Ficheru:Tarantula nebula detail.jpg

Ficheru orixinal(1076 × 1087 píxels, tamañu de ficheru: 1,55 MB, triba MIME: image/jpeg)

Esti ficheru ye de Wikimedia Commons y puen usalu otros proyeutos. La descripción de la páxina de descripción del ficheru s'amuesa darréu.

Descripción Part of the Tarantula Nebula, a giant HII region in the Large Magellanic Cloud. The star cluster at the lower right is Hodge 301.
Fonte http://hubblesite.org/newscenter/archive/releases/1999/12/image/a (direct link)
Autor The Hubble Heritage Team (AURA / STScI / NASA)
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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.

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Data/HoraMiniaturaDimensionesUsuariuComentariu
actual22:19 23 pay 2006Miniatura de la versión a fecha de 22:19 23 pay 20061076 × 1087 (1,55 MB)SiebrandHigh res from [http://hubblesite.org/newscenter/archive/releases/1999/12/image/a hubblesite.org] Downloaded from: [http://imgsrc.hubblesite.org/hu/db/1999/12/images/a/formats/full_jpg.jpg here]
08:22 15 avi 2005Miniatura de la versión a fecha de 08:22 15 avi 2005750 × 756 (144 kB)ChongDaeThis image was copied from wikipedia:en. The original description was: Part of the Tarantula Nebula, a giant HII region in the LMC. The star cluster at the lower right is Hodge 301. Image Credit: NASA and The Hubble Heritage Team (STScI/AURA) A

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