Gravitational Redshift
Predicts that gravity should shift the frequency of light, later called gravitational redshift.
Albert Einstein ยท Source topic
49 Einstein records classified as Astronomy in the supplied World History Database data.

Predicts that gravity should shift the frequency of light, later called gravitational redshift.
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.
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.
During work recorded in a 1912 notebook, Einstein calculated how a foreground mass could bend light from a background source and produce the geometry of a gravitational lens.
Einstein's notebook analysis showed that gravitational deflection could allow light from one distant source to reach an observer along two paths, producing two apparent images.
Einstein worked out a magnification relation for the gravitational-lens configuration, anticipating formulae he would publish when he returned to the subject decades later.
Encourages astronomical testing of gravitational light deflection during a solar eclipse.
Works with Michele Besso on applying the developing gravitational theory to Mercury's orbit, creating calculations that later help solve the perihelion anomaly.
Einstein and Michele Besso calculated Mercury's anomalous perihelion motion with the provisional gravitational theory, creating a detailed test that the Entwurf equations failed to reproduce correctly.
With the completed geometric treatment of gravity, Einstein obtained a solar light-deflection prediction approximately twice the value produced by his earlier equivalence-principle calculation.
Using the completed theory, obtains the full gravitational deflection predicted for starlight grazing the Sun, approximately twice his earlier 1911 estimate.
The relativistic Mercury calculation matched the anomalous perihelion advance using the gravitational theory itself rather than introducing an additional planet or an adjustable correction to Newtonian gravity.
Explains Mercury's anomalous perihelion advance using the emerging general theory of relativity.
Einstein used the emerging general theory to account for Mercury's unexplained perihelion advance, obtaining the observed residual shift that earlier gravitational models had failed to reproduce.
Einstein mentioned the possibility of gravitational lensing in a letter to Heinrich Zangger, revisiting the double-image effect he had calculated in his 1912 notebook.
Predicts gravitational waves as propagating disturbances in spacetime within general relativity.
Einstein adds the cosmological constant to his gravitational field equations to permit a static universe, creating the mathematical term later associated with dark energy.
To support a static cosmological solution, Einstein modified the gravitational field equations with an additional cosmological term that could counterbalance large-scale attraction.
Einstein designed his early relativistic cosmology partly around the hope that inertia would be determined by the overall distribution of matter, reflecting his interpretation of Mach's ideas.
Applies general relativity to the universe and introduces the cosmological constant in a static cosmological model.
Einstein interprets the cosmological constant as a repulsive contribution capable of balancing ordinary gravitational attraction on the largest cosmic scales.
Einstein applied general relativity to the universe as a whole and proposed a spatially closed, homogeneous model intended to remain static on cosmic scales.
Refines gravitational-wave theory and derives the quadrupole form for radiated energy.
British eclipse expeditions photograph stars near the Sun to test Einstein's predicted gravitational deflection.
The total solar eclipse provides observations designed to test the bending of starlight predicted by Einstein's general theory of relativity.
Royal Society and Royal Astronomical Society report eclipse results supporting Einstein's general relativity.
A total solar eclipse expedition at Wallal obtains measurements of gravitational light deflection that provide another observational test of Einstein's relativity prediction.
The Einstein Tower begins operation as a solar observatory designed to test relativistic effects.
Receives the Royal Astronomical Society Gold Medal for relativity and the theory of gravitation.
Adopts an expanding cosmological model and abandons the need for his earlier static-universe construction.
Publishes a non-static cosmological model within general relativity, accepting cosmic expansion and dispensing with the static balance that motivated his cosmological constant.
Receives the Prix Jules Janssen for distinguished work in astronomy and astrophysics.
Einstein abandons the need for a static cosmological model after cosmic expansion becomes established, leaving the cosmological constant without its original motivation.
Abandons his earlier static cosmological model as expanding-universe observations and relativistic cosmology make a dynamical universe the more credible interpretation.
Visits Mount Wilson and discusses observational cosmology, confronting evidence that distant galaxies exhibit the redshift-distance relation associated with cosmic expansion.
With Willem de Sitter, proposes a spatially flat expanding cosmological model without a cosmological constant, providing a simple benchmark solution of general relativity.
With Willem de Sitter, proposes a simple expanding cosmological model with zero cosmological constant.
Einstein showed that exact alignment of source, lens and observer produces a circular image geometry, the configuration later widely known as an Einstein ring.
Publishes a calculation showing how a foreground star can gravitationally lens light from a background star.
Einstein published a short analysis of the lens-like action of a foreground star, giving a compact treatment of image formation and magnification caused by gravitational light bending.
After discussions with Rudi Mandl, Einstein returned to the lensing calculation he had explored in 1912 and agreed to publish the optical effect of gravitational light bending.
Einstein quantified the magnification produced by gravitational deflection in a simple stellar-lens geometry, linking image brightness to the angular alignment of source and lens.
Einstein's lensing note described how imperfect alignment can produce two apparent images of a background star because its light reaches the observer along different curved paths.
Publishes a calculation of the lens-like action of a star's gravitational field, describing how general relativity can produce multiple or magnified images of a background source.
Einstein and Rosen publish a corrected paper showing cylindrical gravitational-wave solutions.
Studies a stationary spherical system of gravitating particles and argues that such configurations do not naturally form the Schwarzschild-type singular surface then under discussion.
Comments on Kurt Godel's rotating cosmological solution, acknowledging that general relativity permits global spacetime structures with profound consequences for the concept of time.