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Home » 2015 » November » 17 » Einstein taught us: It’s all ‘relative’
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Einstein taught us: It’s all ‘relative’

Einstein taught us: It’s all ‘relative’

space time

While still a relatively young scientist, Albert Einstein painted a new picture of the universe. Some of his final brush strokes emerged on November 4, 1915 — a century ago today. That’s when this physicist shared the first of four new papers with the Prussian Academy in Berlin, Germany. Together, those new papers would outline what would be his general theory of relativity.

Before Einstein came along, scientists believed that space always stayed the same. Time moved at a rate that never changed. And gravity pulled massive objects toward each other. Apples fell from trees to the ground because of the Earth’s strong pull.

All of those ideas came from the mind of Isaac Newton, who wrote about them in a famous 1687 book. Albert Einstein was born 192 years later. He grew up to show that Newton was wrong. Space and time were not unvarying, as Newton had described them. And Einstein had a better idea about gravity.

Earlier, Einstein had discovered that time does not always flow at the same rate. It slows down if you are moving very fast. If you were traveling at high speed in a spaceship, any clocks onboard or even your pulse rate would slow down compared with your friends back home on Earth. That clock-slowing is part of what Einstein called his special theory of relativity.


black hole

An artist’s drawing of a black hole named Cygnus X-1. It formed when a large star caved in. It’s seen here pulling in matter from a nearby blue star. Black holes are so massive that nothing can escape their gravitational clutches.


Later, Einstein would realize that space, too, was not always constant. It changed notably in the neighborhood of very massive objects, such as a planet, the sun or a black hole. So a spaceship — or even a ray of light — would move on a curved line through space as it neared a massive object. And that was because that massive object had contorted the shape of the space.


Einstein also showed that the way mass alters space makes bodies move as if they were pulling upon each other, just as Newton had described. So Einstein’s theory was a different way of describing gravity. But it was also a more accurate one. Newton’s idea worked when gravity is not especially strong on all scales, such as near the sun or maybe a black hole. Einstein’s descriptions, by contrast, would work even in these environments.

It took several years for Einstein to figure all of this out. He had to learn new kinds of math. And his first try didn’t really work. But finally, in November 1915, he found the right equation for describing gravity and space. He called this new idea for gravity the general theory of relativity.

Relativity is the key word here. Einstein’s math had indicated that time would not seem to slow down to an observer who was speeding along. It only showed up by comparing that person’s time relative to what it was back on Earth.

Nor was time the only thing that could stretch with relativity. In Einstein’s theory, time and space are closely related. So events in the universe are referred to as locations in spacetime. Matter moves through spacetime along curving pathways. And those pathways are created by the effect of matter on spacetime.

Today scientists believe that Einstein’s theory is the best way to describe not only gravity, but also the entire universe.

Strange — but very useful

Relativity sounds like a very strange theory. So why did anyone believe it? At first, many people didn’t. But Einstein pointed out that his theory was better than Newton’s theory of gravity because it solved a problem about the planet Mercury.

Astronomers keep good records about the orbits of planets moving about the sun. Mercury’s orbit puzzled them. Each trip around the sun, Mercury’s closest approach was a little beyond where it had been the orbit before. Why would the orbit change like that?

Some astronomers said that gravity from other planets must be tugging on Mercury and shifting its orbit a bit. But when they did the calculations, they found that gravity from the known planets couldn’t explain all of the shift. So some thought there might be another planet, closer to the sun, that also tugged on Mercury.



Photo of the planet Mercury passing between the Earth and Sun. Mercury appears as a small black dot silhouetted against the sun’s brilliant surface.


Einstein disagreed, arguing there was no other planet. Using his theory of relativity, he calculated how much Mercury’s orbit should shift. And it was exactly what astronomers had measured.


Still, this did not satisfy everyone. So Einstein recommended another way that scientists might test his theory. He pointed out that the sun’s mass should bend the light from a distant star slightly as its beam passed near to the sun. That bending would make the star’s position in the sky look like it was slightly moved from where it would usually be. Of course, the sun is too bright to see stars just beyond its edges (or anywhere when the sun is shining). But during a total eclipse, the sun’s intense light briefly becomes masked. And now stars become visible.

In 1919, astronomers trekked to South America and Africa to view a total eclipse of the sun. To test Einstein’s theory, they measured the locations of some stars. And the shift in the stars’ location was just what Einstein’s theory had predicted.

From then on, Einstein would be known as the man who replaced Newton’s theory of gravity.

