| Display title | Astronomy:Optical window |
| Default sort key | Optical Window |
| Page length (in bytes) | 6,855 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 837721 |
| 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>AnLinks |
| Date of page creation | 06:46, 6 February 2024 |
| Latest editor | imported>AnLinks |
| Date of latest edit | 06:46, 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 optical window is the portion of the optical spectrum that is not blocked by the Earth's atmosphere. The window runs from around 300 nanometers (ultraviolet-B) up into the range the human eye can detect, roughly 400–700 nm and continues up to approximately 2 μm. Sunlight mostly reaches the ground... |
