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11.10 Parametric Equations

As we have seen in Exercises - in Section, Chapter and most recently in Section, there are scores of interesting curves which, when plotted in the x y -plane, neither represent y as a function of x nor x as a function of y . In this section, we present a new concept which allows us to use functions to study these kinds of curves. To motivate the idea, we imagine a bug crawling across a table top starting at the point O and tracing out a curve C in the plane, as shown below.

Coordinate-plane figure.
Figure 11.292

The curve C does not represent y as a function of x because it fails the Vertical Line Test and it does not represent x as a function of y because it fails the Horizontal Line Test. However, since the bug can be in only one place P ( x , y ) at any given time t , we can define the x -coordinate of P as a function of t and the y -coordinate of P as a (usually, but not necessarily) different function of t . (Traditionally, f ( t ) is used for x and g ( t ) is used for y .) The independent variable t in this case is called a parameter and the system of equations

{ x = f ( t ) y = g ( t )

is called a system of parametric equations or a parametrization of the curve C .1 The parametrization of C endows it with an orientation and the arrows on C indicate motion in the direction of increasing values of t . In this case, our bug starts at the point O , travels upwards to the left, then loops back around to cross its path2 at the point Q and finally heads off into the first quadrant. It is important to note that the curve itself is a set of points and as such is devoid of any orientation. The parametrization determines the orientation and as we shall see, different parametrizations can determine different orientations. If all of this seems hauntingly familiar, it should. By definition, the system of equations { x = cos ( t ) , y = sin ( t ) parametrizes the Unit Circle, giving it a counter-clockwise orientation. More generally, the equations of circular motion { x = r cos ( ω t ) , y = r sin ( ω t ) developed on page in Section are parametric equations which trace out a circle of radius r centered at the origin. If ω > 0 , the orientation is counter-clockwise; if ω < 0 , the orientation is clockwise. The angular frequency ω determines `how fast' the object moves around the circle. In particular, the equations { x = 2960 cos ( π 12 t ) , y = 2960 sin ( π 12 t ) that model the motion of Lakeland Community College as the earth rotates (see Example in Section ) parameterize a circle of radius 2960 with a counter-clockwise rotation which completes one revolution as t runs through the interval [ 0 , 24 ) . It is time for another example.

The curve sketched out in Example Example 1 certainly looks like a parabola, and the presence of the t 2 term in the equation x = t 2 3 reinforces this hunch. Since the parametric equations { x = t 2 3 , y = 2 t 1 given to describe this curve are a system of equations, we can use the technique of substitution as described in Section to eliminate the parameter t and get an equation involving just x and y . To do so, we choose to solve the equation y = 2 t 1 for t to get t = y + 1 2 . Substituting this into the equation x = t 2 3 yields x = ( y + 1 2 ) 2 3 or, after some rearrangement, ( y + 1 ) 2 = 4 ( x + 3 ) . Thinking back to Section, we see that the graph of this equation is a parabola with vertex ( 3 , 1 ) which opens to the right, as required. Technically speaking, the equation ( y + 1 ) 2 = 4 ( x + 3 ) describes the entire parabola, while the parametric equations { x = t 2 3 , y = 2 t 1 for t 2 describe only a portion of the parabola. In this case,3 we can remedy this situation by restricting the bounds on y . Since the portion of the parabola we want is exactly the part where y 5 , the equation ( y + 1 ) 2 = 4 ( x + 3 ) coupled with the restriction y 5 describes the same curve as the given parametric equations. The one piece of information we can never recover after eliminating the parameter is the orientation of the curve.

Eliminating the parameter and obtaining an equation in terms of x and y , whenever possible, can be a great help in graphing curves determined by parametric equations. If the system of parametric equations contains algebraic functions, as was the case in Example Example 1, then the usual techniques of substitution and elimination as learned in Section can be applied to the system { x = f ( t ) , y = g ( t ) to eliminate the parameter. If, on the other hand, the parametrization involves the trigonometric functions, the strategy changes slightly. In this case, it is often best to solve for the trigonometric functions and relate them using an identity. We demonstrate these techniques in the following example.

Now that we have had some good practice sketching the graphs of parametric equations, we turn to the problem of finding parametric representations of curves. We start with the following.

Parametrizations of Common Curves

The reader is encouraged to verify the above formulas by eliminating the parameter and, when indicated, checking the orientation. We put these formulas to good use in the following example.

