| Display title | Astronomy:Poynting–Robertson effect |
| Default sort key | Poynting-Robertson Effect |
| Page length (in bytes) | 12,049 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 637008 |
| Page content language | en - English |
| Page content model | wikitext |
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| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>Rtextdoc |
| Date of page creation | 06:37, 6 February 2024 |
| Latest editor | imported>Rtextdoc |
| Date of latest edit | 06:37, 6 February 2024 |
| Total number of edits | 1 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | The Poynting–Robertson effect, also known as Poynting–Robertson drag, named after John Henry Poynting and Howard P. Robertson, is a process by which solar radiation causes a dust grain orbiting a star to lose angular momentum relative to its orbit around the star. This is related to radiation pressure... |
