| Display title | Physics:Laplace–Runge–Lenz vector |
| Default sort key | Laplace-Runge-Lenz vector |
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| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 650710 |
| Page content language | en - English |
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| Page creator | imported>John Stpola |
| Date of page creation | 06:33, 5 February 2024 |
| Latest editor | imported>John Stpola |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In classical mechanics, the Laplace–Runge–Lenz (LRL) vector is a vector used chiefly to describe the shape and orientation of the orbit of one astronomical body around another, such as a binary star or a planet revolving around a star. For two bodies interacting by Newtonian gravity, the LRL vector is... |
