Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Borealis |
Right ascension | 16h 22m 21.42283s[1] |
Declination | +33° 47′ 56.5880″[1] |
Apparent magnitude (V) | 5.20[2] |
Characteristics | |
Spectral type | M2 III[3] |
B−V color index | 1.64[3] |
Astrometry | |
Radial velocity (Rv) | −13.01±0.12[1] km/s |
Proper motion (μ) | RA: +4.756 mas/yr[1] Dec.: −38.223 mas/yr[1] |
Parallax (π) | 5.0245 ± 0.0843 mas[1] |
Distance | 650 ± 10 ly (199 ± 3 pc) |
Absolute magnitude (MV) | −1.19[3] |
Details[4] | |
Radius | 80.78±2.88 R☉ |
Luminosity | 1,257±70 L☉ |
Temperature | 3,828 K |
Other designations | |
Database references | |
SIMBAD | data |
Nu1 Coronae Borealis is a solitary,[6] red-hued star located in the northern constellation of Corona Borealis. It is faintly visible to the naked eye, having an apparent visual magnitude of 5.20.[2] Based upon an annual parallax shift of 5.02 mas,[1] it is located roughly 650 light years from the Sun. At its distance, the visual magnitude is diminished by an extinction of 0.1 due to interstellar dust.[7] This object is drifting closer with a radial velocity of −13 km/s.[1]
This is an evolved red giant star with a stellar classification of M2 III.[3] It is a variable star of uncertain type, showing a change in brightness with an amplitude of 0.0114 magnitude and a frequency of 0.22675 cycles per day, or 4.41 days/cycle.[8] It has about 81 times the Sun's radius and is radiating nearly 1,300 times the Sun's luminosity from its photosphere at an effective temperature of 3,828 K.[4]
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