Mu Boötis
{{short description|Pair of double stars in the northern constellation of Boötes}}
{{Starbox begin
| name=Mu Boötis
}}
{{Starbox image
| image ={{Location map|100x100
|AlternativeMap=Boötes IAU.svg
|caption=
|alt=Diagram showing star positions and boundaries of the Boötes constellation and its surroundings
|width=250
|lat=64.5 |long=30.6
|mark=Cercle rouge 100%.svg | marksize=12
|float=center
}}| caption=Location of μ Boötis (circled)
}}
{{Starbox observe 3s
| epoch=J2000
| constell=Boötes
| component1=A
| component2=B or Ba
| component3=C or Bb
}}
{{Starbox character
| component1 = Mu1 Boötis
| r-i = 0.15
| component2 = Mu2 Boötis
}}
{{Starbox astrometry
| component1 = A
| radial_v = {{Val|−8.60|0.3}}
| parallax = 26.5759
| p_error = 0.7871
}}
{{Starbox astrometry|no_heading=y
| component1 = B or Ba
| radial_v =
| parallax = 27.2223
| p_error = 0.0168
| absmag_v=
}}
{{Starbox astrometry|no_heading=y
| component1 = C or Bb
| radial_v =
| parallax = 27.2126
| p_error = 0.0181
| absmag_v=
}}
{{Starbox orbit
| primary = Aa
| name=Ab
| period=3.75
| axis=0.099
| eccentricity=0.270
| inclination=129.7
| node=129.4
| periarg=43.5
| periastron=1006.33
}}
{{Starbox orbit
| primary = B
| name=C
| period=265
| axis=1.46
| eccentricity=0.585
| inclination=135.5
| node=174
| periarg=338
| periastron=1864.9
}}
{{Starbox detail
| component1 = Aa
| metal_fe =
| age_gyr=
}}
{{Starbox detail|no_heading=y
| component1 = Ab
| radius =
| luminosity =
| metal_fe =
| age_gyr=
}}
{{Starbox detail|no_heading=y
| component1 = B or Ba
| metal_fe =
}}
{{Starbox detail|no_heading=y
| component1 = C or Bb
| metal_fe =
}}
{{Starbox catalog
| names = {{odlist | name=Alkalurops | name2=Inkalunis | name3=Icalurus | name4=Clava | name5=Venabulum | ADS=9626 | B=μ Boo | F=51 Boötis | FK5=568 | CCDM=15245+3722 }}
| component1=μ1 Boo
| names1={{odlist | BD=+37°2636 | GJ=3903 | HD=137391 | HIP=75411 | HR=5733 | SAO=64686 | GC=20724 }}
| component2=μ2 Boo
| names2={{odlist | BD=+37°2637 | GJ=3904 | HD=137392 | HIP=75415 | HR=5734 | SAO=64687 | GC=20725 }}
}}
{{Starbox reference
| Simbad=mu.+Boo | sn=μ1 Boo
| Simbad2=51+Boo+B | sn2=μ2 Boo
}}
{{Starbox end}}
Mu Boötis, Latinized from μ Boötis, consists of a pair of double stars in the northern constellation of Boötes, 120 light-years from the Sun.
Mu Boötis had the traditional name Alkalurops {{IPAc-en|æ|l|k|ə|ˈ|lj|ʊər|ɒ|p|s}}, although the International Astronomical Union now regards that name as only applying to μ1 Boötis.
System
The primary pair, component A, is designated μ1 Boötis and the two components an angular separation of 0.08″.{{cn|date=April 2023}}
The secondary, consisting of components BC, is designated μ2 Boötis and they have a separation of 2.2″. The two double star systems are separated by 107″, with matching parallaxes and proper motions, suggesting they form a system. However, components BC have a different chemical composition compared to the A pair, indicating this may instead be a close encounter between two binary systems.
Nomenclature
μ Boötis (Latinised to Mu Boötis) is the star's Bayer designation. It also bears the Flamsteed designation 51 Boötis.
The system's traditional name Alkalurops is from the Greek καλαύροψ kalaurops "a herdsman's crook or staff", with the Arabic prefix attached. It has also been known as Inkalunis (from the Alfonsine tables), Clava (Latin 'the club') and Venabulum (Latin 'a hunting spear'). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name Alkalurops for μ¹ Boötis on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.
