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In the example below, note that the process of getting the equation in standard form is identical with hyperbolas and ellipses. The extra last step—rewriting a multiplication by 4 as a division by —can come up with ellipses as easily as with hyperbolas. However, it did not come up in the last example, so it is worth taking note of here.
Graph | The problem. We recognize this as a hyperbola because it has an and a term, and have different signs (one is positive and one negative). |
Group together the terms and the terms, with the number on the other side. | |
Factor out the coefficients of the squared terms. In the case of the for this particular equation, the coefficient is minus 12. | |
Complete the square twice. Adding 9 inside the first parentheses adds 27; adding 1 inside the second set subtracts 12. | |
Rewrite and simplify. | |
Divide by 3, to get a 1 on the right. Note, however, that we are still not in standard form, because of the 4 that is multiplied by . The standard form has numbers in the denominator, but not in the numerator. | |
Dividing by is the same as multiplying by 4, so this is still the same equation. But now we are in standard form, since the number is on the bottom. |
However, the process of graphing a hyperbola is quite different from the process of graphing an ellipse. Even here, however, some similarities lurk beneath the surface.
Graph | The problem, carried over from the example above, now in standard form. |
Center: (3,–1) | Comes straight out of the equation, both signs changed, just as with circles and ellipses. |
The square roots of the denominators, just as with the ellipse. But how do we tell which is which? In the case of a hyperbola, the always goes with the positive term . In this case, the term is positive, so the term under it is . | |
Horizontal hyperbola | Again, this is because the term is positive. If the were the positive term, the hyperbola would be vertical, and the number under the term would be considered . |
Remember that the relationship is different: for hyperbolas, | |
Now we begin drawing. Begin by drawing the center at (3,–1). Now, since this is a horizontal ellipse, the vertices will be aligned horizontally around the center. Since , move 1 to the left and 1 to the right, and draw the vertices there. | |
In the other direction—vertical, in this case—we have something called the “conjugate axis.” Move up and down by ( in this case) to draw the endpoints of the conjugate axis. Although not part of the hyperbola, they will help us draw it. | |
Draw a box that goes through the vertices and the endpoints of the conjugate axis. The box is drawn in dotted lines to show that it is not the hyperbola. | |
Draw diagonal lines through the corners of the box—also dotted, because they are also not the hyperbola.These lines are called the asymptotes , and they will guide you in drawing the hyperbola. The further it gets from the vertices, the closer the hyperbola gets to the asymptotes. However, it never crosses them. | |
Now, at last, we are ready to draw the hyperbola. Beginning at the vertices, approach—but do not cross!—the asymptotes. So you see that the asymptotes guide us in setting the width of the hyperbola, performing a similar function to the latus rectum in parabolas. |
The hyperbola is the most complicated shape we deal with in this course, with a lot of steps to memorize.
But there is also a very important concept hidden in all that, and that is the concept of an asymptote. Many functions have asymptotes, which you will explore in far greater depth in more advanced courses. An asymptote is a line that a function approaches, but never quite reaches. The asymptotes are the easiest way to confirm that a hyperbola is not actually two back-to-back parabolas. Although one side of a hyperbola resembles a parabola superficially, parabolas do not have asymptotic behavior—the shape is different.
Remember our comet? It flew into the solar system at a high speed, whipped around the sun, and flew away in a hyperbolic orbit. As the comet gets farther away, the sun’s influence becomes less important, and the comet gets closer to its “natural” path—a straight line. In fact, that straight line is the asymptote of the hyperbolic path.
Before we leave hyperbolas, I want to briefly mention a much simpler equation: . This is the equation of a diagonal hyperbola. The asymptotes are the and axes.
Although the equation looks completely different, the shape is identical to the hyperbolas we have been studying, except that it is rotated 45°.
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