The Euler (or Eulerian) angles, usually designated

,

, and

, uniquely determine the orientation of a rigid body in three-dimensional space. There are several conflicting conventions for defining the Euler angles, depending on the choice of axes and the order in which rotations about these axes are performed. This Demonstration uses the convention described in
MathWorld, hyperlinked below in Related Links. For topical relevance, NASA's space shuttle is chosen as the rigid body. The angles

and

are analogous to the spherical polar coordinates orienting the main axis of the shuttle, while

describes rotation about this axis. The ranges of the three Euler angles are given by:

,

, and

. In aeronautic or astronautic terminology, the angles

,

, and

are known as pitch, yaw, and roll, respectively. The corresponding motions of a rigid body are termed nutation, precession and intrinsic rotation.
Any rotation of a rigid body can be represented as the product of three successive rotations

, with matrix representations
and successive rotations obey the algebra of quaternion multiplication. The same combination rule pertains to a linear combination of Pauli spin matrices:

, where

is the 2×2 unit matrix and

means

.