Video Transcript
In this video, we’re going to learn
about rotational equilibrium. We’ll see what this term means. And we’ll also learn how to apply
the equations that it indicates. To start out, imagine you’re
participating in a team-building exercise with a group of five of your
coworkers. The exercise requires all six
members of the team to be on a long plank of wood, while the wood is balancing and
not touching the ground. As the last person to get on the
plank, it’s your job to find the location where to stand so that the entire team
balances out equally.
To know where this might be, it
will be helpful to know about rotational equilibrium. Leading in to talking about
equilibrium from a rotational perspective, we know that, from a translational
aspect, equilibrium means that the sum of the forces on an object is equal to
zero. For example, for a mass sitting on
a flat tabletop, the weight force acting on that mass is exactly canceled out by the
normal force of the table pressing up on the mass. So the net force on this mass is
zero. And therefore, it’s in
equilibrium. It’s not accelerating. Force as a translational notion has
a rotational analog. And that’s torque, often symbolized
with the Greek letter 𝜏.
We can think of torque as the
capacity to change an object’s angular acceleration, as in the case of this wheel
which is experiencing a force on the edge of its circumference. For rotational equilibrium then,
you may guess that the mathematical expression of that equilibrium is that the sum
of the torques acting on an object add up to zero, in other words that the net
torque on an object is zero. If we apply this concept to the
previous example of the seesaw that we want to balance, from a problem-solving
approach, our first step would be to choose the rotation point along the plank. Even though the position of the
middle of the plank where it rests on a support naturally suggests itself in this
case, as a general rule, we can choose our rotation point anywhere along the object
we want to experience rotational equilibrium.
And sometimes by making a clever
choice of our rotation point, we can simplify the problem by minimizing the number
of calculations we’ll need to do. Why might this be? Well, recall that the magnitude of
torque is equal to force times distance when the force and the distance vectors are
perpendicular to each other. Whatever point along our object we
choose for our rotation point will naturally have a distance value, 𝑟, of zero. So whatever forces are exerted at
that point will drop out of the calculation.
Our next step in solving a
rotational equilibrium problem involves choosing the plus–minus rotation
directions. If we had a two-dimensional
translational exercise to solve, we’ll probably be helped by going ahead and
choosing the positive 𝑥- and 𝑦-directions for that scenario. In just the same way for rotational
equilibrium, we choose a rotational direction, either clockwise or counterclockwise,
to be considered positive torques. And naturally, the other way are
negative torques. Once we’ve chosen the positive
rotation direction, our next step is to write out all the torques acting on our
object of interest. And then using our expression of
rotational equilibrium, we set that sum equal to zero.
In the case of our team exercise,
if we knew the mass and position from our axis of rotation of every one of our
coworkers and if we knew our own mass, then this equation we create in step three
will let us solve for the distance from that rotation point that we should stand to
create balance. Let’s get some practice now with
rotational equilibrium through working an example.
The forearm shown below is
positioned at an angle 𝜃 with respect to the upper arm. And a 5.0-kilogram mass is held in
the hand. The total mass of the forearm and
hand is 3.0 kilograms. And their center of mass is 15.0
centimeters from the elbow. What is the magnitude of the force
that the bicep muscle exerts on the forearm for 𝜃 equals 60 degrees? What is the magnitude of the force
on the elbow joint for a 𝜃 equals 60 degrees?
We can label the force magnitude of
the bicep 𝐹 sub 𝐵 and the force magnitude on the elbow 𝐹 sub 𝑒. When we consider this scenario, we
have a ball being held motionless. There’s no rotation and there’s no
translation going on. If we consider the forearm of this
arm as the length along which torques and forces are exerted, we can say that the
sum of all the torques exerted on the forearm are zero. We will use this condition along
with the other information we’ve been given about the scenario to solve for the
force exerted by the bicep, 𝐹 sub 𝐵. We can simplify this scenario by
modeling the forearm simply as a rigid extended line segment.
When it comes to the forces that
are acting on this forearm, we know there’s the weight force of the five-kilogram
ball acting down. We’ll label that force 𝑚 sub 𝑏,
the mass of the ball of 5.0 kilograms, times 𝑔, the acceleration due to gravity,
which is 9.8 meters per second squared. We’re also told about the mass of
the arm, that is, the forearm and hand combined. That mass also has a downward force
that is exerted on this line. We’ll call that force 𝑚 sub 𝑎 for
the mass of the arm, given as 3.0 kilograms times 𝑔.
