Pi Coronae Borealis
  | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Corona Borealis[1] |
| Right ascension | 15h 43m 59.299s[2] |
| Declination | +32° 30′ 56.901″[2] |
| Apparent magnitude (V) | 5.578[3] |
| Characteristics | |
| Evolutionary stage | red clump[4] |
| Spectral type | G9 III:[3] or K0 III[5] |
| B−V color index | 1.074[6] |
| Astrometry | |
| Radial velocity (Rv) | −4.94±0.51[6] km/s |
| Proper motion (μ) | RA: −30.287 mas/yr[2] Dec.: −9.363 mas/yr[2] |
| Parallax (π) | 12.5965±0.0411 mas[2] |
| Distance | 258.9 ± 0.8 ly (79.4 ± 0.3 pc) |
| Absolute magnitude (MV) | +1.21[1] |
| Details[6] | |
| Mass | 1.61[3] M☉ |
| Radius | 10 R☉ |
| Luminosity | 39 L☉ |
| Surface gravity (log g) | 2.7 cgs |
| Temperature | 4,667±5 K |
| Metallicity [Fe/H] | −0.15 dex |
| Rotational velocity (v sin i) | 3.5 km/s |
| Age | 4.6[3] Gyr |
| Other designations | |
| Stephanos, π CrB, 9 CrB, BD+32°2621, FK5 3249, GC 21161, HD 140716, HIP 77048, HR 5855, SAO 64870[7] | |
| Database references | |
| SIMBAD | data |
Pi Coronae Borealis is a solitary,[8] orange-hued star in the northern constellation of Corona Borealis. It has the proper name Stephanos;[9] Pi Coronae Borealis is its Bayer designation, which is Latinized from π Coronae Borealis and abbreviated Pi CrB or π CrB. The star has an apparent visual magnitude of 5.58,[3] which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 12.60 mas as measured from Earth,[2] it is located at a distance of about 258.9 light-years (79.4 pc) from the Sun. The star is moving closer to the Sun with a radial velocity of −5 km/s.[6] It is most likely (98% chance) a member of the thin disk population.[4]
This is an evolved G-type giant star with a stellar classification of G9 III:, where the ':' indicates some uncertainty about the classification. (Bartkevicius and Lazauskaite (1997) classify it as K0 III.)[5] The star has 1.61[3] times the mass of the Sun and has expanded to about 10 times the Sun's radius. The abundance of iron is lower than in the Sun: the star is considered metal deficient.[5] It is a red clump giant, fusing helium in its core. It is around 4.6 billion years old and is radiating 39 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,667 K.
Stephanos (Στέφανος), the wreath, is the ancient Greek name of Corona Borealis. The IAU Working Group on Star Names adopted the name Stephanos for this star on 14 May 2026.[9]
References
- 1 2 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 5 6 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 88, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
- 1 2 Soubiran, C.; et al. (2008), "Vertical distribution of Galactic disk stars. IV. AMR and AVR from clump giants", Astronomy and Astrophysics, 480 (1): 91–101, arXiv:0712.1370, Bibcode:2008A&A...480...91S, doi:10.1051/0004-6361:20078788, S2CID 16602121.
- 1 2 3 Bartkevicius, A.; Lazauskaite, R. (December 1997), "Classification of Population II Stars in the Vilnius Photometric System. II. Results", Baltic Astronomy, 6 (4): 499–572, Bibcode:1997BaltA...6..499B, doi:10.1515/astro-1997-0402.
- 1 2 3 4 Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.
- ↑ "pi. CrB". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-04-30.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- 1 2 IAU Catalog of Star Names, retrieved 18 May 2026.