Newton is still mostly right.

Newton’s theory still works pretty well in most instances. But not for everything. For example, Einstein’s theory called for gravity to slow down some clocks. A clock on a beach should tick just a bit slower than one on a mountaintop, where gravity is weaker.



The May 29, 1919, solar eclipse taken by the British astronomer Arthur Eddington on Principe Island, Gulf of Guinea. The stars he saw during this eclipse (not visible in this image) confirmed Einstein's theory of general relativity. Stars near the sun appeared slightly shifted because their light had been curved by the sun’s gravitational field. This shift is only noticeable when the sun's brightness does not obscure the stars, as during this eclipse.


It’s not a big difference, and not even important if all you want to know is when it’s time for lunch. But it can matter big-time for things like the GPS devices you might have seen in cars that give driving directions. These global-positioning-system devices pick up signals from satellites. A GPS device can identify where you are by comparing the differences in the time it takes for a signal to arrive from each of several satellites. Those times have to be adjusted for the way time slows down on the ground compared to in space. Without adjusting for that effect of general relativity, your location could be off by more than a mile. Why? The mismatch in time would grow, second by second, since the ground clock and the satellite’s clock were keeping time at different rates.


But the benefits of general relativity go far beyond just helping us stay on the right road. It helps science explain the universe.

Early on, for instance, scientists studying general relativity realized that the universe might be getting bigger all the time. Only later would astronomers show that the universe actually is expanding. The math used to explain general relativity also led experts to foresee that fantastic objects like black holes could exist. Black holes are regions of space where gravity is so strong that nothing can escape, even light. Einstein’s theory also suggests that gravity can create ripples in space that speed across the universe. Scientists have built huge structures using lasers and mirrors to try to detect those ripples, known asgravitational waves.

Einstein didn’t know about such things as gravitational waves and black holes when he started working on his theory. He was just interested in trying to figure out gravity. Finding the right math to describe gravity, he reasoned, would make sure that scientists could find laws of motion that would not depend on how anybody was moving.

And it makes sense, when you think about it.

The laws of motion should be able to describe how matter moves, and how that motion is affected by forces (such as gravity or magnetism).

Gravity = acceleration?

But what happens when it is two people that are moving in different speeds and directions? Would both use the same laws to describe what they see? Think about it: If you’re riding on a merry-go-round, the movements of people nearby look very different from what they look like to someone standing still.

In his first theory of relativity (known as the “special” one) Einstein showed that two people in motion could both use the same laws — but only as long as each was moving in straight lines at a constant speed. He couldn’t figure out how to make one set of laws work when people moved in a circle or changed speed.

Then he found a clue. One day he was looking out of his office window and imagined someone falling off the roof of a nearby building. Einstein realized that, while falling, that person would feel weightless. (Please do not try jumping off a building to test this, though. Take Einstein’s word for it.)

To someone on the ground, gravity would appear to make the person fall faster and faster. In other words, the speed of their fall would accelerate. Gravity, Einstein suddenly realized, was the same thing as acceleration!

Imagine standing on the floor of a rocket ship. There are no windows. You feel your weight against the floor. If you try to lift your foot, it wants to go back down. So maybe your ship is on the ground. But it is also possible that your ship might be flying. If it is moving upward at a faster and faster speed — accelerating smoothly by just the right amount — your feet will feel pulled to the floor just as they had when the ship was sitting on the ground.


spacetime curvature

Artwork illustrating the curvature of spacetime due to the presence of celestial bodies. As predicted by Einstein, the mass of Earth and its moon creates gravitational dips in the fabric of spacetime. That spacetime is shown here on a two-dimensional grid (with gravitational potential represented by a third dimension). In the presence of a gravitational field, spacetime becomes warped, or curved. So the shortest distance between two points usually is not a straight line but a curved one.


Once Einstein realized that gravity and acceleration are one and the same, he thought he could find a new theory of gravity. He just had to find the math that would describe any possible acceleration for any object. In other words, no matter how the motions of objects appeared from one point of view, you would have a formula to describe them just as correctly from any other point of view.


Finding that formula did not prove easy.

For one thing, objects moving through space with gravity don’t follow straight lines. Imagine an ant walking across a sheet of paper without changing direction. Its path should be straight. But suppose there’s a bump in the path because a marble is under the paper. When walking over the bump, the ant’s path would curve. The same thing happens to a beam of light in space. A mass (like a star) makes a “bump” in space just like the marble under the paper.

