101 Piscium
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Pisces |
Right ascension | 01h 35m 46.44226s[1] |
Declination | +14° 39′ 41.1144″[1] |
Apparent magnitude (V) | 6.23[2] |
Characteristics | |
Spectral type | B9.5 III[3] |
U−B color index | −0.151[4] |
B−V color index | −0.036±0.005[2] |
Astrometry | |
Radial velocity (Rv) | −10.10[5] km/s |
Proper motion (μ) | RA: +3.287[1] mas/yr Dec.: −8.052[1] mas/yr |
Parallax (π) | 2.3343 ± 0.0663 mas[1] |
Distance | 1,400 ± 40 ly (430 ± 10 pc) |
Absolute magnitude (MV) | −2.07[2] |
Details | |
Mass | 4.53±0.51[6] M☉ |
Radius | 3.6[7] R☉ |
Luminosity | 1,037+523 −347[6] L☉ |
Surface gravity (log g) | 2.907±0.028[8] cgs |
Temperature | 10,471+49 −48[6] K |
Rotational velocity (v sin i) | 246[6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
101 Piscium is a star in the zodiac constellation of Pisces,[9] located around 1,400 light years away from the Sun. This appears as a dim, blue-white hued star near the lower limit of visibility to the naked eye at an apparent visual magnitude of 6.23.[2] It is a suspected variable star with the designation NSV 559;[10] 101 Piscium is the Flamsteed designation. The star is moving closer to the Earth with a heliocentric radial velocity of −10 km/s.[5]
This object has a stellar classification of B9.5 III,[3] matching a giant star that has consumed the hydrogen at its core and is evolving away from the main sequence.[6] It is spinning rapidly with a projected rotational velocity of 246[6] km/s, compared to a critical velocity of 270 km/s.[8] The star has 4.5[6] times the mass of the Sun and about 3.6[7] times the Sun's radius. It is radiating around 1,000[6] times the luminosity of the Sun from its photosphere at an effective temperature of 10,471 K.[6]
References
[edit]- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d 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.
- ^ a b Cowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications". Astronomical Journal. 74: 375–406. Bibcode:1969AJ.....74..375C. doi:10.1086/110819.
- ^ Gutierrez-Moreno, Adelina; et al. (1966). "A System of photometric standards". Publications of the Department of Astronomy University of Chile. 1. Publicaciones Universidad de Chile, Department de Astronomy: 1–17. Bibcode:1966PDAUC...1....1G.
- ^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
- ^ a b c d e f g h i Zorec, J.; et al. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and 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.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy and Astrophysics. 367 (Third ed.): 521–524. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID 425754.
- ^ a b Huang, W.; et al. (2010). "A Stellar Rotation Census of B Stars: From ZAMS to TAMS". The Astrophysical Journal. 722 (1): 605–619. arXiv:1008.1761. Bibcode:2010ApJ...722..605H. doi:10.1088/0004-637X/722/1/605. S2CID 118532653.
- ^ a b "35 Psc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-24.
- ^ Samus, N. N.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.