Metadata
Author: WikiMatrix
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English[en]
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 planet revolving around a star.
Latin[la]
Vector Laplace–Runge–Lenz (vel brevius vector LRL) in mechanica classica est vector quo, inter alia, forma et orientatio orbitae unius corporis caelestis circa aliud, ut planetae circa stellam, describitur.