File:Central regions Perseus galaxy cluster.jpg
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
Size of this preview: 631 × 599 pixels. Other resolutions: 253 × 240 pixels | 505 × 480 pixels | 808 × 768 pixels | 1,078 × 1,024 pixels | 2,100 × 1,995 pixels.
Original file (2,100 × 1,995 pixels, file size: 1.43 MB, MIME type: image/jpeg)
File information
Structured data
Captions
Summary
[edit]DescriptionCentral regions Perseus galaxy cluster.jpg |
English: An accumulation of 270 hours of Chandra observations of the central regions of the Perseus galaxy cluster reveals evidence of the turmoil that has wracked the cluster for hundreds of millions of years. One of the most massive objects in the universe, the cluster contains thousands of galaxies immersed in a vast cloud of multimillion degree gas with the mass equivalent of trillions of suns.
Enormous bright loops, ripples, and jet-like streaks are apparent in the image. The dark blue filaments in the center are likely due to a galaxy that has been torn apart and is falling into NGC 1275, a.k.a. Perseus A, the giant galaxy that lies at the center of the cluster. Image is 284 arcsec across. RA 03h 19m 47.60s Dec +41° 30' 37.00" in Perseus. Observation dates: 13 pointings between August 8, 2002 and October 20, 2004. Color code: Energy (Red 0.3-1.2 keV, Green 1.2-2 keV, Blue 2-7 keV). Instrument: ACIS. |
Date | (released) |
Source | http://chandra.harvard.edu/photo/2005/perseus/ (TIFF source) |
Author | NASA/CXC/IoA/A.Fabian et al. |
Permission (Reusing this file) |
Images from NASA usually are free of copyright. |
Licensing
[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.) | ||
Warnings:
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 10:57, 2 July 2017 | 2,100 × 1,995 (1.43 MB) | Huntster (talk | contribs) | Full resolution from TIFF. | |
03:46, 25 November 2009 | 420 × 405 (164 KB) | Marshallsumter (talk | contribs) | {{Information |Description={{en|1=An accumulation of 270 hours of Chandra observations of the central regions of the Perseus galaxy cluster reveals evidence of the turmoil that has wracked the cluster for hundreds of millions of years. One of the most mas |
You cannot overwrite this file.
File usage on Commons
The following 3 pages use this file:
File usage on other wikis
The following other wikis use this file:
- Usage on af.wikipedia.org
- Usage on ar.wikipedia.org
- Usage on bn.wikipedia.org
- Usage on ca.wikipedia.org
- Usage on cs.wikipedia.org
- Usage on de.wikipedia.org
- Usage on en.wikipedia.org
- Usage on en.wikiversity.org
- Plasmas/Plasma objects/Coronal clouds
- Sources/First astronomical X-ray source
- Stars/Surface fusion
- User:Marshallsumter/Radiation astronomy2/Synchrotrons
- Portal:Radiation astronomy
- Portal:Radiation astronomy/Image
- Portal:Radiation astronomy/Image/21
- Portal:Radiation astronomy/Pictures
- Portal:Radiation astronomy/Pictures/27
- Portal:Radiation astronomy/X-ray astronomy article
- Portal:Radiation astronomy/X-ray astronomy article/29
- Usage on fa.wikipedia.org
- Usage on fr.wikipedia.org
- Usage on id.wikipedia.org
- Usage on it.wikipedia.org
- Usage on ja.wikipedia.org
- Usage on ko.wikipedia.org
- Usage on kw.wikipedia.org
- Usage on lb.wikipedia.org
- Usage on sv.wikipedia.org
- Usage on uk.wikipedia.org
- Usage on www.wikidata.org