Nu1 Boötis

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Nu1 Boötis
File:Nu1 Bootis.jpg
ν1 (right) and ν2 Boötis in optical light
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Boötes
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +5.02[2]
Characteristics
Spectral type K4.5 IIIb Ba0.4[3]
U−B Template:Engvar +1.91[2]
B−V Template:Engvar +1.59[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: +10.563 mas/yr[1]
Dec.: Script error: No such module "val". mas/yr[1]
Parallax (π)3.3492±0.077 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−2.22[5]
Details
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".[7] cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]Script error: No such module "val".[7] dex
Rotational velocity (v sin i)4.2[8] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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Nu1 Boötis is an orange-hued star in the northern constellation of Boötes. Its name is a Bayer designation that is Latinized from ν1 Boötis, and abbreviated Nu1 Boo or ν1 Boo. This star has an apparent visual magnitude of +5.02,[2] which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of Script error: No such module "val". as seen from Earth,[1] it is located approximately 970 light years distant from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction of 0.13 due to interstellar dust.[10] It is drifting closer to the Sun with a radial velocity of −11.1 km/s.[4]

This is an evolved K-type giant star with a stellar classification of K4.5 IIIb Ba0.4.[3] The 'Ba0.4' suffix notation indicates this is a weak barium star,[11] which means that the stellar atmosphere has been enhanced by s-process elements most likely provided by what is now an orbiting white dwarf companion.[12] The giant component has 99.8 times the radius of the Sun. It is radiating 2,054[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of about 3,917 K.[7]

Ptolemy considered Nu Boötis to be shared by Hercules, and Bayer assigned it a designation in both constellations: Nu Boötis (ν Boo) and Psi Herculis (ψ Her). When the modern constellation boundaries were fixed in 1930, the latter designation dropped from use.[13]

References

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  4. a b Script error: No such module "citation/CS1".
  5. Script error: No such module "citation/CS1".
  6. a b c Script error: No such module "citation/CS1". Nu1 Boötis' database entry at VizieR.
  7. a b c d Script error: No such module "citation/CS1".
  8. Script error: No such module "citation/CS1".
  9. Template:Cite simbad
  10. Script error: No such module "citation/CS1".
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  13. Script error: No such module "citation/CS1".

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External links

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Template:Stars of Boötes