(Redirected from Gorgonea Secunda )
Star in the constellation Perseus
Pi Persei
Location of π Persei (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Perseus
Right ascension
02 58 45.66858
Declination
+39° 39′ 45.8212″
Apparent magnitude (V)
4.70
Characteristics
Spectral type
A2Vn
U−B color index
+0.12
B−V color index
+0.06
Astrometry Radial velocity (Rv )+14.2 km/s Proper motion (μ) RA: +26.224 mas /yr Dec.: −41.899 mas /yr Parallax (π)10.7797 ± 0.2794 mas Distance 303 ± 8 ly (93 ± 2 pc ) Absolute magnitude (MV )−0.21
Details Mass 2.07 M ☉ Radius 4.8 R ☉ Luminosity 170 L ☉ Surface gravity (log g )3.53 cgs Temperature 9,290 K Rotational velocity (v sin i )186 km/s Age 272 Myr
Other designations Gorgonea Secunda, π Per , 22 Persei , BD +39°681, FK5 2207, GC 3567, HD 18411, HIP 13879, HR 879, SAO 56047
Database references SIMBAD data
π Persei , Latinized as Pi Persei , is a single star in the northern constellation of Perseus . It has the traditional name Gorgonea Secunda /ɡɔːrɡəˈniːə sɪˈkʌndə/ , the second of three Gorgons in the mythology of the hero Perseus . This star has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.7. It is located at a distance of approximately 303 light years from the Sun based on parallax , and is moving further away with a radial velocity of +14 km/s.
This object is an A-type main-sequence star with a stellar classification of A2Vn, where the 'n' suffix indicates broad (nebulous) lines due to rapid rotation. It is spinning with a projected rotational velocity of 186 km/s, which is creating an equatorial bulge that is 6% wider than the polar radius. The star is 272 million years old with double the mass of the Sun . It has 4.8 times the Sun's radius and is radiating 170 times the luminosity of the Sun from its photosphere at an effective temperature of 9,290 K.
References
^ 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 .
^ Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues . 2237 . Bibcode :2002yCat.2237....0D .
^ Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars" . Astrophysical Journal Supplement . 99 : 135. Bibcode :1995ApJS...99..135A . doi :10.1086/192182 .
^ Wilson, R. E. (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication . Carnegie Institution for Science . Bibcode :1953GCRV..C......0W . ISBN 9780598216885 . LCCN 54001336 .
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 . Vizier catalog entry
^ David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal . 804 (2): 146. arXiv :1501.03154 . Bibcode :2015ApJ...804..146D . doi :10.1088/0004-637X/804/2/146 . S2CID 33401607 .
Vizier catalog entry
^ Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics . 352 : 555–562. arXiv :astro-ph/9911002 . Bibcode :1999A&A...352..555A . Vizier catalog entry
^ Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars". Astronomy & Astrophysics . 537 : A120. arXiv :1201.2052 . Bibcode :2012A&A...537A.120Z . doi :10.1051/0004-6361/201117691 . S2CID 55586789 . Vizier catalog entry
Allen, Richard Hinckley (1899). Star-names and Their Meanings . G.E. Stechert. p. 334 .
"pi Per" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-10-12.
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 .
Kaler, James B. (November 21, 2014). "Pi Persei" . STARS . Retrieved 2019-10-12.
van Belle, Gerard T. (March 2012). "Interferometric observations of rapidly rotating stars". The Astronomy and Astrophysics Review . 20 (1): 51. arXiv :1204.2572 . Bibcode :2012A&ARv..20...51V . doi :10.1007/s00159-012-0051-2 . S2CID 119273474 .
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