This is a Featured picture. Click here for more information.
This image was selected for display on the Main Page as the picture of the day. Click here for more information.

File:M104 ngc4594 sombrero galaxy hi-res.jpg

From Wikimedia Commons, the free media repository
Revision as of 12:47, 30 June 2012 by Julia W (talk | contribs) (+link to nom)
Jump to navigation Jump to search

Original file (11,472 × 6,429 pixels, file size: 34.22 MB, MIME type: image/jpeg)

Captions

Captions

Add a one-line explanation of what this file represents
Warning The original file is very high-resolution. It might not load properly or could cause your browser to freeze when opened at full size. Open in ZoomViewer
Description

This image of the Sombrero Galaxy is a mosaic of six images taken by the Hubble Space Telescope's Advanced Camera for Surveys in May and June 2003 (exposition time: 10.2 hours).

English: The famous Sombrero galaxy (M104) is a bright nearby spiral galaxy. The prominent dust lane and halo of stars and globular clusters give this galaxy its name. Something very energetic is going on in the Sombrero's center, as much X-ray light has been detected from it. This X-ray emission coupled with unusually high central stellar velocities cause many astronomers to speculate that a black hole lies at the Sombrero's center - a black hole a billion times the mass of our Sun.
Français : La fameuse galaxie du Sombrero (M104) est une galaxie spirale proche et particulièrement brillante. La bande de poussières et le halo des étoiles et des amas globulaires lui ont donné son nom. Des évènements très énergetiques ont lieu dans le centre de cette galaxie et produisent de nombreux rayons X. Cette forte émission dans le X ainsi que la vitesse anormalement élevée des étoiles près de son centre font que beaucoup d'astronomes supposent qu'un trou noir se trouve au centre de cette galaxie. Un trou noir pesant un milliard de fois la masse du soleil.
Español: La famosa galaxia de Sombrero (M104) es una galaxia de la escalera luminosa de caracol cercana. La senda de polvo prominente, el halo de estrellas y los racimos globulares dan su nombre a esta galaxia. Una energía muy intensa puede observarse en el centro del Sombrero, debido a la gran cantidad de luz proveniente del centro. Esta emisión de la Radiografía (luz potente) acoplada con extraordinarias velocidades estelares centrales altas causa muchas astrónomas especulares por el agujero negro ubicado al centro del Sombrero - un agujero negro un mil millones veces más grande que la masa de nuestro Sol.
Date between May 2003 and June 2003
date QS:P,+2003-00-00T00:00:00Z/9,P1319,+2003-05-00T00:00:00Z/10,P1326,+2003-06-00T00:00:00Z/10
Source
Author NASA/ESA and The Hubble Heritage Team (STScI/AURA)
Permission
(Reusing this file)
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.
Other versions
Infrared light

Featured picture

Wikimedia CommonsWikipedia

This is a featured picture on Wikimedia Commons (Featured pictures) and is considered one of the finest images. See its nomination here.
 With an aspect ratio of 8:5, 16:10, or 16:9, this image is suitable as a widescreen computer wallpaper (see gallery).

Wikipedia
 This is a featured picture on the English language Wikipedia (Featured pictures) and is considered one of the finest images. See its nomination here.
 This is a featured picture on the Spanish language Wikipedia (Recursos destacados) and is considered one of the finest images. See its nomination here.
 This is a featured picture on the Croatian language Wikipedia (Slika tjedna) and is considered one of the finest images. See its nomination here.
 This is a featured picture on the Turkish language Wikipedia (Seçkin resimler) and is considered one of the finest images. See its nomination here.

If you have an image of similar quality that can be published under a suitable copyright license, be sure to upload it, tag it, and nominate it.

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current20:20, 20 July 2009Thumbnail for version as of 20:20, 20 July 200911,472 × 6,429 (34.22 MB)Tryphon (talk | contribs)Better quality.
17:54, 27 April 2005Thumbnail for version as of 17:54, 27 April 200511,472 × 6,429 (7.12 MB)Bricktop (talk | contribs)

The following 58 pages use this file:

File usage on other wikis

The following other wikis use this file:

View more global usage of this file.