Precalculus with Integrated CalculusXYZ Homework Edition

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8.4 Ellipses

In the definition of a circle, Definition 8.2, we fixed a point called the center and considered all of the points which were a fixed distance r from that one point. For our next conic section, the ellipse, we fix two distinct points and a distance d to use in our definition.

Figure: 12 for all on the ellipse
Figure 8.66 d 1 + d 2 = d for all ( x , y ) on the ellipse

We may imagine taking a length of string and anchoring it to two points on a piece of paper. The curve traced out by taking a pencil and moving it so the string is always taut is an ellipse. Each ellipse has an assortment of parameters associated with it which we sketch below.

Coordinate-plane figure.
Figure 8.67

An ellipse with center C ; foci F 1 , F 2 ; and vertices V 1 , V 2

As depicted above, the center of the ellipse is the midpoint of the line segment connecting the two foci. The major axis of the ellipse is the line segment connecting two opposite ends of the ellipse which also contains the center and foci. The minor axis of the ellipse is the line segment connecting two opposite ends of the ellipse which contains the center but is perpendicular to the major axis. The vertices of an ellipse are the points of the ellipse which lie on the major axis.

Notice that the center is also the midpoint of the major axis, hence it is the midpoint of the vertices. Also note that the major axis is the longer of the two axes through the center, hence the moniker `major.' Likewise, the minor axis is the shorter of the two, whence the adjective `minor.'

In order to derive the standard equation of an ellipse, we assume that the ellipse has its center at ( 0 , 0 ) , its major axis along the x -axis, and has foci ( c , 0 ) and ( c , 0 ) and vertices ( a , 0 ) and ( a , 0 ) . We will label the y -intercepts of the ellipse as ( 0 , b ) and ( 0 , b ) (We assume a , b , and c are all positive numbers.)

Coordinate-plane figure.
Figure 8.68

Note that since ( a , 0 ) is on the ellipse, it must satisfy the conditions of Definition 8.4. That is, the distance from ( c , 0 ) to ( a , 0 ) plus the distance from ( c , 0 ) to ( a , 0 ) must equal the fixed distance d . Since all of these points lie on the x -axis, we get

distance from  ( c , 0 )  to  ( a , 0 ) + distance from  ( c , 0 )  to  ( a , 0 ) = d ( a + c ) + ( a c ) = d 2 a = d

In other words, the fixed distance d mentioned in the definition of the ellipse is none other than the length of the major axis. We now use that fact ( 0 , b ) is on the ellipse, along with the fact that d = 2 a to get

distance from  ( c , 0 )  to  ( 0 , b ) + distance from  ( c , 0 )  to  ( 0 , b ) = 2 a ( 0 ( c ) ) 2 + ( b 0 ) 2 + ( 0 c ) 2 + ( b 0 ) 2 = 2 a b 2 + c 2 + b 2 + c 2 = 2 a 2 b 2 + c 2 = 2 a b 2 + c 2 = a

From this, we get a 2 = b 2 + c 2 , or b 2 = a 2 c 2 , which will prove useful later. Now consider a point ( x , y ) on the ellipse. Applying Definition 8.4, we get

distance from  ( c , 0 )  to  ( x , y ) + distance from  ( c , 0 )  to  ( x , y ) = 2 a ( x ( c ) ) 2 + ( y 0 ) 2 + ( x c ) 2 + ( y 0 ) 2 = 2 a ( x + c ) 2 + y 2 + ( x c ) 2 + y 2 = 2 a

In order to make sense of this situation, we need to make good use of Intermediate Algebra.

( x + c ) 2 + y 2 + ( x c ) 2 + y 2 = 2 a ( x + c ) 2 + y 2 = 2 a ( x c ) 2 + y 2 ( ( x + c ) 2 + y 2 ) 2 = ( 2 a ( x c ) 2 + y 2 ) 2 ( x + c ) 2 + y 2 = 4 a 2 4 a ( x c ) 2 + y 2 + ( x c ) 2 + y 2 4 a ( x c ) 2 + y 2 = 4 a 2 + ( x c ) 2 ( x + c ) 2 4 a ( x c ) 2 + y 2 = 4 a 2 4 c x a ( x c ) 2 + y 2 = a 2 c x ( a ( x c ) 2 + y 2 ) 2 = ( a 2 c x ) 2 a 2 ( ( x c ) 2 + y 2 ) = a 4 2 a 2 c x + c 2 x 2 a 2 x 2 2 a 2 c x + a 2 c 2 + a 2 y 2 = a 4 2 a 2 c x + c 2 x 2 a 2 x 2 c 2 x 2 + a 2 y 2 = a 4 a 2 c 2 ( a 2 c 2 ) x 2 + a 2 y 2 = a 2 ( a 2 c 2 )

