HD 1606

Star in the constellation Andromeda From Wikipedia, the free encyclopedia

HD 1606 is a single[14] star in the northern constellation of Andromeda, positioned a few degrees to the northeast of the bright star Alpheratz. It has a blue-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.87.[3] Although it is suspected of variability, none has been conclusively found.[15] The star is located at a distance of approximately 580 light-years (179 parsecs) from the Sun based on parallax,[2] and is drifting further away with a radial velocity of +4 km/s.[8] It has an absolute magnitude of −0.5.[9]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 1606
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[1]
Right ascension 00h 20m 24.40107s[2]
Declination +30° 56 08.2099[2]
Apparent magnitude (V) 5.869[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type B7V[5]
U−B color index −0.45[6]
B−V color index −0.10[6]
Variable type Suspected[7]
Astrometry
Radial velocity (Rv)3.8[8] km/s
Proper motion (μ) RA: 15.734±0.159[2] mas/yr
Dec.: −2.957±0.125[2] mas/yr
Parallax (π)5.5900±0.1069 mas[2]
Distance580 ± 10 ly
(179 ± 3 pc)
Absolute magnitude (MV)−0.5[9]
Details
Mass3.75±0.08[4] M
Radius2.9[10] R
Luminosity245+36
−31
[4] L
Surface gravity (log g)3.988±0.017[11] cgs
Temperature13,186±100[11] K
Rotational velocity (v sin i)113±8[11] km/s
Age211[12] Myr
Other designations
NSV 128, AG+30°32, BD+30°42, GC 408, HD 1606, HIP 1630, HR 78, SAO 53820, PPM 65213[13]
Database references
SIMBADdata
Close

This is a B-type main-sequence star with a stellar classification of B7V,[5] which means it is currently generating energy through hydrogen fusion at its core. It has 3.75[4] times the mass of the Sun and a fairly high rate of spin, showing a projected rotational velocity of 113 km/s.[11] The star is radiating 245[4] times the luminosity of the Sun from its photosphere at an effective temperature of 13,186 K.[11]

References

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