x = a cos(t) → x/a = cos(t) → (x/a)2 = cos2t
y = b sin(t) → y/b = sin(t) → (y/b)2 = sin2t
(x/a)2 + (y/b)2 = cos2t + sin2t
(x/a)2 + (y/b)2 = 1
The property that allowed us to convert the parametric equation to (x/a)2 + (y/b)2 = 1 is a Pythagorean Property: cos2t + sin2t = 1. Sometimes, it is better to see the x-y form of a function, so you can recognize it's graph easily. For example, this function is easily recognizable as an ellipse.
x = 4 cos(t) → x/4 = cos(t) → (x/4)2 = cos2t
y = 7 sin(t) → y/7 = sin(t) → (y/7)2 = sin2t
(x/4)2 + (y/7)2 = cos2t + sin2t
(x/4)2 + (y/7)2 = 1
Ellipse
x = h + a cos t
y = k + a sin t
Here are more conic sections and some of their graphs that will be very helpful to memorize for a Final Exam:
*You will find that isolating the trigonometry operations is very helpful when converting from parametric to x-y form
In the general formula x and y refer to the coordinates of the starting position of the object, v is the intial velocity or magnitude of the object, θ is the angle which the object is moving
x = (vcosθ)t + x
y = (vcosθ)t + y
x = (21cos0°)t - 43
y = (13sin90°)t + 19
x = -43 +21t
y = 19 +13t
Pretty simple! Most of where the difficulty comes into play is analyzing all aspects of the situation, so remember to read directions carefully!
x = 6t + 6cos(1.5π - t)
y = 6 + 6sin(1.5π - t)
x = a(t - sin(t))
y = a(1 - cos(t))
Parametric and polar equations are two different ways to represent functions which are not written in the standard x-y form.
Polar coordinates are a new way of plotting points or equations on a plane. Polar coordinates can be used in physics, specifically spherical physics dealing with mechanics. They can also be used when looking at a radar, or plan-position indicator. While standard algebraic equations are written in x-y form, polar equations are in terms of r (radius) and θ.
Rather than a standard coordinate plane, the polar plane is usually thought of as a circular plane. Like a standard unit circle, angles begin at the positive x-axis and rotate counter-clockwise.
Domain and range are written in terms of angle measurements. For example, in the picture above the domain is 0≤θ≤2π, because the angle begins at 0° and rotates 360° or 2π radians.
Points on the polar plane are written in (r,θ) form. In the example to the left, the point is colinear to a circle with a radius of 2, so the r value is '2.' The point is rotated π/4 radians about the pole (origin of the polar plane, making the θ value 'π/4.' Keep in mind that the point (2, π/4) is the same as (-2, 5π/4), because points can be written in multiple ways on the polar plane.
To the left is a table showing points in the equation r = sin.
So, when we graph these points, we see that it creates a circle with a radius of 1 just above the x-axis.
When we graph the same equation on Desmos, we get the same result. Since cosθ=sinθπ/2, we can conclude that the graph for r = cos(θ) would be identical to the prior, but rotated -π/2 radians.
Spirals in the polar plane can be derived from the equation r = θ.
The greater the coefficient of θ is, the greater the distance of each point will be from the pole.
Equation Above: r = 5θ
Equation Above: r = θ/2
Equations for petaled roses are in the form r=asin(nθ) or r=acos(nθ). The a value is the amplitude of the petals, or the distance from the center. If n is odd, the number of petals is n. If n is even, the number of petals is 2n.
There is a slight rotation between when the trig value is sin and when it is cos. The rotation directly varies with the n value. Using Desmos, you can see how as n increases, the rotation between roses decreases.
Cardioids look like circles, but curve inwards at a certain point, creating a "cusp." The equation for cardioids is r=a±asin(θ) or r=a±acos(θ)
When the equation involves sine, the cusp faces towards the y-axis, and when it includes cosine, the cusp faces towards the x-axis.
Limaçons are similar to cardioids, but have a loop in the center rather than a cusp. They are written in the form r=a±b⋅sin(θ) or r=a±bcos(θ). When a>b, the curve is a convex limaçon. When a<b, the curve is a standard limaçon. When a=b, the curve is a cardioid.
Example of a Convex Limaçon.
Example of a Standard Limaçon.
Note: The length of the cusp (from the intersection) is the value of |b|-|a|.
If you go back to the Polar Art project, you will remember that finding intersection points of polar curves is a bit more difficult than it seems. When given two equations, you can solve algebraically for points of intersection. Although, it is important to remember that not every point that looks like a point of intersection when the equations are graphed actually are solutions. This connects back to the different types of polar curves, as you will need to be able to identify which polar curves are involved in the given equations.
When converting between polar equations and x-y equations, there are 4 main conversions we can use:
Mastering this concept can help you fully understand polar coordinates.
From 11-3 Intersections of Polar Curves
r = 2 + 2sinθ r = 2 - 2cosθ
2 + 2sinθ = 2 - 2cosθ
sinθ = -cosθ
Values for θ in which this is true: 3π/4, 7π/4
Plug both values back in:
r = 2 + 2sin(3π/4) r = 2 + 2sin(7π/4)
r = 2 + 2(√2/2) r = 2 - 2(√2/2)
r = 2+√2 r = 2-√2
(2+√2, 3π/4) and (2-√2, 7π/4)
To the left are the two types of ways that the equations of conics can be written. The variables k, a, and b, all determine that amplitudes of conics, and also effect the type of conic under the rule of eccentricity.
As you may recall from earlier in the year, or even from Algebra II, the complex numbers plane is similar to the standard coordinate plane. Complex numbers are in the form of z=a+bi. For example, the point plotted above is written in the equation z=3-2i. It will be plotted at (3,-2).
When converting complex numbers into polar form, you must find the modulas and the angle of rotation. The modulas can be found using the equation r=√ (a2+b2). The angle of rotation can be found using the equation tan(θ)=b/a.
We can take coordinates of complex numbers and put them in terms of sin and cos.
When we write complex numbers in terms of sin and cos, we shorten r(cosθ+isinθ) to rcisθ. In this form, we can find the roots of complex numbers.
From 11-4 Complex Numbers
Hint: to find the amount of roots in a complex number, you must write the numbers in the form Zn = (rn)cis(nθ).
Using simple arithmetic, we find the three roots.
∛(27cis120)
9cis(1/3)(120+360k) → (k starts at 0 and increases by 1 per root)
Solutions: 3cis40, 3cis160, 3cis280
Practice all the sample problems and go over the important concepts!