- [Narrator] I want to show you how to do
a slightly more sophisticated
centripetal force problem,
and this one's a classic.
This is the one where there's a mass,
tied to a string,
and that string is secured to the ceiling,
and the mass has been given an initial velocity,
so that it swings around in a horizontal circle.
So, this mass is going to maintain a constant height,
it's not moving up or down,
but it revolves in a horizontal circle,
so if you were to view this thing from above,
from below, it looks something like this.
You'd see the ball tracing out a perfect circle.
If you were looking at this from right below.
And the question I want to ask is: two things.
What is the tension in the rope?
And what has to be the speed of the mass?
And these are given variables.
We know the mass is three kilograms.
We know the length of the rope is two meters.
And this rope is making an angle of thirty degrees,
with respect to this vertical line right here.
Now this problem's a classic for a good reason.
If you don't have a clean conceptual understanding
of what we really mean by the terms
when dealing with centripetal forces.
And if you don't have a problem solving
strategy to use to tackle problems,
this problem will expose you.
So that's why we should go over this,
to make sure you have a clean understanding
of exactly what we mean by all the different terms
and to show you there's a strategy you could use
to solve any centripetal force problem.
And that strategy is this.
First, draw a quality force diagram
for the object or objects in your problem.
So, let's do that first.
The forces that are acting on this three kilogram sphere
are the force of gravity.
You'll have a force of gravity straight down.
That's gonna be m times g.
So the way we find the force of gravity
is with the formula mass times 9.8.
And the only other object that's touching this mass
is the rope.
So the only other force on this mass
is the force of tension.
So I'm gonna to label that force
with a capital T.
This'll be the total force of tension
from the rope.
And, really, the only other step
in this problem solving strategy,
there's really only two steps,
use Newton's second law.
But only use it for one direction at a time.
And we typically only have two directions.
I mean, we've got this vertical direction
or we've got this horizontal direction.
We've got a 50-50 shot.
I mean, we've gotta pick one of the two.
It's not like you can pick the wrong direction.
If you pick the wrong direction,
it'll just mean that you can't solve
because there'll be too many variables.
But what you write down in that process
is probably gonna be useful later in the problem anyway,
so don't erase it.
If you pick a direction that you can't solve,
because you have too many variables,
just go to the other direction, and pick that direction.
I know what direction to pick,
cause I've done this one before.
But if you don't know,
the worst thing you do is freeze up.
You gotta try something.
If you try the wrong direction,
no big deal,
there's only one other direction to pick.
So I'm gonna choose to analyze these forces
in the vertical direction.
So I'm gonna say that the acceleration
in the vertical direction,
this y direction,
is equal to the net force
in the y direction divided by the mass.
And now I simply ask myself,
what is the acceleration in the vertical direction?
It's not 9.8.
A lot of people want to say negative 9.8.
But that's only if this ball were free-falling.
And this ball is not free-falling.
In fact, this ball is not even changing
it's vertical height.
It's remaining at the same constant height,
and that means not only is there no vertical velocity,
there's no vertical acceleration.
Since the ball's not even moving vertically.
So, on the left hand side here,
this is great,
we can put a zero.
Zero's are wonderful.
They make calculations easier.
So this is going to equal the net force
in the vertical direction.
So one force is gonna to be
the force of gravity.
So I'll put that in here.
You'll have m times g.
That force is definitely a vertical force.
But you gotta be careful,
if we're gonna consider upward is positive,
this mg is a negative force.
So in terms of y-directed forces,
downward, typically,
the convention is that you choose that to be negative.
So I'm gonna say that mg is negative.
And now we ask ourselves,
are there any other vertical forces?
Well, we just look at our force diagram.
So our force diagram will tell us
if there's any other vertical forces.
We look over here,
the only other force is this tension force.
And part of this tension force
is vertical.
We can't put in the entire tension
into this formula.
We could only do that if this tension
was directed vertically upward,
but it's not.
Part of it's vertically upward,
and part of it's horizontal.
So part of this tension force
is directed this way.
I'm gonna call that the x component
of the tension.