We note that the formulas given on page offer only one of literally infinitely many ways to parametrize the common curves listed there. At times, the formulas offered there need to be altered to suit the situation. Two easy ways to alter parametrizations are given below.

Adjusting Parametric Equations

We demonstrate these techniques in the following example.

We put our answer to Example Example 4 number to good use to derive the equation of a cycloid . Suppose a circle of radius r rolls along the positive x -axis at a constant velocity v as pictured below. Let θ be the angle in radians which measures the amount of clockwise rotation experienced by the radius highlighted in the figure.

Coordinate-plane figure.
Figure 11.306

Our goal is to find parametric equations for the coordinates of the point P ( x , y ) in terms of θ . From our work in Example Example 4 number, we know that clockwise motion along the Unit Circle starting at the point ( 0 , 1 ) can be modeled by the equations { x = sin ( θ ) , y = cos ( θ ) for 0 θ < 2 π . (We have renamed the parameter ` θ ' to match the context of this problem.) To model this motion on a circle of radius r , all we need to do11 is multiply both x and y by the factor r which yields { x = r sin ( θ ) , y = r cos ( θ ) . We now need to adjust for the fact that the circle isn't stationary with center ( 0 , 0 ) , but rather, is rolling along the positive x -axis. Since the velocity v is constant, we know that at time t , the center of the circle has traveled a distance v t down the positive x -axis. Furthermore, since the radius of the circle is r and the circle isn't moving vertically, we know that the center of the circle is always r units above the x -axis. Putting these two facts together, we have that at time t , the center of the circle is at the point ( v t , r ) . From Section, we know v = r θ t , or v t = r θ . Hence, the center of the circle, in terms of the parameter θ , is ( r θ , r ) . As a result, we need to modify the equations { x = r sin ( θ ) , y = r cos ( θ ) by shifting the x -coordinate to the right r θ units (by adding r θ to the expression for x ) and the y -coordinate up r units12 (by adding r to the expression for y ). We get { x = r sin ( θ ) + r θ , y = r cos ( θ ) + r , which can be written as { x = r ( θ sin ( θ ) ) , y = r ( 1 cos ( θ ) ) . Since the motion starts at θ = 0 and proceeds indefinitely, we set θ 0 .

We end the section with a demonstration of the graphing calculator.

Exercises

In Exercises -, plot the set of parametric equations by hand. Be sure to indicate the orientation imparted on the curve by the parametrization.

