Alcyone (star)

Alcyone, η Tau

Alcyone is the bright star at the center of the map.
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 03h 47m 29.0765s[1]
Declination 24° 06′ 18.494″[1]
Apparent magnitude (V) 2.873[1]
Characteristics
Spectral type B7IIIe[2]
U−B color index -0.35[3]
B−V color index -0.09[3]
Variable type suspected
Astrometry
Radial velocity (Rv) 10.1[1] km/s
Proper motion (μ) RA: 19.35[1] mas/yr
Dec.: -43.11[1] mas/yr
Parallax (π) 8.87 ± 0.99[4] mas
Distance approx. 370 ly
(approx. 110 pc)
Absolute magnitude (MV) -2.39
Details
Mass 6[5] M
Radius ~10[5] R
Luminosity 2,400[5] L
Temperature 13,000[5] K
Rotation 215 km/s[2]
Other designations
η Tau, 25 Tau, HR 1165, HD 23630, BD+23 541, FK5 139, HIP 17702, SAO 76199, GC 4541, BDS 1875, CCDM 03474+2407
Database references
SIMBAD data

Coordinates: 03h 47m 29.0765s, +24° 06′ 18.494″

Alcyone (η Tau, η Tauri, Eta Tauri) is a star system in the constellation Taurus. It is the brightest star in the Pleiades open cluster, which is a young cluster, aged at less than 50 million years. Alcyone is approximately 370 light years from Earth. It is named after the mythological figure Alcyone, one of the mythological Pleiades. It is known as 昴宿六 (the Sixth Star of the Hairy Head) in Chinese.

Contents

Overview

The main star, known as Alcyone A, is a blue-white B-type giant similar to many of the other B-type stars in the Pleiades cluster. It has an apparent magnitude of +2.87 (absolute magnitude = −2.39), and a radius almost 10 times that of the Sun.[5] Its temperature is approximately 13,000 K giving it a total luminosity that is 2,400 times solar. The spectral type of B7IIIe indicates that emission lines are present in its spectrum. Like many Be stars, Alcyone A has a high rotational velocity of 215 km/s,[2] which has created a gaseous disk flung into orbit around the star from its equator.

Star System

Alcyone is an eclipsing binary, and the two components have a separation of 0.031 arcseconds, or about the distance from the Sun to Jupiter.

The binary star is orbited by three companions. Alcyone B and Alcyone C are both 8th magnitude white A-type dwarfs and are separated from A by 117 and 181 arcseconds respectively. Alcyone D is a yellow-white F-type dwarf, 191 arcseconds from the primary. It has an apparent magnitude of +8.7. Alcyone C is classified as a Delta Scuti type variable star and its brightness varies from magnitude +8.25 to +8.30 over 1.13 hours.

See also

References

  1. ^ a b c d e f "SIMBAD query result: ALCYONE -- Be Star". Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=Alcyone&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id. Retrieved 2010-06-30. 
  2. ^ a b c "Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR. Centre de Données astronomiques de Strasbourg. http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HR%201165. Retrieved 2010-06-30. 
  3. ^ a b Johnson, H. L.; Iriarte, B.; Mitchell, R. I.; Wisniewski, W. Z. (1966). "UBVRIJKL photometry of the bright stars." (PDF). Comm. Lunar Plan. Lab., 4. Bibcode 1966CoLPL...4...99J. 
  4. ^ Perryman, M. A. C. et al. (1997), "The Hipparcos Catalogue", Astronomy & Astrophysics 323: L49–L52, Bibcode 1997A&A...323L..49P 
  5. ^ a b c d e Professor James B. (Jim) Kaler. "ALCYONE (Eta Tauri)". University of Illinois. http://www.astro.uiuc.edu/~kaler/sow/alcyone.html. Retrieved 2010-06-30. 

External links