Beta Eridani

β Eridani

Template:Location mark Location of β Eridani (circled)
Observation data Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation	Eridanus
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	2.796
Characteristics
Spectral type	A3 III var
U−B Template:Engvar	+0.124
B−V Template:Engvar	+0.110
R−I Template:Engvar	+0.08
Astrometry
Radial velocity (Rv)	−3.6 km/s
Proper motion (μ)	RA: −82.82 mas/yr Dec.: −75.39 mas/yr
Parallax (π)	36.2456±0.3575 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	+0.59
Details
Mass	2.55 Template:Solar mass
Radius	Template:Solar radius
Luminosity	45 Template:Solar luminosity
Surface gravity (log g)	3.58 cgs
Temperature	K
Metallicity [Fe/H]	+ dex
Rotational velocity (v sin i)	196 km/s
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Cursa/Kursa, Dhalim, β Eri, Beta Eridani, Beta Eri, 67 Eridani, 67 Eri, BD−05 1162, CCDM J05079-0506A, FK5 188, GC 6274, GJ 9175, HD 33111, HIP 23875, HR 1666, IDS 05030-0513 A, PPM 187729, SAO 131794, WDS 05078-0505A.
Database references
SIMBAD	data

Beta Eridani (β Eridani, abbreviated Beta Eri, β Eri), formally named Cursa Template:IPAc-en, is the second-brightest star in the constellation of Eridanus, located in the northeast end of this constellation near the shared border with Orion. The apparent visual magnitude of this star is 2.796, so it can be viewed with the naked eye in dark skies. Parallax measurements yield an estimated distance of about from the Earth.

Nomenclature

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β Eridani is the second-brightest star, above center. The brightest star, towards the lower left (southeast), is Rigel. In between is the reflection nebula IC 2118.

Beta Eridani is the star's Bayer designation. It has the traditional name Cursa derived from , "the Chair (or "Footstool") of the Central One". This is the name of the star association consisting of this star along with Lambda Eridani, Psi Eridani and Tau Orionis. According to a NASA catalogue of stars, was the title of three stars: β Eri is Cursa, Psi Eridani , and Lambda Eridani (excluding Tau Orionis). In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Cursa for this star.

In Chinese, (), "the Jade Well", refers to an asterism consisting of β Eridani, λ Eridani, ψ Eridani and τ Orionis. Consequently, the Chinese name for β Eridani itself is "the third star of Jade Well" ( ). In older texts, was also spelt .

Properties

β Eridani has a spectral type of A3 III, with the luminosity class III indicating that this is a giant star which has consumed the hydrogen at its core and evolved away from the main sequence. The effective temperature of the outer envelope is about 8,360 K, which gives the star a white hue typical of A-type stars. The projected rotational velocity is a rapid 196 km s⁻¹, compared to 2 km s⁻¹ along the Sun's equator. The star is known to vary in apparent visual magnitude, ranging between 2.72 and 2.80. A particularly strong flare-up was reported in 1985.

The location and trajectory of this star suggest that it is a member of the Ursa Major supergroup, an association of stars that share a common origin and motion through space. However, its photometric properties indicate that it may instead be an interloper. Beta Eridani has an optical companion star with an apparent magnitude 10.90 at an angular separation of 120 arcseconds and a position angle of 148°. It has the catalogue identifier CCDM J05079-0506B.