  1. { x = 4 t 3 y = 6 t 2 for  0 t 1
  2. { x = 4 t 1 y = 3 4 t for  0 t 1
  3. { x = 2 t y = t 2 for  1 t 2
  4. { x = t 1 y = 3 + 2 t t 2 for  0 t 3
  5. { x = t 2 + 2 t + 1 y = t + 1 for  t 1
  6. { x = 1 9 ( 18 t 2 ) y = 1 3 t for  t 3
  7. { x = t y = t 3 for  < t <
  8. { x = t 3 y = t for  < t <
  9. { x = cos ( t ) y = sin ( t ) for  π 2 t π 2
  10. { x = 3 cos ( t ) y = 3 sin ( t ) for  0 t π
  11. { x = 1 + 3 cos ( t ) y = 4 sin ( t ) for  0 t 2 π
  12. { x = 3 cos ( t ) y = 2 sin ( t ) + 1 for  π 2 t 2 π
  13. { x = 2 cos ( t ) y = sec ( t ) for  0 t < π 2
  14. { x = 2 tan ( t ) y = cot ( t ) for  0 < t < π 2
  15. { x = sec ( t ) y = tan ( t ) for  π 2 < t < π 2
  16. { x = sec ( t ) y = tan ( t ) for  π 2 < t < 3 π 2
  17. { x = tan ( t ) y = 2 sec ( t ) for  π 2 < t < π 2
  18. { x = tan ( t ) y = 2 sec ( t ) for  π 2 < t < 3 π 2
  19. { x = cos ( t ) y = t for  0 t π
  20. { x = sin ( t ) y = t for  π 2 t π 2
  21. { x = t 3 3 t y = t 2 4 for  2 t 2
  22. { x = 4 cos 3 ( t ) y = 4 sin 3 ( t ) for  0 t 2 π
  23. { x = e t + e t y = e t e t for  2 t 2
  24. { x = cos ( 3 t ) y = sin ( 4 t ) for  0 t 2 π
  25. the directed line segment from ( 3 , 5 ) to ( 2 , 2 )
  26. the directed line segment from ( 2 , 1 ) to ( 3 , 4 )
  27. the curve y = 4 x 2 from ( 2 , 0 ) to ( 2 , 0 ) .
  28. the curve y = 4 x 2 from ( 2 , 0 ) to ( 2 , 0 ) (Shift the parameter so t = 0 corresponds to ( 2 , 0 ) .)
  29. the curve x = y 2 9 from ( 5 , 2 ) to ( 0 , 3 ) .
  30. the curve x = y 2 9 from ( 0 , 3 ) to ( 5 , 2 ) . (Shift the parameter so t = 0 corresponds to ( 0 , 3 ) .)
  31. the circle x 2 + y 2 = 25 , oriented counter-clockwise
  32. the circle ( x 1 ) 2 + y 2 = 4 , oriented counter-clockwise
  33. the circle x 2 + y 2 6 y = 0 , oriented counter-clockwise
  34. the circle x 2 + y 2 6 y = 0 , oriented clockwise (Shift the parameter so t begins at 0 .)
  35. the circle ( x 3 ) 2 + ( y + 1 ) 2 = 117 , oriented counter-clockwise
  36. the ellipse ( x 1 ) 2 + 9 y 2 = 9 , oriented counter-clockwise
  37. the ellipse 9 x 2 + 4 y 2 + 24 y = 0 , oriented counter-clockwise
  38. the ellipse 9 x 2 + 4 y 2 + 24 y = 0 , oriented clockwise (Shift the parameter so t = 0 corresponds to ( 0 , 0 ) .)
  39. the triangle with vertices ( 0 , 0 ) , ( 3 , 0 ) , ( 0 , 4 ) , oriented counter-clockwise (Shift the parameter so t = 0 corresponds to ( 0 , 0 ) .)
  40. Use parametric equations and a graphing utility to graph the inverse of f ( x ) = x 3 + 3 x 4 .
  41. Every polar curve r = f ( θ ) can be translated to a system of parametric equations with parameter θ by { x = r cos ( θ ) = f ( θ ) cos ( θ ) , y = r sin ( θ ) = f ( θ ) sin ( θ ) . Convert r = 6 cos ( 2 θ ) to a system of parametric equations. Check your answer by graphing r = 6 cos ( 2 θ ) by hand using the techniques presented in Section and then graphing the parametric equations you found using a graphing utility.
  42. Use your results from Exercises and in Section to find the parametric equations which model a passenger's position as they ride the London Eye .

In Exercises -, plot the set of parametric equations with the help of a graphing utility. Be sure to indicate the orientation imparted on the curve by the parametrization.

In Exercises -, find a parametric description for the given oriented curve.

Suppose an object, called a projectile, is launched into the air. Ignoring everything except the force gravity, the path of the projectile is given by15

{ x = v 0 cos ( θ ) t y = 1 2 g t 2 + v 0 sin ( θ ) t + s 0 for  0 t T

where v 0 is the initial speed of the object, θ is the angle from the horizontal at which the projectile is launched,16 g is the acceleration due to gravity, s 0 is the initial height of the projectile above the ground and T is the time when the object returns to the ground. (See the figure below.)

Coordinate-plane figure.
Figure 11.313
  1. Carl's friend Jason competes in Highland Games Competitions across the country. In one event, the `hammer throw', he throws a 56 pound weight for distance. If the weight is released 6 feet above the ground at an angle of 42 with respect to the horizontal with an initial speed of 33 feet per second, find the parametric equations for the flight of the hammer. (Here, use g = 32 ft. s 2 .) When will the hammer hit the ground? How far away will it hit the ground? Check your answer using a graphing utility.
  2. Eliminate the parameter in the equations for projectile motion to show that the path of the projectile follows the curve

    y = g sec 2 ( θ ) 2 v 0 2 x 2 + tan ( θ ) x + s 0

    Use the vertex formula (Equation ) to show the maximum height of the projectile is

    y = v 0 2 sin 2 ( θ ) 2 g + s 0 when x = v 0 2 sin ( 2 θ ) 2 g

  3. In another event, the `sheaf toss', Jason throws a 20 pound weight for height. If the weight is released 5 feet above the ground at an angle of 85 with respect to the horizontal and the sheaf reaches a maximum height of 31.5 feet, use your results from part to determine how fast the sheaf was launched into the air. (Once again, use g = 32 ft. s 2 .)
  4. Suppose θ = π 2 . (The projectile was launched vertically.) Simplify the general parametric formula given for y ( t ) above using g = 9.8 m s 2 and compare that to the formula for s ( t ) given in Exercise in Section. What is x ( t ) in this case?

