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The solar system is another example of how conservation of angular momentum works in our universe. Our solar system was born from a huge cloud of gas and dust that initially had rotational energy. Gravitational forces caused the cloud to contract, and the rotation rate increased as a result of conservation of angular momentum ( [link] ).

An illustration of the formation of the solar system from a cloud of gas and dust. At first, the gas cloud is rotating with angular velocity omega and has angular momentum L. It forms a fairly continuous disc in the plane of rotation. Later, the disc is rotating with angular velocity omega prime but still has angular momentum L. The disc starts to break up into concentric rings. The gaps between the rings grow. Eventually, the gas in the rings forms a star in the center and planets whose orbits trace the rings from which they came. In all cases, the angular velocity is in the same direction as that of the original gas cloud and the angular momentum is L.
The solar system coalesced from a cloud of gas and dust that was originally rotating. The orbital motions and spins of the planets are in the same direction as the original spin and conserve the angular momentum of the parent cloud. (credit: modification of work by NASA)

We continue our discussion with an example that has applications to engineering.

Coupled flywheels

A flywheel rotates without friction at an angular velocity ω 0 = 600 rev / min on a frictionless, vertical shaft of negligible rotational inertia. A second flywheel, which is at rest and has a moment of inertia three times that of the rotating flywheel, is dropped onto it ( [link] ). Because friction exists between the surfaces, the flywheels very quickly reach the same rotational velocity, after which they spin together. (a) Use the law of conservation of angular momentum to determine the angular velocity ω of the combination. (b) What fraction of the initial kinetic energy is lost in the coupling of the flywheels?

In the drawing on the left, two flywheels are shown. Their axes are vertical and aligned, and the wheels face each other, but the wheels are separate from one another. The lower wheel has moment to inertia I sub 0 and is spinning counterclockwise as viewed from above. The upper wheel has moment to inertia 3 I sub 0 and is at rest. In the drawing on the right, the wheels are coupled together and spin counterclockwise as viewed from above.
Two flywheels are coupled and rotate together.

Strategy

Part (a) is straightforward to solve for the angular velocity of the coupled system. We use the result of (a) to compare the initial and final kinetic energies of the system in part (b).

Solution

a. No external torques act on the system. The force due to friction produces an internal torque, which does not affect the angular momentum of the system. Therefore conservation of angular momentum gives

I 0 ω 0 = ( I 0 + 3 I 0 ) ω , ω = 1 4 ω 0 = 150 rev / min = 15.7 rad / s .

b. Before contact, only one flywheel is rotating. The rotational kinetic energy of this flywheel is the initial rotational kinetic energy of the system, 1 2 I 0 ω 0 2 . The final kinetic energy is 1 2 ( 4 I 0 ) ω 2 = 1 2 ( 4 I 0 ) ( ω 0 4 ) 2 = 1 8 I 0 ω 0 2 .

Therefore, the ratio of the final kinetic energy to the initial kinetic energy is

1 8 I 0 ω 0 2 1 2 I 0 ω 0 2 = 1 4 .

Thus, 3/4 of the initial kinetic energy is lost to the coupling of the two flywheels.

Significance

Since the rotational inertia of the system increased, the angular velocity decreased, as expected from the law of conservation of angular momentum. In this example, we see that the final kinetic energy of the system has decreased, as energy is lost to the coupling of the flywheels. Compare this to the example of the skater in [link] doing work to bring her arms inward and adding rotational kinetic energy.

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Check Your Understanding A merry-go-round at a playground is rotating at 4.0 rev/min. Three children jump on and increase the moment of inertia of the merry-go-round/children rotating system by 25 % . What is the new rotation rate?

Using conservation of angular momentum, we have
I ( 4.0 rev/min ) = 1.25 I ω f , ω f = 1.0 1.25 ( 4.0 rev / min ) = 3.2 rev / min

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Dismount from a high bar

An 80.0-kg gymnast dismounts from a high bar. He starts the dismount at full extension, then tucks to complete a number of revolutions before landing. His moment of inertia when fully extended can be approximated as a rod of length 1.8 m and when in the tuck a rod of half that length. If his rotation rate at full extension is 1.0 rev/s and he enters the tuck when his center of mass is at 3.0 m height moving horizontally to the floor, how many revolutions can he execute if he comes out of the tuck at 1.8 m height? See [link] .

A drawing of a gymnast dismounting from a 3 m tall high bar. He starts the dismount at full extension above the bar, then tucks when he is moving horizontally to the floor, level with the bar. The gymnast is 1.8 meters tall.
A gymnast dismounts from a high bar and executes a number of revolutions in the tucked position before landing upright.

Strategy

Using conservation of angular momentum, we can find his rotation rate when in the tuck. Using the equations of kinematics, we can find the time interval from a height of 3.0 m to 1.8 m. Since he is moving horizontally with respect to the ground, the equations of free fall simplify. This will allow the number of revolutions that can be executed to be calculated. Since we are using a ratio, we can keep the units as rev/s and don’t need to convert to radians/s.

Solution

The moment of inertia at full extension is I 0 = 1 12 m L 2 = 1 12 80.0 kg ( 1 . 8 m ) 2 = 21.6 kg · m 2 .

The moment of inertia in the tuck is I f = 1 12 m L f 2 = 1 12 80.0 kg ( 0 . 9 m ) 2 = 5.4 kg · m 2 .

Conservation of angular momentum: I f ω f = I 0 ω 0 ω f = I 0 ω 0 I f = 21.6 kg · m 2 ( 1.0 rev / s ) 5.4 kg · m 2 = 4.0 rev / s .

Time interval in the tuck: t = 2 h g = 2 ( 3.0 1.8 ) m 9.8 m / s = 0.5 s .

In 0.5 s, he will be able to execute two revolutions at 4.0 rev/s.

Significance

Note that the number of revolutions he can complete will depend on how long he is in the air. In the problem, he is exiting the high bar horizontally to the ground. He could also exit at an angle with respect to the ground, giving him more or less time in the air depending on the angle, positive or negative, with respect to the ground. Gymnasts must take this into account when they are executing their dismounts.

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Practice Key Terms 1

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Source:  OpenStax, University physics volume 1. OpenStax CNX. Sep 19, 2016 Download for free at http://cnx.org/content/col12031/1.5
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