6.5: Angular Momentum and Its Conservation
Learning Objectives
- Understand the analogy between angular momentum and linear momentum.
- Observe the relationship between torque and angular momentum.
- Apply the law of conservation of angular momentu
Why does Earth keep on spinning? What started it spinning to begin with? And how does an ice skater manage to spin faster and faster simply by pulling her arms in? Why does she not have to exert a torque to spin faster? Questions like these have answers based in angular momentum, the rotational analog to linear momentum.
By now the pattern is clear—every rotational phenomenon has a direct translational analog. It seems quite reasonable, then, to define angular momentum \(L\) as
\[L=I \omega. \nonumber \]
This equation is an analog to the definition of linear momentum as \(p=m v\). Units for linear momentum are \(\mathrm{kg} \cdot \mathrm{m} / \mathrm{s}\) while units for angular momentum are \(\mathrm{kg} \cdot \mathrm{m}^{2} / \mathrm{s}\). As we would expect, an object that has a large moment of inertia \(I\), such as Earth, has a very large angular momentum. An object that has a large angular velocity \(\omega\), such as a centrifuge, also has a rather large angular momentum.
Example \(\PageIndex{1}\): Calculating Angular Momentum of the Earth
Strategy
No information is given in the statement of the problem; so we must look up pertinent data before we can calculate \(L=I \omega\). First, according to Figure 10.3.3 from [link] , the formula for the moment of inertia of a sphere is
\[I=\frac{2 M R^{2}}{5} \nonumber\]
so that
\[L=I \omega=\frac{2 M R^{2} \omega}{5}. \nonumber\]
Earth’s mass \(M\) is \(5.979 \times 10^{24} \mathrm{~kg}\) and its radius \(R\) is \(6.376 \times 10^{6} \mathrm{~m}\). The Earth’s angular velocity \(\omega\) is, of course, exactly one revolution per day, but we must covert \(\omega\) to radians per second to do the calculation in SI units.
Solution
Substituting known information into the expression for \(L\) and converting \(\omega\) to radians per second gives
\[\begin{aligned}
L &=0.4\left(5.979 \times 10^{24} \mathrm{~kg}\right)\left(6.376 \times 10^{6} \mathrm{~m}\right)^{2}\left(\frac{1 \; \mathrm{rev}}{\mathrm{d}}\right) \\
&=9.72 \times 10^{37} \mathrm{~kg} \cdot \mathrm{m}^{2} \cdot \mathrm{rev} / \mathrm{d}.
\end{aligned} \nonumber\]
Substituting \(2 \pi\) rad for \(1\) rev and \(8.64 \times 10^{4}\) for 1 day gives
\[\begin{aligned}
L &=\left(9.72 \times 10^{37} \mathrm{~kg} \cdot \mathrm{m}^{2}\right)\left(\frac{2 \pi \; \mathrm{rad} / \mathrm{rev}}{8.64 \times 10^{4} \mathrm{~s} / \mathrm{d}}\right)(1 \; \mathrm{rev} / \mathrm{d}) \\
&=7.07 \times 10^{33} \mathrm{~kg} \cdot \mathrm{m}^{2} / \mathrm{s}.
\end{aligned} \nonumber\]
Discussion
This number is large, demonstrating that Earth, as expected, has a tremendous angular momentum. The answer is approximate, because we have assumed a constant density for Earth in order to estimate its moment of inertia.
When you push a merry-go-round, spin a bike wheel, or open a door, you exert a torque. If the torque you exert is greater than opposing torques, then the rotation accelerates, and angular momentum increases. The greater the net torque, the more rapid the increase in \(L\). The relationship between torque and angular momentum is
\[\text { net } \tau=\frac{\Delta L}{\Delta t}. \nonumber \]
This expression is exactly analogous to the relationship between force and linear momentum, \(F=\Delta p / \Delta t\). The equation \(\text { net } \tau=\frac{\Delta L}{\Delta t}\) is very fundamental and broadly applicable. It is, in fact, the rotational form of Newton’s second law.
Example \(\PageIndex{2}\): Calculating the Torque Putting Angular Momentum Into a Lazy Susan
Figure \(\PageIndex{1}\) shows a Lazy Susan food tray being rotated by a person in quest of sustenance. Suppose the person exerts a 2.50 N force perpendicular to the lazy Susan’s 0.260-m radius for 0.150 s. (a) What is the final angular momentum of the lazy Susan if it starts from rest, assuming friction is negligible? (b) What is the final angular velocity of the lazy Susan, given that its mass is 4.00 kg and assuming its moment of inertia is that of a disk?
Strategy
We can find the angular momentum by solving \(\text { net } \tau=\frac{\Delta L}{\Delta t}\) for \(\Delta L\), and using the given information to calculate the torque. The final angular momentum equals the change in angular momentum, because the lazy Susan starts from rest. That is, \(\Delta L=L\). To find the final velocity, we must calculate \(\omega\) from the definition of \(L\) in \(L=I \omega\).
