| Display title | Astronomy:Mira variable |
| Default sort key | Mira Variable |
| Page length (in bytes) | 25,382 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 620761 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>WikiEd2 |
| Date of page creation | 09:55, 6 February 2024 |
| Latest editor | imported>WikiEd2 |
| Date of latest edit | 09:55, 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. | Mira variables (named for the prototype star Mira) are a class of pulsating stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths. They are red giants in the very late stages of stellar... |