In Exercises -, we explore the hyperbolic cosine function, denoted cosh ( t ) , and the hyperbolic sine function, denoted sinh ( t ) , defined below:

cosh ( t ) = e t + e t 2 and sinh ( t ) = e t e t 2

  1. Using a graphing utility as needed, verify that the domain of cosh ( t ) is ( , ) and the range of cosh ( t ) is [ 1 , ) .
  2. Using a graphing utility as needed, verify that the domain and range of sinh ( t ) are both ( , ) .
  3. Show that { x ( t ) = cosh ( t ) , y ( t ) = sinh ( t ) parametrize the right half of the `unit' hyperbola x 2 y 2 = 1 . (Hence the use of the adjective `hyperbolic.')
  4. Compare the definitions of cosh ( t ) and sinh ( t ) to the formulas for cos ( t ) and sin ( t ) given in Exercise in Section.
  5. Four other hyperbolic functions are waiting to be defined: the hyperbolic secant sech ( t ) , the hyperbolic cosecant csch ( t ) , the hyperbolic tangent tanh ( t ) and the hyperbolic cotangent coth ( t ) . Define these functions in terms of cosh ( t ) and sinh ( t ) , then convert them to formulas involving e t and e t . Consult a suitable reference (a Calculus book, or this entry on the hyperbolic functions ) and spend some time reliving the thrills of trigonometry with these `hyperbolic' functions.
  6. If these functions look familiar, they should. Enjoy some nostalgia and revisit Exercise in Section, Exercise in Section and the answer to Exercise in Section.

Answers

  1. { x = 4 t 3 y = 6 t 2 for  0 t 1

    Coordinate-plane figure.
    Figure 11.314
  2. { x = 4 t 1 y = 3 4 t for  0 t 1

    Coordinate-plane figure.
    Figure 11.315
  3. { x = 2 t y = t 2 for  1 t 2

    Coordinate-plane figure.
    Figure 11.316
  4. { x = t 1 y = 3 + 2 t t 2 for  0 t 3

    Coordinate-plane figure.
    Figure 11.317
  5. { x = t 2 + 2 t + 1 y = t + 1 for  t 1

    Coordinate-plane figure.
    Figure 11.318
  6. { x = 1 9 ( 18 t 2 ) y = 1 3 t for  t 3

    Coordinate-plane figure.
    Figure 11.319
  7. { x = t y = t 3 for  < t <

    Coordinate-plane figure.
    Figure 11.320
  8. { x = t 3 y = t for  < t <

    Coordinate-plane figure.
    Figure 11.321
  9. { x = cos ( t ) y = sin ( t ) for  π 2 t π 2

    Coordinate-plane figure.
    Figure 11.322
  10. { x = 3 cos ( t ) y = 3 sin ( t ) for  0 t π

    Coordinate-plane figure.
    Figure 11.323
  11. { x = 1 + 3 cos ( t ) y = 4 sin ( t ) for  0 t 2 π

    Coordinate-plane figure.
    Figure 11.324
  12. { x = 3 cos ( t ) y = 2 sin ( t ) + 1 for  π 2 t 2 π

    Coordinate-plane figure.
    Figure 11.325
  13. { x = 2 cos ( t ) y = sec ( t ) for  0 t < π 2

    Coordinate-plane figure.
    Figure 11.326
  14. { x = 2 tan ( t ) y = cot ( t ) for  0 < t < π 2

    Coordinate-plane figure.
    Figure 11.327
  15. { x = sec ( t ) y = tan ( t ) for  π 2 < t < π 2

    Coordinate-plane figure.
    Figure 11.328
  16. { x = sec ( t ) y = tan ( t ) for  π 2 < t < 3 π 2

    Coordinate-plane figure.
    Figure 11.329
  17. { x = tan ( t ) y = 2 sec ( t ) for  π 2 < t < π 2

