| Display title | Astronomy:Kepler-88 |
| Default sort key | Kepler-88 |
| Page length (in bytes) | 6,456 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 15796 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 3 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>DanMescoff |
| Date of page creation | 06:12, 6 February 2024 |
| Latest editor | imported>DanMescoff |
| Date of latest edit | 06:12, 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. | Kepler-88 is a Sun-like star in the constellation of Lyra, with three confirmed planets. In April 2012, scientists discovered that a Kepler candidate known as KOI-142.01 (Kepler-88b) exhibited very significant transit-timing variations caused by a non-transiting planet. Timing variations were large enough... |
