ISBN: | 978-5-5109-8474-3 |
High Quality Content by WIKIPEDIA articles! Differential rotation is seen when different parts of a rotating object move with different angular velocities (rates of rotation) at different latitudes and/or depths of the body and/or in time. This indicates that the object is not solid. In fluid objects, such as accretion disks, this leads to shearing. Galaxies and protostars usually show differential rotation; and examples in our solar system include the Sun, Jupiter and Saturn.