11 Canis Minoris

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Template:Short description

11 Canis Minoris
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Canis Minor
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.25[2]
Characteristics
Spectral type A1Vnn[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: −29.902[1] mas/yr
Dec.: −25.275[1] mas/yr
Parallax (π)10.4262±0.2007 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.42[2]
Details
Mass2.23[5] Template:Solar mass
Radius2.5[6] Template:Solar radius
Luminosity65.26[2] Template:Solar luminosity
Surface gravity (log g)3.60[5] cgs
TemperatureScript error: No such module "val".[5] K
Age149[5] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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11 Canis Minoris is a single[8] star in the equatorial constellation of Canis Minor,[7] located around 313 light years away from the Sun.[1] It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.25.[2] This object is moving away from the Earth with a heliocentric radial velocity of +28 km/s,[4] having come to within Script error: No such module "convert". some 2.35 million years ago.[2]

This is an A-type main-sequence star with a stellar classification of A1Vnn,[3] where the 'n' notation indicates (very) "nebulous" lines due to rapid rotation. However, Gray and Garrison (1987) found a class of A0.5 IVnn,[9] which would instead match an evolving subgiant star. It is a suspected variable star of unknown type.[10] This object is 149[5] million years old with 2.23[5] times the mass of the Sun and about 2.5[6] times the Sun's radius. It is radiating 65[2] times the Sun's luminosity from its photosphere at an effective temperature of 9,972 K.[5]

References

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Template:Stars of Canis Minor