Early Solar Deflection Numerical Estimate
Einstein calculated an early value for the deflection of starlight passing close to the Sun and proposed that a total solar eclipse could make the displacement observable.
Explore 4 historical events and records for Austria-Hungary in 1911.
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Einstein calculated an early value for the deflection of starlight passing close to the Sun and proposed that a total solar eclipse could make the displacement observable.
Einstein encouraged astronomer Erwin Freundlich to pursue eclipse observations capable of testing the predicted gravitational bending of starlight near the Sun.
Einstein argued that clocks deeper in a gravitational field should run more slowly than clocks at higher gravitational potential, giving gravity a measurable effect on elapsed time.
Einstein published a study of how gravitation affects light, deriving observable consequences from the equivalence principle while his full theory of curved spacetime was still incomplete.
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