General Relativity is Einstein’s theory explaining gravity not as a force, but as the effect of mass and energy bending the fabric of spacetime. Massive objects like stars and planets curve spacetime around them, and this curvature guides the motion of other objects, causing what we perceive as gravitational attraction. The theory revolutionized our understanding of the universe, predicting phenomena like black holes, gravitational waves, and the bending of light near massive bodies.
General Relativity is Einstein’s theory explaining gravity not as a force, but as the effect of mass and energy bending the fabric of spacetime. Massive objects like stars and planets curve spacetime around them, and this curvature guides the motion of other objects, causing what we perceive as gravitational attraction. The theory revolutionized our understanding of the universe, predicting phenomena like black holes, gravitational waves, and the bending of light near massive bodies.
What is General Relativity?
General Relativity is Einstein's theory that gravity arises from mass-energy bending spacetime, and that objects move along the straightest possible paths (geodesics) in that curved geometry rather than being pulled by a force.
How does mass-energy bend spacetime?
Mass and energy tell spacetime how to curve; the greater the mass-energy, the stronger the curvature, which changes how nearby objects and light move.
What is a geodesic, and how does it relate to gravity?
A geodesic is the straightest path through curved spacetime; freely falling objects follow geodesics, so gravity is explained by geometry rather than a force.
How does curved spacetime explain orbits and light bending?
Planets follow geodesics around massive bodies to form orbits, and light also follows curved spacetime, leading to phenomena like gravitational lensing and gravitational time dilation near massive objects.