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Theorem

Euler's Rotation Theorem

Geometry

Euler's rotation theorem is a result in geometry stating that any displacement of a rigid body in three dimensional space that leaves one point fixed is equivalent to a single rotation about some axis running through that fixed point. Leonhard Euler proved the result in 1775 using spherical geometry. Composing two such rotations yields another rotation, giving the set of rotations a group structure known as the rotation group, and in linear algebra terms a non identity rotation matrix has one eigenvalue equal to one, whose eigenvector marks the axis of rotation, with the other two eigenvalues either complex conjugates or both equal to minus one. This description is adapted from Wikipedia contributors under CC BY-SA 4.0; changes were made. https://creativecommons.org/licenses/by-sa/4.0/

Connections

Named After

Leonhard Euler, Mathematicians

Derived from the theorem's own name (unambiguous possessive-token match to exactly one live mathematician entity, w-bfill-g5-0924 browse backfill)

Sources
Euler's rotation theorem (Wikipedia)
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