| Display title | Astronomy:Galactic bulge |
| Default sort key | Galactic bulge |
| Page length (in bytes) | 18,290 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 1007201 |
| 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>WikiG |
| Date of page creation | 12:09, 6 February 2024 |
| Latest editor | imported>WikiG |
| Date of latest edit | 12:09, 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, a galactic bulge (or simply bulge) is a tightly packed group of stars within a larger star formation. The term almost exclusively refers to the central group of stars found in most spiral galaxies (see galactic spheroid). Bulges were historically thought to be elliptical galaxies that happened... |
