| Display title | Astronomy:Small planet radius gap |
| Default sort key | Small planet radius gap |
| Page length (in bytes) | 9,505 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 312588 |
| 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>WikiGary |
| Date of page creation | 13:12, 6 February 2024 |
| Latest editor | imported>WikiGary |
| Date of latest edit | 13:12, 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. | The small planet radius gap (also called the Fulton gap, photoevaporation valley, or Sub-Neptune Desert) is an observed scarcity of planets with radii between 1.5 and 2 times Earth's radius, likely due to photoevaporation-driven mass loss. A bimodality in the Kepler exoplanet population was first observed... |
