HD 220105

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Template:Short description

HD 220105
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 6.24[3]
Characteristics
Evolutionary stage main sequence[4][2]
Spectral type A5 Vn[5]
U−B Template:Engvar 0.10[3]
B−V Template:Engvar 0.14[3]
Astrometry
Radial velocity (Rv)−1.8[6] km/s
Proper motion (μ) RA: −9.582[2] mas/yr
Dec.: −37.026[2] mas/yr
Parallax (π)13.7783±0.0277 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.87[1]
Details
Mass1.85[7] Template:Solar mass
Radius1.8[2] Template:Solar radius
Luminosity18.6[2] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[7] cgs
TemperatureScript error: No such module "val".[7] K
Rotational velocity (v sin i)259[4] km/s
Age525[7] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 220105 is a star in the northern constellation of Andromeda, and a member of the Sirius supercluster.[9] It lies near the lower limit of visibility to the naked eye at an apparent visual magnitude of 6.24, and can be a challenge to spot under normal viewing conditions. The star is located 238 light years away, based upon an annual parallax shift of Script error: No such module "val".. It is moving closer to the Earth with a heliocentric radial velocity of −2 km/s.

This is an A-type main-sequence star with a stellar classification of A5 Vn, where the 'n' notation indicates "nebulous" absorption lines due to rapid rotation. It is around 525 million years old with a high projected rotational velocity of 259 km/s. The star has 1.85 times the mass of the Sun and is radiating 19 times the Sun's luminosity from its photosphere at an effective temperature of 8,367 K.

HD 220105 has a magnitude 10.13 companion located at an angular separation of Script error: No such module "val". along a position angle of 178°, as of 2015,[10] and it is listed as a close binary by Zorec and Royer (2012).[4] These coordinates are a source for X-ray emission with a luminosity of Script error: No such module "val"., which is most likely coming from the faint companion.[11]

References

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  2. a b c d e f g h Template:Cite Gaia DR3
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External links

Template:Stars of Andromeda