Beta Ophiuchi

Beta Ophiuchi

Template:Location mark Location of β Ophiuchi (circled)
Observation data Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation	Ophiuchus
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	2.749 (2.75 to 2.77)
Characteristics
Spectral type	K2 III
U−B Template:Engvar	+1.253
B−V Template:Engvar	+1.170
Astrometry
Radial velocity (Rv)	−12.53 km/s
Proper motion (μ)	RA: Template:Val mas/yr Dec.: Template:Val mas/yr
Parallax (π)	39.2284±0.2027 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	+0.77 ± 0.04
Details
Mass	Template:ValTemplate:SndTemplate:Val Template:Solar mass
Radius	Template:Val Template:Solar radius
Luminosity	Template:Val Template:Solar luminosity
Surface gravity (log g)	Template:Val cgs
Temperature	Template:Val K
Metallicity [Fe/H]	Template:Val dex
Rotational velocity (v sin i)	5.4 km/s
Age	Template:Val Gyr
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBAD	data

Beta Ophiuchi or β Ophiuchi, also named Cebalrai Template:IPAc-en, is a star in the equatorial constellation of Ophiuchus. The apparent visual magnitude of this star is 2.7, which is readily visible to the naked eye even from urban skies. The distance to this star can be estimated using parallax measurements, yielding a value of Template:Convert from the Sun.

Nomenclature

β Ophiuchi (Latinised to Beta Ophiuchi) is the star's Bayer designation.

It bore the traditional names Cebalrai, Celbalrai, Cheleb and Kelb Alrai (or sometimes just Alrai), all derived from the Arabic كلب الراعي kalb al-rā‘ī "the shepherd's dog". 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 Cebalrai for this star on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.

Namesake

USS Cheleb (AK-138) was a United States Navy Crater class cargo ship named after the star.

Properties

This is a giant star with a stellar classification of K2 III. Although it is only 2.75 billion years old, 60% of the solar age, it has reached a stage in its evolution where the atmosphere has expanded to about 12 times the Sun's radius and is radiating 58 times the luminosity of the Sun. Its outer envelope is relatively cool with an effective temperature of 4,559 K, giving it the orange hue typical of K-type stars. Like some other K-type giants, β Ophiuchi has been found to vary very slightly (0.02 magnitudes) in brightness.^,

Cebalrai is a member of the thin disk population. It is following a low eccentricity orbit through the Milky Way galaxy that carries it between a distance of Template:Convert from the Galactic Center and up to Template:Convert above or below the galactic plane.

Radial velocity variations with a period of 142 days are likely explained by periodic radial pulsations caused by intrinsic stellar variability.