# Rotation

# Rotation

A rotation, in geometry, is a transformation where a figure is turned about a point (the center of rotation). It is one of three rigid motions that move a figure in a plane without changing its size or shape. As its name implies, a rotation moves a figure by rotating it around a center somewhere on a plane. This center can be somewhere inside or on the figure, or outside the figure completely. A rotation completely around the central point is called a full turn. It consists of a rotation of 360 degrees. A one-half rotation involves a rotation of 180 degrees, and it is called a half turn. The two other rigid motions are reflections and translations.

Figure 1 illustrates a rotation of 30° around a point C. This rotation is counterclockwise, which is considered positive. Clockwise rotations are negative. The product of two rotations, that is, following one rotation with another, is also a rotation. This assumes that the center of rotation is the same for both. When one moves a heavy box across the room by rotating it first on one corner then on the other, that product is not a rotation because the movement was not about the same central point.

Rotations are so commonplace that it is easy to forget how important they are. A person orients a map by rotating it. A clock shows time by the rotation of its hands. A person fits a key in a lock by rotating the key until its grooves match the pattern on the keyhole. Rotating the letter M 180° changes it into a letter W; while 6s and 9s are alike except for a rotation.

Rotary motions are one of the two basic motions of parts in a machine. An automobile wheel converts rotary (circular) motion into translational (straight-line) motion, and propels the car. A drill bores a hole by cutting away material as it turns. The Earth rotates on its axis. Earth and its Moon rotate around their centers of gravity, and so on.

Astronomy prior to Polish astronomer Nicolaus Copernicus (1473–1543) was greatly complicated by trying to use Earth as the center of the rotation of the planets. When German astronomer and mathematician Johannes Kepler (1571–1630) and Copernicus made the sun the gravitational center, the motions of the planets became far easier to predict and explain (but even with the sun as the center, planetary motion is not strictly rotational).

When points are represented by coordinates, a rotation can be effected algebraically. How difficult this is to do depends upon the location of the center of

rotation and on the kind of coordinate system that is used. In the two most commonly employed systems, the rectangular Cartesian coordinate system and the polar coordinate system, the center of choice is the origin or pole.

In either of these systems a rotation can be thought of as moving the points and leaving the axes fixed, or vice versa. The mathematical connection between these alternatives is a simple one: rotating a set of points clockwise is equivalent to rotating the axes, particularly with reflections, it is usually preferable to leave the axes in place and move the points.

When a point or a set of points is represented with polar coordinates, the equations that connect a point (r, θ) with the rotated image (r’, θ’) are particularly simple (Figure 2). If θ_{1} is the angle of rotation:

r’ = θ

θ’ = θ + θ^{1}

Thus, if the points are rotated 30° counterclockwise, (7,80°) is the image of 7,50°). If the set of points described by the equation r = θ/2 is rotated π units clockwise, its image is described by r = (θ - π)/2. Rectangular coordinates are related to polar coordinates by the equations x = r cos θ and y = r sin θ.

Therefore the equations that connect a point (x, y) with its rotated image (x’, y’) are

θ’ = θ + θ^{1}

Using the trigonometric identities for cos (θ + θ_{1}) and sin (θ + θ_{1}), these can be written x’ = x cos θ_{1} - y sin θ _{1}and y’ = x sin θ_{1} + y cos θ_{1} or, after solving for x and y: x = x’ cos θ_{1} + y sin θ_{1} and y = -x’ sin θ_{1} + y cos θ_{1}.

To use these equations one must resort to a table of sines and cosines, or use a calculator with SIN and COS keys.

One can use the equations for a rotation many ways. One use is to simplify an equation such as x^{2} -xy + y^{2} = 5. For any second-degree polynomial equation in x and y there is a rotation that will eliminate the xy term. In this case, the rotation is 45°, and the resulting equation, after dropping the primes, is 3x^{2}+y^{2} = 10.

Another area in which rotations play an important part is in rotational symmetry. A figure has rotational symmetry if there is a rotation such that the original figure and its image coincide. A square, for example, has rotational symmetry because any rotation about the square’s center, which is a multiple of 90° will result in a square that coincides with the original. An ordinary gear has rotational symmetry. So do the numerous objects such as vases and bowls that are decorated repetitively around the edges. Actual objects can be checked for rotational symmetry by looking at them. Geometric figures described analytically can be tested using the equations for rotations. For example, the spiral r = 28 has two-fold rotational symmetry. When the spiral is rotated 180° the image coincides with the original spiral.

### KEY TERMS

**Rotation—** The spinning of an object on its axis.

**Rotational symmetry—** A property of a figure that allows it to coincide with its image after a suitable rotation.

## Resources

### BOOKS

Jeffrey, Alan. *Mathematics for Engineers and Scientists.* Boca Raton, FL: Chapman & Hall/CRC, 2005.

Noronha, Maria Helena. *Euclidean and Non-Euclidean Geometries.* Upper Saddle River, NJ: Prentice Hall, 2002.

Setek, William M. *Fundamentals of Mathematics.* Upper Saddle River, NJ: Pearson Prentice Hall, 2005.

Silvester, John R. *Geometry: Ancient and Modern.* Oxford, UK, and New York: Oxford University Press, 2001.

Slavin, Stephen L. *Geometry: A Self-teaching Guide.* Hoboken, NJ: John Wiley & Sons, 2005.

Thomas, David Allen. *Modern Geometry.* Pacific Grove, CA: Brooks/Cole, 2001.

J. Paul Moulton

# Rotation

# Rotation

A rotation is one of three rigid motions that move a figure in a **plane** without changing its size or shape. As its name implies, a rotation moves a figure by rotating it around a center somewhere on a plane. This center can be somewhere inside or on the figure, or outside the figure completely. The two other rigid motions are **reflections** and **translations** .