We are nearly finished. Recall that b 2 = a 2 c 2 so that

( a 2 c 2 ) x 2 + a 2 y 2 = a 2 ( a 2 c 2 ) b 2 x 2 + a 2 y 2 = a 2 b 2 x 2 a 2 + y 2 b 2 = 1

This equation is for an ellipse centered at the origin. To get the formula for the ellipse centered at ( h , k ) , we could use the transformations from Section 5.4 or re-derive the equation using Definition 8.4 and the distance formula to obtain the formula below.

Some remarks about Equation 8.5 are in order. First note that the values a and b determine how far in the x and y directions, respectively, one counts from the center to arrive at points on the ellipse.

Also note that if a > b , then we have an ellipse whose major axis is horizontal, and hence, the foci lie to the left and right of the center. In this case, as we've seen in the derivation, the distance from the center to the focus, c , can be found by c = a 2 b 2 .

If b > a , the roles of the major and minor axes are reversed, and the foci lie above and below the center. In this case, c = b 2 a 2 . In either case, it's best to just remember that c is the distance from the center to each focus, and, formulaically, c = bigger denominator smaller denominator .

Finally, it is worth mentioning that if we compare Equation 8.5 with the alternate standard equation of the circle, Equation 8.4, the only difference between the forms is that with a circle, the denominators are the same, and with an ellipse, they are different.

If we take a transformational approach, we can consider both Equations 8.5 and 8.4 as shifts and stretches of the Unit Circle x 2 + y 2 = 1 in Definition 8.3. Replacing x with ( x h ) and y with ( y k ) causes the usual horizontal and vertical shifts. Replacing x with x a and y with y b causes the usual vertical and horizontal stretches.

In other words, it is perfectly fine to think of an ellipse as the deformation of a circle in which the circle is stretched farther in one direction than the other.

As seen in Example 8.4.1 above, it is often necessary to algebraically manipulate a given equation into the standard form of Equation 8.5 in order to graph. We summarize one approach below.

To Write the Equation of an Ellipse in Standard Form

  1. Group common variables together on one side of the equation and put the constant on the other.
  2. Complete the square on both variables as needed.
  3. Divide both sides, if needed, to obtain 1 on one side of the equation.

If we think of a circle as being `perfectly round,' then ellipses, being deformed circles, have varying degrees of `roundness.' We quantify this idea with the notion of eccentricity defined formally below.

In an ellipse, the foci are closer to the center than the vertices, so 0 < e < 1 . The ellipse below on left has eccentricity e 0.66 ; for the ellipse below on the right, e 0.98 . In general, the closer the eccentricity is to 0 , the less `eccentric' or more `circular' the ellipse appears. On the other hand, the closer the eccentricity is to 1 , the more `eccentric' the ellipse is and it appears less `circular.'

Coordinate-plane figure.
Figure 8.75
Coordinate-plane figure.
Figure 8.76

e 0.66

e 0.98

According to Kepler's Laws of Planetary Motion , each planet orbits the Sun in an elliptical path with the Sun at one focus. The eccentricity is therefore an important orbital parameter. We investigate the orbit of Mercury in the following example.

As with parabolas, ellipses have a reflective property. If we imagine the dashed lines below representing sound waves, then it can be shown that the waves emanating from one focus reflect off the top of the ellipse and head towards the other focus.

Coordinate-plane figure.
Figure 8.78

Such geometry is exploited in the construction of so-called `Whispering Galleries'. If a person whispers at one focus, a person standing at the other focus will hear the first person as if they were standing right next to them. We explore the Whispering Galleries in our last example.

Exercises

In Exercises -, graph the ellipse in the x y -plane. Find the center, the lines which contain the major and minor axes, the vertices, the endpoints of the minor axis, the foci and the eccentricity.

