Tugna:A Swarm of Ancient Stars - GPN-2000-000930.jpg

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Afaylu agi yusad seg : Wikimedia Commons. Ahat yeseqdec deg isenfaṛen nniḍen. Aglam-is ɣef asebter n aglam ye beqqeḍ ddaw-agi.

Aglam
English: This stellar swarm is M80 (NGC 6093), one of the densest of the 147 known globular star clusters in the Milky Way galaxy. Located about 28,000 light-years from Earth, M80 contains hundreds of thousands of stars, all held together by their mutual gravitational attraction. Globular clusters are particularly useful for studying stellar evolution, since all of the stars in the cluster have the same age (about 12 billion years), but cover a range of stellar masses. Every star visible in this image is either more highly evolved than, or in a few rare cases more massive than, our own Sun. Especially obvious are the bright red giants, which are stars similar to the Sun in mass that are nearing the ends of their lives.
Azemz
Aɣbalu Great Images in NASA Description
Ameskar NASA, The Hubble Heritage Team, STScI, AURA
Tasiregt
(Tulsa n useqdec n ufaylu-agi)
Public domain This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org. For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
Cette image ou vidéo a été cataloguée par le
Space Telescope Science Institute
de la
National Aeronautics and Space Administration
 (NASA) des États-Unis sous Photo ID : GPN-2000-000930 ; et Alternate ID : PR99-26.

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Star Swarms

Éléments décrits dans ce fichier

igellem

type MIME Tafransist

image/jpeg

somme de contrôle Tafransist

71a8b3eb2ddd1ab70f006560b8467fd3edcc4f69

méthode de détermination Tafransist : SHA-1 Tafransist

taille des données Tafransist

4 224 281 octet

hauteur Tafransist

1 864 pixel

largeur Tafransist

1 777 pixel

Amazray n ufaylu

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Azemz/SsaɛaAqmamaḍIseggiwenAmseqdacAwennit
Lux a4 Meɣres 2010 à 14:08Tugna tamectuḥt i lqem n 4 Meɣres 2010 à 14:081 777 × 1 864 (4,03 MB/MO)TryphonFrom original source http://hubblesite.org/newscenter/archive/releases/1999/26/image/a/ (http://imgsrc.hubblesite.org/hu/db/images/hs-1999-26-a-full_jpg.jpg).
9 Yebrir 2009 à 00:54Tugna tamectuḥt i lqem n 9 Yebrir 2009 à 00:541 777 × 1 864 (3,98 MB/MO)BotMultichillT{{Information |Description={{en|1=This stellar swarm is M80 (NGC 6093), one of the densest of the 147 known globular star clusters in the Milky Way galaxy. Located about 28,000 light-years from Earth, M80 contains hundreds of thousands of stars, all held

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Iwikiyen-agi-nniḍen seqdacen afaylu-agi:

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