Because of this effect of mass on space, the math for describing straight lines on a flat sheet of paper doesn’t work anymore. That flat-paper math is known as Euclidean geometry. It describes things like shapes made from segments of lines and angles where lines cross. And it works fine on flat surfaces, but not on bumpy surfaces or curved surfaces (such as the outside of a ball). And it doesn’t work in space where mass makes space bumpy or curved.

So Einstein needed a new kind of geometry. Luckily, some mathematicians had already invented what he needed. It is called, not surprisingly, non-Euclidean geometry. At the time, Einstein didn’t know anything about it. So he got help from a math teacher from his school days. With his new knowledge about this improved geometry, Einstein was now able to move ahead.

Until he got stuck again. That new math worked for many points of view, he found, but not all possible ones. He concluded that this was the best he — or anybody — could do. Nature just wouldn’t allow the complete theory of gravity that Einstein wanted.

Or so he thought.

But then he got a new job. He moved to Berlin, to a physics institute where he did not have to teach. He could spend all of his time thinking about gravity, undistracted. And, here, in 1915, he saw a way to make his theory work. In November, he wrote four papers outlining the details. He presented them to a major German science academy.  

The really big picture

Soon afterwards, Einstein began thinking about what his new theory of gravity would mean for understanding the whole universe. To his surprise, his equations suggested that space could be expanding or shrinking. The universe would have to be getting bigger or it would collapse as gravity pulled everything together. But at that time, everybody thought the size of the universe today was as it had always been and always would be. So Einstein tweaked his equation to make sure the universe would stay still.

Years later, Einstein admitted that had been a mistake. In 1929, the American astronomer Edwin Hubble discovered that the universe truly is expanding. Galaxies, huge clumps of stars, flew apart from each other in all directions as space expanded. This meant that Einstein’s math had been right the first time.

Based largely on Einstein’s theory, astronomers today have figured out that the universe we live in began in a big explosion. Called the Big Bang, it took place almost 14 billion years ago. The universe started out tiny but has been growing bigger ever since.



Born in 1879, Albert Einstein was 36 years old when he issued the papers that would describe general relativity and soon change how the world viewed both space and time. Six years later he would claim the 1921 Nobel Prize in physics (although it wouldn’t be issued to him until 1922). He did not win for relatively but instead for what the Nobel Committee described as “his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect.”


Over the years, many experiments and discoveries have shown that Einstein’s theory is the best explanation that scientists have for gravity and many features of the universe. Weird things in space, like black holes, were predicted by people studying general relativity long before astronomers discovered them. Whenever new measurements are made of things like the bending of light or the slowing of time, general relativity’s math always gets the right answer.


Clifford Will works at the University of Florida, in Gainesville, where is an expert on relativity. “It is remarkable that this theory, born 100 years ago out of almost pure thought, has managed to survive every test,” he has written.

Without Einstein’s theory, scientists wouldn’t understand very much about the universe at all.

Yet when Einstein died, in 1955, very few scientists were studying his theory. Since then, the physics of general relativity has grown to become one of the most important theories in the history of science. It helps scientists explain not only gravity, but also how the whole universe works. Scientists have used general relativity to map how matter is arranged in the universe. It’s also used to study the mysterious “dark matter” that doesn’t shine like stars. General relativity’s effects also help in the search for faraway worlds now known as exoplanets.

“The implications for the further reaches of the universe,” the famous physicist Stephen Hawking once wrote, “were more surprising than even Einstein ever realized.”

Power Words

(for more about Power Words, click here)

acceleration    A change in the speed or direction of some object.

astronomy    The area of science that deals with celestial objects, space and the physical universe. People who work in this field are called astronomers.

Big Bang  The rapid expansion of dense matter that, according to current theory, marked the origin of the universe. It is supported by physics’ current understanding of the composition and structure of the universe.

black hole  A region of space having a gravitational field so intense that no matter or radiation (including light) can escape.

dark matter  Physical objects or particles that emit no detectable radiation of their own. They are believed to exist because of unexplained gravitational forces that they appear to exert on other, visible astronomical objects.

eclipse    The temporary masking of one celestial body (such as the sun or moon) by another passing in front of it (from our vantage point on Earth). An eclipse can be full, where the more distant object totally disappears for a time, or partial, where some part of it remains visible at all times to viewers on Earth.

equation  In mathematics, the statement that two quantities are equal. In geometry, equations are often used to determine the shape of a curve or surface.

