39 Andromedae

Double star in the constellation Andromeda From Wikipedia, the free encyclopedia

39 Andromedae, abbreviated 39 And, is a double star in the northern constellation Andromeda. 39 Andromedae is the Flamsteed designation. Its apparent visual magnitude is 5.95,[1] which indicates it is near the lower limit on visibility to the naked eye. The distance to this star, as estimated from its annual parallax shift of 9.57 mas,[2] is 341 light years. It is a suspected member of the Ursa Major Moving Group, although King et al. (2003) list it as a probable non-member.[10]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
39 Andromedae
Location of 39 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[1]
Right ascension 01h 02m 54.25471s[2]
Declination +41° 20 42.7688[2]
Apparent magnitude (V) 5.95[1]
Characteristics
Spectral type kA3hA7VmA9[3]
B−V color index +0.161±0.009[1]
Astrometry
Radial velocity (Rv)+3.1±0.9[4] km/s
Proper motion (μ) RA: −18.380[2] mas/yr
Dec.: −18.498[2] mas/yr
Parallax (π)9.5651±0.1226 mas[2]
Distance341 ± 4 ly
(105 ± 1 pc)
Absolute magnitude (MV)0.80[1]
Details
Mass2.01[5] M
Radius3.02[5] R
Luminosity37[5] L
Surface gravity (log g)3.78[5] cgs
Temperature8,203[5] K
Metallicity [Fe/H]−0.01[6] dex
Rotation30.4 days[7]
Rotational velocity (v sin i)34[8] km/s
Age670[6] Myr
Other designations
39 And, BD+40°209, HD 6116, HIP 4903, HR 290, SAO 36874, PPM 43575, WDS J01029+4121A[9]
Database references
SIMBADdata
Close

The brighter component is a confirmed Am star[11] with a stellar classification of kA3hA7VmA9.[3] This notation indicates its spectrum displays the calcium K line of an A3 star, the hydrogen lines of an A7 V, or A-type main-sequence star, and the metal lines of an A9 star. It is radiating 37 times the Sun's luminosity from its photosphere at an effective temperature of 8,203 K.[5] As of 2015, the magnitude 12.48 companion star is located at an angular separation of 20.5 along a position angle of 3° from the primary.[12]

References

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