Rotation is the movement of an object in a circular motion. A two-dimensional object rotates around a center of rotation. A three-dimensional object rotates around a line called an axis. If the axis of rotation is within the body, the body is said to rotate upon itself; spin implies a quick rotation, perhaps freely-moving with angular momentum. A circular motion about an external point, for example the Earth around the Sun, is more properly called orbital revolution.
Mathematically, a rotation is a rigid body movement which keeps a point fixed; unlike a translation. This definition is applicable both for rotations in a plane (two dimensions) and in space (three dimensions). It turns out that a rotation in the three-dimensional space keeps fixed not just a single point, but rather an entire line; that is to say, any rotation in the three dimensional space is a rotation around an axis. This is a consequence of Euler's rotation theorem.
Any rigid body movement is in fact either a rotation, or a translation, or a combination of the two.
If one does a rotation around a point (axis), followed by another rotation around the same point (axis), the total result is yet another rotation. The reverse (inverse) of a rotation is also a rotation. It follows that the rotations around a point or axis form a group. If however one performs rotation around a point (axis) followed by rotation around another point (axis), the overall movement may not be a rotation anymore; it can for example be a translation.
See also: curl, cyclic permutation, Euler angles, rigid body, rotation around a fixed axis, rotation group, rotation matrix, isometry.
In astronomy, rotation is a commonly observed phenomenon. Stars, planets and similar bodies all spin around on their axes (the plural of axis).
This rotation induces a centrifugal acceleration which slightly counteracts the effect of gravity the closer one is to the equator. One effect is that an object weighs slightly less at the equator. Another is that the Earth is slightly deformed into a oblate spheroid.
Another consequence of the rotation of a planet is the phenomenon of precession. Like a gyroscope, the overall effect is a slight "wobble" in the movement of the axis of a planet. Currently the tilt of the Earth's axis to its orbital plane (obliquity of the ecliptic) is 66.5 degrees, but this angle changes slowly (over thousands of years). (See also Precession of the equinoxes and Pole star.)
Moons also revolve about their planet, planets revolve about their star (such as the Earth around the Sun); and stars slowly revolve about their galaxial center. The motion of the components of galaxies is complex, but it usually includes a rotation component.
The Moon makes one complete rotation during one complete revolution around the Earth (a effect called tidal locking) so that the same side of the Moon always faces the Earth (the other side is called the far side of the Moon).
Most planets in our solar system, including Earth, spin in the same direction as they orbit the Sun. The exceptions are Venus, Uranus, and Pluto. Uranus rotates nearly on its side relative to its orbit. Current speculation is that Uranus started off with a typical prograde orientation and was knocked on its side by a large impact early in its history. Venus may be thought of as rotating slowly backwards (or being "upside down").
The speed of rotation is given by the angular frequency (rad/s) or frequency (turns/s, turns/min), or period (seconds, days, etc.). The time-rate of change of angular frequency is angular acceleration (rad/s²), This change is caused by torque. The ratio of the two (how heavy is it to start, stop, or otherwise change rotation) is given by the moment of inertia.
The angular velocity vector also describes the direction of the axis of rotation. Similarly the torque is a vector.
According to the right-hand rule, the direction away from the observer is associated with clockwise rotation and the direction towards the observer with counterclockwise rotation, like a screw.
Euclidean geometry | Celestial mechanics
Rotace | Rotation | Rotation (Physik) | Rotación | Rotacio | Rotation | Rotación | Rotazione | Rotatie (voorwerp) | 自転 | Obrót | Вращение | Vrtenje | Rotation | 自转
This article is licensed under the GNU Free Documentation License.
It uses material from the
"Rotation".
Home Page • arts • business • computers • games • health • hospitals • home • kids & teens • news • physicians • recreation• reference • regional • science • shopping • society • sports • world