| Display title | Physics:Shapiro time delay |
| Default sort key | Shapiro time delay |
| Page length (in bytes) | 13,007 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 443315 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
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| 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>LinXED |
| Date of page creation | 06:28, 5 February 2024 |
| Latest editor | imported>LinXED |
| Date of latest edit | 06:28, 5 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. | The Shapiro time delay effect, or gravitational time delay effect, is one of the four classic Solar System tests of general relativity. Radar signals passing near a massive object take slightly longer to travel to a target and longer to return than they would if the mass of the object were not present... |
