Uniform circular motion

Lightning Round Questions

gr7: [lightning:: 2]
gr10: [lightning:: 4]

Demonstration

Attach a spring to the shaft of the drill and spin with a weight attached.

If the centripetal force is mr\omega { #2} , what would happen to the surface of a bowl of water if you were to spin it at a fixed speed?

Concept summary and connections

Lesson content with examples

An object moving in a circle is always accelerating. After all, it's velocity vector is changing, so there must be acceleration happening. This is where we finally break the idea that accelerating = going faster once and for all! You can go in a circle without changing speed, forever. If the planets were it perfectly circular orbits, this is exactly what they would do (for some values of "forever" including "a really, really long time").

So how can that be? How can you accelerate forever without any energy going in to the system? How is it that your velocity can be constantly changing but your speed is constant? The answer to both is from one idea:

In circular motion, the acceleration always points toward the center of the rotation

We know from geometry that that a line from the center of a circle is always perpendicular to the circle where it crosses. We also know that work only happens when some component of the motion is parallel to the force. Taking those together, we can see that the centripetal force doesn't do any work! It's always perpendicular to the object, so it doesn't change its kinetic energy.

The math

Centripetal acceleration is inversely proportional to the radius of the arc, and directly proportional to the squared speed of the motion. The larger the arc, the lower the acceleration. The higher the speed, the higher the acceleration. ac=v2r. We usually write this using angular velocity though:

v=ωr, so v2=ω2r2r=ω2r

So, we can write ac=ω2r, or centripetal acceleration is the angular velocity squared time the radius of the turn.

We also know that force=mass×acceleration, so the centripetal force must be fc=mω2r

From that, we can figure out a whole bunch of neat stuff.

Media resources

Guided practice

Homework