Display title | Astronomy:Leonard–Merritt mass estimator |
Default sort key | Leonard-Merritt Mass Estimator |
Page length (in bytes) | 4,353 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 375798 |
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 |
HandWiki item ID | None |
Edit | Allow all users (infinite) |
Move | Allow all users (infinite) |
Page creator | imported>Scavis |
Date of page creation | 18:06, 6 March 2023 |
Latest editor | imported>Scavis |
Date of latest edit | 18:06, 6 March 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. | The Leonard–Merritt mass estimator is a formula for estimating the mass of a spherical stellar system using the apparent (angular) positions and proper motions of its component stars. The distance to the stellar system must also be known.
Like the virial theorem, the Leonard–Merritt estimator yields... |