And then part of this tension is directed vertically.
I'll call that the y component of the tension.
So we can only plug in this y component
of tension into this formula over here,
since we're plugging in y-directed
forces into this equation.
So I could just write plus Ty.
But I don't wanna do that.
I wanna solve for what T is,
not what Ty is.
So I wanna write this Ty in terms of T.
And I can do that.
Look at the triangle this is making.
This tension and this Ty
is gonna make an angle right here.
And that angle has to be the same angle
that the rope makes with this vertical line.
So the tension is not the rope.
The tension is a force exerted by the rope.
And the tension lies along the same direction as the rope.
But the tension is not the rope.
This is a really common misconception.
Sometimes people think,
oh, the tension is two meters, right?
No.
That's not even a force.
That's the length of the rope.
And, yes, the length of the rope
lies along the same direction as the tension force,
but the tension is different
from the length of the rope.
However, this angle between the tension
and this vertical component of the tension
is the same as the angle between this rope
and the vertical direction.
So that means we can label this
as thirty degrees right here.
And now I can figure out
what is the vertical component of the tension
in terms of T and in terms of theta?
I got a right triangle.
Here's a right angle.
This side that I wanna find out,
Ty, is adjacent to this thirty degrees.
Since it's adjacent, we're gonna use cosine.
In other words,
we're gonna say that cosine of theta
equals adjacent over hypotenuse.
People get confused sometimes.
They're like, wait,
I thought vertical was always the opposite side.
It'd be the opposite side if we knew this angle,
But we don't know that angle.
We know this vertical angle.
And that means that this vertical side
is adjacent to that angle.
Since we know the angle,
we can write the cosine of thirty degrees
is gonna equal the adjacent side.
Now the adjacent side is Ty.
And the hypotenuse is gonna be T.
People get freaked out here.
They're like, I've got too many variables.
But that's okay.
We can label this total hypotenuse is T.
Even though we don't know it, it's alright.
We're gonna manipulate symbols
and we're gonna solve for Ty.
If I multiply both sides by T, I get Ty.
The vertical component of the tension
is equal to the total tension
times cosine of thirty degrees.
This is the vertical component of the tension.
And this is the force that I can plug into
my vertical net force.
So I'm gonna add,
cause this points upward,
T, the total tension,
times cosine of thirty.
And then I have to divide by my mass.
So I can solve this for T now.
If I multiply both sides by m.
M times zero is gonna be zero.
I'll move the mg over
and then I divide by cosine of thirty.
To get that the tension in the rope
is gonna equal mg,
the force of gravity divided by
cosine of thirty.
And if we plug in numbers
we'll get that T equals,
the mass was 3 kilograms,
g is always 9.8.
Divided by cosine of thirty.
Gives us a tension of about 33.9 Newtons.
I'll just say that that's 34 Newtons.
So that's the tension in the rope.
That's the first thing we wanted to find.
We just found it over here.
That is the tension in the rope.
So let's do the next part.
Let's try to find the speed.
People get a little concerned now.
They're like, what do I do?
Don't deviate from the plan.
We drew our force diagram.
We used Newton's second law
for one of the directions.
You still got work to do,
then do Newton's second law for another direction.
We're just gonna do this for the x direction.
So we'll do the x direction.
I'll see that the acceleration in the x direction
equals the net force in the x direction
divided by the mass.
And I'll ask myself the same question.
Is there any acceleration in the x direction?
There wasn't any acceleration in the y direction.
You might think there's not any in the x direction.
But there is.
This mass is going in a circle.
That means there's gonna be centripetal
acceleration in this direction.
So this horizontal direction is, essentially,
just the centripetal direction.
So to make that more clear,
I'm just gonna put ac and Fc.
And whenever you have centripetal acceleration,
we can replace that with v squared.
The speed squared divided by the radius.
And that's gonna equal the net centripetal force
over the mass.
What force is acting in the centripetal direction?
Well, you can figure that out.
It's just the force that was acting in the x direction.
Cause this is the x direction.
