File:Messier 90 - HST.png

Page contents not supported in other languages.
This is a file from the Wikimedia Commons
From Wikipedia, the free encyclopedia

Original file ‎(4,073 × 3,961 pixels, file size: 33.31 MB, MIME type: image/png)

Summary

Description

Also known as M90 or Messier 90, this spiral galaxy exhibits less star formation than usual due to a phenomenon called ram pressure stripping. Gas that could have collapsed to form stars was instead stripped away as the galaxy moved through the intracluster medium between galaxies. Space may be mostly empty, but a galaxy moving fast enough through it can feel it.

This galaxy was observed as part of the wonderful PHANGS-HST. archive.stsci.edu/proposal_search.php?mission=hst&id=...

Red: WFC3/UVIS F814W Green: WFC3/UVIS F555W WFC3/UVIS F438W+F336W

North is 18.79° counter-clockwise from up.
Date
Source NGC 4569
Author Judy Schmidt from USA

Licensing

w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 2.0 Generic license.
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://flickr.com/photos/54209675@N00/49652791637. It was reviewed on 14 March 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

14 March 2020

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

depicts

some value

inception

12 March 2020

File history

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

Date/TimeThumbnailDimensionsUserComment
current21:51, 12 March 2020Thumbnail for version as of 21:51, 12 March 20204,073 × 3,961 (33.31 MB)Fabian RRRR=={{int:filedesc}}== {{Information |Description=Also known as M90 or Messier 90, this spiral galaxy exhibits less star formation than usual due to a phenomenon called ram pressure stripping. Gas that could have collapsed to form stars was instead stripped away as the galaxy moved through the intracluster medium between galaxies. Space may be mostly empty, but a galaxy moving fast enough through it can feel it. This galaxy was observed as part of the wonderful PHANGS-HST. [https://archive.sts...
The following pages on the English Wikipedia use this file (pages on other projects are not listed):

Global file usage

The following other wikis use this file:

Retrieved from "https://en.wikipedia.org/wiki/File:Messier_90_-_HST.png"