Display title | Astronomy:Main sequence |
Default sort key | Main sequence |
Page length (in bytes) | 64,343 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 375987 |
Page content language | en - English |
Page content model | wikitext |
Indexing by robots | Allowed |
Number of redirects to this page | 1 |
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>LinuxGuru |
Date of page creation | 14:28, 6 February 2024 |
Latest editor | imported>LinuxGuru |
Date of latest edit | 14:28, 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 main sequence is a classification of stars which appear on plots of stellar color versus brightness as a continuous and distinctive band. Stars on this band are known as main-sequence stars or dwarf stars, and positions of stars on and off the band are believed to indicate their physical... |