| Display title | Astronomy:Very-long-baseline interferometry |
| Default sort key | Very-long-baseline interferometry |
| Page length (in bytes) | 22,437 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 412157 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
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| 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>Rjetedi |
| Date of page creation | 10:44, 6 February 2024 |
| Latest editor | imported>Rjetedi |
| Date of latest edit | 10:44, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar, is collected at multiple radio telescopes on Earth or in space. The distance between the radio telescopes is then calculated... |