The x direction is the direction
that happens to be pointing
toward the center of the circle.
That's why the x direction here
is just the centripetal direction.
So to figure out which forces are centripetal,
I just look at my force diagram.
I drew this for a reason.
I drew this so when I look at it,
I can figure out what forces are vertical,
to put in over here,
and what forces are centripetal,
i.e. horizontal,
to put in over here.
The only force that's horizontal
is the horizontal component of the tension.
That's this Tx.
But, again, instead of just plugging in Tx,
we'll plug in what this component is.
in terms of the angle and the total tension.
Just like we did over here.
Ty was T cosine thirty.
So it might not be that big of a surprise
that Tx, the horizontal component,
is just gonna be T sine thirty.
If you don't believe that,
you can prove it to yourself.
Think about it.
This Tx component is the opposite to this angle.
And for opposite we use sine.
So we can say sine of thirty would be
the x component, which is the opposite side,
over the hypotenuse, which is T.
And if you solve this for Tx,
you multiple both sides by T,
you, indeed, get that Tx is just T,
the total tension, times sine thirty.
So we can plug that back in over here.
We know that the only component
that's acting as a centripetal force,
i.e. that's pointing towards the center of the circle,
is this x component,
which we just found is T sine thirty degrees.
Now you see why picking this direction first
wouldn't have allowed us to solve,
cause we wouldn't have known the speed, v,
and we wouldn't have known the tension T.
Only because we chose the y direction first,
we were able to find the tension.
And now that we know this tension,
being 34 Newtons,
we can plug that in over here
and solve for our speed.
But there's a really common mistake that people make here.
People really wanna plug in r as two meters,
cause they're like,
hey, you gave me two meters over here,
I'm gonna use it.
That's an r, right?
Isn't that r?
No, that is not r.
R here, always, in the centripetal formula
for the acceleration, this r represents
the radius of the circle that the object
is moving in.
And this object doesn't move in a circle
with a radius of two.
The radius of the circle this object's
traveling in looks like this.
That's the radius of the circle.
And that's not two meters.
How do we find that?
We'll again use trigonometry.
We're just gonna say that we've got a right triangle.
This time, though, we're gonna make a right triangle
out of the length,
not of the force.
Not of this tension.
We're making a right triangle out of the length.
But, again, we know that side's a right angle.
We know that this side's thirty degrees.
So we say that this radius is the opposite side
of that thirty degrees.
So we're gonna use sine theta.
We're gonna say that the sine of theta,
which is thirty,
equals the opposite side,
and that's r,
divided by the total length of the string, L.
And, so if I solve this for the radius,
I get the radius of the circle
that this ball is traveling in
would be L times sine of thirty,
where L would be this two meters.
So we'll plug that back in over here.
We'll say that v squared divided by
r, which is L sine thirty,
is gonna equal T sine 30 divided by the mass.
And now we can solve,
we can multiple both sides by L sine thirty.
And we get that v squared is gonna equal
T sine thirty
times L sine thirty
divided by the mass of the sphere.
And since I want to find v not v squared,
I'll take a square root of both sides,
and when I take a square root of both sides,
I end up with v is the square root
of t sine thirty, L sine thirty over the mass.
So if we plug in our numbers,
we get that v is the square root of T,
which is 34 Newtons,
times sine of 30, times L,
and this L is referring to this total length
which is two meters,
times sine of thirty.
All divided by the mass, which was three kilograms.
Which, if you solve, gives you a speed of about 2.38.
So I'll just say 2.4 meters per second.
Which is the speed that we were trying to find.
So, recapping, when you're solving
a sophisticated centripetal force problem,
be sure to draw a quality force diagram.
Then use Newton's second law for a single direction.
And only plug forces in that direction
into the net force.
If the direction you choose
happens to lie along the centripetal direction,
i.e. it points toward the center of the circle,
then you can use v squared over r,
for your centripetal acceleration,
But, again, only plug in forces
that lie along that direction
for the centripetal force.
And make sure that you understand when we say the radius,
we're talking about the radius of the circle
that the object is traveling in.