HD 47536

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Template:Short description

HD 47536
File:Giant Star HD 47536.jpg
Sky area of 10 x 10 square arcmin around the 6th-magnitude giant star HD 47536.
Reproduced from the Digital Sky Survey.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) +5.25[1]
Characteristics
Evolutionary stage red giant branch[3]
Spectral type K1 III[4]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)7.9902±0.0535 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[5]
Details[5]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val".[6] Template:Solar radius
LuminosityScript error: No such module "val".[6] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val".[6] K
Metallicity [Fe/H]−0.68 dex
Rotation625 days[7]
Rotational velocity (v sin i)Script error: No such module "val".[3] km/s
AgeScript error: No such module "val". Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 47536 is a single[9] star in the southern constellation of Canis Major. It has an orange hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.25.[1] The star is located at a distance of approximately 408 light years from the Sun based on parallax. It is drifting further away with a radial velocity of 80 km/s.[2]

This is an aging, metal-poor giant star with a stellar classification of K1 III.[4] It is about 9.3 billion years old with 94% of the mass of the Sun. Having exhausted the supply of hydrogen at its core, the star cooled and expanded to 23 times the Sun's radius.[6] The star is spinning slowly, taking Script error: No such module "convert". to complete its sidereal rotation. It is radiating 177[6] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,384 K.[6] As of 2015, at least one planet is known to orbit this star.[10]

Planetary system

A planetary companion to this star, HD 47536 b, was discovered in 2003 by a team led by J. Setiawan.[11][3] A second planet, HD 47536 c, was claimed in 2007.[12] However, a follow-up study by Soto et al. in 2015 failed to detect the signal of the second planet, so it remains unconfirmed.[10]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet Template:OrbitboxPlanet hypothetical

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See also

References

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  2. a b c d e f Template:Cite Gaia DR3
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  5. a b Script error: No such module "Citation/CS1".
  6. a b c d e f Template:Cite Gaia DR2
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  8. Template:Cite simbad
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  10. a b Script error: No such module "Citation/CS1".
  11. Script error: No such module "citation/CS1".
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External links

Template:Sky

Template:Stars of Canis Major