1. Learning objectives

Learning objectives

Graph an ellipse with center at the origin

Find the equation of an ellipse with center at the origin

Graph an ellipse with center not at the origin

Solve application with ellipses

2. Graph an Ellipse with Center at the Origin

Graph an Ellipse with Center at the Origin

The next conic section we will look at is an ellipse. We define an ellipse as all points in a plane where the sum of the distances from two fixed points is constant. Each of the given points is called a focus of the ellipse.

An ellipse is all points in a plane where the sum of the distances from two fixed points is constant. Each of the fixed points is called a focus of the ellipse.

We can draw an ellipse by taking some fixed length of flexible string and attaching the ends to two thumbtacks. We use a pen to pull the string taut and rotate it around the two thumbtacks. The figure that results is an ellipse.

A line drawn through the foci intersect the ellipse in two points. Each point is called a vertex of the ellipse. The segment connecting the vertices is called the major axis. The midpoint of the segment is called the center of the ellipse. A segment perpendicular to the major axis that passes through the center and intersects the ellipse in two points is called the minor axis.

We mentioned earlier that our goal is to connect the geometry of a conic with algebra. Placing the ellipse on a rectangular coordinate system gives us that opportunity. In the figure, we placed the ellipse so the foci $((-c,0),(c,0))$ are on the x-axis and the center is the origin.

The definition states the sum of the distance from the foci to a point $(x,y)$ is constant. So ${d}_{1}+{d}_{2}$ is a constant that we will call $2a$ so, ${d}_{1}+{d}_{2}=2a.$ We will use the distance formula to lead us to an algebraic formula for an ellipse.

\begin{array}{lccclccrlccc} \begin{array}{l} \mathrm{Use the distance formula to find}\,{d}_{1},{d}_{2}. \\ \end{array} & & & \begin{array}{clcll} {d}_{1} & + & {d}_{2} & = & 2a \\ \sqrt{{(x-(-c))}^{2}+{(y-0)}^{2}} & + & \sqrt{{(x-c)}^{2}+{(y-0)}^{2}} & = & 2a \\ \end{array} \\ \begin{array}{l} \mathrm{After eliminating radicals and simplifying,} \\ \mathrm{we get:} \\ \end{array} & & & \frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{a}^{2}-{c}^{2}}\,=\,1\, \\ \begin{array}{l} \mathrm{To simplify the equation of the ellipse, we} \\ \mathrm{let}\,{a}^{2}-{c}^{2}={b}^{2}. \\ \end{array} & & & \\ \begin{array}{l} \mathrm{So, the equation of an ellipse centered at the} \\ \mathrm{origin in standard form is:} \\ \end{array} & & & \frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}}\,=\,1\, \\ \end{array}

To graph the ellipse, it will be helpful to know the intercepts. We will find the x-intercepts and y-intercepts using the formula.

\begin{array}{lccllcclcccccccccccccccccccccccccccc} \begin{array}{cccllcclcccccc} & & & \,y\mathrm{-intercepts} \\ \begin{array}{l} \mathrm{Let}\,x=0. \\ \end{array} & & & \begin{array}{rll} \frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}} & = & 1 \\ \frac{{0}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}} & = & 1 \\ \frac{{y}^{2}}{{b}^{2}} & = & 1 \\ {y}^{2} & = & {b}^{2} \\ y & = & \pm{}b \\ \end{array} \\ \end{array} & & & \begin{array}{cccllcclcccccc} & & & \,x\mathrm{-intercepts} \\ \begin{array}{l} \mathrm{Let}\,y=0. \\ \end{array} & & & \begin{array}{rll} \frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}} & = & 1 \\ \frac{{x}^{2}}{{a}^{2}}+\frac{{0}^{2}}{{b}^{2}} & = & 1 \\ \frac{{x}^{2}}{{a}^{2}} & = & 1 \\ {x}^{2} & = & {a}^{2} \\ x & = & \pm{}a \\ \end{array} \\ \end{array} \\ \mathrm{The}\,y\mathrm{-intercepts are}\,(0,b)\,\mathrm{and}\,(0,-b). & & & \mathrm{The}\,x\mathrm{-intercepts are}\,(a,0)\,\mathrm{and}\,(-a,0). \\ \end{array}