  1. x 2 169 + y 2 25 = 1
  2. x 2 9 + y 2 25 = 1
  3. ( x 2 ) 2 4 + ( y + 3 ) 2 9 = 1
  4. ( x + 5 ) 2 16 + ( y 4 ) 2 1 = 1
  5. ( x 1 ) 2 10 + ( y 3 ) 2 11 = 1
  6. ( x 1 ) 2 9 + ( y + 3 ) 2 4 = 1
  7. ( x + 2 ) 2 16 + ( y 5 ) 2 20 = 1
  8. ( x 4 ) 2 8 + ( y 2 ) 2 18 = 1

In Exercises -, put the equation in standard form. Find the center, the lines which contain the major and minor axes, the vertices, the endpoints of the minor axis, the foci and the eccentricity.6

  1. 9 x 2 + 25 y 2 54 x 50 y 119 = 0
  2. 12 x 2 + 3 y 2 30 y + 39 = 0
  3. 5 x 2 + 18 y 2 30 x + 72 y + 27 = 0
  4. x 2 2 x + 2 y 2 12 y + 3 = 0
  5. 9 x 2 + 4 y 2 4 y 8 = 0
  6. 6 x 2 + 5 y 2 24 x + 20 y + 14 = 0
  7. For each of the odd numbered equations given in Exercises -, find two or more explicit functions of x represented by each of the equations. (See Example 8.2.2 in Section 8.2.)

In Exercises -, graph each function by recognizing it as a semi ellipse.

  1. f ( x ) = 16 4 x 2
  2. g ( x ) = 1 2 6 x x 2
  3. f ( x ) = 2 3 2 x x 2
  4. g ( x ) = 2 + 2 9 x 2

In Exercises -, find an equation for the ellipse or semi ellipse whose graph is given.

  1. Coordinate-plane figure.
    Figure 8.80
  2. Coordinate-plane figure.
    Figure 8.81
  3. Figure: ,-intercept
    Figure 8.82 x , y -intercept ( 0 , 0 )
  4. Figure: ,-intercept
    Figure 8.83 x , y -intercept ( 0 , 0 )

In Exercises -, find the standard form of the equation of the ellipse which has the given properties.

  1. Center ( 3 , 7 ) , Vertex ( 3 , 2 ) , Focus ( 3 , 3 )
  2. Foci ( 0 , ± 5 ) , Vertices ( 0 , ± 8 ) .
  3. Foci ( ± 3 , 0 ) , length of the Minor Axis 10
  4. Vertices ( 3 , 2 ) , ( 13 , 2 ) ; Endpoints of the Minor Axis ( 8 , 4 ) , ( 8 , 0 )
  5. Center ( 5 , 2 ) , Vertex ( 0 , 2 ) , eccentricity 1 2
  6. All points on the ellipse are in Quadrant IV except ( 0 , 9 ) and ( 8 , 0 ) . (One might also say that the ellipse is “tangent to the axes” at those two points.)
  7. Repeat Example 8.4.3 for a whispering gallery 200 feet wide and 75 feet tall.
  8. An elliptical arch is constructed which is 6 feet wide at the base and 9 feet tall in the middle. Find the height of the arch exactly 1 foot in from the base of the arch. Compare your result with your answer to Exercise in Section 8.2.
  9. The Earth's orbit around the sun is an ellipse with the sun at one focus and eccentricity e 0.0167 . The length of the semimajor axis (that is, half of the major axis) is defined to be 1 astronomical unit (AU). The vertices of the elliptical orbit are given special names: `aphelion' is the vertex farthest from the sun, and `perihelion' is the vertex closest to the sun. Find the distance in AU between the sun and aphelion and the distance in AU between the sun and perihelion.
  10. This exercise is a follow-up to Example 8.4.2. Find the equation of the ellipse which models the orbit of Mercury. Graph the ellipse using a graphing utility, and comment on the `roundness' of the orbit.
  11. Some famous examples of whispering galleries include St. Paul's Cathedral in London, England, National Statuary Hall in Washington, D.C., and The Cincinnati Museum Center . With the help of your classmates, research these whispering galleries. How does the whispering effect compare and contrast with the scenario in Example 8.4.3?
  12. With the help of your classmates, research “extracorporeal shock-wave lithotripsy”. It uses the reflective property of the ellipsoid to dissolve kidney stones.

Answers

  1. x 2 169 + y 2 25 = 1

    Center ( 0 , 0 ) Major axis along y = 0 Minor axis along x = 0 Vertices ( 13 , 0 ) , ( 13 , 0 ) Endpoints of Minor Axis ( 0 , 5 ) , ( 0 , 5 ) Foci ( 12 , 0 ) , ( 12 , 0 ) e = 12 13

    Coordinate-plane figure.
    Figure 8.84
  2. x 2 9 + y 2 25 = 1

    Center ( 0 , 0 ) Major axis along x = 0 Minor axis along y = 0 Vertices ( 0 , 5 ) , ( 0 , 5 ) Endpoints of Minor Axis ( 3 , 0 ) , ( 3 , 0 ) Foci ( 0 , 4 ) , ( 0 , 4 ) e = 4 5

