Axial parallelism

Axial parallelism (also called gyroscopic stiffness, inertia or rigidity, or "rigidity in space") is the characteristic of a rotating body in which the direction of the axis of rotation remains fixed as the object moves through space. In astronomy, this characteristic is found in astronomical bodies in orbit. It is the same effect that causes a gyroscope's axis of rotation to remain constant as Earth rotates, allowing the devices to measure Earth's rotation.^[1]

^ Kumar, B.; DeRemer, D.; Marshall, D. (2005). An Illustrated Dictionary of Aviation. McGraw-Hill Education. p. 326. ISBN 978-0-07-139606-6. Retrieved 2022-12-03. Because of rigidity in space, a gyroscope does not tilt its axis of rotation as the earth rotates.

[Kumar_DeRemer_Marshall_2005_p.-1] Kumar, B.; DeRemer, D.; Marshall, D. (2005). An Illustrated Dictionary of Aviation. McGraw-Hill Education. p. 326. ISBN 978-0-07-139606-6. Retrieved 2022-12-03. Because of rigidity in space, a gyroscope does not tilt its axis of rotation as the earth rotates.

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