55 Persei is a single,[9] blue-white hued star in the northern constellation Perseus. It is faintly visible to the naked eye under good seeing conditions, having an apparent visual magnitude of 5.73.[2] Based upon an annual parallax shift of 8.50±0.38 mas[4] as seen from Earth's orbit, the star is located about 380 light years from the Sun. At that distance, the visual magnitude is diminished by an extinction of 0.39[5] due to interstellar dust.
 55 Persei in optical light | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Perseus |
| Right ascension | 04h 24m 29.1556s[1] |
| Declination | 34° 07′ 50.728″[1] |
| Apparent magnitude (V) | 5.73[2] |
| Characteristics | |
| Spectral type | B8 V[2] |
| B−V color index | −0.054±0.004[2] |
| Astrometry | |
| Radial velocity (Rv) | 8.5±3.5[3] km/s |
| Proper motion (μ) | RA: 21.092 [1] mas/yr Dec.: −34.137 [1] mas/yr |
| Parallax (π) | 8.50 ± 0.38 mas[4] |
| Distance | 380 ± 20 ly (118 ± 5 pc) |
| Absolute magnitude (MV) | −0.39[5] |
| Details | |
| Mass | 3.44±0.07[6] M☉ |
| Radius | 3.0[7] R☉ |
| Luminosity | 193 24 −21[6] L☉ |
| Temperature | 12,246±85[6] K |
| Rotational velocity (v sin i) | 288[6] km/s |
| Age | 197[5] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
This is a B-type main-sequence star with a stellar classification of B8 V;[2] a massive star that is generating energy through hydrogen fusion at its core. It has 3.44[6] times the mass of the Sun and about 3[7] times the Sun's radius. The star is about 197[5] million years old and is spinning rapidly with a projected rotational velocity of 288 km/s.[6] It is radiating roughly 193[6] times the Sun's luminosity from its photosphere at an effective temperature of 12,246 K.[6]
References
edit- ^ a b c d Brown, A. G. A; et al. (2016), "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties", Astronomy and Astrophysics, 595, A2, arXiv:1609.04172, Bibcode:2016A&A...595A...2G, doi:10.1051/0004-6361/201629512, S2CID 1828208.
- ^ a b c d e 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, S2CID 119257644.
- ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 86351347, A61.
- ^ a b van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.653-664&rft.date=2007&rft_id=info:arxiv/0708.1752&rft_id=https://api.semanticscholar.org/CorpusID:18759600#id-name=S2CID&rft_id=info:doi/10.1051/0004-6361:20078357&rft_id=info:bibcode/2007A&A...474..653V&rft.aulast=van Leeuwen&rft.aufirst=F.&rfr_id=info:sid/en.wikipedia.org:55 Persei" class="Z3988">
- ^ a b c d Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.694-706&rft.date=2012-11&rft_id=info:arxiv/1606.09028&rft_id=https://api.semanticscholar.org/CorpusID:119108982#id-name=S2CID&rft_id=info:doi/10.1134/S1063773712110035&rft_id=info:bibcode/2012AstL...38..694G&rft.aulast=Gontcharov&rft.aufirst=G. A.&rfr_id=info:sid/en.wikipedia.org:55 Persei" class="Z3988">
- ^ a b c d e f g h Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (2) (3rd ed.): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.521-524&rft.date=2001-02&rft_id=info:arxiv/astro-ph/0012289&rft_id=https://api.semanticscholar.org/CorpusID:425754#id-name=S2CID&rft_id=info:doi/10.1051/0004-6361:20000451&rft_id=info:bibcode/2001A&A...367..521P&rft.aulast=Pasinetti Fracassini&rft.aufirst=L. E.&rft.au=Pastori, L.&rft.au=Covino, S.&rft.au=Pozzi, A.&rfr_id=info:sid/en.wikipedia.org:55 Persei" class="Z3988">
- ^ "55 Per". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-03-08.
- ^ 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 14878976.869-879&rft.date=2008-09&rft_id=info:arxiv/0806.2878&rft_id=https://api.semanticscholar.org/CorpusID:14878976#id-name=S2CID&rft_id=info:doi/10.1111/j.1365-2966.2008.13596.x&rft_id=info:bibcode/2008MNRAS.389..869E&rft.aulast=Eggleton&rft.aufirst=P. P.&rft.au=Tokovinin, A. A.&rfr_id=info:sid/en.wikipedia.org:55 Persei" class="Z3988">