    Coordinate-plane figure.
    Figure 8.85
  3. ( x 2 ) 2 4 + ( y + 3 ) 2 9 = 1

    Center ( 2 , 3 ) Major axis along x = 2 Minor axis along y = 3 Vertices ( 2 , 0 ) , ( 2 , 6 ) Endpoints of Minor Axis ( 0 , 3 ) , ( 4 , 3 ) Foci ( 2 , 3 + 5 ) , ( 2 , 3 5 ) e = 5 3

    Coordinate-plane figure.
    Figure 8.86
  4. ( x + 5 ) 2 16 + ( y 4 ) 2 1 = 1

    Center ( 5 , 4 ) Major axis along y = 4 Minor axis along x = 5 Vertices ( 9 , 4 ) , ( 1 , 4 ) Endpoints of Minor Axis ( 5 , 3 ) , ( 5 , 5 ) Foci ( 5 + 15 , 4 ) , ( 5 15 , 4 ) e = 15 4

    Coordinate-plane figure.
    Figure 8.87
  5. ( x 1 ) 2 10 + ( y 3 ) 2 11 = 1

    Center ( 1 , 3 ) Major axis along x = 1 Minor axis along y = 3 Vertices ( 1 , 3 + 11 ) , ( 1 , 3 11 ) Endpoints of the Minor Axis ( 1 10 , 3 ) , ( 1 + 10 , 3 ) Foci ( 1 , 2 ) , ( 1 , 4 ) e = 11 11

    Coordinate-plane figure.
    Figure 8.88
  6. ( x 1 ) 2 9 + ( y + 3 ) 2 4 = 1

    Center ( 1 , 3 ) Major axis along y = 3 Minor axis along x = 1 Vertices ( 4 , 3 ) , ( 2 , 3 ) Endpoints of the Minor Axis ( 1 , 1 ) , ( 1 , 5 ) Foci ( 1 + 5 , 3 ) , ( 1 5 , 3 ) e = 5 3

    Coordinate-plane figure.
    Figure 8.89
  7. ( x + 2 ) 2 16 + ( y 5 ) 2 20 = 1

    Center ( 2 , 5 ) Major axis along x = 2 Minor axis along y = 5 Vertices ( 2 , 5 + 2 5 ) , ( 2 , 5 2 5 ) Endpoints of the Minor Axis ( 6 , 5 ) , ( 2 , 5 ) Foci ( 2 , 7 ) , ( 2 , 3 ) e = 5 5

    Coordinate-plane figure.
    Figure 8.90
  8. ( x 4 ) 2 8 + ( y 2 ) 2 18 = 1

    Center ( 4 , 2 ) Major axis along x = 4 Minor axis along y = 2 Vertices ( 4 , 2 + 3 2 ) , ( 4 , 2 3 2 ) Endpoints of the Minor Axis ( 4 2 2 , 2 ) , ( 4 + 2 2 , 2 ) Foci ( 4 , 2 + 10 ) , ( 4 , 2 10 ) e = 5 3

    Coordinate-plane figure.
    Figure 8.91
  9. ( x 3 ) 2 25 + ( y 1 ) 2 9 = 1 Center ( 3 , 1 ) Major Axis along y = 1 Minor Axis along x = 3 Vertices ( 8 , 1 ) , ( 2 , 1 ) Endpoints of Minor Axis ( 3 , 4 ) , ( 3 , 2 ) Foci ( 7 , 1 ) , ( 1 , 1 ) e = 4 5
  10. x 2 3 + ( y 5 ) 2 12 = 1 Center ( 0 , 5 ) Major axis along x = 0 Minor axis along y = 5 Vertices ( 0 , 5 2 3 ) , ( 0 , 5 + 2 3 ) Endpoints of Minor Axis ( 3 , 5 ) , ( 3 , 5 ) Foci ( 0 , 2 ) , ( 0 , 8 ) e = 3 2
  11. ( x 3 ) 2 18 + ( y + 2 ) 2 5 = 1 Center ( 3 , 2 ) Major axis along y = 2 Minor axis along x = 3 Vertices ( 3 3 2 , 2 ) , ( 3 + 3 2 , 2 ) Endpoints of Minor Axis ( 3 , 2 + 5 ) , ( 3 , 2 5 ) Foci ( 3 13 , 2 ) , ( 3 + 13 , 2 ) e = 26 6
  12. ( x 1 ) 2 16 + ( y 3 ) 2 8 = 1 Center ( 1 , 3 ) Major Axis along y = 3 Minor Axis along x = 1 Vertices ( 5 , 3 ) , ( 3 , 3 ) Endpoints of Minor Axis ( 1 , 3 + 2 2 ) , ( 1 , 3 2 2 ) Foci ( 1 + 2 2 , 3 ) , ( 1 2 2 , 3 ) e = 2 2
  13. x 2 1 + 4 ( y 1 2 ) 2 9 = 1 Center ( 0 , 1 2 ) Major Axis along x = 0 (the y -axis) Minor Axis along y = 1 2 Vertices ( 0 , 2 ) , ( 0 , 1 ) Endpoints of Minor Axis ( 1 , 1 2 ) , ( 1 , 1 2 ) Foci ( 0 , 1 + 5 2 ) , ( 0 , 1 5 2 ) e = 5 3
  14. ( x 2 ) 2 5 + ( y + 2 ) 2 6 = 1 Center ( 2 , 2 ) Major Axis along x = 2 Minor Axis along y = 2 Vertices ( 2 , 2 + 6 ) , ( 2 , 2 6 ) Endpoints of Minor Axis ( 2 5 , 2 ) , ( 2 + 5 , 2 ) Foci ( 2 , 1 ) , ( 2 , 3 ) e = 6 6
  15. For number:

    • f ( x ) = 5 13 169 x 2 represents the upper half of the ellipse.
    • g ( x ) = 5 13 169 x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 3 + 3 2 4 x x 2 represents the upper half of the ellipse.
    • g ( x ) = 3 3 2 4 x x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 3 + 1 10 990 + 220 x 110 x 2 represents the upper half of the ellipse.
    • g ( x ) = 3 1 10 990 + 220 x 110 x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 5 + 1 2 60 20 x 5 x 2 represents the upper half of the ellipse.
    • g ( x ) = 5 1 2 60 20 x 5 x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 1 + 3 5 16 + 6 x x 2 represents the upper half of the ellipse.
    • g ( x ) = 1 3 5 16 + 6 x x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 2 + 1 6 90 + 60 x 10 x 2 represents the upper half of the ellipse.
    • g ( x ) = 2 1 6 90 + 60 x 10 x 2 represents the lower half of the ellipse.

    For number:

    • f ( x ) = 1 2 + 3 2 1 x 2 represents the upper half of the ellipse.
    • g ( x ) = 1 2 3 2 1 x 2 represents the lower half of the ellipse.
  16. f ( x ) = 16 4 x 2

    Coordinate-plane figure.
    Figure 8.92
  17. g ( x ) = 1 2 6 x x 2

    Coordinate-plane figure.
    Figure 8.93
  18. f ( x ) = 2 3 2 x x 2

    Coordinate-plane figure.
    Figure 8.94
  19. g ( x ) = 2 + 2 9 x 2

    Coordinate-plane figure.
    Figure 8.95
  20. ( x 1 ) 2 9 + y 2 16 = 1
  21. ( x 4 ) 2 16 + ( y 4 ) 2 9 = 1
  22. y = 3 3 4 16 x 2
  23. y = 2 8 x x 2 12
  24. ( x 3 ) 2 9 + ( y 7 ) 2 25 = 1
  25. x 2 39 + y 2 64 = 1
  26. x 2 34 + y 2 25 = 1
  27. ( x 8 ) 2 25 + ( y 2 ) 2 4 = 1
  28. ( x 5 ) 2 25 + 4 ( y 2 ) 2 75 = 1
  29. ( x 8 ) 2 64 + ( y + 9 ) 2 81 = 1
  30. Jamie and Jason should stand 100 25 7 33.86 feet from opposite ends of the gallery.
  31. The arch can be modeled by the upper half of x 2 9 + y 2 81 = 1 . One foot in from the base of the arch corresponds to either x = ± 2 . Plugging in x = ± 2 gives y = ± 3 5 and since y represents a height, we choose y = 3 5 6.71 feet.
  32. Distance from the sun to aphelion 1.0167 AU. Distance from the sun to perihelion 0.9833 AU.
  33. ( x 7.4 ) 2 1296 + y 2 1241.24 = 1 . Graphing this equation7 reveals a very `round' orbit.

Adapted from Precalculus, Preliminary 4th Edition (integrated calculus), by Carl Stitz and Jeff Zeager (stitz-zeager.com), licensed under CC BY-NC-SA 3.0. Changes were made: reformatted as an accessible XYZ web edition. License: CC-BY-NC-SA-3.0.

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