| Display title | Astronomy:Exozodiacal dust |
| Default sort key | Exozodiacal Dust |
| Page length (in bytes) | 8,330 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 569419 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>JTerm |
| Date of page creation | 12:26, 6 February 2024 |
| Latest editor | imported>JTerm |
| Date of latest edit | 12:26, 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. | File:Artist’s impression of bright exozodiacal light.ogv
Exozodiacal dust is 1–100 micrometre-sized grains of amorphous carbon and silicate dust that fill the plane of extrasolar planetary systems. It is the exoplanetary analog of zodiacal dust, the 1–100 micrometre-sized dust grains observed in the... |
