Mada za sehemu hiiCoordinate Geomrtry 2Mada 6
The ellipse is a conic section defined as the locus of a point that moves such that the ratio of its distance from a fixed point (focus) to its distance from a fixed line (directrix) is constant. It can also be defined as the locus of points such that the sum of the distances from any point to the two foci is constant. This constant is equal to , where is the semi-major axis. The eccentricity of an ellipse is less than 1.
The standard equation of an ellipse
Figure below represents an ellipse with foci and , moving point , and directrix .
From the definition, . Also, .
Derivation from :
Substituting into :
Rearranging:
Squaring both sides:
Squaring both sides again:
Let :
Dividing by :
From the right-angled triangle formed by , , and , using Pythagoras' theorem:
From the definition using directrix and focus: , where and so . Similarly, and so .
Solving these gives and .
The foci are and the directrices are .
If , then or with foci , directrices , and vertices . The lengths of the major and minor axes are and , respectively.
If , then or with foci , directrices , and vertices . The lengths of the major and minor axes are and , respectively.
Example 1
Given the equation , find:
- Lengths of the major and minor axes.
- Coordinates of the foci.
- Equations of the directrices.
- Coordinates of the vertices.
Solution:
Standard form: . Here, and . Since , the major axis is along the x-axis.
- Major axis: ; Minor axis:
- , so . Foci:
- . Directrices:
- Vertices:
Example 2
An ellipse is defined by . Find:
- The coordinates of the foci.
- The lengths of the major and minor axes.
- The equations of the directrices.
- The coordinates of the vertices.
Solution:
Standard form: . Here, and . Since , the major axis is along the y-axis.
- , so . Foci:
- Major axis: ; Minor axis:
- . Directrices:
- Vertices:
Example 3
Astronomers have revealed that planets revolve around the sun in an elliptical orbit and that the sun is always at one of the foci of the elliptical orbit. Pluto is said to be the farthest from the sun with an eccentricity of 0.248. Astronomers have also revealed that Pluto's orbit is at a distance about 30 Astronomical Unit (AU) from the sun at its closest point to the sun (perihelion). The length of its major axis is about 79 AU.
- Sketch the Pluto's orbit showing the position of the sun. (See Diagram: Sketch of Pluto's orbit)
- Find the length of the semi-minor axis of the orbit.
- Find the distance of Pluto from the sun at its farthest point (aphelion).
Solution:
a. (See Diagram: Sketch of Pluto's orbit)
b. The length of the major axis is AU, so AU.
The distance at perihelion is AU. Since , we have .
Now, we use :
The length of the semi-minor axis is approximately 38.3 AU.
c. The distance at aphelion is AU
Like the graph of a parabola, the graph of an ellipse can be translated. If an ellipse centered at is translated units horizontally and units vertically, then the center of the ellipse will be . This translation changes the standard equation by replacing with and with .
Thus, the standard form of the equation of an ellipse with center is:
The standard equation of the translated ellipse , for has the following features:
- The vertices are and co-vertices are .
- The foci are .
- The directrices are .
- The lengths of major and minor axes are and , respectively.
- The eccentricity, .
Example 1
Given the ellipse . Find each of the following:
- Center
- Foci
- Eccentricity
- Directrices
- Vertices
- Length of major axis
Solution:
(a) Comparing with the standard equation , we have , , , and . Therefore, the center is at .
(b) Since , , so . The foci are .
(c)
(d) The directrices are
(e) The vertices are , which are and .
(f) Length of major axis .
Example 2
Given the ellipse . Find each of the following:
(a) Center (b) Foci (c) Vertices (d) Directrices
In order to sketch the graph, identify the x and y-intercepts as follows:
When x = 0, . This is a quadratic equation in y. Using the quadratic formula:
So, the y-intercepts are approximately and .
When y = 0, . This is a quadratic equation in x. Using the quadratic formula:
So, the x-intercepts are approximately and .
Solution (Calculations):
(a) Rearrange and complete the square:
Divide by 225:
Comparing with the translated equation, , , , . Thus, the center is .
(b) Since , , so . The foci are , which are and .
(c) The vertices are , which are and .
(d) . The directrices are , which are and .
Similar to the parabola, we can determine the equations of the tangent and normal to an ellipse at any given point. The gradient of a tangent at the point of tangency is the same as the gradient of the ellipse at that point.
One way to find the equation of the tangent and normal is by differentiating the equation of the ellipse to determine its gradient at the point of tangency.
The equation of the tangent to the ellipse at the point is:
The equation of the normal to the ellipse at the point is:
Example 1
Find the equations of the tangent and normal to the ellipse at the point .
Solution:
Standard form: . Here and . The point of tangency is .
Tangent:
Normal:
Example 2
Find the equations of the tangent and normal to the ellipse at the point .
Solution:
Rewrite the equation: or
Differentiating implicitly with respect to x:
At : which is incorrect. This means the tangent is vertical. The point is on the ellipse so the tangent is x=5 and the normal is y=1.
Using the translated formula:
Example 3
Prove that the condition for the line to be a tangent to the ellipse is .
Solution:
Substitute into :
For tangency, the discriminant must be zero:
Divide by :
The line segment is the latus rectum of the ellipse.
Since the coordinate point of the focus is , the two coordinate points and satisfy the equation .
Substituting into the equation of the ellipse gives:
Solving for :
Thus, the coordinates of and are and , respectively.
Length of latus rectum = length of :
But, which means .
Substitute this result into the equation of the length of the latus rectum:
Therefore, the length of the latus rectum is units for . A similar approach can be used to show that the length of the latus rectum is units for .
Example 1
The lengths of the latus rectum and major axis of the ellipse are units and 20 units, respectively. If the major axis is along the y-axis, find the equation of the ellipse.
Solution:
Since the major axis is along the y-axis, the length of the latus rectum is . We are given that this length is , so:
The length of the major axis is , so . (Equation ii)
Substitute Equation ii into Equation i:
Substitute these values ( and ) into the standard equation :
Example 2
Find the length of the latus rectum of an ellipse whose equation is .
Solution:
Given the equation .
Here, and , so and . Since , the length of the latus rectum is :
The equation of an ellipse can also be written in parametric form. Consider the standard equation of the ellipse:
This equation resembles the trigonometric identity .
From Figure 1.9, it can be observed that and are associated with cosine and sine, respectively.
To express the equation of an ellipse in parametric form, compare the terms of the two equations as follows:
This implies that:
Thus, equations (1.13) and (1.14) are parametric equations of a standard ellipse with the center at the origin and foci on the x-axis. When the major axis is on the y-axis, or the center of the ellipse is at , the parametric equations change slightly.
Example 1
Express the ellipse in parametric form.
Solution:
Given the ellipse . This implies that and . The standard parametric equations of the ellipse are:
Substituting the values of and gives:
Example 2
The equation of the ellipse is given in parametric form as and . Find its:
(a) Corresponding Cartesian equation.
(b) Length of the latus rectum.
Solution:
(a) Given and .
Rearrange the equations:
Squaring and adding:
Since , the Cartesian equation is:
(b) From the Cartesian equation, and , so and . Since b>a, the length of the latus rectum is .
Example 3
The equation of the ellipse is given in Cartesian form as . Find the corresponding parametric equations of the ellipse.
Solution:
Given .
Rearranging and completing the square:
Divide by 36:
The center is , so , and so .
The parametric equations of the translated ellipse are:
Substituting the values , , , and gives:
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