The standard form of the equation of an ellipse with center $(0,0),$ is

\frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}}=1

The x-intercepts are $(a,0)$ and $(-a,0).$ The y-intercepts are $(0,b)$ and $(0,-b).$

Notice that when the major axis is horizontal, the value of a will be greater than the value of b and when the major axis is vertical, the value of b will be greater than the value of a. We will use this information to graph an ellipse that is centered at the origin.

$\frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}}=1$ · $a>b$ · $b>a$ Major axis · on the x- axis. · on the y-axis.

x-intercepts · $(-a,0),$ $(a,0)$ y-intercepts · $(0,-b),$ $(0,b)$

Table

11.2

3. Example 11.20

Example 11.20

How to Graph an Ellipse with Center (0, 0)

Graph: $\frac{{x}^{2}}{4}+\frac{{y}^{2}}{9}=1.$

We summarize the steps for reference.

How to Graph an Ellipse with Center $(0,0).$

Step 1. Write the equation in standard form.
Step 2. Determine whether the major axis is horizontal or vertical.
Step 3. Find the endpoints of the major axis.
Step 4. Find the endpoints of the minor axis
Step 5. Sketch the ellipse.

Sometimes our equation will first need to be put in standard form.

4. Example 11.21

Example 11.21

Graph ${x}^{2}+4{y}^{2}=16.$

Solution

5. Find the Equation of an Ellipse with Center at the Origin

Find the Equation of an Ellipse with Center at the Origin

If we are given the graph of an ellipse, we can find the equation of the ellipse.

6. Example 11.22

Example 11.22

Find the equation of the ellipse shown.

Solution

We recognize this as an ellipse that is centered at the origin. · $\frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}}=1$ Since the major axis is horizontal and the distance from the center to the vertex is 4, we know $a=4$ and so ${a}^{2}=16$ . · $\frac{{x}^{2}}{16}+\frac{{y}^{2}}{{b}^{2}}=1$ The minor axis is vertical and the distance from the center to the ellipse is 3, we know $b=3$ and so ${b}^{2}=9$ . · $\frac{{x}^{2}}{16}+\frac{{y}^{2}}{9}=1$

7. Graph an Ellipse with Center Not at the Origin

Graph an Ellipse with Center Not at the Origin

The ellipses we have looked at so far have all been centered at the origin. We will now look at ellipses whose center is $(h,k).$

The equation is $\frac{{(x-h)}^{2}}{{a}^{2}}+\frac{{(y-k)}^{2}}{{b}^{2}}=1$ and when $a>b,$ the major axis is horizontal so the distance from the center to the vertex is a. When $b>a,$ the major axis is vertical so the distance from the center to the vertex is b.

The standard form of the equation of an ellipse with center $(h,k),$ is

\frac{{(x-h)}^{2}}{{a}^{2}}+\frac{{(y-k)}^{2}}{{b}^{2}}=1

When $a>b,$ the major axis is horizontal so the distance from the center to the vertex is a.

When $b>a,$ the major axis is vertical so the distance from the center to the vertex is b.

8. Example 11.23

Example 11.23

Graph: $\frac{{(x-3)}^{2}}{9}+\frac{{(y-1)}^{2}}{4}=1.$

Solution

If we look at the equations of $\frac{{x}^{2}}{9}+\frac{{y}^{2}}{4}=1$ and $\frac{{(x-3)}^{2}}{9}+\frac{{(y-1)}^{2}}{4}=1,$ we see that they are both ellipses with $a=3$ and $b=2.$ So they will have the same size and shape. They are different in that they do not have the same center.

Notice in the graph above that we could have graphed $\frac{{(x-3)}^{2}}{9}+\frac{{(y-1)}^{2}}{4}=1$ by translations. We moved the original ellipse to the right 3 units and then up 1 unit.

