Chi Ursae Majoris
{{short description|Star in the constellation Ursa Major}}
{{Starbox begin}}
{{Starbox image
| image =
{{Location mark
| image=Ursa Major IAU.svg
| float=center | width=250 | position=right
| mark=Red circle.svg | mark_width=10 | mark_link=χ UMa
| x%=41.3 | y%=47.8
}}
| caption=Location of χ Ursae Majoris (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Ursa Major
| dec = {{DEC|+47|46|45.8553}}
}}
{{Starbox character
| r-i =
| variable =
}}
{{Starbox astrometry
| radial_v = {{Val|−9.02|0.20}}
| prop_mo_ra = {{val|-138.297}}
| prop_mo_dec = +28.66
| parallax = 16.438
| p_error = 0.113
| absmag_v = {{Val|0.10|0.02}}
}}
{{Starbox detail
| luminosity = {{val|170.1|5.3}}
| temperature = {{Val|4331|33|fmt=commas}}
| gravity = 2.2
| metal_fe = −0.44
| rotational_velocity = 2.3
| age_myr =
}}
{{Starbox catalog
| names = {{odlist | name=Alkaphrah | name2=El Koprah | name3=Taiyangshou | B=Chi UMa, χ UMa | F=63 Ursae Majoris | BD=+48°1966 | FK5=441 | HD=102224 | HIP=57399 | HR=4518 | SAO=43886 }}
}}
{{Starbox reference
| Simbad = chi+UMa
}}
{{Starbox end}}
Chi Ursae Majoris or χ Ursae Majoris, formally named Taiyangshou {{IPAc-en|,|t|ai|,|j|æ|N|'|sh|ou}},{{cite web | url=https://www.iau.org/public/themes/naming_stars/ | title=Naming Stars |publisher=IAU.org |accessdate=16 December 2017}} is a single 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. It is located at a distance of approximately 198 light-years from the Sun based on parallax, but is drifting closer with a radial velocity of −9 km/s.
Nomenclature
File:NGC3877-LB3-2010May16.jpg]]
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.[https://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Ursa_Major*.html Richard Hinckley Allen: Star Names — Their Lore and Meaning: Ursa Major] 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.
In 2016, the IAU organized a Working Group on Star Names (WGSN){{cite web | url=https://www.iau.org/science/scientific_bodies/working_groups/280/ | title=IAU Working Group on Star Names (WGSN)|accessdate=22 May 2016}} 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.
Properties
Chi Ursae Majoris is an evolved, orange hued K-type giant with a stellar classification of K0.5 IIIb. It is a red clump giant, which means it is on the horizontal branch and is generating energy through helium fusion at its core. This star has expanded to 23 times the radius of the Sun with 1.49 times the Sun's mass. It is radiating 170 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,331 K.
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
{{reflist|refs=
{{citation | title=The Cambridge Guide to the Constellations | first1=Michael E. | last1=Bakich | publisher=Cambridge University Press | year=1995 | isbn=0521449219 | pages=112, 116 | url=https://books.google.com/books?id=tLMXiFhTnRYC&pg=PA112}}
{{citation | last1=Jennens | first1=P. A. | last2=Helfer | first2=H. L. | title=A new photometric metal abundance and luminosity calibration for field G and K giants | journal=Monthly Notices of the Royal Astronomical Society | volume=172 | pages=667–679 | date=September 1975 | issue=3 | postscript=. | bibcode=1975MNRAS.172..667J | doi=10.1093/mnras/172.3.667 | doi-access=free}}
{{citation | postscript=. | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | s2cid=14878976 | bibcode=2008MNRAS.389..869E | arxiv=0806.2878}}
{{cite simbad | title=chi UMa | accessdate=2017-02-22 | postscript=.}}
{{cite DR3|786420645182229504}}
}}