Epsilon Coronae Borealis

Epsilon Coronae Borealis, Latinized from ε Coronae Borealis, is a multiple star system in the constellation Corona Borealis located around 230 light-years from the Solar System. It shines with a combined apparent magnitude of 4.13, meaning it is visible to the unaided eye in all night skies except those brightly lit in inner city locations. It is an orange giant around 1.7 times as massive as the Sun of spectral type K2III, which has exhausted its core fuel supply of hydrogen and swollen to 21 times the Sun's diameter and 151 times its luminosity. That is, Epsilon Coronae Borealis's diameter is about one-quarter of Mercury's orbit. Its surface temperature has been calculated to be 4365 ± 9 K, or 4406 ± 15 K. It is thought to be around 1.74 billion years old.

ε Coronae Borealis
Location of ε Coronae Borealis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Corona Borealis
Right ascension 15h 57m 35.25147s
Declination +26° 52 40.3635
Apparent magnitude (V) 4.13
Characteristics
Spectral type K2 III
U−B color index +1.28
B−V color index +1.235
Astrometry
Radial velocity (Rv)–32.42 km/s
Proper motion (μ) RA: –77.07 mas/yr
Dec.: –60.61 mas/yr
Parallax (π)13.4922 ± 0.1023 mas
Distance242 ± 2 ly
(74.1 ± 0.6 pc)
Absolute magnitude (MV)−0.02
Details
Mass1.44±0.18 M
Radius21 R
Luminosity (bolometric)151 L
Surface gravity (log g)1.94±0.15 cgs
Temperature4,365±28 K
Metallicity [Fe/H]−0.22±0.03 dex
Rotational velocity (v sin i)2.4 km/s
Age4.13 Gyr
Other designations
13 Coronae Borealis, BD+27°2558, HD 143107, HIP 78159, HR 5947, SAO 84098, 2MASS J15573523+2652400
Database references
SIMBADdata

Epsilon Coronae Borealis B is a companion star thought to be an orange dwarf of spectral types K3V to K9V that orbits at a distance of 135 astronomical units, completing one orbit every 900 years.

A faint (magnitude 11.5) star, 1.5 arc minutes away, has been called Epsilon Coronae Borealis C although it is only close by line of sight and is unrelated to the system.

Epsilon Coronae Borealis lies one degree north of (and is used as a guide for) the variable T Coronae Borealis.

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