Fiveable

๐Ÿ“Honors Pre-Calculus Unit 10 Review

QR code for Honors Pre-Calculus practice questions

10.1 The Ellipse

10.1 The Ellipse

Written by the Fiveable Content Team โ€ข Last updated August 2025
Written by the Fiveable Content Team โ€ข Last updated August 2025
๐Ÿ“Honors Pre-Calculus
Unit & Topic Study Guides
Pep mascot

Ellipse Equation and Graphing

An ellipse is a set of all points where the sum of the distances to two fixed points (called foci) is constant. Understanding the equation of an ellipse lets you identify its shape, orientation, size, and position on a coordinate plane.

Pep mascot
more resources to help you study

Standard Form of Ellipse Equations

For an ellipse centered at the origin, the standard form is:

x2a2+y2b2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1

  • aa is the semi-axis length in the horizontal direction (distance from center to the ellipse along the x-axis)
  • bb is the semi-axis length in the vertical direction (distance from center to the ellipse along the y-axis)

Whichever denominator is larger tells you the direction of the major axis (the longer one). If a>ba > b, the ellipse is wider than it is tall (horizontal major axis). If b>ab > a, it's taller than it is wide (vertical major axis). When a=ba = b, you just have a circle.

For an ellipse centered at (h,k)(h, k), the equation shifts accordingly:

(xโˆ’h)2a2+(yโˆ’k)2b2=1\frac{(x-h)^2}{a^2} + \frac{(y-k)^2}{b^2} = 1

The (h,k)(h, k) values translate the entire ellipse so its center sits at that point instead of the origin. Notice that the signs inside the parentheses are subtracting hh and kk, so if you see (xโˆ’3)225+(y+2)29=1\frac{(x-3)^2}{25} + \frac{(y+2)^2}{9} = 1, the center is at (3,โˆ’2)(3, -2), not (3,2)(3, 2).

Standard form of ellipse equations, Writing Equations of Ellipses in Standard Form | College Algebra

Graphing Ellipses with Various Centers

Ellipse centered at the origin (0,0)(0, 0):

  1. Identify a2a^2 and b2b^2 from the denominators, then take their square roots to get aa and bb.
  2. Plot the center at (0,0)(0, 0).
  3. From the center, move aa units left and right to plot (a,0)(a, 0) and (โˆ’a,0)(-a, 0).
  4. From the center, move bb units up and down to plot (0,b)(0, b) and (0,โˆ’b)(0, -b).
  5. Sketch a smooth oval through all four points.

Ellipse centered at (h,k)(h, k):

  1. Identify aa, bb, hh, and kk from the equation.
  2. Plot the center at (h,k)(h, k).
  3. From the center, move aa units left and right to plot (h+a,k)(h+a, k) and (hโˆ’a,k)(h-a, k).
  4. From the center, move bb units up and down to plot (h,k+b)(h, k+b) and (h,kโˆ’b)(h, k-b).
  5. Sketch a smooth oval through all four points.

The four points you plot in steps 3โ€“4 are the vertices (endpoints of the major axis) and co-vertices (endpoints of the minor axis). Which pair is which depends on whether aa or bb is larger.

Standard form of ellipse equations, The Ellipse ยท Precalculus

Ellipse Features vs. Equation Components

The values of aa and bb control more than just size:

  • Major axis length = 2ร—2 \times (the larger of aa or bb)
  • Minor axis length = 2ร—2 \times (the smaller of aa or bb)
  • Orientation: If a>ba > b, the major axis is horizontal. If b>ab > a, the major axis is vertical.

Finding the foci: The foci always lie on the major axis, each a distance cc from the center, where:

c2=(largerย denominator)โˆ’(smallerย denominator)c^2 = (\text{larger denominator}) - (\text{smaller denominator})

More specifically:

  • Horizontal major axis (a>ba > b): c2=a2โˆ’b2c^2 = a^2 - b^2, foci at (hยฑc,โ€…โ€Šk)(h \pm c,\; k)
  • Vertical major axis (b>ab > a): c2=b2โˆ’a2c^2 = b^2 - a^2, foci at (h,โ€…โ€Škยฑc)(h,\; k \pm c)

Eccentricity measures how "stretched" the ellipse is: e=c(semi-majorย axisย length)e = \frac{c}{(\text{semi-major axis length})}. An eccentricity near 0 means the ellipse is nearly circular; closer to 1 means it's very elongated.

Area of an ellipse: A=ฯ€abA = \pi ab

Real-World Applications of Ellipses

  • Planetary orbits follow elliptical paths with the Sun at one focus (Kepler's First Law). Earth's orbit, for example, has an eccentricity of about 0.017, so it's very close to circular.
  • Whispering galleries are elliptical rooms (like the one in St. Paul's Cathedral) where a whisper at one focus reflects off the walls and converges at the other focus, making it clearly audible across the room.
  • Architecture and engineering use elliptical arches and gears. The Colosseum in Rome has an elliptical footprint.

Solving applied problems typically requires you to:

  1. Extract known information (foci locations, axis lengths, specific points on the ellipse).
  2. Use that information to find aa, bb, and the center.
  3. Write the standard form equation, then answer whatever the problem asks (coordinates of foci, area, etc.).

Additional Ellipse Properties

  • An ellipse is a conic section, formed when a plane slices through a cone at an angle that isn't steep enough to produce a parabola or hyperbola.
  • The defining property ties back to the foci: for any point PP on the ellipse, the sum of distances PF1+PF2=2aPF_1 + PF_2 = 2a (where aa is the semi-major axis length). This constant-sum property is what gives the ellipse its shape.
  • Each ellipse has two directrices, lines perpendicular to the major axis. The ratio of a point's distance to a focus versus its distance to the corresponding directrix equals the eccentricity ee.
  • The latus rectum is a chord through a focus, perpendicular to the major axis. Its length is 2b2a\frac{2b^2}{a} (when aa is the semi-major axis). This value is useful for understanding how "wide" the ellipse is near each focus.
  • The auxiliary circle has the same center as the ellipse and a radius equal to the semi-major axis. It's a helpful construction for parametric representations of the ellipse.