We also know that the bicep muscle
exerts an upward force on the forearm in order to help support the weight of the
ball. This is the force we want to solve
for. And we’re presuming that these
three forces are acting around a rotation axis at the elbow joint. Our next step is to calculate the
torque created about this rotation point at the elbow joint by each of these three
forces. Recalling that torque magnitude is
equal to force times distance from the axis of rotation multiplied by the sine of
the angle between these two vectors, and since we’re told that, in our case, the
angle 𝜃, which is also the same as the 𝜃 shown in this general equation, is equal
to 60 degrees. We’re almost ready to write out the
torques created by these three forces acting on the forearm.
But before we do, let’s choose
which direction of rotation about our rotation point we want to consider
positive. We’ll choose clockwise rotation as
positive rotation. This choice means that 𝑚 sub 𝑎
times 𝑔 and 𝑚 sub 𝑏 times 𝑔 will create positive torques and 𝐹 sub 𝐵, our
bicep force, will create a negative torque. When we enter the expression 𝐹
times 𝑟 times the sin of 𝜃 for each one of the three forces acting on our forearm
and set that sum equal to zero, we use the fact that the mass of the arm is said to
have a center of gravity 15.0 centimeters from the elbow. And the ball is 35.0 centimeters
from the elbow joint, while the bicep is only 4.0 centimeters away.
Since the sin of 60 degrees is
common to all the terms on the left-hand side of our equation, we can divide both
sides of the equation by that term and cancel it out. Now since we want to solve for 𝐹
sub 𝐵, we rearrange to isolate that on one side of the equation. When we do and also factor out the
acceleration due to gravity 𝑔, we see that our expression for 𝐹 sub 𝐵 is in terms
of known values 𝑚 sub 𝑎, 𝑚 sub 𝑏, and our distances, as well as 𝑔. We’ll now plug in for those masses
as well as convert our distances from units of centimeters to meters. When we enter this expression on
our calculator, we find that, to two significant figures, 𝐹 sub 𝐵 is 540
newtons. That’s the force exerted by the
bicep on the forearm in order to ensure rotational equilibrium.
The next thing we wanna do is solve
for the force that’s exerted on the elbow joint. Now you might say, “What force? I thought we were in
equilibrium.” It’s true that we’re in rotational
equilibrium with the three forces we’ve named about the axis we’ve chosen at the
elbow joint. But the equilibrium we’ll use to
solve for 𝐹 sub 𝑒 is a translational equilibrium. That is, the whole arm isn’t moving
up, down, left, or right at all. The implication is that not only is
the sum of torques on this forearm zero, but the sum of the forces on the forearm is
zero as well. If we look back at our original
diagram and specifically at the elbow joint, if we had to guess a direction for the
force exerted on that joint because of the rest of this scenario. We could say that because bones
tend to exert force while under compression that that elbow force would point in the
same direction as the weight force on the ball and the arm.
If we decide to set up the
convention that downward direction is positive force, then because all the forces on
the forearm add up to zero, we can write that 𝐹 sub 𝑒 plus 𝑔 times the quantity
𝑚 sub 𝑎 plus 𝑚 sub 𝑏 minus 𝐹 sub 𝐵 is equal to zero. Or 𝐹 sub 𝑒 is equal to 𝐹 sub 𝐵
minus 𝑔 times the quantity 𝑚 𝑎 plus 𝑚 𝑏. We’ve been given the values for 𝑚
sub 𝑎 and 𝑚 sub 𝑏. We know 𝑔 since it’s a
constant. And we solved for 𝐹 sub 𝐵 in a
previous part. So we’re ready to plug in and solve
for 𝐹 sub 𝑒. When we enter this expression on
our calculator, again to two significant figures, we find that 𝐹 sub 𝑒 is 460
newtons. That’s the force magnitude exerted
on the elbow joint.
Let’s summarize what we’ve learned
about rotational equilibrium. We’ve seen that rotational
equilibrium means something very specific. Mathematically, it means that the
sum of all the torques acting on an object is zero. In other words, the object has no
angular acceleration. We’ve also seen that we can choose
the axis of rotation to be anywhere along the length of an object that’s
experiencing torque. Our choice can be led by what
simplifies calculations and leads us to our answer most directly.
And finally, we saw that if an
object is in rotational as well as translational equilibrium, then the sum of
torques on the object is zero, as well as the sum of forces on the object. By applying these two conditions to
a scenario we may encounter, often they help us generate a set of independent
equations that let us solve for properties of interest.