Euclid   A famous ancient mathematician born around 325 B.C. and who has come to be known as the father of geometry. He taught in Alexandria, Egypt, and wrote a book that would serve as the foundation for mathematical teaching over the next two millennia. It was known simply as The Elements.

Euclidian geometry  It describes the mathematical relationships between points, lines and other shapes on a flat plane. For instance, it showed that in this environment, the shortest path between two points is a straight line; the sum of all angles in any triangle equals 180 degrees; and that parallel lines will never cross, no matter how long they are extended.

geometry   The mathematical study of shapes, especially points, lines, planes, curves and surfaces.

global positioning system  Best known by its acronym GPS, this system uses a device to calculate the position of individuals or things (in terms of latitude, longitude and elevation — or altitude) from any place on the ground or in the air. The device does this by comparing how long it takes signals from different satellites to reach it.

gravity waves (also known as gravitational waves) Ripples in the fabric of space that are produced when masses undergo sudden acceleration. Some are believed to have been unleashed during the Big Bang, when the universe got its explosive start.

gravity Schools tend to teach that gravity is the force that attracts anything with mass, or bulk, toward any other thing with mass. The more mass that something has, the greater its gravity. But Einstein’s general theory of relativity redefined it, showing that gravity is not an ordinary force, but instead a property of space-time geometry. Gravity essentially can be viewed as a curve in spacetime, because as a body moves through space, it follows a curved path owing to the far greater mass of one or more objects in its vicinity.

Isaac Newton    This English physicist and mathematician became most famous for describing his law of gravity. Born in 1642, he developed into a scientist with wide-ranging interests. Among some of his discoveries: that white light is made from a combination of all the colors in the rainbow, which can be split apart again using a prism; the mathematics that describe the orbital motions of things around a center of force; that the speed of sound waves can be calculated from the density of air; early elements of the mathematics now known as calculus; and an explanation for why things “fall:” the gravitational pull of one object towards another, which would be proportional to the mass of each. Newton died in 1727.

laser  A device that generates an intense beam of coherent light of a single color. Lasers are used in drilling and cutting, alignment and guidance, in data storage and in surgery.

magnetism  The attractive influence, or force, created by certain materials, called magnets, or by the movement of electric charges.

mass A number that shows how much an object resists speeding up and slowing down — basically a measure of how much matter that object is made from. 

matter Something which occupies space and has mass. Anything with matter will weigh something on Earth.

orbit  The curved path of a celestial object or spacecraft around a star, planet or moon. One complete circuit around a celestial body.

physics     The scientific study of the nature and properties of matter and energy. Classical physics is an explanation of the nature and properties of matter and energy that relies on descriptions such as Newton’s laws of motion. Quantum physics, a field of study which emerged later, is a more accurate way of  explaining the motions and behavior of matter. A scientist who works in that field is known as a physicist.

planet   A celestial object that orbits a star, is big enough for gravity to have squashed it into a roundish balland it must have cleared other objects out of the way in its orbital neighborhood. To accomplish the third feat, it must be big enough to pull neighboring objects into the planet itself or to sling-shot them around the planet and off into outer space. Astronomers of the International Astronomical Union (IAU) created this three-part scientific definition of a planet in August 2006 to determine Pluto’s status. Based on that definition, IAU ruled that Pluto did not qualify. The solar system now includes eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

relativity    A theory developed by physicist Albert Einstein showing that neither space nor time are constant, but instead affected by one’s velocity and and the mass of things in your vicinity.

satellite     A moon orbiting a planet or a vehicle or other manufactured object that orbits some celestial body in space.

spacetime   A term made essential by Einstein’s theory of relativity, it describes a designation for some spot given in terms of its three-dimensional coordinates in space, along with a fourth coordinate corresponding to time.

star  Thebasic building block from which galaxies are made. Stars develop when gravity compacts clouds of gas. When they become dense enough to sustain nuclear-fusion reactions, stars will emit light and sometimes other forms of electromagnetic radiation. The sun is our closest star.

theory  (in science)  A description of some aspect of the natural world based on extensive observations, tests and reason. A theory can also be a way of organizing a broad body of knowledge that applies in a broad range of circumstances to explain what will happen. Unlike the common definition of theory, a theory in science is not just a hunch. Ideas or conclusions that are based on a theory — and not yet on firm data or observations — are referred to as theoretical. Scientists who use mathematics and/or existing data to project what might happen in new situations are known as theorists.

universe The entire cosmos: All things that exist throughout space and time. It has been expanding since its formation during an event known as the Big Bang, some 13.8 billion years ago (give or take a few hundred million years).

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