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Three-body problem, in astronomy, the problem of determining the motion of three celestial bodies moving under no influence other than that of their mutual gravitation.
Lemaître also did research on cosmic rays and on the three-body problem, which concerns the mathematical description of the motion of three mutually attracting bodies in space.
For example, Euler studied the difficult problem of describing the motion of three masses under mutual gravitational attraction (now known as the three-body problem).
The motion of three bodies proved less tractable indeed, nobody could solve the "three-body problem"—and here was Oscar asking for the solution to a ten-body problem (or something like a thirty-body problem if one includes the satellites of the planets and a many-thousand-body problem if one includes asteroids).
Generally, the motion of three bodies is now known to be nonrepeating.
Firstly, the self-synchronization motion of three ERs is analyzed according to self-synchronization theory.
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She sees a bulge in the snake, and the tiny motion of one last featherless nestling still alive at the back of the hole.
As practically attacked, it consists of the problem of determining the perturbations (disturbances) in the motion of one of the bodies around the principal, or central, body that are produced by the attraction of the third.
(b) Particle motion of two horizontal components.
(c) Particle motion of two horizontal components.
More complicated macroscopic motion of two immiscible incompressible liquids is governed by the Muskat problem.
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Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com