Original file (4,073 × 3,961 pixels, file size: 33.31 MB, MIME type: image/png)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 21:51, 12 March 2020 |
![]() | 4,073 × 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... |
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Original file (4,073 × 3,961 pixels, file size: 33.31 MB, MIME type: image/png)
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:51, 12 March 2020 |
![]() | 4,073 × 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 other wikis use this file: