In todays geometry lesson, were going to review Rotation Rules.
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Youre going to learn about rotational symmetry, back-to-back reflections, and common reflections about the origin.
Lets dive in and see how this works!
A rotation is an isometric transformation that turns every point of a figure through a specified angle and direction about a fixed point.
To describe a rotation, you need three things:
The most common rotations are 180° or 90° turns, and occasionally, 270° turns, about the origin, and affect each point of a figure as follows:
When rotating a point 90 degrees counterclockwise about the origin our point A(x,y) becomes A'(-y,x). In other words, switch x and y and make y negative.
When rotating a point 180 degrees counterclockwise about the origin our point A(x,y) becomes A'(-x,-y). So all we do is make both x and y negative.
When rotating a point 270 degrees counterclockwise about the origin our point A(x,y) becomes A'(y,-x). This means, we switch x and y and make x negative.
And just as we saw how two reflections back-to-back over parallel lines is equivalent to one translation, if a figure is reflected twice over intersecting lines, this composition of reflections is equal to one rotation.
In fact, the angle of rotation is equal to twice that of the acute angle formed between the intersecting lines.
Lastly, a figure in a plane has rotational symmetry if the figure can be mapped onto itself by a rotation of 180° or less. This means that if we turn an object 180° or less, the new image will look the same as the original preimage. And when describing rotational symmetry, it is always helpful to identify the order of rotations and the magnitude of rotations.
For more information, please visit what direction is counterclockwise.
The order of rotations is the number of times we can turn the object to create symmetry, and the magnitude of rotations is the angle in degree for each turn, as nicely stated by Math Bits Notebook.
In the video that follows, youll look at how to:
38 min
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