File:Comp galcen.jpg
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Comp_galcen.jpg (160 × 240 pixels, file size: 14 KB, MIME type: image/jpeg)
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[edit]DescriptionComp galcen.jpg |
Deutsch: NASA: Vergleich des Zentrums der Milchstraße bei verschiedenen Wellenlängen
English: The image of the central region of our own Milky Way Galaxy shows how areas which cannot be seen in visible light can show up very brightly in the infrared. The top row shows these regions in visible red light. At this wavelength we are seeing the light from billions of stars, particularly the largest, brightest ones. Note the dark bands where vast clouds of dust block our view of more distant objects.The middle row shows the same regions in the near-infrared (infrared wavelengths closest to visible light). The bottom row shows the same regions in the far-infrared.
IPAC: The Infrared Processing and Analysis Center (IPAC) is NASA's multi-mission center of expertise for long-wavelength astrophysics. |
Source | http://coolcosmos.ipac.caltech.edu/cosmic_classroom/ir_tutorial/importance.html |
Author | NASA |
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[edit]Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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[edit]The original description page was here. All following user names refer to de.wikipedia.
- 2004-03-30 10:45 Srbauer 160×240× (14468 bytes) NASA: Vergleich des Zentrums der Milchstraße bei verschiedenen Wellenlängen
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 16:00, 14 October 2011 | 160 × 240 (14 KB) | File Upload Bot (Magnus Manske) (talk | contribs) | {{BotMoveToCommons|de.wikipedia|year={{subst:CURRENTYEAR}}|month={{subst:CURRENTMONTHNAME}}|day={{subst:CURRENTDAY}}}} {{Information |Description={{de|NASA: Vergleich des Zentrums der Milchstraße bei verschiedenen Wellenlängen von http://coolcosmos.ip |
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JPEG file comment | File written by Adobe Photoshop¨ 4.0 |
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