Solution for (a)
Solving \(\text { net } \tau=\frac{\Delta L}{\Delta t}\) for \(\Delta L\) gives
\[\Delta L=(\operatorname{net} \tau) \Delta \mathrm{t}. \nonumber\]
Because the force is perpendicular to \(R\), we see that \(\text { net } \tau=r F\), so that
\[\begin{aligned}
L &=\mathrm{rF} \Delta t=(0.260 \mathrm{~m})(2.50 \mathrm{~N})(0.150 \mathrm{~s}) \\
&=9.75 \times 10^{-2} \mathrm{~kg} \cdot \mathrm{m}^{2} / \mathrm{s}.
\end{aligned} \nonumber\]
Solution for (b)
The final angular velocity can be calculated from the definition of angular momentum,
\[L=I \omega. \nonumber\]
Solving for \(\omega\) and substituting the formula for the moment of inertia of a disk into the resulting equation gives
\[\omega=\frac{L}{I}=\frac{L}{\frac{1}{2} M R^{2}}. \nonumber\]
And substituting known values into the preceding equation yields
\[\omega=\frac{9.75 \times 10^{-2} \mathrm{~kg} \cdot \mathrm{m}^{2} / \mathrm{s}}{(0.500)(4.00 \mathrm{~kg})(0.260 \mathrm{~m})}=0.721 \mathrm{rad} / \mathrm{s}. \nonumber\]
Discussion
Note that the imparted angular momentum does not depend on any property of the object but only on torque and time. The final angular velocity is equivalent to one revolution in 8.71 s (determination of the time period is left as an exercise for the reader), which is about right for a lazy Susan.
MAKING CONNECTIONS: CONSERVATION LAWS
Angular momentum, like energy and linear momentum, is conserved. This universally applicable law is another sign of underlying unity in physical laws. Angular momentum is conserved when net external torque is zero, just as linear momentum is conserved when the net external force is zero.
Conservation of Angular Momentum
We can now understand why Earth keeps on spinning. As we saw in the previous example, \(\Delta L=(\operatorname{net} \tau) \Delta t\). This equation means that, to change angular momentum, a torque must act over some period of time. Because Earth has a large angular momentum, a large torque acting over a long time is needed to change its rate of spin. So what external torques are there? Tidal friction exerts torque that is slowing Earth’s rotation, but tens of millions of years must pass before the change is very significant. Recent research indicates the length of the day was 18 h some 900 million years ago. Only the tides exert significant retarding torques on Earth, and so it will continue to spin, although ever more slowly, for many billions of years.
What we have here is, in fact, another conservation law. If the net torque is zero , then angular momentum is constant or conserved . We can see this rigorously by considering \(\text { net } \tau=\frac{\Delta L}{\Delta t}\) for the situation in which the net torque is zero. In that case,
\[\operatorname{net} \tau=0 \nonumber \]
implying that
\[\frac{\Delta L}{\Delta t}=0. \nonumber \]
If the change in angular momentum \(\Delta L\) is zero, then the angular momentum is constant; thus,
\[L=\text { constant }(\text { net } \tau=0) \nonumber \]
or
\[L=L^{\prime}(\operatorname{net} \tau=0) . \nonumber \]
These expressions are the law of conservation of angular momentum . Conservation laws are as scarce as they are important.
An example of conservation of angular momentum is seen in Figure \(\PageIndex{2}\), in which an ice skater is executing a spin. The net torque on her is very close to zero, because there is relatively little friction between her skates and the ice and because the friction is exerted very close to the pivot point. (Both \(F\) and \(R\) are small, and so \(\tau\) is negligibly small.) Consequently, she can spin for quite some time. She can do something else, too. She can increase her rate of spin by pulling her arms and legs in. Why does pulling her arms and legs in increase her rate of spin? The answer is that her angular momentum is constant, so that
\[L=L^{\prime}. \nonumber \]
Expressing this equation in terms of the moment of inertia,
\[I \omega=I^{\prime} \omega^{\prime}, \nonumber \]
where the primed quantities refer to conditions after she has pulled in her arms and reduced her moment of inertia. Because \(I^{\prime}\) is smaller, the angular velocity \(\omega^{\prime}\) must increase to keep the angular momentum constant. The change can be dramatic, as the following example shows.
Example \(\PageIndex{3}\): Calculating the Angular Momentum of a Spinning Skater
Suppose an ice skater, such as the one in Figure \(\PageIndex{2}\), is spinning at 0.800 rev/ s with her arms extended. She has a moment of inertia of \(2.34 \mathrm{~kg} \cdot \mathrm{m}^{2}\) with her arms extended and of \(0.363 \mathrm{~kg} \cdot \mathrm{m}^{2}\) with her arms close to her body. (These moments of inertia are based on reasonable assumptions about a 60.0-kg skater.) (a) What is her angular velocity in revolutions per second after she pulls in her arms? (b) What is her rotational kinetic energy before and after she does this?
