Omicron Coronae Borealis
  | |
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Corona Borealis[1] |
| Right ascension | 15h 20m 08.559s[2] |
| Declination | +29° 36′ 58.35″[2] |
| Apparent magnitude (V) | +5.53[3] |
| Characteristics | |
| Evolutionary stage | red clump[4] |
| Spectral type | K0 III[5] |
| U−B color index | +0.786[3] |
| B−V color index | +1.009[3] |
| Astrometry | |
| Radial velocity (Rv) | −54.15±0.20[6] km/s |
| Proper motion (μ) | RA: −117.972 mas/yr[2] Dec.: −42.922 mas/yr[2] |
| Parallax (π) | 11.9113±0.0572 mas[2] |
| Distance | 274 ± 1 ly (84.0 ± 0.4 pc) |
| Absolute magnitude (MV) | +0.92[1] |
| Details[6] | |
| Mass | 1.07±0.19 M☉ |
| Radius | 10.13±0.40 R☉ |
| Luminosity | 50.1 L☉ |
| Surface gravity (log g) | 2.70±0.06 cgs |
| Temperature | 4,812±13 K |
| Metallicity [Fe/H] | −0.24±0.01 dex |
| Rotational velocity (v sin i) | 0.47±0.61 km/s |
| Age | 5.54±2.79 Gyr |
| Other designations | |
| o CrB, 1 Coronae Borealis, NSV 7032, BD+30°2647, GC 20619, HD 136512, HIP 75049, HR 5709, SAO 83768, WDS J15201+2937A, 2MASS J15200853+2936584[7] | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
Omicron Coronae Borealis is a star in the northern constellation of Corona Borealis. Its name is a Bayer designation that is Latinized from o Coronae Borealis, and is abbreviated Omicron CrB or o CrB. This is a faint star but visible to the naked eye on a dark night with an apparent visual magnitude of +5.53.[3] The annual parallax shift of the star as seen from Earth is 11.91 mas,[2] which provides a distance estimate of approximately 274 light-years (84 pc). It is moving closer to the Sun with a radial velocity of −54 km/s.[6]
Based upon the spectrum of this star, it has a stellar classification of K0 III.[1] This indicates this is an evolved K-type giant star that has exhausted the hydrogen at its core and has left the main sequence. It is a red clump star,[4] which means it is now generating energy through helium fusion at its core. This star has 107% of the mass of the Sun and has expanded to over ten times the Sun's radius. It is radiating 50 times the Sun's luminosity from its expanded photosphere at an effective temperature of 4,812 K.[4]
Planetary system
Omicron Coronae Borealis has one confirmed planet, believed to be, along with HD 100655 b, one of the two least massive planets known around red clump giants.[4] The planet was detected by measuring changes in radial velocity of the host star caused by gravitational perturbation of the orbiting object. It is orbiting with a period of 188 days, at a semimajor axis 83% of the mean separation between the Earth and the Sun, and an eccentricity of 0.19.[4]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination (°) |
Radius |
|---|---|---|---|---|---|---|
| b | >1.5 MJ | 0.83 | 187.83 ± 0.54 | 0.191 ± 0.085 | — | — |
References
- 1 2 3 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015 XHIP record for this object at VizieR.
- 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023), "Gaia Data Release 3. Summary of the content and survey properties", Astronomy and Astrophysics, 674: A1, arXiv:2208.00211, Bibcode:2023A&A...674A...1G, doi:10.1051/0004-6361/202243940, S2CID 244398875 Gaia DR3 record for this source at VizieR.
- 1 2 3 4 Jennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants", Monthly Notices of the Royal Astronomical Society, 172 (3): 667–679, Bibcode:1975MNRAS.172..667J, doi:10.1093/mnras/172.3.667.
- 1 2 3 4 5 6 Sato, Bun'ei; et al. (2012), "Substellar Companions to Seven Evolved Intermediate-Mass Stars", Publications of the Astronomical Society of Japan, 64 (6), 135, arXiv:1207.3141, Bibcode:2012PASJ...64..135S, doi:10.1093/pasj/64.6.135, S2CID 119197073.
- ↑ Roman, Nancy G. (December 1955), "A Catalogue of High-Velocity Stars", The Astrophysical Journal Supplement Series, 2: 195, Bibcode:1955ApJS....2..195R, doi:10.1086/190021, eISSN 1538-4365, ISSN 0067-0049, S2CID 123076474.
- 1 2 3 Jofré, E; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy & Astrophysics, 574: A50, arXiv:1410.6422, Bibcode:2015A&A...574A..50J, doi:10.1051/0004-6361/201424474, S2CID 53666931, A50.
- ↑ "omi CrB", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2026-07-14.
