Epsilon Coronae Borealis
| 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 |
| Distance | 242 ± 2 ly (74.1 ± 0.6 pc) |
| Absolute magnitude (MV) | −0.02 |
| Details | |
| Mass | 1.37±0.24 M☉ |
| Radius | 21.87+0.98 −0.99 R☉ |
| Luminosity (bolometric) | 162.9±9.4 L☉ |
| Surface gravity (log g) | 1.94±0.15 cgs |
| Temperature | 4,408±109 K |
| Metallicity [Fe/H] | −0.22±0.03 dex |
| Rotational velocity (v sin i) | 2.4 km/s |
| Age | 3.24±1.81 Gyr |
| Other designations | |
| 13 Coronae Borealis, BD+27°2558, HD 143107, HIP 78159, HR 5947, SAO 84098, 2MASS J15573523+2652400 | |
| Database references | |
| SIMBAD | data |
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.
This star has a stellar spectrum matching the class K2III, which indicate it is a giant star that exhausted its hydrogen supply at its core and evolved. Being 40% more massive than the Sun and 3.2 billion years old, it expanded to over 20 times the Sun's size and cooled to an effective temperature of 4,408 K. That is, Epsilon Coronae Borealis's diameter is about one-quarter of Mercury's orbit. The star radiates with 160 times the Sun's luminosity.
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.