Light and waves

29 May 1919

Starlight bends

Arthur Eddington, Frank Dyson and the eclipse expeditions

Can the Sun bend starlight?

During a total eclipse, expeditions to Príncipe and Sobral photographed stars near the darkened Sun. Their positions had shifted, as if the Sun’s gravity bent their light by about the amount Einstein predicted. Newspapers made Einstein famous overnight.

How they figured it out

Arthur Eddington, a Quaker who refused to fight in the First World War, championed the work of Einstein, a scientist from an enemy country, while the war was still on. With Astronomer Royal Frank Dyson he planned expeditions for the total eclipse of 29 May 1919: one to the island of Príncipe, one to Sobral in Brazil.

It was cloudy at Príncipe until the last moments. When the results were announced in London in November, newspapers declared a revolution in science, and Einstein became world-famous overnight. Historians have since debated how precise those plates really were; later measurements, especially with radio telescopes, confirmed the bending firmly.

The equation

δθ=4GMc2b≈1.75′′\delta\theta = \frac{4GM}{c^2 b} \approx 1.75''

Light grazing the Sun is bent by about 1.75 arcseconds, twice the simple Newtonian guess.

Everyday echoGalaxies bend light from behind them, acting as giant natural lenses.

See it in real life

The bottom of a wine glass

Look at a candle through the stem and base of a wine glass and you see it smeared into an arc or a ring. Massive galaxies bend the light of galaxies behind them the same way, making rings and arcs astronomers use as natural telescopes.

Where engineers use it

  • Testing predictions

    A clear, risky prediction tested by measurement is how every engineering model earns trust.