How to Understand Einstein's Theory of Gravity

Einstein's general relativity may be complicated, but it's our best way of understanding the universe.

By Devin Powell
May 24, 2019 3:01 PMApr 26, 2020 9:28 PM
Einstein Ring, Hubble - NASA
A phenomenon known as an "Einstein Ring" created when light is bent by gravity around a large object. In this case, the large red galaxy in the middle is causing light from a much more distant blue galaxy directly behind it to be bent around into the shape of a ring. (Credit: ESA/Hubble/NASA)


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An astronaut wakes up in a spaceship, with no memory of how she got there. Sitting alone in a chair, she wonders: “Where in the universe am I?”

The ship has no windows. Its instruments are dead. The only clue is the push of the chair against her body. Phew, there’s gravity, she thinks. Her vessel must still be on Earth.

But then a second possibility occurs to her. The ship could be accelerating through space, pressing her into the seat like a race car picking up speed. From inside the vessel, there is — terrifyingly — no way to tell.

This spacefarer’s dilemma would have been familiar to Albert Einstein. His 1915 general theory of relativity built on the notion that gravity and acceleration are not just easily confused, but are one and the same. This equivalence, “the happiest thought” of Einstein’s life, was his starting point for redefining gravity.

General relativity grew out of Einstein’s theory of special relativity, which describes how the speed of light (in a vacuum) can always be constant.

According to relativity, anything that can happen inside of a box picking up speed — i.e., accelerating — also happens in the presence of gravity. Imagine, for example, a horizontal laser inside an elevator that’s accelerating upward. As the light travels sideways, the elevator rises, causing the beam to strike a spot on the wall slightly lower than where it started. If the elevator accelerates quickly enough, the beam visibly bends toward the floor.

Einstein showed the same thing happens to a beam inside a stationary elevator within a powerful gravitational field; the gravity bends the light. Similarly, he expected a beam of starlight should bend when passing through the sun’s gravity. This prediction proved correct when the stars moved during the 1919 solar eclipse.

Relativity describes why a clock on a satellite ticks a few dozen microseconds faster than a clock on Earth; without accounting for that discrepancy, GPS technologies wouldn’t work.

To link acceleration and gravity in this way, Einstein overthrew one of his own heroes: Isaac Newton. You may have learned that Newton described gravity as a force, an invisible rubber band that pulls together objects with mass. Newton’s math did a good job at predicting how everything from projectiles to planets moved — but it kept gravity separate from acceleration.

Einstein argued that gravity isn’t a force at all. He described it as a curvature of time and space caused by mass and energy. Confused? The German physicist was, too, and he struggled with the theory for nearly a decade. He got help from mathematician Marcel Grossmann, an old friend who shared his notes when a young Einstein skipped class.

Their math, laid down in 10 equations, explained how gravity could move around objects via a warped reality, accelerating without ever feeling any mysterious Newtonian forces.

An apple feeling no force usually stays in the same place (left). But when gravity curves space and time (right), as Einstein's general theory of relativity predicts, the fruit winds up on the ground without feeling a force. (Credit: Alison Mackey/Discover; Collage elements: Envato Elements, Vanatchanan/Shutterstock)

The Relative Basics

The main takeaways behind Einstein’s general theory of relativity:

1. Time and space are neither flat nor fixed; they are curved and distorted by mass and energy.

2. Gravity is not a force, but rather a distortion of time and space.

3. The effects of gravity are indistinguishable from the effects of acceleration, over a small space.

Einstein's inspiration for general relativity struck while he was a patent clerk in Switzerland in 1907. (Credit: Heritage Image Partnership Ltd/Alamy Stock Photo)

Einstein’s Peculiar Predictions

Relativity makes numerous bizarre predictions, many of them experimentally verified. They only seem bizarre because we don’t notice them in our daily lives — we live, for the most part, in Newton’s reality. But beyond that lies Einstein’s universe, where gravity bends space and time to its will. Here are some of the theory’s strangest side effects:

  • Gravity literally slows down time. Waves of light emitted by stars stretch out because of this time bending, and objects closer to a massive object age more slowly. Super-precise clocks, which tick according to the vibrations of atoms, have verified that gravity alters time’s flow.

  • Satellites have shown that rotating celestial bodies twirl the fabric of the cosmos around themselves, like honey twisted by a spoon, affecting the motion of gyroscopes.

  • One prediction solved a long-standing dilemma, a weird wobble in Mercury’s orbit that Newton’s math couldn’t account for. (Astronomers had initially blamed a hidden planet called Vulcan.) Relativity explained the wonky orbit in terms of the warping of space by the sun’s powerful gravity.

  • Tiny ripples in reality, caused by colliding black holes, have tripped sensors in highly sensitive instruments buried underground on Earth.

This story originally appeared in print as "It's All Relative."

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