Epsilon Coronae Australis

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) 4.83±0.02
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
(2.39 + 4.98)
Orbit
Period (P)0.59145447(30) days
Semi-major axis (a)3.82±0.02 R
Eccentricity (e)0
Inclination (i)74.02±0.14°
Longitude of the node (Ω)2.0113 ± 0.0033°
Periastron epoch (T)HJD 3966.6892(0.0696)
Semi-amplitude (K1)
(primary)
36.40±0.05 km/s
Semi-amplitude (K2)
(secondary)
273.70±0.05 km/s
Details
ε CrA A
Mass1.89±0.16 M
Radius2.14±0.09 R
Luminosity8.9±1.8 L
Temperature6,820±200 K
Rotational velocity (v sin i)148.5 km/s
Age2.83±0.28 Gyr
ε CrA B
Mass0.25±0.04 M
Radius0.84±0.04 R
Luminosity0.85±0.14 L
Surface gravity (log g)3.99±0.03 cgs
Temperature6,050±100 K
Age2.83±0.28 Gyr
Other designations
ε CrA, CD−37°13001, CPD−37°8433, HD 175813, HIP 93174, HR 7152, SAO 210781
Database references
SIMBADdata

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.