World Library  
Flag as Inappropriate
Email this Article

Castor (star)

Article Id: WHEBN0000245159
Reproduction Date:

Title: Castor (star)  
Author: World Heritage Encyclopedia
Language: English
Subject: Gemini (constellation), Pollux (star), Punarvasu, Star system, Canis Minor
Publisher: World Heritage Encyclopedia

Castor (star)


Castor within the constellation Gemini
Observation data
Epoch J2000      Equinox J2000
Constellation Gemini
Right ascension 07h 34m 35.863s[1]
Declination +31° 53′ 17.79″[1]
Apparent magnitude (V) 1.93[1]
Right ascension 07h 34m 36.100s[1]
Declination +31° 53′ 18.57″[1]
Apparent magnitude (V) 2.97[1]
Right ascension 07h 34m 37.584s[1]
Declination +31° 53′ 17.8160″[1]
Apparent magnitude (V) 9.83[1]
Spectral type A1V + dM1e[2]
B−V color index +0.03[3]
Spectral type Am + dM1e[2]
B−V color index +0.04[3]
Spectral type dM1e + dM1e[2]
U−B color index +1.04[4]
B−V color index +1.49[4]
Variable type BY Dra[5]
Proper motion (μ) RA: –191.45[6] mas/yr
Dec.: –145.19[6] mas/yr
Parallax (π) 64.12 ± 3.75[6] mas
Distance 51 ± 3 ly
(15.6 ± 0.9 pc)
Radial velocity (Rv) +6.0[7] km/s
Absolute magnitude (MV) +0.986[3]
Radial velocity (Rv) –1.2[7] km/s
Absolute magnitude (MV) +1.886[3]
Radial velocity (Rv) +2.5[8] km/s
Absolute magnitude (MV) +8.950[9]
α Gem Aa
Mass 2.76[10] M
Radius 2.4[11] R
Surface gravity (log g) 4.2[11] cgs
Temperature 10,286[12] K
Metallicity [Fe/H] 0.98[12] dex
Rotational velocity (v sin i) 18[13] km/s
α Gem Ba
Mass 2.98[10] M
Radius 3.3[11] R
Surface gravity (log g) 4.0[11] cgs
Temperature 8,842[12] K
Metallicity [Fe/H] 0.45[12] dex
Rotational velocity (v sin i) 33[13] km/s
Mass 0.5992[9] M
Radius 0.6191[9] R
Luminosity 0.0733[9] L
Surface gravity (log g) 4.6317[9] cgs
Temperature 3,820[9] K
Metallicity [Fe/H] ~0.0[9] dex
Rotational velocity (v sin i) 37[9] km/s
Age 370[9] Myr
Primary α Gem A
Companion α Gem B
Period (P) 445[10] yr
Semi-major axis (a) 7.369"
Eccentricity (e) 0.360
Inclination (i) 112.9°
Longitude of the node (Ω) 41.7°
Periastron epoch (T) 2401950.650
Argument of periastron (ω)
Primary α Gem A1
Companion α Gem A2
Period (P) 9.2128 days
Eccentricity (e) 0.5
Periastron epoch (T) 2427543.938
Argument of periastron (ω)
Semi-amplitude (K1)
12.9 km/s
Primary α Gem B1
Companion α Gem B2
Period (P) 2.9283 days
Periastron epoch (T) 2427501.703
Argument of periastron (ω)
Semi-amplitude (K1)
31.9 km/s
Primary α Gem AB
Companion α Gem C
Period (P) 14,000 yr
Semi-amplitude (K1)
121.0 km/s
Semi-amplitude (K2)
119.0 km/s
Primary α Gem C1
Companion α Gem C2
Period (P) 0.814 days
Eccentricity (e) 0
Inclination (i) 86.29 ± 0.10°
Longitude of the node (Ω) 7.315°
Other designations
Castor, α Gem, 66 Gem, FK5 287, Gliese 278, HIP 36850, SAO 60198
A: BD+32°1581A, PLX 1785.00, HR 2891, HD 60179
B: BD+32°1581B, HR 2890, HD 60178
C: YY Gem, BD +32° 1582
Database references
SIMBAD Castor A data
SIMBAD Castor B data
SIMBAD Castor C data

Castor (α Gem, α Geminorum, Alpha Geminorum) is the second brightest star in the constellation Gemini and one of the brightest stars in the night sky. Although it has the Bayer designation "alpha", it is actually fainter than Beta Geminorum (Pollux).


  • The Castor System 1
  • Physical characteristics 2
  • Etymology and culture 3
  • References 4
  • External links 5

The Castor System

Castor A and B

Castor was recorded as a visual binary in 1718 by James Pound. It may have been resolved in 1678 by Cassini. The separation of the two stars has increased from 2" in 1907[15] to 7" in 1997.[14] The two stars form a visual double, with magnitudes of 1.9 and 3.0.

