Mu1 Scorpii

μ¹ Scorpii

Template:Location mark Location of μ1 Scorpii (circled)
Observation data Epoch J2000      Equinox J2000
Constellation	Scorpius
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	2.94 - 3.22
Characteristics
Spectral type	B1.5 V + B6.5 V
U−B Template:Engvar	−0.859
B−V Template:Engvar	−0.202
Variable type	β Lyr
Astrometry
Radial velocity (Rv)	−25 km/s
Proper motion (μ)	RA: −10.58 mas/yr Dec.: −22.06 mas/yr
Parallax (π)	6.51±0.91 mas
Distance	approx. Template:Rnd ly (approx. Template:Rnd pc)
Absolute magnitude (MV)	Template:Val
Orbit
Period (P)	1.44627 days
Semi-major axis (a)	Template:Solar radius
Eccentricity (e)	0.0
Inclination (i)	Template:Val°
Longitude of the node (Ω)	123.21Template:Rp°
Periastron epoch (T)	2412374.434 HJD
Details
μ1 Sco A
Mass	Template:Val Template:Solar mass
Radius	Template:Val Template:Solar radius
Surface gravity (log g)	Template:Val cgs
Temperature	Template:Val K
Rotational velocity (v sin i)	191.5 km/s
μ1 Sco B
Mass	Template:Val Template:Solar mass
Radius	Template:Val Template:Solar radius
Surface gravity (log g)	Template:Val cgs
Temperature	Template:Val K
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Rotational velocity (v sin i)	165.0 km/s
Other designations
Xamidimura, CD−37°11033, FK5 1439, HD 151890, HIP 82514, HR 6247, SAO 208102, WDS 16519-3803
Database references
SIMBAD	data

Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius. The combined apparent visual magnitude of the pair is about magnitude 3, making it one of the brighter members of Scorpius. Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). This system is a member of the Scorpius–Centaurus association, the nearest OB association of co-moving stars to the Sun.

The primary (Mu¹ Scorpii Aa) is formally named Xamidimura Template:IPAc-en, from the Khoekhoe 'the (two) eyes of the lion'.

Properties

File:Mu1ScoLightCurve.png

A light curve for Mu¹ Scorpii, plotted from TESS data

Mu¹ Scorpii is an eclipsing binary of the Beta Lyrae type. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. The two stars revolve each other along a circular orbit with the components separated by 12.9 times the Sun's radius. Due to occultation of each component by the other, the apparent magnitude of the system decreased by 0.3 and 0.4 magnitudes over the course of the binary's orbit, which takes 34 hours 42.6 minutes to complete.

The primary component is a B-type main sequence star with a stellar classification of B1.5 V. It has 8.3 times the mass of the Sun and 3.9 times the Sun's radius. The secondary is a smaller B-type main sequence star with a classification of about B6.5 V, having 3.6 times the Sun's mass and 4.6 times the radius of the Sun. The effective temperature of the outer atmosphere for each star is 24,000 K for the primary and 17,000 K for the secondary. At these temperatures, the two stars glow with a blue-white hue.

Nomenclature

μ¹ Scorpii (Latinised to Mu¹ Scorpii) is the system's Bayer designation. The designations of the primary as Mu¹ Scorpii Aa derives from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).

The pair of stars Mu¹ and Mu² Scorpii are known as the xami di mura 'eyes of the lion' by the Khoikhoi people of South Africa.

In 2016, the IAU organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. It approved the name Xamidimura for the component Mu¹ Scorpii Aa on 5 September 2017 (along with Pipirima for the partner of Mu¹ Scorpii) and it is now so included in the List of IAU-approved Star Names.

In Chinese, (), meaning Tail, refers to an asterism consisting of Mu¹ Scorpii, Epsilon Scorpii, Zeta¹ Scorpii and Zeta² Scorpii, Eta Scorpii, Theta Scorpii, Iota¹ Scorpii and Iota² Scorpii, Kappa Scorpii, Lambda Scorpii and Upsilon Scorpii. Consequently, the Chinese name for Mu¹ Scorpii itself is (), "the First Star of Tail".