Translational, Rotational and Vibrational Energy

Main Idea

In many cases, analyzing the kinetic energy of an object is in fact more difficult than just applying the formula [math]\displaystyle{ K = \cfrac{1}{2}mv^2 }[/math]. When you throw a ball, for example, the ball is traveling through the air, but will also rotate around its own axis. When analyzing more complicated movements like this one, it is necessary to break kinetic energy into different parts and analyze each one separately.

The kinetic energy associated to the movement of the center of mass of the object is called the translational kinetic energy. In terms of the example above, this would be the kinetic energy of the movement of the center of mass of the ball through the air.

The kinetic energy associated to the rotation or vibration of the atoms of the object around its center or axis is called the relative kinetic energy. This kinetic energy is the energy of the ball rotating on its own axis. If this is difficult to visualize, think about how an american football rotates about its center axis when you throw it correctly.

A Mathematical Model

As we just saw, kinetic energy can be divided into two energies: translational kinetic energy and rotational kinetic energy. Therefore, the total kinetic energy of a system is equal to the sum of those two kinetic energies:

[math]\displaystyle{ K_{total} = K_{translational} + K_{relative} }[/math]

The relative kinetic energy term can itself be divided into two other terms. The energy of the atoms of the object relative to its center or axis can either be rotational (this is the case of the football thrown in the air) or vibrational. Therefore, we have:

[math]\displaystyle{ K_{total} = K_{translational} + K_{relative} = K_{translational} + K_{rotational} + K_{vibrational} }[/math]

Because the translational kinetic energy is associated to the movement of the center of mass of the object, it is important to know how to calculate the location of the center of mass.

[math]\displaystyle{ r_{CM} = \cfrac{m_1r_1 + m_2r_2+m_3r_3 + ...}{Mass} }[/math]

The velocity of the center of mass is given by the equation:

[math]\displaystyle{ v_{CM} = \cfrac{m_1v_1 + m_2v_2+m_3v_3 + ...}{Mass} }[/math]

Using the total mass and the velocity of the center of mass, we can thus calculate the translational energy of an object:

[math]\displaystyle{ K_{translational} = \cfrac{1}{2}M_{total}v_{CM}^2 }[/math]

Similarly, we can calculate rotational kinetic energy with the following formula:

[math]\displaystyle{ K_{rotational} = \cfrac{1}{2}M_{total}v{CM}^2 }[/math]

But rotational kinetic energy can also be calculated with the moment of inertia and the angular speed of an object. The moment of inertia of an object is the sum of the products of the mass of each particle in the object with the square of their distance from the axis of rotation. The general formula for calculating the moment of inertia of an object is:

[math]\displaystyle{ I = m_1r_{\perp,1}^2 + m_2r_2{\perp,2}^2 + m_3r_{\perp,3}^2 +... }[/math] [math]\displaystyle{ kg.m^2 }[/math]

Some examples of moments of inertia:

For a ring, the moment of inertia formula leads to [math]\displaystyle{ I = MR^2 }[/math] because all of the atoms in the ring are at equal distance from the center.

For a long thin rod, we get [math]\displaystyle{ I = \cfrac{1}{12}ML^2 }[/math], where L is the length of the rod.

For a cylinder of length L and radius R, the formula leads us to [math]\displaystyle{ \cfrac{1}{12}ML^2 + \cfrac{1}{4}MR^2 }[/math]

For a disk, [math]\displaystyle{ I = \cfrac{1}{2}MR^2 }[/math]

For a sphere , [math]\displaystyle{ I = \cfrac{2}{5}MR^2 }[/math]

The angular speed is a calculation of how fast the object is rotating. It can be calculated from the period, T, with the following formula : [math]\displaystyle{ \omega = \cfrac{2\pi}{T} }[/math]

The rotational kinetic energy can thus be calculated using these two variables: [math]\displaystyle{ = K_{rotational} = \cfrac{1}{2}I\omega^2 }[/math].

A Computational Model

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