한국어로 읽기 Secrets of Spacetime and Black Holes

All scenes › Chapter 3 Strong gravity slows time

Light bends too

What the 1919 eclipse showed

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Starlight passing the Sun

When spacetime bends, light follows the bend too. Light from a star just behind the Sun bends slightly as it passes the Sun, then reaches our eyes. So the star looks a little farther out than where it really is. During a total solar eclipse in 1919, astronomers photographed stars next to the Sun and confirmed this prediction.

Why?Normally the Sun is far too bright for us to see the stars right next to it. Only during a total eclipse, when the Moon covers the Sun completely, could those stars be photographed.

Learn moreLight grazing the edge of the Sun bends by about 1.75 arcseconds. One arcsecond is a tiny angle, one degree divided by 3,600, so the screen exaggerates it hugely. Very heavy things like galaxies can bend the light of galaxies behind them so much that they look like rings. This is called gravitational lensing.

Clock we are watching
A clock on the Sun’s surface
How much slower
About 0.2 s slower per day
Clock rate
0.9999979

seconds this clock ticks while a clock far away in empty space ticks one second · calculated with the formulas of relativity

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Wikipedia: Eddington experiment · Wikipedia: Gravitational lens

More in the series

The numbers come from the textbook formulas of relativity (for a non-spinning, ball-shaped mass) and official constants. Sizes, depths and angles in the 3D view are exaggerated so you can see them.