In the next example we will use the translation method to graph the ellipse.

9. Example 11.24

Example 11.24

Graph $\frac{{(x+4)}^{2}}{16}+\frac{{(y-6)}^{2}}{9}=1$ by translation.

Solution

This ellipse will have the same size and shape as $\frac{{x}^{2}}{16}+\frac{{y}^{2}}{9}=1$ whose center is $(0,0).$ We graph this ellipse first.

When an equation has both an ${x}^{2}$ and a ${y}^{2}$ with different coefficients, we verify that it is an ellipsis by putting it in standard form. We will then be able to graph the equation.

10. Example 11.25

Example 11.25

Write the equation ${x}^{2}+4{y}^{2}-4x+24y+24=0$ in standard form and graph.

Solution

We put the equation in standard form by completing the squares in both x and y.

11. Solve Application with Ellipses

Solve Application with Ellipses

The orbits of the planets around the sun follow elliptical paths.

12. Example 11.26

Example 11.26

Pluto (a dwarf planet) moves in an elliptical orbit around the Sun. The closest Pluto gets to the Sun is approximately 30 astronomical units (AU) and the furthest is approximately 50 AU. The Sun is one of the foci of the elliptical orbit. Letting the ellipse center at the origin and labeling the axes in AU, the orbit will look like the figure below. Use the graph to write an equation for the elliptical orbit of Pluto.

Solution

We recognize this as an ellipse that is centered at the origin. · $\,\frac{{x}^{2}}{{a}^{2}}+\frac{{y}^{2}}{{b}^{2}}=1$ Since the major axis is horizontal and the distance from the center to the vertex is 40, we know $a=40$ and so ${a}^{2}=1600$ . · $\,\frac{{x}^{2}}{1600}+\frac{{y}^{2}}{{b}^{2}}=1$ The minor axis is vertical but the end points aren’t given. To find $b$ we will use the location of the Sun. Since the Sun is a focus of the ellipse at the point $(10,0)$ , we know $c=10$ . Use this to solve for ${b}^{2}$ . · $\,\begin{array}{l} {b}^{2}={a}^{2}-{c}^{2} \\ {b}^{2}={40}^{2}-{10}^{2} \\ {b}^{2}=1600-100 \\ {b}^{2}=1500 \\ \end{array}$ Substitute ${a}^{2}$ and ${b}^{2}$ into the standard form of the ellipse. · $\frac{{x}^{2}}{1600}+\frac{{y}^{2}}{1500}=1$

13. Section 11.3 Exercises

Section 11.3 Exercises

Graph an Ellipse with Center at the Origin

In the following exercises, graph each ellipse.

Find the Equation of an Ellipse with Center at the Origin

In the following exercises, find the equation of the ellipse shown in the graph.

Graph an Ellipse with Center Not at the Origin

In the following exercises, graph each ellipse.

In the following exercises, graph each equation by translation.

In the following exercises, ⓐ write the equation in standard form and ⓑ graph.

In the following exercises, graph the equation.

Solve Application with Ellipses

Writing Exercises

ⓐ After completing the exercises, use this checklist to evaluate your mastery of the objectives of this section.

ⓑ What does this checklist tell you about your mastery of this section? What steps will you take to improve?

14. Practice 1

Graph: $\frac{{x}^{2}}{4}+\frac{{y}^{2}}{16}=1.$

Graph: $\frac{{x}^{2}}{9}+\frac{{y}^{2}}{16}=1.$

Graph $9{x}^{2}+16{y}^{2}=144.$

15. Practice 2

Graph $16{x}^{2}+25{y}^{2}=400.$

Find the equation of the ellipse shown.

Find the equation of the ellipse shown.

16. Practice 3

Graph: $\frac{{(x+3)}^{2}}{4}+\frac{{(y-5)}^{2}}{16}=1.$

Graph: $\frac{{(x-1)}^{2}}{25}+\frac{{(y+3)}^{2}}{16}=1.$

Graph $\frac{{(x-5)}^{2}}{9}+\frac{{(y+4)}^{2}}{4}=1$ by translation.