Figure 1 illustrates a rotation of 30° around a point C. This rotation is counterclockwise, which is considered positive. Clockwise rotations are **negative** . The "product" of two rotations, that is, following one rotation
with another, is also a rotation. This assumes that the center of rotation is the same for both. When one moves a heavy box across the room by rotating it first on one corner then on the other, that "product" is not a rotation.

Rotations are so commonplace that it is easy to forget how important they are. A person orients a map by rotating it. A clock shows **time** by the rotation of its hands. A person fits a key in a **lock** by rotating the key until its grooves match the pattern on the keyhole. Rotating an M 180° changes it into a W; 6s and 9s are alike except for a rotation.

Rotary motions are one of the two basic motions of parts in a machine. An **automobile** wheel converts rotary **motion** into translational motion, and propels the car. A drill bores a hole by cutting away material as it turns. The **earth** rotates on its axis. The earth and the **moon** rotate around their centers of gravity, and so on.

**Astronomy** prior to Copernicus was greatly complicated by trying to use the earth as the center of the rotation of the planets. When Kepler and Copernicus made the **sun** the gravitational center, the motions of the planets became far easier to predict and explain (but even with the sun as the center, planetary motion is not strictly rotational).

When points are represented by coordinates, a rotation can be effected algebraically. How hard this is to do depends upon the location of the center of rotation and on the kind of coordinate system which is used. In the two most commonly employed systems, the rectangular Cartesian coordinate system and the polar coordinate system, the center of choice is the origin or pole.

In either of these systems a rotation can be thought of as moving the points and leaving the axes fixed, or vice versa. The mathematical connection between these alternatives is a simple one: rotating a set of points clockwise is equivalent to rotating the axes, particularly with reflections, it is usually preferable to leave the axes in place and move the points.

When a point or a set of points is represented with **polar coordinates** , the equations that connect a point (r, θ) with the rotated image (r', θ') are particularly simple. If θ1 is the **angle** of rotation:

Thus, if the points are rotated 30° counterclockwise, (7,80°) is the image of 7,50°). If the set of points described by the equation r = θ/2 is rotated π units clockwise, its image is described by r = θ - π)/2. Rectangular coordinates are related to polar coordinates by the equations x = r cos θ and y = r sin θ.

Therefore the equations which connect a point (x, y) with its rotated image (x', y') are

Using the trigonometric identities for cos (θ + θ1) and sin (θ + θ1), these can be written x' = x cos θ1 - y sin θ1 and y' = x sin θ1 + y cos θ1 or, after solving for x and y: x = x' cos θ1 + y sin θ1 and y = -x' sin θ1 + y cos θ1.

To use these equations one must resort to a table of sines and cosines, or use a **calculator** with SIN and COS keys.

One can use the equations for a rotation many ways. One use is to simplify an equation such as x2 - xy + y2 = 5. For any second-degree polynomial equation in x and y there is a rotation which will eliminate the xy **term** . In this case the rotation is 45°, and the resulting equation, after dropping the primes, is 3x2 + y2 = 10.

Another area in which rotations play an important part is in rotational **symmetry** . A figure has rotational symmetry if there is a rotation such that the original figure and its image coincide. A square, for example, has rotational symmetry because any rotation about the square's center which is a multiple of 90° will result in a square that coincides with the original. An ordinary gear has rotational symmetry. So do the numerous objects such as vases and bowls which are decorated repetitively around the edges. Actual objects can be checked for rotational symmetry by looking at them. Geometric figures described analytically can be tested using the equations for rotations. For example, the **spiral** r = 28 has two-fold rotational symmetry. When the spiral is rotated 180°, the image coincides with the original spiral.

## Resources

### books

Coxeter, H.S.M., and S. L. Greitzer. *Geometry Revisited.* Washington, DC: The Mathematical Association of America, 1967.

Hilbert, D., and S. Cohn-Vossen. *Geometry and the Imagination.* New York: Chelsea Publishing Co., 1952.

Pettofrezzo, Anthony. *Matrices and Transformations.* New York: Dover Publications, 1966.

Yaglom, I.M. *Geometric Transformations.* Washington, DC: The Mathematical Association of America, 1962.

### periodicals

Alperin, Jonathan. "Groups and Symmetry." In *Mathematics**Today,* edited by Lynn Arthur Steen. New York: Springer-Verlag, 1978.

Weyl, Hermann. "Symmetry." In *The World of Mathematics,* edited by James Newman. New York: Simon and Schuster, 1956.

J. Paul Moulton

## KEY TERMS

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .**Rotation**—The spinning of an object on its axis.

**Rotational symmetry**—A property of a figure that allows it to coincide with its image after a suitable rotation.

# rotation

ro·ta·tion / rōˈtāshən/ •
n. the action of rotating around an axis or center: *the moon moves in the same direction as the earth's rotation.* ∎ (also crop ro·ta·tion) the action or system of rotating crops. ∎ Forestry the cycle of planting, felling, and replanting. ∎ the passing of a privilege or responsibility from one member of a group to another in a regularly recurring succession: *it has become common for senior academics to act as heads of department in rotation.* ∎ a tour of duty, esp. by a medical practitioner in training:

*she was completing a rotation in trauma surgery.*∎ Math. the conceptual operation of turning a system around an axis. ∎ Math. another term for curl (sense 2).DERIVATIVES: ro·ta·tion·al / -shənl/ adj.ro·ta·tion·al·ly / -shənl-ē/ adv.

# rotation

**rotation** Turning of a body about its axis. In the Solar System, the Sun and all the planets, with the exception of Uranus and Venus, rotate from w to e.

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#### NEARBY TERMS

**rotation**