16 Aurigae

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

Template:Short description

16 Aurigae
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.552[2]
Characteristics
Spectral type K2.5 IIIb CN-0.5[3]
U−B Template:Engvar +1.26[4]
B−V Template:Engvar +1.276[2]
Astrometry
Radial velocity (Rv)−28.44[2] km/s
Proper motion (μ) RA: Script error: No such module "val".[1] mas/yr
Dec.: Script error: No such module "val".[1] mas/yr
Parallax (π)14.04±0.58 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)0.28[5]
Orbit[6][7]
Period (P)Script error: No such module "val".
Semi-major axis (a)Script error: No such module "val".
Eccentricity (e)Script error: No such module "val".
Inclination (i)Script error: No such module "val".°
Longitude of the node (Ω)Script error: No such module "val".°
Periastron epoch (T)Script error: No such module "val".
Argument of periastron (ω)
(secondary)
Script error: No such module "val".°
Details
16 Aur A
Mass1.30[2] Template:Solar mass
RadiusScript error: No such module "val".[8] Template:Solar radius
LuminosityScript error: No such module "val".[8] Template:Solar luminosity
Surface gravity (log g)1.87[9] cgs
TemperatureScript error: No such module "val".[2] K
Metallicity [Fe/H]−0.40[9] dex
Rotational velocity (v sin i)0.0[10] km/s
Age5.07[2] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[11]
Database references
SIMBADdata

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

16 Aurigae is a triple star[12] system located 232 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.547,[13] and is located about 2/3 of the way from Capella toward Beta Tauri. It also lies in the midst of the Melotte 31 cluster, but is merely a line-of-sight interloper.[6] The system has a relatively high proper motion, advancing across the celestial sphere at the rate of 0.166 arc seconds per annum,[14] and is moving closer to the Earth with a heliocentric radial velocity of −28 km/s.[2]

The primary component is a single-lined spectroscopic binary with an orbital period of Script error: No such module "convert". and an eccentricity of 0.1189.[6] The visible member is an aging K-type giant star with a stellar classification of K2.5 IIIb CN-0.5;[3] sometimes just given as K3 III. The notation of the former class indicates weak lines of CN in the spectrum.[6] This star is an estimated five[2] billion years old with 1.30[2] times the mass of the Sun. As a consequence of exhausting the hydrogen at its core, it has expanded to 20 times the Sun's radius. The star is radiating 127[8] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,264 K.[2]

A third component is an magnitude 10.6 star at an angular separation of Script error: No such module "val"..[12] It shows a common proper motion with the primary and thus is a likely third member of the system.[6]

References

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

  1. a b c d e Script error: No such module "Citation/CS1".
  2. a b c d e f g h i j Script error: No such module "Citation/CS1".
  3. a b Script error: No such module "Citation/CS1".
  4. Script error: No such module "Citation/CS1".
  5. Script error: No such module "Citation/CS1".
  6. a b c d e Script error: No such module "Citation/CS1".
  7. Script error: No such module "citation/CS1".
  8. a b c Script error: No such module "Citation/CS1".
  9. a b Script error: No such module "Citation/CS1".
  10. Script error: No such module "Citation/CS1".
  11. Template:Cite simbad
  12. a b Script error: No such module "Citation/CS1".
  13. Script error: No such module "Citation/CS1".
  14. Script error: No such module "Citation/CS1".

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

External links

Template:Stars of Auriga