A third star is 73" distant from the main components.[14] It was discovered to vary in brightness with a regular period and was thought to be an eclipsing binary, but the variations are now considered to be due to areas of different brightness on the surface of one or both stars. It was given the variable star designation YY Geminorum.[9]

All three of the visual components are actually spectroscopic binaries and Castor is a complex multiple star system made up of six individual stars. Castor A and B both have orbits of a few days with a much fainter companion. The Castor C components orbit in less than a day. Castor C is believed to be in orbit around the bright pair, but with an extremely long period of several thousand years. [14]

The combined apparent magnitude of all six stars is +1.58.

Physical characteristics

Castor is 51 light years away from Earth, determined from its large annual parallax. The two brightest stars are both A-class main sequence stars, more massive and brighter than the sun. The properties of their red dwarf companions are difficult to determine, but are both thought to have less than half the mass of the sun.[14] The two red dwarfs of Castor C are almost identical, with masses around a half M and luminosities less than 10% of the sun.[9]

Castor B is an Am star, with particularly strong spectral lines of certain metals.

Castor C is a variable star, classified as a BY Dra type. BY Draconis variables are cool dwarf stars which vary as they rotate due to star spots or other variations in their photospheres.

All the red dwarfs in the Castor system have emissions lines in their spectra, and all are Flare stars.[11]

Etymology and culture

Castor and Pollux are the two "heavenly twin" stars that give the constellation Gemini (meaning twins in Latin) its name. The name Castor refers specifically to Castor, one of the twin sons of Zeus and Leda. The star was annotated by the Arabic description Al-Ras al-Taum al-Muqadim, which translates as the head of the foremost twin. In the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, this star was designated Aoul al Dzira, which was translated into Latin as Prima Brachii, meaning the first in the paw.[16]

In Chinese, 北河 (Běi Hé), meaning North River, refers to an asterism consisting of Castor, ρ Geminorum, and Pollux.[17] Consequently, Castor itself is known as 北河二 (Běi Hé èr, English: the Second Star of North River.)[18] The Chinese recognized Castor as Yin, which is, according to the Chinese, one of the two fundamental principles upon which all things depend.


  1. ^ a b c d e f g h i Fabricius, C.; et al. (March 2002), "The Tycho double star catalogue", Astronomy and Astrophysics 384: 180–189,  
  2. ^ a b c Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics 424 (2): 727–732.  
  3. ^ a b c d Barrado y Navascues, D. (1998). "The Castor moving group. The age of Fomalhaut and VEGA". Astronomy and Astrophysics 339: 831.  
  4. ^ a b 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: 0.  
  5. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007–2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S 1: 02025.  
  6. ^ a b c van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664,  
  7. ^ a b Evans, D. S. (1967), Batten, Alan Henry; Heard, John Frederick, eds., "Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30 held at the University of Toronto 20-24 June, 1966", Determination of Radial Velocities and their Applications (Academic Press, London) 30: 57,  
  8. ^ Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Washington (Washington: Carnegie Institution of Washington): 0,  
  9. ^ a b c d e f g h i j k l Torres, Guillermo; Ribas, Ignasi (2002). "Absolute Dimensions of the M‐Type Eclipsing Binary YY Geminorum (Castor C): A Challenge to Evolutionary Models in the Lower Main Sequence". The Astrophysical Journal 567 (2): 1140–1165.  
  10. ^ a b c Tokovinin, A. (September 2008), "Comparative statistics and origin of triple and quadruple stars", Monthly Notices of the Royal Astronomical Society 389 (2): 925–938,  
  11. ^ a b c d e Stelzer, B.; Burwitz, V. (May 2003), "Castor A and Castor B resolved in a simultaneous Chandra and XMM-Newton observation", Astronomy and Astrophysics 402 (2): 719–728,  
  12. ^ a b c d Smith, M. A. (April 1974), "Metallicism in border regions of the Am domain. III. Analysis of the hot stars Alpha Geminorum A and B and Theta Leonis", Astrophysical Journal 189: 101–111,  
  13. ^ a b Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682,  
  14. ^ a b c d e f g h Tokovinin, A. A. (1997). "MSC - a catalogue of physical multiple stars". Astronomy and Astrophysics Supplement Series 124 (1): 75–84.  
  15. ^ Heintz, W. D. (1980). "Micrometer Observations of Double Stars and New Pairs - Part Ten". The Astrophysical Journal Supplement Series 44: 111.  
  16. ^ Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket".  
  17. ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  18. ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.

External links

  • "Castor 6". SolStation. Retrieved December 5, 2005. 

This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.

Copyright © World Library Foundation. All rights reserved. eBooks from World eBook Library are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.