Chi Ursae Majoris

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Template:Short description

Chi Ursae Majoris
Template:Location mark
Location of χ Ursae Majoris (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Ursa Major
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.72[2]
Characteristics
Evolutionary stage Horizontal branch[3]
Spectral type K0.5 IIIb[4]
U−B Template:Engvar +1.16[2]
B−V Template:Engvar +1.18[2]
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[1]
Dec.: +28.66 mas/yr[1]
Parallax (π)16.438±0.113 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[5]
Details[2]
Mass1.49[6] Template:Solar mass
RadiusScript error: No such module "val".[7] Template:Solar radius
LuminosityScript error: No such module "val".[7] Template:Solar luminosity
Surface gravity (log g)2.2 cgs
TemperatureScript error: No such module "val".[7] K
Metallicity [Fe/H]−0.44 dex
Rotational velocity (v sin i)2.3 km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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Chi Ursae Majoris or χ Ursae Majoris, formally named Taiyangshou Template:IPAc-en,[9] is a single[10] star in the northern circumpolar constellation of Ursa Major. The star has an orange hue and is visible to the naked eye at night with an apparent visual magnitude of 3.72.[2] It is located at a distance of approximately 198 light-years from the Sun based on parallax,[1] but is drifting closer with a radial velocity of −9 km/s.[2]

Nomenclature

File:NGC3877-LB3-2010May16.jpg
Chi Ursae Majoris and NGC 3877

χ Ursae Majoris (Latinised to Chi Ursae Majoris) is the star's Bayer designation.

It bore the traditional name Tai Yang Show, "the Sun Governor", from Chinese astronomy.[11] The name was possibly derived from the word 太陽守, Pinyin: Tàiyángshǒu, meaning Guard of the Sun, because this star is marking itself and standing alone in the Guard of the Sun asterism, Purple Forbidden enclosure (see : Chinese constellations). It also bore traditional names of Arabic origin: Alkafzah, Alkaphrah, and El Koprah.[12]

In 2016, the IAU organized a Working Group on Star Names (WGSN)[13] to catalog and standardize proper names for stars. The WGSN approved the name Taiyangshou for this star on 30 June 2017 and it is now so included in the List of IAU-approved Star Names.[9]

Properties

Chi Ursae Majoris is an evolved, orange hued K-type giant with a stellar classification of K0.5 IIIb.[4] It is a red clump giant,[3] which means it is on the horizontal branch and is generating energy through helium fusion at its core. This star has expanded to 23[7] times the radius of the Sun with 1.49 times the Sun's mass.[6] It is radiating 170 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,331 K.[7]

The spiral galaxy in Ursa Major, NGC 3877 (= H I.201), type Sc, is best found from Chi Ursae Majoris, which is almost exactly 15 arcminutes north of the galaxy.

References

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  1. a b c d e Template:Cite DR3
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  3. a b Script error: No such module "citation/CS1".
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  6. a b Script error: No such module "citation/CS1".
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  8. Template:Cite simbad
  9. a b Script error: No such module "citation/CS1".
  10. Script error: No such module "citation/CS1".
  11. Richard Hinckley Allen: Star Names — Their Lore and Meaning: Ursa Major
  12. Script error: No such module "citation/CS1".
  13. Script error: No such module "citation/CS1".

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External links

Template:Stars of Ursa Major