    Coordinate-plane figure.
    Figure 11.330
  18. { x = tan ( t ) y = 2 sec ( t ) for  π 2 < t < 3 π 2

    Coordinate-plane figure.
    Figure 11.331
  19. { x = cos ( t ) y = t for  0 < t < π

    Coordinate-plane figure.
    Figure 11.332
  20. { x = sin ( t ) y = t for  π 2 < t < π 2

    Coordinate-plane figure.
    Figure 11.333
  21. { x = t 3 3 t y = t 2 4 for  2 t 2

    Coordinate-plane figure.
    Figure 11.334
  22. { x = 4 cos 3 ( t ) y = 4 sin 3 ( t ) for  0 t 2 π

    Coordinate-plane figure.
    Figure 11.335
  23. { x = e t + e t y = e t e t for  2 t 2

    Coordinate-plane figure.
    Figure 11.336
  24. { x = cos ( 3 t ) y = sin ( 4 t ) for  0 t 2 π

    Coordinate-plane figure.
    Figure 11.337
  25. { x = 3 5 t y = 5 + 7 t for  0 t 1
  26. { x = 5 t 2 y = 1 3 t for  0 t 1
  27. { x = t y = 4 t 2 for  2 t 2
  28. { x = t 2 y = 4 t t 2 for  0 t 4
  29. { x = t 2 9 y = t for  2 t 3
  30. { x = t 2 6 t y = 3 t for  0 t 5
  31. { x = 5 cos ( t ) y = 5 sin ( t ) for  0 t < 2 π
  32. { x = 1 + 2 cos ( t ) y = 2 sin ( t ) for  0 t < 2 π
  33. { x = 3 cos ( t ) y = 3 + 3 sin ( t ) for  0 t < 2 π
  34. { x = 3 cos ( t ) y = 3 3 sin ( t ) for  0 t < 2 π
  35. { x = 3 + 117 cos ( t ) y = 1 + 117 sin ( t ) for  0 t < 2 π
  36. { x = 1 + 3 cos ( t ) y = sin ( t ) for  0 t < 2 π
  37. { x = 2 cos ( t ) y = 3 sin ( t ) 3 for  0 t < 2 π
  38. { x = 2 cos ( t π 2 ) = 2 sin ( t ) y = 3 3 sin ( t π 2 ) = 3 + 3 cos ( t ) for  0 t < 2 π
  39. { x ( t ) , y ( t ) where:

    x ( t ) = { 3 t , 0 t 1 6 3 t , 1 t 2 0 , 2 t 3 y ( t ) = { 0 , 0 t 1 4 t 4 , 1 t 2 12 4 t , 2 t 3

  40. The parametric equations for the inverse are { x = t 3 + 3 t 4 y = t for  < t <
  41. r = 6 cos ( 2 θ ) translates to { x = 6 cos ( 2 θ ) cos ( θ ) y = 6 cos ( 2 θ ) sin ( θ ) for  0 θ < 2 π .
  42. The parametric equations which describe the locations of passengers on the London Eye are { x = 67.5 cos ( π 15 t π 2 ) = 67.5 sin ( π 15 t ) y = 67.5 sin ( π 15 t π 2 ) + 67.5 = 67.5 67.5 cos ( π 15 t ) for  < t <
  43. The parametric equations for the hammer throw are { x = 33 cos ( 42 ) t y = 16 t 2 + 33 sin ( 42 ) t + 6 for t 0 . To find when the hammer hits the ground, we solve y ( t ) = 0 and get t 0.23 or 1.61 . Since t 0 , the hammer hits the ground after approximately t = 1.61 seconds after it was launched into the air. To find how far away the hammer hits the ground, we find x ( 1.61 ) 39.48 feet from where it was thrown into the air.
  44. We solve y = v 0 2 sin 2 ( θ ) 2 g + s 0 = v 0 2 sin 2 ( 85 ) 2 ( 32 ) + 5 = 31.5 to get v 0 = ± 41.34 . The initial speed of the sheaf was approximately 41.34 feet per second.

Adapted from Precalculus, 3rd corrected edition, by Carl Stitz and Jeff Zeager (stitz-zeager.com), licensed under CC BY-NC-SA 3.0. Changes were made: reformatted as an accessible XYZ web edition. License: CC-BY-NC-SA-3.0.