 17.4103″[2] |
Apparent magnitude (V) | 6.13 – 6.17[3] |
Characteristics | |
Spectral type | K0Ve[3][4] |
U−B color index | +0.30[5] |
B−V color index | +0.755[5] |
Variable type | BY Dra[3] |
Astrometry | |
Radial velocity (Rv) | −6.9±0.2[4] km/s |
Proper motion (μ) | RA: 380.092±0.060[2] mas/yr Dec.: −177.573±0.037[2] mas/yr |
Parallax (π) | 72.5764 ± 0.0498 mas[2] |
Distance | 44.94 ± 0.03 ly (13.779 ± 0.009 pc) |
Absolute magnitude (MV) | 5.41[6] |
Details | |
Mass | 0.889[7] M☉ |
Radius | 0.9172±0.0090[7] R☉ |
Luminosity | 0.6078±0.0099[7] L☉ |
Surface gravity (log g) | 4.49±0.09[8] cgs |
Temperature | 5509±34[8] K |
Metallicity [Fe/H] | 0.00±0.03[8] dex |
Rotation | 6.23±0.01 days[9] |
Rotational velocity (v sin i) | 4.1 [9] km/s |
Age | 78±28[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 166 or V439 Andromedae (ADS 69 A) is a 6th magnitude star in the constellation Andromeda, approximately 45 light years away from Earth. It is a variable star of the BY Draconis type, varying between magnitudes 6.13 and 6.18 with a 6.23 days periodicity.[3] It appears within one degree of the star Alpha Andromedae[10] and is a member of the Hercules-Lyra association moving group.[4] It also happens to be less than 2 degrees from right ascension 00h 00m.
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