The effect where a rotating massive body drags spacetime around it, predicted by Einstein.Frame dragging is a consequence of Einstein's general relativity where a rotating massive body twists the fabric of spacetime around itself. Instead of space being a passive stage, it is dragged along with the rotation, like a whirlpool in a fluid. This effect is also known as the Lense-Thirring effect, named after the physicists who first calculated it in 1918.
The effect was predicted in 1918 by Austrian physicists Josef Lense and Hans Thirring, who derived it from Einstein's field equations. It was later measured precisely by the Gravity Probe B mission, which launched in 2004 and confirmed the effect to within 19% of the predicted value.
In general relativity, mass and energy curve spacetime, and rotation adds a twist to that curvature. A spinning object, such as a planet or a black hole, drags nearby spacetime around with it. This affects the motion of gyroscopes, particles, and even light passing close to the rotating body, causing their paths to deviate from what Newtonian gravity would predict.
Frame dragging is crucial for understanding the behavior of matter around rotating black holes and neutron stars, and it must be accounted for in precise satellite navigation and orbital mechanics.
The Earth's rotation drags spacetime so slightly that a gyroscope in polar orbit would shift its axis by only about 0.000011 degrees per year.








