| Display title | Astronomy:Dissociative recombination |
| Default sort key | Dissociative Recombination |
| Page length (in bytes) | 2,516 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374687 |
| 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>HamTop |
| Date of page creation | 11:20, 6 February 2024 |
| Latest editor | imported>HamTop |
| Date of latest edit | 11:20, 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. | Dissociative recombination is a chemical process in which a positive polyatomic ion recombines with an electron, and as a result, the neutral molecule dissociates. This reaction is important for interstellar and atmospheric chemistry. On Earth, dissociative recombination rarely occurs naturally, as free... |