It is known as 七公六, Qī Gōng liù (the Sixth Star of the Seven Excellencies) in Chinese.{{in lang|zh}} [http://aeea.nmns.edu.tw/2006/0606/ap060626.html AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 26 日] {{Webarchive|url=https://web.archive.org/web/20110522121442/http://aeea.nmns.edu.tw/2006/0606/ap060626.html |date=2011-05-22 }}
Properties
μ1 Boötis is a yellow-white F-type subgiant with an apparent magnitude of +4.31.
Separated from its brighter companion by 108 arcseconds in the sky is the binary star μ2 Boötis, which has a combined spectral type of G1V and a combined brightness of +6.51 magnitudes. The components of μ2 Boötis have apparent magnitudes of +7.2 and +7.8 and are separated by 2.2 arcseconds.{{cn|date=April 2023}} They complete one orbit about their common centre of mass every 260 years.
{{Clear left}}
References
{{reflist|refs=
{{cite Gaia DR3|1387349379494809600}}
{{cite Gaia DR3|1387349065967311744}}
{{cite Gaia DR3|1387349065960639232}}
{{Citation|postscript=.|last=Tokovinin|first=Andrei|date=2018-03-01|title=The Updated Multiple Star Catalog|journal=The Astrophysical Journal Supplement Series|volume=235|issue=1|pages=6|doi=10.3847/1538-4365/aaa1a5|issn=0067-0049|arxiv=1712.04750|bibcode=2018ApJS..235....6T|s2cid=119047709 |doi-access=free }}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters | arxiv=1108.4971
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015
| s2cid=119257644 | postscript=. }}
{{citation | display-authors=1
| last1=Johnson | first1=H. L. | last2=Iriarte | first2=B.
| last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z.
| title=UBVRIJKL photometry of the bright stars
| journal=Communications of the Lunar and Planetary Laboratory
| volume=4 | issue=99 | pages=99 | date=1966
| bibcode=1966CoLPL...4...99J | postscript=. }}
| last1=Zorec | first1=J. | last2=Royer | first2=F.
| title=Rotational velocities of A-type stars. IV. Evolution of rotational velocities
| journal=Astronomy & Astrophysics
| volume=537 | page=A120 | date=January 2012
| doi=10.1051/0004-6361/201117691 | bibcode=2012A&A...537A.120Z
| arxiv=1201.2052 | s2cid=55586789 | postscript=. }}
| last1=Gontcharov | first1=G. A.
| title=Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system
| journal=Astronomy Letters
| volume=32| issue=11| pages=759–771| date=November 2006
| doi=10.1134/S1063773706110065 | bibcode=2006AstL...32..759G
| arxiv=1606.08053 | s2cid=119231169
| postscript=. }}
| author=Mamajek, Eric |display-authors=etal | date=June 30, 2017
| publisher=IAU Division C Working Group on Star Names
| url=http://www.pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt
| title=IAU Catalog of Star Names | access-date=28 July 2016 }}
| url=https://www.iau.org/science/scientific_bodies/working_groups/280/
| title=IAU Working Group on Star Names (WGSN)
| publisher=International Astronomical Union
| access-date=22 May 2016 | postscript=. }}
| title=The multiple system ADS 9626: A quadruple star or an encounter of two binaries?
| display-authors=1 | last1=Kiyaeva | first1=O. V.
| last2=Zhuchkov | first2=R. Ya. | last3=Malogolovets | first3=E. V.
| last4=Orlov | first4=V. V. | last5=Glukhova | first5=A. V.
| last6=Balega | first6=Yu. Yu. | last7=Bikmaev | first7=I. F.
| journal=Astronomy Reports | postscript=.
| volume=58 | issue=11 | pages=835–848 | date=November 2014
| doi=10.1134/S106377291411002X | bibcode=2014ARep...58..835K | s2cid=122667185 }}
| last1=Malagnini | first1=M. L. | last2=Morossi | first2=C.
| title=Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars
| journal=Astronomy and Astrophysics Supplement Series
| volume=85 | issue=3 | pages=1015–1019 | date=November 1990
| bibcode=1990A&AS...85.1015M | postscript=. }}
}}
External links
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%205733 HR 5733]
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%205734 HR 5734]
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?CCDM%20J15245%2b3722A CCDM J15245+3722]
- [http://aladin.u-strasbg.fr/AladinPreview?-c=15+24+29.4278%2B37+22+37.800&ident=NSV++7063&submit=Aladin+previewer Image Mu Boötis]
{{Stars of Boötes|state=collapsed}}
{{DEFAULTSORT:Mu Bootis}}