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Bill Nye explains about momentum

Momentum describes how strong a moving thing is. Things that aren't moving have no momentum. Moving things have less momentum if they are light or moving slowly, and more momentum if they are heavy or moving fast.

Because of momentum, a planet or a star that is moving in space will generally keep moving in the same direction unless something happens to push it another way. The Sun keeps going around the Milky Way, and the Earth keeps going around the Sun. But on Earth, friction with the ground or the air will gradually push an object and make it stop.

One way to think of momentum is that momentum measures how hard it will be to stop the object. An object has more momentum if it is bigger, or if it is going faster - momentum is equal to mass times velocity (speed). So if a car (something with a lot of mass) is rolling down the street towards you, it's hard to stop it even if it is going pretty slowly. Or, if someone hits a baseball at you, it's hard to stop it even though it is pretty small, because it is going so fast. But a car going fast will be even harder to stop - then the car will have both a big mass and a fast speed. That's why it's dangerous to walk on train tracks - a train is big and goes fast, and so it takes a long time to stop one. The driver can't just stop the train as soon as he or she sees you.

A special kind of momentum is "angular momentum". This is when the object spins around and around like a top instead of going straight like the baseball or the car. Again, bigger things and faster things are harder to stop. In space, nebulae, stars, black holes, and planets all have angular momentum, and they all spin around.

The law of conservation of momentum tells us that you can't just lose momentum - it has to go somewhere. If a thing gets bigger, like a snowball rolling down a hill, then it gains more momentum. If a thing gets smaller (so it has less mass), then it has to spin faster, so that it has the same total momentum. If a wind stops moving forward, it starts to spin around to conserve momentum, making a hurricane or a tornado. Big nebulae spin around slowly. But when parts of them form into stars, the stars spin a little faster. And when those stars become supernovas and then tiny black holes, the black holes spin fastest of all.

Learn by Doing: Building a Roller-Coaster

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Professor Carr

Karen Eva Carr, PhD.
Assoc. Professor Emerita, History
Portland State University

Professor Carr holds a B.A. with high honors from Cornell University in classics and archaeology, and her M.A. and PhD. from the University of Michigan in Classical Art and Archaeology. She has excavated in Scotland, Cyprus, Greece, Israel, and Tunisia, and she has been teaching history to university students for a very long time.

Professor Carr's PSU page

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