17. Practice 4

Graph $\frac{{(x+6)}^{2}}{16}+\frac{{(y+2)}^{2}}{25}=1$ by translation.

ⓐ Write the equation $6{x}^{2}+4{y}^{2}+12x-32y+34=0$ in standard form and ⓑ graph.

ⓐ Write the equation $4{x}^{2}+{y}^{2}-16x-6y+9=0$ in standard form and ⓑ graph.

18. Practice 5

A planet moves in an elliptical orbit around its sun. The closest the planet gets to the sun is approximately 20 AU and the furthest is approximately 30 AU. The sun is one of the foci of the elliptical orbit. Letting the ellipse center at the origin and labeling the axes in AU, the orbit will look like the figure below. Use the graph to write an equation for the elliptical orbit of the planet.

A planet moves in an elliptical orbit around its sun. The closest the planet gets to the sun is approximately 20 AU and the furthest is approximately 50 AU. The sun is one of the foci of the elliptical orbit. Letting the ellipse center at the origin and labeling the axes in AU, the orbit will look like the figure below. Use the graph to write an equation for the elliptical orbit of the planet.

$\frac{{x}^{2}}{4}+\frac{{y}^{2}}{25}=1$

19. Practice 6

$\frac{{x}^{2}}{25}+\frac{{y}^{2}}{36}=1$

$\frac{{x}^{2}}{36}+\frac{{y}^{2}}{16}=1$

${x}^{2}+\frac{{y}^{2}}{4}=1$

20. Practice 7

$4{x}^{2}+25{y}^{2}=100$

$16{x}^{2}+36{y}^{2}=576$

$\frac{{(x+1)}^{2}}{4}+\frac{{(y+6)}^{2}}{25}=1$

21. Practice 8

$\frac{{(x+4)}^{2}}{4}+\frac{{(y-2)}^{2}}{9}=1$

$\frac{{(x-3)}^{2}}{4}+\frac{{(y-7)}^{2}}{25}=1$

$\frac{{(x-5)}^{2}}{9}+\frac{{(y+4)}^{2}}{25}=1$

22. Practice 9

$25{x}^{2}+9{y}^{2}-100x-54y-44=0$

$4{x}^{2}+25{y}^{2}-24x-64=0$

$x=-2{(y-1)}^{2}+2$

23. Practice 10

${(x+5)}^{2}+{(y+2)}^{2}=4$

$\frac{{(x+3)}^{2}}{16}+\frac{{(y+1)}^{2}}{4}=1$

$\frac{{x}^{2}}{25}+\frac{{y}^{2}}{36}=1$

24. Practice 11

${x}^{2}+{y}^{2}=64$

$y=6{x}^{2}+2x-1$

A planet moves in an elliptical orbit around its sun. The closest the planet gets to the sun is approximately 10 AU and the furthest is approximately 30 AU. The sun is one of the foci of the elliptical orbit. Letting the ellipse center at the origin and labeling the axes in AU, the orbit will look like the figure below. Use the graph to write an equation for the elliptical orbit of the planet.

25. Practice 12

A comet moves in an elliptical orbit around a sun. The closest the comet gets to the sun is approximately 15 AU and the furthest is approximately 85 AU. The sun is one of the foci of the elliptical orbit. Letting the ellipse center at the origin and labeling the axes in AU, the orbit will look like the figure below. Use the graph to write an equation for the elliptical orbit of the comet.

In your own words, define an ellipse and write the equation of an ellipse centered at the origin in standard form. Draw a sketch of the ellipse labeling the center, vertices and major and minor axes.

Compare and contrast the graphs of the equations $\frac{{x}^{2}}{4}+\frac{{y}^{2}}{9}=1$ and $\frac{{x}^{2}}{9}+\frac{{y}^{2}}{4}=1.$