Theory of General Relativity
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science20th Century

Theory of General Relativity

Year1915
LocationBerlin, Germany / Zurich, Switzerland
Key figuresAlbert Einstein, Arthur Eddington
Impact
97
Difficulty
100

Context

Newton's law of universal gravitation had reigned for over 200 years, but it couldn't explain certain anomalies, like the precession of Mercury's orbit. Einstein, already famous for special relativity (1905), spent a grueling decade developing a more comprehensive theory that would reconcile gravity with the geometry of space and time.

The Deed

Einstein presented his field equations to the Prussian Academy of Sciences in November 1915. The mathematics were extraordinarily complex, replacing Newton's gravitational force with the curvature of four-dimensional spacetime. The theory made bold predictions: light should bend around massive objects, time should slow near gravity wells, and gravitational waves should ripple through space. In 1919, Eddington's observations during a solar eclipse confirmed the light-bending prediction, making Einstein an overnight global celebrity.

Why It Matters

General relativity is one of the two pillars of modern physics (alongside quantum mechanics). GPS satellites must correct for relativistic time dilation or they'd drift by 10 kilometers per day. The theory predicted black holes, gravitational lensing, and the expansion of the universe, all later confirmed. LIGO's 2015 detection of gravitational waves opened an entirely new window on the cosmos.

Brutal Truth

Einstein spent the last 30 years of his life trying to unify general relativity with quantum mechanics and failed. The two theories remain fundamentally incompatible. Despite its elegance, general relativity breaks down at singularities and cannot explain dark energy or dark matter, which make up 95% of the universe.

By the Numbers

  • 10 years of work to develop the theory
  • GPS would drift 10 km/day without relativistic corrections
  • Gravitational waves detected in 2015, 100 years after prediction
  • Mercury's orbital precession: 43 arcseconds per century, exactly as predicted
physicsgravityspacetimeNobel Prize

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