| Display title | Astronomy:DI Herculis |
| Default sort key | DI Herculis |
| Page length (in bytes) | 9,018 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 567948 |
| 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>DanMescoff |
| Date of page creation | 03:17, 27 June 2023 |
| Latest editor | imported>DanMescoff |
| Date of latest edit | 03:17, 27 June 2023 |
| 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. | DI Herculis is an Algol-type eclipsing binary star in the constellation of Hercules. The system has an apparent magnitude of about +8.5 and consists of two young blue stars of spectral type B5 and B4. It is about two thousand light years from Earth.
The orbit of the stars around their mutual centre of... |
