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In celestial mechanics, the Lagrange points (/ləˈɡrɑːndʒ/), also called the Lagrangian points or libration points, are points of equilibrium for small-mass objects under the gravitational influence of two massive orbiting bodies. Mathematically, this involves the solution of the restricted three-body problem.
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earth sun points l2 lagrange two l1 l5 point l4 orbit space l3 bodies mass orbits around gravitational moon solar
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| the Solar System does not contain these periodic orbits | instance of | A full n-body dynamical system | 0.80 | text |
| but does contain quasi-periodic | instance of | A full n-body dynamical system | 0.80 | text |
| Lagrange point | related to External links | What | 0.60 | section |
| Lagrange point | related to External links | Lagrange | 0.60 | section |
| Lagrange point | related to External links | European Space Agency | 0.60 | section |
| Lagrange point | related to External links | NASA | 0.60 | section |
| Lagrange point | related to External links | John | 0.60 | section |
| Lagrange point | related to External links | BaezLocations | 0.60 | section |
| Lagrange point | related to External links | David Peter SternAstronomy Cast | 0.60 | section |
| Lagrange point | related to External links | Ep | 0.60 | section |
| Lagrange point | related to External links | Lagrange Points | 0.60 | section |
| Lagrange point | related to External links | Fraser Cain | 0.60 | section |
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