| Display title | Physics:Mantle convection |
| Default sort key | Mantle Convection |
| Page length (in bytes) | 19,685 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 429395 |
| 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) |
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| Page creator | imported>AstroAI |
| Date of page creation | 07:00, 5 February 2024 |
| Latest editor | imported>AstroAI |
| Date of latest edit | 07:00, 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. | Mantle convection is the very slow creeping motion of Earth's solid silicate mantle as convection currents carry heat from the interior to the planet's surface.
The Earth's surface lithosphere rides atop the asthenosphere and the two form the components of the upper mantle. The lithosphere is divided... |
