Kappa Arae

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

Kappa Arae
Template:Location mark
The location of κ Arae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ara
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.200±0.009[2]
Characteristics
Evolutionary stage Giant[3]
Spectral type G8 III[4]
B−V Template:Engvar +1.03±0.01[2]
Astrometry
Radial velocity (Rv)+17.8±0.1[5] km/s
Proper motion (μ) RA: +13.004 mas/yr[1]
Dec.: +7.554 mas/yr[1]
Parallax (π)7.5862±0.0741 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.49±0.06[2]
Details[2]
Mass3.23±0.24 Template:Solar mass
Radius18.22±0.60 Template:Solar radius
Luminosity166.1±8.9 Template:Solar luminosity
Surface gravity (log g)2.56±0.15 cgs
Temperature4,855±48 K
Metallicity [Fe/H]−0.058±0.037 dex
Rotational velocity (v sin i)1.0[6] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

Kappa Arae is a single[8] star in the southern constellation of Ara. Its name is a Bayer designation that is Latinized from κ Arae, and abbreviated Kappa Ara or κ Ara. With an apparent visual magnitude of 5.20,[2] this star is faintly visible to the naked eye. Based upon parallax measurements, it is approximately Script error: No such module "convert". distant from Earth, give or take a 4 light-year margin of error.[1] It is receding from the Sun with a radial velocity of +17.8 km/s.[5]

This is a giant star with a stellar classification of G8 III,[4] having exhausted the hydrogen at its core and evolved away from the main sequence. With 3.2 times the mass of the Sun, its outer envelope has expanded to about 18 times the Sun's radius. It is radiating 166 times the luminosity of the Sun from its photosphere at an effective temperature of 4,855 K.[2] This is hot enough for it to shine with the golden-hued glow of a G-type star.[9] It is a source for coronal X-ray emission and has been reported as a mild barium star, although the latter is questionable.[10]

Kappa Arae has two 14th magnitude optical companions that are at an angular distance of 25 and 30 arcseconds.[11]

References

<templatestyles src="Reflist/styles.css" />

  1. a b c d e Template:Cite Gaia DR3
  2. a b c d e f Script error: No such module "citation/CS1".
  3. Script error: No such module "citation/CS1".
  4. a b Script error: No such module "citation/CS1".
  5. a b Script error: No such module "citation/CS1".
  6. Script error: No such module "citation/CS1".
  7. Template:Cite simbad
  8. Script error: No such module "citation/CS1".
  9. Script error: No such module "citation/CS1".
  10. Script error: No such module "citation/CS1".
  11. Script error: No such module "citation/CS1".

Script error: No such module "Check for unknown parameters".

External links

Template:Stars of Ara