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Most stars in our Universe are constantly rotating. In the presence of a rotating massive object, such as Earth, the spacetime in its vicinity becomes twisted or dragged along with the rotation of the object. This effect is a consequence of the object's mass and angular momentum warping the fabric of spacetime. As a result, the orientation of nearby objects, including other celestial bodies or even the paths of particles, can be influenced by this dragging of spacetime. This phenomenon is known as frame-dragging.