| Display title | Astronomy:Intracluster medium |
| Default sort key | Intracluster Medium |
| Page length (in bytes) | 12,669 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375666 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>John Marlo |
| Date of page creation | 07:39, 6 February 2024 |
| Latest editor | imported>John Marlo |
| Date of latest edit | 07:39, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In astronomy, the intracluster medium (ICM) is the superheated plasma that permeates a galaxy cluster. The gas consists mainly of ionized hydrogen and helium and accounts for most of the baryonic material in galaxy clusters. The ICM is heated to temperatures on the order of 10 to 100 megakelvins, emitting... |
