FrameDraggingPhänomene

Frame-dragging, also known as the Lense-Thirring effect, is a phenomenon predicted by Einstein's theory of general relativity. It describes the warping of spacetime caused by the rotation of a massive object, such as a planet or a star. This effect is analogous to the way a spinning object drags the space around it, causing nearby objects to be pulled along in the direction of rotation.

The Lense-Thirring effect was first proposed by Josef Lense and Hans Thirring in 1918, but it was not until the 1960s that it was confirmed through experimental evidence. The effect is relatively weak and has only been observed in the vicinity of massive, rapidly rotating objects, such as neutron stars and black holes. It has been studied using various methods, including gravitational wave detection and the analysis of the orbits of satellites and other celestial bodies.

Frame-dragging has important implications for our understanding of the universe. It provides further evidence for the validity of general relativity and helps to explain the behavior of celestial bodies in strong gravitational fields. Additionally, it has practical applications in fields such as satellite navigation and the design of spacecraft trajectories.

Despite its importance, the Lense-Thirring effect remains a topic of ongoing research. Scientists continue to study this phenomenon to gain a deeper understanding of the fundamental nature of spacetime and the forces that shape our universe.