PR Persei
Appearance
Location of PR Persei (circled) near the Double Cluster (north is down) | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Perseus |
| Right ascension | 02h 21m 42.41s[1] |
| Declination | +57° 51′ 46.1″[1] |
| Apparent magnitude (V) | 7.7 – 8.2[2] |
| Characteristics | |
| Evolutionary stage | Red supergiant |
| Spectral type | M1 Iab-Ib[2] |
| Variable type | LC[2] |
| Astrometry | |
| Radial velocity (Rv) | −45.9[1] km/s |
| Proper motion (μ) | RA: −0.857[1] mas/yr Dec.: −1.059[1] mas/yr |
| Parallax (π) | 0.3621±0.0239 mas[1] |
| Distance | 9,000 ± 600 ly (2,800 ± 200 pc) |
| Details | |
| Mass | 9.2[3] M☉ |
| Radius | 401[4] R☉ |
| Luminosity | 27,542[5] L☉ |
| Surface gravity (log g) | 0.89[6] cgs |
| Temperature | 3,715[5] K |
| Metallicity [Fe/H] | −0.22[6] dex |
| Other designations | |
| PR Persei, BD+57°550, HD 14404, HIP 10995, SAO 23234, TIC 348442493, TYC 3694-152-1, IRAS 02181+5738, 2MASS J02214241+5751460[7] | |
| Database references | |
| SIMBAD | data |
PR Persei (also known as HD 14404, HIP 10995, or BD+57 550) is a red supergiant star located in the constellation of Perseus in the northern celestial hemisphere. Classified as a variable star of spectral type M1-Iab-Ib, it exhibits mild brightness variations due to pulsations in its outer layers. It resides in the Milky Way galaxy, approximately 9,000 light-years from the Solar System. It can be seen near the Double Cluster of Perseus through a telescope or binoculars.
Charecterstics
[edit]
PR Persei is a cool, luminous red supergiant with a spectral type of M1 Iab-Ib, indicating an intermediate luminosity class between Iab and Ib supergiants.[9]
References
[edit]- ^ a b c d e f 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.
- ^ a b c "PR Persei". International Variable Star Index. AAVSO. Retrieved 2025-10-26.
- ^ Anders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardèvol, J.; Casamiquela, L.; Figueras, F.; Jiménez-Arranz, Ó.; Jordi, C.; Monguió, M.; Romero-Gómez, M.; Altamirano, D.; Antoja, T.; Assaad, R.; Cantat-Gaudin, T.; Castro-Ginard, A.; Enke, H.; Girardi, L.; Guiglion, G.; Khan, S.; Luri, X.; Miglio, A.; Minchev, I.; Ramos, P.; Santiago, B. X.; Steinmetz, M. (2022). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G = 18.5". Astronomy and Astrophysics. 658: A91. arXiv:2111.01860. Bibcode:2022A&A...658A..91A. doi:10.1051/0004-6361/202142369.
- ^ Fetherolf, Tara; Pepper, Joshua; Simpson, Emilie; Kane, Stephen R.; Močnik, Teo; English, John Edward; Antoci, Victoria; Huber, Daniel; Jenkins, Jon M.; Stassun, Keivan; Twicken, Joseph D.; Vanderspek, Roland; Winn, Joshua N. (2023). "Variability Catalog of Stars Observed during the TESS Prime Mission". The Astrophysical Journal Supplement Series. 268 (1): 4. arXiv:2208.11721. Bibcode:2023ApJS..268....4F. doi:10.3847/1538-4365/acdee5.
- ^ a b Dorn-Wallenstein, Trevor Z.; Levesque, Emily M.; Neugent, Kathryn F.; Davenport, James R. A.; Morris, Brett M.; Gootkin, Keyan (2020). "Short-term Variability of Evolved Massive Stars with TESS. II. A New Class of Cool, Pulsating Supergiants". The Astrophysical Journal. 902 (1): 24. arXiv:2008.11723. Bibcode:2020ApJ...902...24D. doi:10.3847/1538-4357/abb318.
- ^ a b Huson, Dylan; Cowan, Indiana; Sizemore, Logan; Kounkel, Marina; Hutchinson, Brian (2025). "Gaia Net: Toward Robust Spectroscopic Parameters of Stars of all Evolutionary Stages". The Astrophysical Journal. 984 (1): 58. arXiv:2503.02958. Bibcode:2025ApJ...984...58H. doi:10.3847/1538-4357/adc2fa.
- ^ "PR Persei". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2025-10-15.
- ^ EAS (1997). "The HIPPARCOS and TYCHO catalogues". Astrometric and Photometric Star Catalogues Derived from the ESA Hipparcos Space Astrometry Mission. ESA SP Series. 1200. Noordwijk, Netherlands: ESA Publications Division. Bibcode:1997HIP...C......0E. ISBN 9290923997. Retrieved 26 October 2025.
- ^ Dorn-Wallenstein, Trevor Z.; Levesque, Emily M.; Neugent, Kathryn F.; Davenport, James R. A.; Morris, Brett M.; Gootkin, Keyan (2020-10-01). "Short-term Variability of Evolved Massive Stars with TESS. II. A New Class of Cool, Pulsating Supergiants". The Astrophysical Journal. 902 (1): 24. arXiv:2008.11723. Bibcode:2020ApJ...902...24D. doi:10.3847/1538-4357/abb318. ISSN 0004-637X.