How far would you have to go to escape gravity? - Rene Laufer

566,272 views ・ 2018-11-06

TED-Ed


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More than six thousand light years
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from the surface of the earth,
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a rapidly spinning neutron star
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called the Black Widow pulsar
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blasts its companion brown dwarf star with radiation
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as the two orbit each other every 9 hours.
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Standing on our own planet,
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you might think you’re just an observer of this violent ballet.
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But in fact, both stars are pulling you towards them.
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And you’re pulling back,
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connected across trillions of kilometers
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by gravity.
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Gravity is the attractive force between two objects with mass—
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any two objects with mass.
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Which means that every object in the universe attracts every other object:
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every star, black hole,
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human being, smartphone, and atom
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are all constantly pulling on each other.
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So why don’t we feel pulled in billions of different directions?
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Two reasons: mass and distance.
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The original equation describing the gravitational force between two objects
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was written by Isaac Newton in 1687.
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Scientists’ understanding of gravity has evolved since then,
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but Newton’s Law of Universal Gravitation
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is still a good approximation in most situations.
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It goes like this:
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the gravitational force between two objects
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is equal to the mass of one
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times the mass of the other,
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multiplied by a very small number
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called the gravitational constant,
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and divided by the distance between them, squared.
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If you doubled the mass of one of the objects,
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the force between them would double, too.
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If the distance between them doubled,
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the force would be one-fourth as strong.
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The gravitational force between you and the Earth pulls you towards its center,
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a force you experience as your weight.
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Let’s say this force is about 800 Newtons
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when you’re standing at sea level.
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If you traveled to the Dead Sea,
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the force would increase by a tiny fraction of a percent.
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And if you climbed to the top of Mount Everest, the force would decrease—
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but again, by a minuscule amount.
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Traveling higher would make a bigger dent in gravity’s influence,
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but you won’t escape it.
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Gravity is generated by variations in the curvature of spacetime—
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the three dimensions of space plus time—
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which bend around any object that has mass.
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Gravity from Earth reaches the International Space Station,
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400 kilometers above the earth,
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with almost its original intensity.
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If the space station was stationary on top of a giant column,
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you’d still experience ninety percent
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of the gravitational force there that you do on the ground.
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Astronauts just experience weightlessness
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because the space station is constantly falling towards earth.
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Fortunately, it’s orbiting the planet fast enough that it never hits the ground.
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By the time you made it to the surface of the moon,
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around 400,000 kilometers away,
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Earth’s gravitational pull would be
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less than 0.03 percent of what you feel on earth.
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The only gravity you’d be aware of would be the moon’s,
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which is about one sixth as strong as the earth’s.
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Travel farther still
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and Earth’s gravitational pull on you will continue to decrease,
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but never drop to zero.
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Even safely tethered to the Earth,
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we’re subject to the faint tug of distant celestial bodies and nearby earthly ones.
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The Sun exerts a force of about half a Newton on you.
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If you’re a few meters away from a smartphone, you'll experience
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a mutual force of a few piconewtons.
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That’s about the same as the gravitational pull
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between you and the Andromeda Galaxy,
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which is 2.5 million light years away
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but about a trillion times as massive as the sun.
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But when it comes to escaping gravity,
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there’s a loophole.
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If all the mass around us is pulling on us all the time,
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how would Earth’s gravity change
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if you tunneled deep below the surface,
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assuming you could do so without being cooked or crushed?
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If you hollowed out the center of a perfectly spherical Earth—
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which it isn’t, but let’s just say it were—
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you’d experience an identical pull from all sides.
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And you’d be suspended, weightless,
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only encountering the tiny pulls from other celestial bodies.
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So you could escape the Earth’s gravity in such a thought experiment—
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but only by heading straight into it.
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