Strategy
In the first part of the problem, we are looking for the skater’s angular velocity \(\omega^{\prime}\) after she has pulled in her arms. To find this quantity, we use the conservation of angular momentum and note that the moments of inertia and initial angular velocity are given. To find the initial and final kinetic energies, we use the definition of rotational kinetic energy given by
\[\mathrm{KE}_{\mathrm{rot}}=\frac{1}{2} I \omega^{2}. \nonumber\]
Solution for (a)
Because torque is negligible (as discussed above), the conservation of angular momentum given in \(I \omega=I^{\prime} \omega^{\prime}\) is applicable. Thus,
\[L=L^{\prime} \nonumber\]
or
\[I \omega=I^{\prime} \omega^{\prime} \nonumber\]
Solving for \(\omega^{\prime}\) and substituting known values into the resulting equation gives
\[\begin{aligned}
\omega^{\prime} &=\frac{I}{I^{\prime}} \omega=\left(\frac{2.34 \mathrm{~kg} \cdot \mathrm{m}^{2}}{0.363 \mathrm{~kg} \cdot \mathrm{m}^{2}}\right)(0.800 \mathrm{rev} / \mathrm{s}) \\
&=5.16 \mathrm{rev} / \mathrm{s}.
\end{aligned} \nonumber\]
Solution for (b)
Rotational kinetic energy is given by
\[\mathrm{KE}_{\mathrm{rot}}=\frac{1}{2} I \omega^{2}. \nonumber\]
The initial value is found by substituting known values into the equation and converting the angular velocity to rad/s:
\[\begin{aligned}
\mathrm{KE}_{\mathrm{rot}} &=(0.5)\left(2.34 \mathrm{~kg} \cdot \mathrm{m}^{2}\right)((0.800 \mathrm{rev} / \mathrm{s})(2 \pi \mathrm{rad} / \mathrm{rev}))^{2} \\
&=29.6 \mathrm{~J}.
\end{aligned} \nonumber\]
The final rotational kinetic energy is
\[\mathrm{KE}_{\mathrm{rot}}^{\prime}=\frac{1}{2} I^{\prime} \omega^{\prime 2}. \nonumber\]
Substituting known values into this equation gives
\[\begin{aligned}
K E_{\text {rot }}^{\prime} &=(0.5)\left(0.363 \mathrm{~kg} \cdot \mathrm{m}^{2}\right)[(5.16 \mathrm{rev} / \mathrm{s})(2 \pi \mathrm{rad} / \mathrm{rev})]^{2} \\
&=191 \mathrm{~J}.
\end{aligned} \nonumber\]
Discussion
In both parts, there is an impressive increase. First, the final angular velocity is large, although most world-class skaters can achieve spin rates about this great. Second, the final kinetic energy is much greater than the initial kinetic energy. The increase in rotational kinetic energy comes from work done by the skater in pulling in her arms. This work is internal work that depletes some of the skater’s food energy.
There are several other examples of objects that increase their rate of spin because something reduced their moment of inertia. Tornadoes are one example. Storm systems that create tornadoes are slowly rotating. When the radius of rotation narrows, even in a local region, angular velocity increases, sometimes to the furious level of a tornado. Earth is another example. Our planet was born from a huge cloud of gas and dust, the rotation of which came from turbulence in an even larger cloud. Gravitational forces caused the cloud to contract, and the rotation rate increased as a result. (See Figure \(\PageIndex{3}\).)
In case of human motion, one would not expect angular momentum to be conserved when a body interacts with the environment as its foot pushes off the ground. Astronauts floating in space aboard the International Space Station have no angular momentum relative to the inside of the ship if they are motionless. Their bodies will continue to have this zero value no matter how they twist about as long as they do not give themselves a push off the side of the vessel.
Exercise \(\PageIndex{1}\)
Is angular momentum completely analogous to linear momentum? What, if any, are their differences?
- Answer
-
Yes, angular and linear momentums are completely analogous. While they are exact analogs they have different units and are not directly inter-convertible like forms of energy are.
Section Summary
- Every rotational phenomenon has a direct translational analog , likewise angular momentum \(L\) can be defined as \(L=I \omega\).
- This equation is an analog to the definition of linear momentum as \(p=m v\). The relationship between torque and angular momentum is \(\text { net } \tau=\frac{\Delta L}{\Delta t}\).
- Angular momentum, like energy and linear momentum, is conserved. This universally applicable law is another sign of underlying unity in physical laws. Angular momentum is conserved when net external torque is zero, just as linear momentum is conserved when the net external force is zero.
Glossary
- rotational kinetic energy
- the kinetic energy due to the rotation of an object. This is part of its total kinetic energy