14 Canis Minoris

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Template:Short description

14 Canis Minoris
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Minor
Right ascension Template:RA[1]
Declination Template:DEC[2]
Apparent magnitude (V) +5.30[3]
Characteristics
Evolutionary stage red clump[4]
Spectral type G8 IIIb[5]
B−V Template:Engvar Script error: No such module "val".[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[6] km/s
Proper motion (μ) RA: −156.144[1] mas/yr
Dec.: +98.798[1] mas/yr
Parallax (π)13.50±0.34 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.95[3]
Details[6]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val". Template:Solar radius
LuminosityScript error: No such module "val". Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]Script error: No such module "val". dex
AgeScript error: No such module "val". Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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14 Canis Minoris, also known as HD 65345, is a single[8] star in the equatorial constellation of Canis Minor. It is faintly visible to the naked eye with an apparent visual magnitude of +5.30.[3] The distance to this star, as determined from an annual parallax shift of Script error: No such module "val".,[2] is approximately 242 light years. 14 CMI has a relatively large proper motion, traversing the celestial sphere at the rate of Script error: No such module "val"..[9] It is moving further from the Sun with heliocentric radial velocity of +42.6 km/s.[6]

This is an evolved G-type giant star with a stellar classification of G8 IIIb.[5] At the age of around 550 million years old, it is a red clump giant, which means it has already undergone helium flash and is generating energy through helium fusion at its core.[4] The star has an estimated 2.5 times the mass of the Sun and has expanded to 8.7 times the Sun's radius. It is radiating roughly 48 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,070 K.[6]

References

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Template:Stars of Canis Minor