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Timeline of Gravitational Physics and Relativity

  • 1640 – Ismael Bullialdus suggests an inverse-square gravitational force
    law
  • 1665 – Isaac Newton deduces the inverse-square gravitational force law
    from the “falling” of the Moon
  • 1684 – Isaac Newton proves that planets moving under an inverse-square
    force law will obey Kepler’s laws
  • 1686 – Isaac Newton uses a fixed length pendulum with weights of
    varying composition to test the weak equivalence principle to 1 part in
    1000
  • 1798 – Henry Cavendish measures the gravitational constant
  • 1846 – Urbain Le Verrier and John Couch Adams, studying Uranus orbit,
    independently prove that another, farther planet must exist. The planet
    will be found at the predicted moment and position, and will be called
    Neptune.
  • 1855 – Leverrier observes a 35″ per century excess precession of
    Mercury’s orbit and attributes it to another planet, inside Mercury’s
    orbit. The planet will never be found.
  • 1876 – William Clifford suggests that the motion of matter may be due
    to changes in the geometry of space
  • 1882 – Simon Newcomb observes a 43 per century excess precession of
    Mercury’s orbit
  • 1887 – Albert Michelson and Edward Morley in their experiment do not
    detect the ether drift
  • 1889 – Roland von Eotvos uses a torsion fiber balance to test the weak
    equivalence principle to 1 part in one billion
  • 1893 – Ernst Mach states Mach’s principle; first constructive attack on
    the idea of Newtonian absolute space
  • 1905 – Albert Einstein completes his theory of special relativity and
    states the law of mass-energy conservation: E=mc2
  • 1907 – Albert Einstein introduces the principle of equivalence of
    gravitation and inertia and uses it to predict the gravitational
    redshift
  • 1915 – Albert Einstein completes his theory of general relativity. The
    new theory perfectly matches Mercury’s strange motions that baffled
    Urbain Le Verrier.
  • 1916 – Albert Einstein shows that the field equations of general
    relativity admit wavelike solutions
  • 1918 – J. Lense and Hans Thirring find the gravitomagnetic precession
    of gyroscopes in the equations of general relativity
  • 1919 – Arthur Eddington leads a solar eclipse expedition which claims
    to detect gravitational deflection of light by the Sun
  • 1921 – T. Kaluza demonstrates that a five-dimensional version of
    Einstein’s equations unifies gravitation and electromagnetism
  • 1937 – Fritz Zwicky states that galaxies could act as gravitational
    lenses
  • 1937 – Albert Einstein, Leopold Infeld, and Banesh Hoffman show that
    the geodesic equations of general relativity can be deduced from its
    field equations
  • 1957 – John Wheeler discusses the breakdown of classical general
    relativity near singularities and the need for quantum gravity
  • 1960 – Robert Pound and Glen Rebka test the gravitational redshift
    predicted by the equivalence principle to approximately 1%
  • 1962 – Robert Dicke, Peter Roll, and R. Krotkov use a torsion fiber
    balance to test the weak equivalence principle to 2 parts in 100
    billion
  • 1964 – Irwin Shapiro predicts a gravitational time delay of radiation
    travel as a test of general relativity
  • 1965 – Joseph Weber puts the first Weber bar gravitational wave
    detector into operation
  • 1968 – Irwin Shapiro presents the first detection of the Shapiro delay
  • 1968 – Kenneth Nordtvedt studies a possible violation of the weak
    equivalence principle for self-gravitating bodies and proposes a new
    test of the weak equivalence principle based on observing the relative
    motion of the Earth and Moon in the Sun’s gravitational field
  • 1976 – Robert Vessot and Martin Levine use a hydrogen maser clock on a
    Scout Drocket to test the gravitational redshift predicted by the
    equivalence principle to approximately 0.007%
  • 1979 – Dennis Walsh, Robert Carswell, and Ray Weymann discover the
    gravitationally lensed quasar Q0957+561
  • 1982 – Joseph Taylor and Joel Weisberg show that the rate of energy
    loss from the binary pulsar PSR1913+16 agrees with that predicted by
    the general relativistic quadrupole formula to within 5%
  • 2002 – Edward B. Fomalout and Sergei Kopeikin showed that the speed of
    gravity equals the speed of light within the 20% experimental error,
    almost confirming one prediction of loop quantum gravity
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