Epsilon Coronae Australis

Epsilon Coronae Australis (ε CrA), is a star system located in the constellation Corona Australis. Varying in brightness between apparent magnitudes of 4.74 to 5 over 14 hours, it is the brightest W Ursae Majoris variable (low mass contact binary) in the night sky.

Epsilon Coronae Australis

A light curve for Epsilon Coronae Australis plotted from TESS data
Observation data
Epoch J2000      Equinox J2000
Constellation Corona Australis
Right ascension 18h 58m 43.37714s
Declination −37° 06 26.4865
Apparent magnitude (V) +4.75
Characteristics
Spectral type F4V Fe-0.8
U−B color index +0.01
B−V color index +0.39
Variable type W UMa
Astrometry
Radial velocity (Rv)57.90 ± 1.2 km/s
Proper motion (μ) RA: 132.40 mas/yr
Dec.: 110.62 mas/yr
Parallax (π)33.13 ± 0.33 mas
Distance98.4 ± 1.0 ly
(30.2 ± 0.3 pc)
Absolute magnitude (MV)2.21
Orbit
Period (P)0.59143357 ± 0.00000016 d
Semi-major axis (a)3.795 ± 0.052 R
Eccentricity (e)0
Inclination (i)73.05 ± 0.16°
Longitude of the node (Ω)2.0113 ± 0.0033°
Periastron epoch (T)JD 2442296.95907 ± 0.0070
Details
ε CrA A
Mass1.9 M
Radius2.167 R
Temperature6481 ± 20 K
Rotational velocity (v sin i)148.5 km/s
ε CrA B
Mass0.24 M
Radius0.869 R
Temperature5939 ± 19 K
Other designations
ε CrA, CD−37°13001, CPD−37°8433, HD 175813, HIP 93174, HR 7152, SAO 210781
Database references
SIMBADdata
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