13 Andromedae

Star in the constellation Andromeda From Wikipedia, the free encyclopedia

13 Andromedae, abbreviated 13 And, is a single,[11] blue-white hued variable star[4] in the northern constellation of Andromeda. 13 Andromedae is the Flamsteed designation, while it bears the variable star designation V388 Andromedae. With a typical apparent visual magnitude of around 5.75,[1] it is dimly visible to the naked eye under good seeing conditions. The distance to this star can be directly estimated from its annual parallax shift of 10.4 mas,[2] yielding a range of 315 light years. At that distance, its brightness is diminished by an extinction of 0.13 magnitude due to interstellar dust.[6] The star is moving closer to the Earth with a heliocentric radial velocity of −8 km/s.[5]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
13 Andromedae
Location of 13 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[1]
Right ascension 23h 27m 07.40s[2]
Declination +42° 54 43.2[2]
Apparent magnitude (V) 5.75[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type B9 III or B9 Mn[3]
B−V color index −0.007±0.004[1]
Variable type α2 CVn[4]
Astrometry
Radial velocity (Rv)−8.1±1.6[5] km/s
Proper motion (μ) RA: +87.132[2] mas/yr
Dec.: +17.127[2] mas/yr
Parallax (π)10.3618±0.0465 mas[2]
Distance315 ± 1 ly
(96.5 ± 0.4 pc)
Absolute magnitude (MV)0.98[6]
Details
Mass2.5[7] M
Radius2.4[7] R
Luminosity48[7] L
Surface gravity (log g)4.08[7] cgs
Temperature9,790[7] K
Rotational velocity (v sin i)75[8] km/s
Age339[6] Myr
Other designations
13 And, V388 Andromedae, BD+42°4672, HD 220885, HIP 115755, HR 8913, SAO 53039, PPM 64250[9]
Database references
SIMBADdata
Close
The visual band light curve of 13 Andromedae, adapted from Adelman (2005)[10]

The variability of 13 Andromedae was first detected in Hipparcos satellite data, and it received its variable star designation in 1999.[12][13]

This is a magnetic chemically peculiar star that has been assigned stellar classifications of B9 III or B9 Mn.[3] It is a variable star of the Alpha2 Canum Venaticorum type, ranging in magnitude from 5.73 down to 5.77[4] with a period of 1.47946 days.[3] The star has a high rate of spin, showing a projected rotational velocity of 75 km/s.[8] 13 Andromedae is around 339 million years old[6] and shines with 48 times the Sun's luminosity.[7]

References

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