56 Andromedae

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Template:Short description

56 Andromedae
Template:Location mark
Location of 56 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.69[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type K0 III[4]
B−V Template:Engvar +1.060[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: +183.659[1] mas/yr
Dec.: +11.670[1] mas/yr
Parallax (π)9.8863±0.1292 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+0.76[2]
Details
MassScript error: No such module "val".[6] Template:Solar mass
Radius11[5] Template:Solar radius
Luminosity56.2[5] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[7] cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]Script error: No such module "val".[7] dex
Rotational velocity (v sin i)0.0[5] km/s
AgeScript error: No such module "val".[6] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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56 Andromedae, abbreviated 56 And, is a probable binary star[9] system in the northern constellation of Andromeda. 56 Andromedae is the Flamsteed designation. It has a combined apparent visual magnitude of 5.69,[2] which is just bright enough to be dimly visible to the naked eye under good seeing conditions. The distance to this system can be ascertained from its annual parallax shift, measured at Script error: No such module "val".[1] with the Gaia space observatory, which yields a separation of 330 light years. It is moving further from the Earth with a heliocentric radial velocity of +62 km/s[5] and is traversing the celestial sphere at a relatively high rate of Script error: No such module "val". per year.[10] This pair is positioned near the line of sight to the open cluster NGC 752, located Script error: No such module "convert". away.[11]

The brighter primary is an aging giant star[7] with a stellar classification of K0 III,[4] having exhausted the hydrogen at its core and evolved off the main sequence. It is a red clump giant, having undergone helium flash and is presently generating energy at its core through helium fusion.[3] The star is about 3.1[6] billion years old with a negligible observable rotation rate, so the rotation axis of the star is likely pointing towards us.[5] It has 1.3[6] times the mass of the Sun and has expanded to 11[5] times the Sun's radius The star is radiating 56[5] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,765 K.[7]

The faint secondary component is a magnitude 11.93 star located at an angular separation of Script error: No such module "val". along a position angle (PA) of 77°, as of 2001. This has changed little since 1903 when it was at a separation of Script error: No such module "val". along a PA of 80°.[12]

References

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External links

Template:Stars of Andromeda