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O Grande Aglomerado Globular de Hércules (também conhecido como Aglomerado Globular de Hércules, Objeto Messier 13, Messier 13, M13, ou NGC 6205) é um aglomerado globular na Constelação de Hércules em ascensão reta 16 41.7 e declinação +36° 28'. Foi descoberto por Edmond Halley em 1714 e catalogado por Charles Messier em 1 de Junho de 1764. Com uma magnitude aparente de 5.8, é muito pouco visível a olho nu em uma noite de céu limpo. More information...

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  • A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite. Globular clusters are very tightly bound by gravity, which gives them their spherical shapes and relatively high stellar densities toward their centers. The name of this category of star cluster is derived from the Latin globulus—a small sphere. A globular cluster is sometimes known more simply as a globular.
    http://commons.wikipedia.org/wiki/File:Messier75.jpg
  • Messier 4 or M4 (also designated NGC 6121) is a globular cluster in the constellation of Scorpius. It was discovered by Philippe Loys de Chéseaux in 1746 and catalogued by Charles Messier in 1764. It was the first globular cluster in which individual stars were resolved.
    http://commons.wikipedia.org/wiki/File:Celestia.png
  • Messier 14 (also known as M14 or NGC 6402) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier in 1764. At a distance of about 30,000 light-years, M14 contains several hundreds of thousands of stars. At an apparent magnitude +7.6 it can be easily observed with binoculars. Medium-sized telescopes will show some hint of the individual stars of which the brightest is of magnitude +14.
    http://commons.wikipedia.org/wiki/File:Celestia.png
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    http://commons.wikipedia.org/wiki/File:Celestia.png
  • Globular Cluster M107 (also known as Messier Object 107 or NGC 6171) is a very loose globular cluster in the constellation Ophiuchus. It was discovered by Pierre Méchain in April 1782 and independently by William Herschel in 1793. It wasn't until 1947 that Helen Sawyer Hogg added it and three other objects discovered by Méchain to the list of Messier objects. M107 is close to the galactic plane at a distance of about 20,900 light-years from Earth.
    http://commons.wikipedia.org/wiki/File:Messier_107_Hubble_WikiSky.jpg
  • Omega Centauri or NGC 5139 is a globular cluster seen in the constellation of Centaurus, discovered by Edmond Halley in 1677 who listed it as a nebula. Omega Centauri had been listed in Ptolemy's catalog 2000 years ago as a star. Lacaille included it in his catalog as number I.5. It was first recognized as a globular cluster by the English astronomer John William Herschel in the 1830s.
    http://commons.wikipedia.org/wiki/File:07-0325_omega_centauri_martinez_fal_vcastro_IMG_5227.JPG
  • Messier 3 (also known as M3 or NGC 5272) is a globular cluster in the constellation Canes Venatici. It was discovered by Charles Messier in 1764, and resolved into stars by William Herschel around 1784. This cluster is one of the largest and brightest, and is made up of around 500,000 stars. It is located at a distance of about 33,900 light-years away from Earth. M3 has an apparent magnitude of 6.2, making it visible to the naked eye under dark conditions.
    http://commons.wikipedia.org/wiki/File:Star_cluster_in_the_Small_Magellanic_Cloud.jpg
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    http://commons.wikipedia.org/wiki/File:M72_Hubble_WikiSky.jpg
  • NGC 6397 is a globular cluster in the Ara constellation. It is located about 7,200 light-years from Earth, making it one of the two nearest globular clusters to Earth (the other one being Messier Object 4). The cluster contains around 400,000 stars. NGC 6397 is one of the at least 20 globulars of our Milky Way Galaxy which have undergone a core collapse, meaning that its core has contracted to a very dense stellar agglomeration.
    http://commons.wikipedia.org/wiki/File:P0321a.jpg
  • Messier 2 or M2 (also designated NGC 7089) is a globular cluster in the constellation Aquarius, five degrees north of the star Beta Aquarii. It was discovered by Jean-Dominique Maraldi in 1746 and is one of the largest known globular clusters.
    http://commons.wikipedia.org/wiki/File:Messier_2_Hubble_WikiSky.jpg

 

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