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Spica

 
Dictionary: Spi·ca   (spī') pronunciation
n.
A spectroscopic binary star, 245 light-years from Earth, one of the brightest stars in the sky and the brightest star in the constellation Virgo.

[Latin Spīca, from spīca, ear of grain.]


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A 1st-magnitude star in the constellation Virgo. Spica (α Virginis) is a hot main-sequence star of spectral type B1, effective temperature about 25,000 K (45,000°F), at a distance of 80 parsecs from the Sun (2.59 × 1015 km or 1.61 × 1015 mi). See also Spectral type.

It is a double-line spectroscopic binary with an orbital period of almost exactly 4 days. The system constitutes an example of an ellipsoidal variable, where the separation between the two stars is so small that powerful tidal forces distort the stars. The changing aspect of the primary as seen from Earth causes light variations with a period equal to the orbital period. The separation between the two stars is only about 3.5 times the radius of the primary. The primary itself is an intrinsic variable of the β Cephei type and is pulsating with a period of about 4 h. See also Binary star; Star; Variable star.


 
Spica (spī'), brightest star in the constellation Virgo; Bayer designation Alpha Virginis; 1992 position R.A. 13h24.8m, Dec. −11°07′. A bluish-white star of spectral class B1 V, its apparent magnitude averages about 0.96, making it one of the 20 brightest stars in the sky. Because it is an eclipsing binary star, the magnitude ranges from 0.91 to 1.01 as the two components orbit about each other within a four-day period. Spica is at a distance of about 200 light-years. Its name is Latin for "ear of grain," referring to an ear of grain held by the figure traditionally associated with the constellation Virgo.


WordNet: Spica
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Note: click on a word meaning below to see its connections and related words.

The noun has one meaning:

Meaning #1: the brightest star in Virgo


Wikipedia: Spica
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Alpha Virginis A/B
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Pronunciation /ˈspaɪkə/
Right ascension 13h 25m 11.6s
Declination −11° 09' 41"
Apparent magnitude (V) +1.04
Characteristics
Spectral type B1III-IV/B2V
U-B color index −0.93
B-V color index −0.13[citation needed]
Variable type β Cep,
Rotating ellipsoid
Astrometry
Radial velocity (Rv) +1.0 km/s
Proper motion (μ) RA: −42.50 mas/yr
Dec.: −31.73 mas/yr
Parallax (π) 12.44 ± 0.86 mas
Distance 260 ± 20 ly
(80 ± 6 pc)
Absolute magnitude (MV) −3.55
Details
Mass 11/7 M
Radius 7.8/4.0 R
Luminosity 13,400/1,700 L
Temperature 22,400/18,500 K
Other designations
Spica, Aztec 角宿一, Spica Virginis, Alaraph, Dana, α Virginis, 67 Virginis, HR 5056, BD -10°3672, HD 116658, GCTP 18144, FK5 498, CCDM 13252-1109, SAO 157923, HIP 65474.
Every year around October 17 the Sun approaches Spica (the bright one below the Sun). Photo: SOHO.
How to locate the star Spica.

Spica (α Vir / α Virginis / Alpha Virginis) is the brightest star in the constellation Virgo, and the 15th brightest star in the nighttime sky. It is 260 light years distant from Earth. A blue giant, it is a variable of the Beta Cephei type.

Contents

Observation history

Spica is believed to be the star that provided Hipparchus with the data which enabled him to discover precession of the equinoxes.[1] A temple to Menat (an early Hathor) at Thebes was oriented with reference to Spica when it was constructed in 3200 BC and, over time, precession resulted in a slow but noticeable change in the location of Spica relative to the temple.[2] Nicolaus Copernicus made many observations of Spica with his home-made triquetrum for his researches on precession.[3][4]

Characteristics

Spica is the brightest of the rotating ellipsoidal variables. Its apparent magnitude varies between +0.92 and +1.04, with a period of 4.0142 days. This slight dip in magnitude is barely noticeable visually. It is also a variable of the Beta Cephei type. Spica has a luminosity about 2,300 times that of the Sun. Spica is a double star, but the distance between the two stars is so small that it distorts the image, and makes the two stars seem like one, with very slight brightness variations.

