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Licensed under Creative Commons Attribution-Share Alike 4.0 (Andrejdam).

This article is about the rotation of an object around a single axis (a one-dimensional rotation). For the kinetic energy of an object that rotates in three dimensions, see rigid rotor.

**Rotational energy** or **angular kinetic energy** is kinetic energy due to the rotation of an object and is part of its total kinetic energy. Looking at rotational energy separately around an object's axis of rotation, the following dependence on the object's moment of inertia is observed:

- $E_{\mathrm {rotational} }={\frac {1}{2}}I\omega ^{2}$

where

- $\omega \$ is the angular velocity
- $I\$ is the moment of inertia around the axis of rotation
- $E\$ is the kinetic energy

The mechanical work required for / applied during rotation is the torque times the rotation angle. The instantaneous power of an angularly accelerating body is the torque times the angular velocity. For free-floating (unattached) objects, the axis of rotation is commonly around its center of mass.

Note the close relationship between the result for rotational energy and the energy held by linear (or translational) motion:

- $E_{\mathrm {translational} }={\frac {1}{2}}mv^{2}$

In the rotating system, the moment of inertia, *I*, takes the role of the mass, *m*, and the angular velocity, $\omega$, takes the role of the linear velocity, *v*. The rotational energy of a rolling cylinder varies from one half of the translational energy (if it is massive) to the same as the translational energy (if it is hollow).

An example is the calculation of the rotational kinetic energy of the Earth. As the Earth has a period of about 23.93 hours, it has an angular velocity of 7.29×10^{−5} rad/s. The Earth has a moment of inertia, I = 8.04×10^{37} kg·m^{2}.^{[1]} Therefore, it has a rotational kinetic energy of 2.138×10^{29} J.

Another example of actually using earth's rotational energy is the locating of opportune spaceports. The European spaceport in French Guiana (on S. American continent). <Wiki: Guiana Space Centre>. This is within about 5 degrees of the equator, so space rocket launches (for primarily geo-stationary satellites) from here to the east obtain nearly all of the full rotational speed of the earth at the equator (about 1,000 mph, sort of a "sling-shot benefit). Rocket launches easterly from Kennedy (USA) on the other hand obtain only about 400 mph added benefit <Wikipedia/Guiana Space Centre>, due to the lower relative rotational speed of the earth at that northerly latitude. This saves significant rocket fuel per launch, so this tends to be a relatively more economic spaceport.

Part of the earth's rotational energy can also be tapped using tidal power. Additional friction of the two global tidal waves creates energy in a physical manner, infinitesimally slowing down Earth's angular velocity *ω*. Due to the conservation of angular momentum, this process transfers angular momentum to the Moon's orbital motion, increasing its distance from Earth and its orbital period (see tidal locking for a more detailed explanation of this process).

Chebychev–Grübler–Kutzbach criterionWind turbineMembraneRotor (electric)Solar thermal energyWind turbine designRenewable energyTorqueEnergyThermal conduction

This article uses material from the Wikipedia article "Rotational energy", which is released under the Creative Commons Attribution-Share-Alike License 3.0. There is a list of all authors in Wikipedia

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