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2013-05-08 10:41:47
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37 Geminorum is a star located at the northwest part of the constellation Gemini. Its distance from our Sun is about 56.3 light years. It is a solitary, yellow-white main sequence dwarf. No extrasolar planets have yet been discovered around this star. 37 Geminorum has many physical properties in common with the Sun and is one of the nearest solar twins. Due to this fact some scientists believe that the prospects for life in its vicinity are good. More information...

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    • Algol (β Per / Beta Persei), known colloquially as the Demon Star, is a bright star in the constellation Perseus. It is one of the best known eclipsing binaries, the first such star to be discovered, and also one of the first variable stars to be discovered. Algol is actually a three-star system (Beta Persei A, B, and C) in which the large and bright primary Beta Persei A is regularly eclipsed by the dimmer Beta Persei B.
      http://commons.wikipedia.org/wiki/File:Position_Beta_Per.png
    • Arcturus (α Boo / α Boötis / Alpha Boötis) is the brightest star in the constellation Boötes. With a visual magnitude of −0.05, it is also the third brightest star in the night sky, after Sirius and Canopus. It is, however, fainter than the combined light of the two main components of Alpha Centauri, which are too close together for the eye to resolve as separate sources of light, making Arcturus appear to be the fourth brightest.
      http://commons.wikipedia.org/wiki/File:Bootes_constellation_map.png
    • Altair (Alpha Aquilae / Alpha Aql / α Aquilae / α Aql / Atair) is the brightest star in the constellation Aquila and the twelfth brightest star in the night sky. It is an A-type main sequence star with an apparent visual magnitude of 0.77 and is one of the vertices of the Summer Triangle; the other two are Deneb and Vega. Altair rotates rapidly, with a velocity at the equator of approximately 286 km/s.
      http://en.wikipedia.org/wiki/File:PR_image6-crop.png
    • Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and the Latin genitive of the constellation it lies in (see List of constellations for a list of constellations and the genitive forms of their names). Flamsteed designation contained 2554 stars.
    • Sirius is the brightest star in the night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The name "Sirius" is derived from the Ancient Greek Seirios ("scorcher"), possibly because the star's appearance was associated with summer. The star has the Bayer designation α Canis Majoris (α CMa, or Alpha Canis Majoris).
      http://commons.wikipedia.org/wiki/File:Sirius_A_and_B_artwork.jpg
    • Vega (α Lyr / α Lyrae / Alpha Lyrae) is the brightest star in the constellation Lyra, the fifth brightest star in the night sky and the second brightest star in the northern celestial hemisphere, after Arcturus. It is a relatively nearby star at only 25 light-years from Earth, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood.
      http://commons.wikipedia.org/wiki/File:Vega_in_lyra.png
    • 61 Cygni, sometimes called Bessel's Star or Piazzi's Flying Star, is a binary star system in the constellation Cygnus. It consists of a pair of K-type dwarf stars that orbit each other in a period of about 659 years, forming a visual binary. At fifth and sixth apparent magnitudes, they are among the least conspicuous stars visible in the night sky to an observer without an optical instrument. 61 Cygni first attracted the attention of astronomers because of its large proper motion.
      http://commons.wikipedia.org/wiki/File:Compare_61_cygni.png
    • 70 Virginis is a yellow dwarf star approximately 59 light-years away in the constellation Virgo. It is rather unusually bright for its spectral type and may be just starting to evolve into the subgiant phase. In 1996, 70 Virginis was discovered to have an extrasolar planet in orbit around it. There is also a dust disc with a maximum temperature of 153 K located at a minimum distance of 3.4 AU from the star.
      http://commons.wikipedia.org/wiki/File:Celestia.png
    • Albireo (β Cyg / β Cygni / Beta Cyg / Beta Cygni) is the fifth brightest star in the constellation Cygnus. Although it has the Bayer designation beta, it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni. Albireo appears to the naked eye to be a single star but can be resolved with a telescope into a double star, consisting of a brighter yellow star (actually a binary system of two stars in orbit) and a fainter blue star.
      http://commons.wikipedia.org/wiki/File:Position_beta_Cyg.png
    • Alpha Arietis (Alpha Ari / α Ari / α Arietis), which also has the traditional names Hamal and El Nath, is the brightest star in the constellation Aries. Its Flamsteed designation is 13 Arietis, but this is very rarely used because it has a Bayer designation. α Arietis has spectral type K2 IIICa-1, which means that it is a K-type giant star, slightly cooler than the Sun and much larger. The Ca portion of the spectral type indicates that it shows calcium lines in its spectrum.
      http://commons.wikipedia.org/wiki/File:Aries_constellation_map.png

     

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