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  1. Examples of general relativity are1234:
    • Black holes, which are regions of space where gravity is so strong that nothing can escape.
    • Gravitational waves, which are ripples in space-time caused by accelerating masses.
    • Gravitational lensing, which is the bending of light by massive objects.
    • Gravitational time dilation, which is the slowing of time near a strong gravitational field.
    • Gravitational redshift, which is the shift of light to lower frequencies near a strong gravitational field.
    • The orbit of Mercury, which deviates from Newtonian predictions due to the curvature of space-time.
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    General relativity describes new phenomena, which the old Newtonian law of gravity could not predict: examples of this are black holes (in principle, Newtonian gravity can predict they exist, but not describe them to the extent of GR) and gravitational waves (this is a totally unique phenomenon to GR).
    profoundphysics.com/general-relativity-for-dummies/
    Einstein made a series of predictions using General Relativity. For example, using his theory, he explained why Mercury’s orbit drifts – because of this distortion of space-time.
    scienceissimple.com/general-relativity/
    Gravitational time dilation, gravitational lensing, the gravitational redshift of light, gravitational time delay, and singularities/black holes are examples of such differences.
    www.vedantu.com/physics/general-relativity
    General relativity has been experimentally verified by observations of gravitational lenses, the orbit of the planet Mercury, the dilation of time in Earth ’s gravitational field, and gravitational waves from merging black holes.
    www.britannica.com/science/general-relativity
  2. People also ask
    The physical consequences of general relativity are in fact quite applicable to everyday life. Gravitational time dilation turns out to affect the times measured by GPS satellites to non-negligible extents.
    San Francisco: Pearson. General relativity is Einstein's theory of gravity, in which gravitational forces are presented as a consequence of the curvature of spacetime. In general relativity, objects moving under gravitational attraction are merely flowing along the "paths of least resistance" in a curved, non-Euclidean space.
    Further tests of general relativity include precision measurements of the Shapiro effect or gravitational time delay for light, measured in 2002 by the Cassini space probe. One set of tests focuses on effects predicted by general relativity for the behavior of gyroscopes travelling through space.
    Another general feature of general relativity is the appearance of spacetime boundaries known as singularities. Spacetime can be explored by following up on timelike and lightlike geodesics—all possible ways that light and particles in free fall can travel.
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