Let's say I have some object that's
traveling in a circular path just like this.
And what I've drawn here is its velocity vector
at different points along that path.
And so this right over here is going to be v1,
velocity vector 1.
This is going to be velocity vector 2.
And this right over here is going to be velocity vector 3.
And what we're going to assume, in this video,
is that the magnitude of these velocity vectors is constant.
Or another way to think about it is that the speed is constant.
So I'll just say lowercase v without the arrow on top--
so this is going to be a scalar quantity-- I'll call this
the speed.
Or you could call this the magnitude of these vectors.
And this is going to be constant.
So this is going to be equal to the magnitude of vector
1, which is equal to the magnitude of vector 2.
The direction is clearly changing,
but the magnitude is going to be the same, which
is equal to the magnitude of vector 3.
And we're going to assume that it's traveling in a path,
in a circle with radius r.
And what I'm going to do is, I'm going
to draw a position vector at each point.
So let's call r1-- actually I'll just do it in pink-- let's call
r1 that right over there.
That's position vector r1.
That is position vector r2.
So the position is clearly changing.
That's position vector r2.
And that is position vector r3.
But the magnitude of our position vectors
are clearly the same.
And I'm going to call the magnitude of our position
vectors r.
And that's just the radius of the circle.
It's this distance right over here.
So r is equal to the magnitude of r1,
which is equal to the magnitude of r2, which
is equal to the magnitude of r3.
Now what I want to do, in this video,
is prove to you visually, that given this radius
and given this speed, that the magnitude
of the centripetal acceleration-- and I'll
just write that as a sub c, I don't have an arrow on top,
so this is a scalar quantity.
So the magnitude of the centripetal acceleration
is going to be equal to our speed squared,
our constant speed squared, divided
by the radius of the circle.
I want you to feel good that this is indeed
the case by the end of this video.
And to understand that, what I want to do
is I want to re-plot these velocity
vectors on another circle and just
think about how the vectors themselves are changing.
So let's copy and paste this.
So let me copy and paste v1.
So copy and paste.
So that is v-- actually I want to do it from the center
--so that is v1.
Then let me do the same thing for v2.
So let me copy and paste it.
That is v2.
And then let me do it also for v3.
I'll just get the vector part; I don't have to get the label.
So copy and paste it.
And that right over there is vector v3.
And let me clean this up a little bit.
So that's clearly v2.
I don't think we have to label anymore.
We know that v2 is in orange.
And what is the radius of this circle
going to be right over here?
Well, the radius of this circle is
going to be the magnitude of the velocity vectors.
And we already know the magnitude of the velocity
vectors is this quantity v, this scalar quantity.
So the radius of this circle is v. The radius of this circle,
we already know, is equal to r.
And just as the velocity vector is
what's giving us the change in position
over time, the change in position vector over time,
what's the vector that's going to give us
the change in our velocity vector over time?
Well, that's going to be our acceleration vectors.
So you will have some acceleration.
We'll call this a1.
We'll call this a2.
And I'll call this a3.
And I want to make sure that you get
the analogy that's going on here.
As we go around in this circle, the position
vectors first they point out to the left, then the upper,
kind of in a maybe 11 o'clock position,
or I guess the top left, and then to the top.
So it's pointing in these different directions
like a hand in a clock.
And what's moving it along there is the change
in position vector over time, which
are these velocity vectors.
Over here, the velocity vectors are moving around
like the hands of a clock.
And what is doing the moving around
are these acceleration vectors.
And over here, the velocity vectors
are tangential to the path, which is a circle.
They're perpendicular to a radius.
And you learned that in geometry--
that a line that is tangent to a circle
is perpendicular to a radius.
And it's also going to be the same thing right over here.
And just going back to what we learned
when we learned about the intuition
of centripetal acceleration, if you look at a1 right over here,
and you translate this vector, it'll be going just like that.
It is going towards the center.
a2, once again, is going towards the center.
a3, once again, if you translate that,
that is going towards the center.
So all of these are actually center-seeking vectors.
And you see that right over here.
These are actually centripetal acceleration vectors
right over here.
Here we're talking about just the magnitude of it.
And we're going to assume that all of these
have the same magnitude.
So we're going to assume that they all
have a magnitude of what we'll call a sub c.
So that's the magnitude.
And it's equal to the magnitude of a1.
That vector, it's equal to the magnitude of a2.
And it's equal to the magnitude of a3.
Now what I want to think about is how long is it
going to take for this thing to get
from this point on the circle to that point on that circle
right over there?
So the way to think about it is, what's the length of the arc
that it traveled?
The length of this arc that it traveled right over there.
That's 1/4 around the circle.
It's going to be 1/4 of the circumference.
The circumference is 2 pi r.
It Is going to be 1/4 of that.
So that is the length of the arc.
And then how long will it take it to go that?
Well, you would divide the length
of your path divided by the actual speed, the actual thing
that's nudging it along that path.
So you want to divide that by the magnitude of your velocity,
or your speed.
This is the magnitude of velocity, not velocity.
This is not a vector right over here, this is a scalar.
So this is going to be the time to travel along that path.
Now the time to travel along this path
is going to be the exact same amount of time
it takes to travel along this path for the velocity vector.
So this is for the position vector to travel like that.
This is for the velocity vector to travel like that.
So it's going to be the exact same T.
And what is the length of this path?
And now think of it in the purely geometrical sense.
We're looking at a circle here.
The radius of the circle is v. So the length
of this path right over here is going to be 1/4.
It is going to be-- I'll do it in that same color
so you see the analogy-- it's equal to 1/4 times
the circumference of the circle.
The circumference of this circle is 2 pi times
the radius of the circle, which is v.
Now what is nudging it along this circle?
What is nudging it along this path?
What is the analogy for speed right over here?
Speed is what's nudging it along the path over here.
It is the magnitude of the velocity vector.
So what's nudging it along this arc right over here
is the magnitude of the acceleration vector.
So it is going to be a sub c.
And these times are going to be the exact same thing.
The amount of time it takes for this vector
to go like that, for the position vector,
is the same amount of time it takes the velocity
vector to go like that.
So we can set these 2 things equal each other.
So we get, on this side, we get 1/4 2 pi r over v
is equal to 1/4 2 pi v over the magnitude of our acceleration
vector.
And now we can simplify it a little bit.
We can divide both sides by 1/4.
Get rid of that.
We can divide both sides by 2 pi, get rid of that.
Let me rewrite it.
So then we get r/v is equal to v over
the centripetal acceleration.
And now you can cross multiply.
And so you get v times v. So I'm just
cross multiplying right over here. v times v,
you get v squared, is equal to a c times r.
And cross multiplying, remember, is really just the same thing
as multiplying both sides by both denominators,
by multiplying both sides times v and ac.
So it's not some magical thing.
If you multiply both sides times v and ac, these v's cancel out.
These ac's cancel out.
You get v times v is v squared, is equal to a sub c times r.
And now to solve for the magnitude
of our centripetal acceleration, you
just divide both sides by r.
And you are left with-- and I guess
we've earned a drum roll now-- the magnitude
of our centripetal acceleration is
equal to the magnitude, our constant magnitude
of our velocity.
So this right here is our speed, divided
by the radius of the circle.
And we're done!