File:NGC 4889 HST.png
![File:NGC 4889 HST.png](https://upload.wikimedia.org/wikipedia/commons/thumb/1/14/NGC_4889_HST.png/618px-NGC_4889_HST.png?20150524214349)
Original file (4,000 × 3,880 pixels, file size: 23.39 MB, MIME type: image/png)
Captions
Captions
Summary
[edit]DescriptionNGC 4889 HST.png |
A dominant member of the Coma Cluster, remarkable elliptical shell galaxy NGC 4889 looms large over its domain. Within the cluster, only NGC 4874 (not shown) is brighter, and only just barely. The faintly visible shells of the galaxy are evidence that the monstrous galaxy recently merged with a smaller galaxy. Other details to notice include smaller and/or more distant elliptical galaxies, some of which are ghostly and faint. I have seen them called them fluffy galaxies in this recent press release. The nature of these ultra-diffuse galaxies and specifically how they manage to form as they do is still a matter of speculation. Very few Milky Way stars are visible within the field. As usual, the ones with four spikes are most likely foreground stars. The hundreds of tiny, fainter point-like objects are globular clusters, many of which are likely orbiting NGC 4889. Do you think that maybe some background galaxies show a curious alignment? You might not be imagining it. It's possible that some weak gravitational lensing is going on. Weak gravitational lensing is detectable by taking measurements of all the background galaxies and seeing if they all seem a bit squished in a certain direction. One final curiosity that I would like to note about NGC 4889: If you measure the brightness of the center of its nucleus, it is actually not as bright as NGC 4886, which is the smaller elliptical galaxy just above it in this image (that one skinny galaxy is kind of pointing toward it). The way some elliptical galaxies have diffuse cores while others have very sharp ones is something that perplexes me. It seems that even though NGC 4889 is much larger than NGC 4886, its nucleus is notably less dense than NGC 4886's. Red: ACS / WFC F814W (jb2i02020_drc) Green: Pseudo Blue: ACS / WFC F475W (jb2i02010_drc & jb2i03010_drc) North is NOT up. It is 43.6° counter-clockwise from up. |
Date | |
Source | NGC 4889 |
Author | Judy Schmidt from Fresh Meadows, NY, USA |
Licensing
[edit]![w:en:Creative Commons](https://upload.wikimedia.org/wikipedia/commons/thumb/7/79/CC_some_rights_reserved.svg/90px-CC_some_rights_reserved.svg.png)
![attribution](https://upload.wikimedia.org/wikipedia/commons/thumb/1/11/Cc-by_new_white.svg/24px-Cc-by_new_white.svg.png)
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
![]() |
This image was originally posted to Flickr by geckzilla at https://www.flickr.com/photos/54209675@N00/17803982215. It was reviewed on 24 May 2015 by FlickreviewR and was confirmed to be licensed under the terms of the cc-by-2.0. |
24 May 2015
Annotations InfoField | This image is annotated: View the annotations at Commons |
NGC 4889
NGC 4886
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:43, 24 May 2015 | ![]() | 4,000 × 3,880 (23.39 MB) | Fabian RRRR (talk | contribs) | {{Information |Description=A dominant member of the [http://en.wikipedia.org/wiki/Coma_Cluster Coma Cluster], remarkable elliptical shell galaxy NGC 4889 looms large over its domain. Within the cluster, only NGC 4874 (not shown) is brighter, and only j... |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
File usage on other wikis
The following other wikis use this file:
- Usage on ar.wikipedia.org
- Usage on arz.wikipedia.org
- Usage on az.wikipedia.org
- Usage on be.wikipedia.org
- Usage on bs.wikipedia.org
- Usage on ce.wikipedia.org
- Usage on de.wikipedia.org
- Usage on diq.wikipedia.org
- Usage on en.wikipedia.org
- Usage on fr.wikipedia.org
- Usage on hr.wikipedia.org
- Usage on it.wikibooks.org
- Usage on kk.wikipedia.org
- Usage on mk.wikipedia.org
- Usage on nl.wikipedia.org
- Usage on pl.wikipedia.org
- Usage on sk.wikipedia.org
- Usage on tt.wikipedia.org
- Usage on uk.wikipedia.org
- Usage on uz.wikipedia.org
- Usage on www.wikidata.org
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Software used | |
---|---|
Date and time of digitizing | 16:56, 17 May 2015 |
File change date and time | 20:15, 17 May 2015 |
Date metadata was last modified | 20:15, 17 May 2015 |
Unique ID of original document | xmp.did:69912ace-6b68-9a42-b35e-4cf4d5e31653 |
Contact information |
|