| Display title | Astronomy:Synchronous frame |
| Default sort key | Synchronous frame |
| Page length (in bytes) | 45,013 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 37077 |
| 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>Dennis Ross |
| Date of page creation | 06:31, 6 February 2024 |
| Latest editor | imported>Dennis Ross |
| Date of latest edit | 06:31, 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. | A synchronous frame is a reference frame in which the time coordinate defines proper time for all co-moving observers. It is built by choosing some constant time hypersurface as an origin, such that has in every point a normal along the time line and a light cone with an apex in that point can be constructed... |
