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.
Albert Einstein · Place
10 Einstein records associated with Prague.

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.
Derives the expectation that light climbing through a gravitational field should lose frequency, providing an early relativistic prediction of gravitational redshift.
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.
Uses his Prague professorship to intensify work on a relativistic theory of gravitation, concentrating on how acceleration, clocks and light behave in gravity.
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.
Becomes professor of theoretical physics at the German University in Prague.
Urges astronomers to test gravitational light bending during a total solar eclipse, linking his theoretical calculation directly to a possible astronomical observation.
Calculates that the Sun's gravitational field should bend passing starlight, turning the emerging gravitational theory into a prediction accessible to eclipse astronomy.
Predicts that gravity should bend starlight and proposes a solar-eclipse test.