Mu1 Boötis

Binary star in the northern constellation of Boötes From Wikipedia, the free encyclopedia

Mu1 Boötis is a binary star in the northern constellation of Boötes. Its name is a Bayer designation that is Latinized from μ1 Boötis, and abbreviated Mu1 Boo or μ1 Boo. This system had the traditional name Alkalurops, pronounced /ælkəˈljʊərɒps/.[8] Based on parallax measurements, the system is located at a distance of 123 light-years.

Right ascension15h 24m 29.43147s[1]
Declination+37° 22 37.7613[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
Mu1 Boötis
Diagram showing star positions and boundaries of the Boötes constellation and its surroundings
Diagram showing star positions and boundaries of the Boötes constellation and its surroundings

Location of μ1 Boötis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes
Right ascension 15h 24m 29.43147s[1]
Declination +37° 22 37.7613[1]
Apparent magnitude (V) 4.31[2]
Characteristics
Spectral type F2IV[3]
U−B color index +0.06[4]
B−V color index +0.31[4]
R−I color index 0.15
Astrometry
Radial velocity (Rv)−8.60±0.3[5] km/s
Proper motion (μ) RA: −149.928[1] mas/yr
Dec.: +89.573[1] mas/yr
Parallax (π)26.5759±0.7871 mas[1]
Distance123 ± 4 ly
(38 ± 1 pc)
Absolute magnitude (MV)1.47[6]
Orbit[3]
PrimaryAa
NameAb
Period (P)3.75 years
Semi-major axis (a)0.099″
Eccentricity (e)0.270
Inclination (i)129.7°
Longitude of the node (Ω)129.4°
Periastron epoch (T)1006.33
Argument of periastron (ω)
(secondary)
43.5°
Details
Aa
Mass1.6[3] M
Radius1.9[2] R
Luminosity20[7] L
Surface gravity (log g)3.4[3] cgs
Temperature7,000[3] K
Rotational velocity (v sin i)89[3] km/s
Ab
Mass1.5[3] M
Surface gravity (log g)3.6[3] cgs
Temperature7,000[3] K
Rotational velocity (v sin i)40[3] km/s
Other designations
Alkalurops, Inkalunis, Icalurus, Clava, Venabulum, μ Boo, 51 Boötis A, BD+37°2636, FK5 568, GC 20724, GJ 3903, HD 137391, HIP 75411, HR 5733, SAO 64686, ADS 9626, CCDM 15245+3722
Database references
SIMBADdata
Close

The components of the system have an angular separation of 0.10.[9] They form a spectroscopic binary system with an orbital period of 3.75 years.[3] The visible component is a yellow-white F-type subgiant with an apparent magnitude of +4.31.

The system μ2 Boötis, separated by 109", makes an optical double with μ1, and even has a similar distance from Earth and comparable proper motions, but has a substantially different metallicity, and therefore is not a gravitationally bound companion.[3]

Nomenclature

μ1 Boötis (Latinised to Mu1 Boötis) is the star's Bayer designation.

The system's traditional name Alkalurops is from the Greek καλαύροψ kalaurops "a herdsman's crook or staff", with the Arabic prefix attached.[10] It has also been known as Inkalunis (from the Alfonsine tables), Clava (Latin 'the club') and Venabulum (Latin 'a hunting spear').[11] In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[12] 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.[8]

It is known as 七公六, Qī Gōng liù (the Sixth Star of the Seven Excellencies) in Chinese.[13]

References

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