Visibility

Located close to the ecliptic, Spica can be occulted by the Moon and sometimes by the planets. The last planetary occultation of Spica occurred when Venus passed in front of the star (as seen from Earth) on November 10, 1783. The next occultation will occur September 2, 2197, when Venus again passes in front of Spica. The Sun passes a little more than 2º north of Spica around October 16 every year, and the star's heliacal rising occurs about two weeks later. Every 8 years, Venus passes Spica around the time of the star's heliacal rising, as in 2009 when it will pass 3.5o north of the star on November 3.[2]

An easy way to find Spica is to follow the arc of the handle of the Big Dipper to Arcturus, and then continue on the same distance to Spica ("follow the arc to Arcturus and speed on to Spica").

Etymology and cultural significance

The name Spica derives from Latin spīca virginis "Virgo's ear of grain" (usually wheat). In Chinese astronomy, the star is known as Jiao Xiu 1 (角宿一) in Jiao Xiu, one of the Chinese constellations. In Hindu astronomy, Spica corresponds to the Nakshatra Chitra. The 17th century German astronomer Bayer and others referred to the star as Arista.

Medieval names include Azimech, from Arabic السماك الأعزل al-simāk al-a‘zal 'the Undefended', and Alarph, Arabic for 'the Grape Gatherer'.[citation needed]

In medieval astrology, it was a Behenian fixed star, associated with the emerald and sage. In his De Occulta Philosophia, Cornelius Agrippa attributes its kabbalistic symbol Agrippa1531 Spica.png to Hermes Trismegistus.

A blue star represents Spica on the flag of the Brazilian state of Pará. Spica is also the star representing Pará on the Brazilian flag.

Spica was used in the novel Pushing Ice by Alastair Reynolds as the distant star to which the protagonists are carried by alien technology.

The Japanese manga and series Twin Spica was named after the star. Spica is two stars that circle each other, though from a distance they appear as one, which parallels the series' running theme of friendship.

References

  1. ^ Evans, James (1998). The History and Practice of Ancient Astronomy. Oxford University Press. pp. 259. ISBN 0195095391. http://books.google.com.au/books?id=nS51_7qbEWsC&pg=PA259&lpg=PA259&dq=spica+hipparchus&source=bl&ots=c1dkQmjFl8&sig=I1zqqn_pb4V65A5Rlzx7FKA9AuU&hl=en&ei=zMrGSeiaI5iy6wP5rqG6Bw&sa=X&oi=book_result&resnum=6&ct=result. 
  2. ^ Allen, Richard Hinckley (2003). Star Names and Their Meanings. Kessinger Publishing. pp. 468. ISBN 0766140288. http://books.google.com.au/books?id=_GUDis0bETgC&pg=PA468&lpg=PA468&dq=spica+thebes+temple+menat&source=bl&ots=6SYdIUUyKg&sig=f3v7K4DaebtOi1kDByXpczmzhkg&hl=en&ei=bszGSfzYI5iVkAWp2-nNDA&sa=X&oi=book_result&resnum=10&ct=result. 
  3. ^ Rufus, W. Carl (April 1943). "Copernicus, Polish Astronomer, 1473–1543". The Journal of the Royal Astronomical Society of Canada 37 (4): 134. Bibcode1943JRASC..37..129R. http://articles.adsabs.harvard.edu//full/1943JRASC..37..129R/0000129.000.html. 
  4. ^ Kristian P. Moesgaard: Copernican influence on Tycho Brahe, in Jerzy Dobrzycki: The reception of Copernicus' heliocentric theory: proceedings of a symposium organized by the Nicolas Copernicus Committee of the International Union of the History and Philosophy of Science, Toruń, Poland, 1973, Studia Copernicana, Springer, 1972 ISBN 9027703116, 9789027703118 [1]

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