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Ellipses Worksheets

HSG-GPE.A.3
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Aligned To Common Core Standard:

Expressing Properties - HSG-GPE.A.3

How to find the Equation of an Ellipse - Before deriving an equation of an ellipse, here are a few important points that need to remembered: A set of all points (x, y)(x ,y) in a plane such that the sum of distances from two fixed points is a constant, is known as Ellipse. Each fixed point is known as the "focus". Each ellipse has two axes of symmetry. The axis that is longer is known as the major axis, while the shorter axis is known as the minor axis. The endpoint of each major axis is known as the vertex, while the endpoints of the minor axis are considered the co-vertex. The midpoint of the major and minor axis is known as the center. Remember that the axes are perpendicular at the center of the figure. The foci are always situated on the major axis. The distance between the foci is less than the sum of the distances from the foci to any point on the ellipse. For deriving the equation, the first step is the identification of the key information from the graph and place them in the pattern. For a horizontal ellipse, the pattern is : [(x - h)2 / a2] + [(y - k)2 / b2] = 1 For a vertical ellipse, the pattern is: [(x - h)2 / b2] + [(y - k)2 / a2] = 1 Here, (h, k) is the center point, a is the distance from the center point to the end of the major axis while b is the distance from the center point to the end of the major axis. These worksheets and lessons are really helpful for understanding the structure of an ellipse and how to map it.

Printable Worksheets And Lessons




Homework Sheets

What is the equation of an figure after being given its vertices and foci?

  • Homework 1 - To write the equation in standard form, the center, a2 and b2 must be found. The x-coordinate of the vertices and foci given are 0, so the center has to be (0,0).
  • Homework 2 - |a| = length of semi-major axis, |b|= length of semi-minor axis
  • Homework 3 - To find b2, use the foci equation. c is the distance from the center to the foci.



Practice Worksheets

We want all of these figures to be in standard form.

  • Practice 1 - Find the equations of an ellipse (in standard form) that has foci at (0,-9) and (0,9) and vertices at (0,-15) and (0,15).
  • Practice 2 - Now that we have the values for b and c, we can substitute the values into the equation and simplify to find b.
  • Practice 3 - Substitute 0 for h and k, the square root of 0 for b and 11 for a into the standard form equation.



Math Skill Quizzes

The questions get a lot more mixed here.

  • Quiz 1 - Write the standard equation of each figure. For example: 16x2 + 9y2 = 144
  • Quiz 2 - Find the foci, vertices, and covertices of each ellipse: x2 /400 + y2/4 = 1
  • Quiz 3 - There are basically three forms of problems here.


The Importance of Ellipses in Astronomy

This geometric shape is one of the classical conic sections that can be formed by cutting a cone with a plane. It is one of the four common conic sections, the others being the circle, the hyperbola, and the parabola. The common version of the equation of this figure, as we studied in the above worksheets and lessons, is driven using Cartesian coordinates. The origin of this shape is located somewhere on the x-axis between the foci. The general nature of this figure is often described by its eccentricity which basically defines how un-circular something is. To help you relative understand this, a circle has zero eccentricity. A hyperbola has an eccentricity value greater than one. Ellipses generally fall somewhere between these two values. In astronomy these shapes are often used to describe and model the motions of celestial objects and their orbits that are dictated by gravity that is exerted by larger bodies. In our solar system (The Milky Way), the sun serves as the core focus for all orbits. In fact, Johannes Kepler's laws of planetary motion are based on the mathematical fundamentals of this shape. These laws of motion can be used to not only predict the orbital path of planets, but also asteroids and comets.