
Impossible Zero G Skyscraper
Season 2 Episode 7 | 6m 33sVideo has Closed Captions
What happens when you keep building a skyscraper higher and higher?
What happens when you keep building a skyscraper higher and higher? You may run into some problems with the laws physics. The higher you build, the faster the top of the building moves around the earth, and you end up with strong centrifugal forces. What could possibly go wrong?
Problems playing video? | Closed Captioning Feedback
Problems playing video? | Closed Captioning Feedback

Impossible Zero G Skyscraper
Season 2 Episode 7 | 6m 33sVideo has Closed Captions
What happens when you keep building a skyscraper higher and higher? You may run into some problems with the laws physics. The higher you build, the faster the top of the building moves around the earth, and you end up with strong centrifugal forces. What could possibly go wrong?
Problems playing video? | Closed Captioning Feedback
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Learn Moreabout PBS online sponsorship[MUSIC PLAYING] Hello!
I'm Diana, and you're watching "Physics, Girl!"
So the idea for this video came from a conversation with a friend where we were talking about tall buildings, because Earth is spinning, and tall buildings are spinning around with it especially fast at the equator from the perspective of someone looking down at Earth.
So you could imagine a building so tall where the end of it is going around it like the speed of light.
Obviously not.
You can't go at the speed of light.
But it's interesting to think about how tall that building might be, if only Newtonian physics applied.
And at some point, a different question popped up, which is that if you dropped a penny from the top of the building, how tall would the building need to be in order for the penny to go into orbit?
So this could actually work, hypothetically.
Like I said, the Earth is rotating, and everything's sticking out of it.
Like me and the buildings are all rotating at the same angular speed-- that is, they do a full rotation of 360 degrees every 24 hours.
Because that's what a day is!
Well, 23 hours, 56 minutes, and 4 seconds.
But even though everything is spinning at the same angular rate, different parts of the building and different parts of the inside of the Earth are moving at different linear speeds, depending on how far away they are from Earth's axis of rotation.
That's this.
This is just like when you go on a merry-go-round, and you move faster on the edges than sitting in the middle.
So people are spinning around the equator at a pretty fast 1,040 miles per hour.
But if you dug down deep into the Earth and settled down in the nice molten core, you could find a place where you're going a comfortable 100 miles an hour.
So all this means that if you are standing on the equator, your head would be further away from Earth's axis of rotation than your feet, so it would be moving faster linearly-- at a rate of a tenth of a millimeter per second, so it's not noticeable.
But also, if you were standing on one of Earth's poles, it wouldn't be noticeable either, because you would only be spinning in this direction.
So now instead of digging down into the Earth, imagine you go the other way, and you build up in a super tall building-- the one we talked about at the beginning of the video-- where the top of your building is going the speed of light!
You can't do that.
[ALARM SOUNDING] 58 00:02:10,189 --> 00:02:11,730 But how tall would this building have to be if Newton were doing the calculation, before Einstein discovered the theory of relativity?
Well, he'd find that your building would have to be-- OK, well, it would do one revolution per 86,164 seconds.
And our revolution is 2 pi r per 86,164 seconds, which we'll set to this.
So my radius is this.
Subtract the radius of the Earth to get the height of the building-- though our number doesn't change much-- to get 4,111,175,472,000 meters, or 27.5 astronomical units.
That means the top of your building would stick out past the sun, past Jupiter's orbit, and somewhere between Uranus and Neptune's orbit.
That is an awesome calculation!
But unfortunately, not realistic, because Newtonian physics is so 1800s.
And there would be so many problems before even getting to that point, like structural integrity of the building, or not having an atmosphere because you're out in space at that point.
So the problems are many.
For example, we established before with the merry-go-round that as you build a building up higher, the top of your building is going faster than the bottom of your building.
And when you're going around in a circle, you feel like you're being pushed toward the outside of the circle.
Just like when you're turning a car to the left, you feel like you're being pushed to the right.
Do you see where I'm going with this?
That feeling is just your inertia wanting to keep you going in a straight line as you get accelerated around in the circle.
But Newton's laws don't really work in an accelerating reference frame.
So we can define a fake force that you feel outward and call it the centrifugal force.
We add this fake force into Newton's laws and pretend that it's actually a force in every other way to do our calculations.
Centrifugal force-- the force that physics teachers hate.
Such is the weirdness of rotating frames, that you need to make up forces in order to use Newton's laws.
But think about it.
The idea of creating artificial gravity is often a circular craft that's spinning, and that's kind of what we're doing here.
The top of the building is spinning around, and that fake centrifugal force feels like it's pulling you away from Earth like a fake or artificial force of gravity.
And it's pulling in the opposite direction of the real force of gravity.
We don't notice this counteraction even standing at the equator of the Earth where Earth is spinning, because the effect is only about 0.03 meters per second squared, which would change the precious 9.81 meters per second squared to 9.78 meters per second squared.
But, like, the bulges of mass around the Earth effect gravity on the same order, so it's not noticeable.
OK, so now as you climb up the building, from an outsider's perspective, your linear speed increases, so your acceleration increases.
And from your perspective, your centrifugal acceleration counteracts the acceleration of gravity more and more.
As you go up in your spinning building, it feels like gravity gets weaker and weaker until the point when you feel weightless.
Gravity is also getting weaker as you move away from Earth.
But way before it goes to 0, you get to a point where the centrifugal force balances the gravitational force.
This is the point when if you drop the penny out of the top of the building, it will go into orbit.
So from your perspective, as you drop the penny out the window, it'll look like it's just floating there, because it would be moving sideways with the tower.
And it would have just enough sideways motion so that it doesn't fall down to Earth, but not so much that it would fly off into space.
That's orbiting.
And that magic altitude is 35,786 kilometers above Earth's surface.
At that height, you could put any object of any mass into orbit.
Maybe you want to attempt to orbit yourself!
Anything you want, out the window!
Orbit!
Another fun thing to think about-- if you keep going up in your tower past this point, you'd start to feel an acceleration in the other direction.
At some point, you'd get out so far that you'd feel 9.8 meters per second squared pushing you against the ceiling.
But now the quadrillion dollar question is, could you ever build a building of heights like this?
Well, short of using futuristic carbon nanotubes, we probably won't be making anything this tall anytime soon.
Thanks for watching, and happy physicsing!
While researching this video, I found a video by [INAUDIBLE] that had an eerily similar title to the question I was wondering about.
But as Michael does, he talked about a ton of different things, including the really tall buildings that we have here on Earth.
It's a great video.
It's called "How High Can We Build?
I'll link it in the description.
You should check it out.
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