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Parametric Functions

Formulas & Definitions
Core Definition

Parametric functions express coordinate variables (such as xxx, yyy, and zzz) as independent functions of a shared auxiliary variable called a parameter (usually denoted by ttt representing time or ΞΈ\thetaΞΈ representing an angle):

x=x(t),y=y(t),z=z(t)forΒ a≀t≀bx = x(t), \quad y = y(t), \quad z = z(t) \quad \text{for } a \leq t \leq bx=x(t),y=y(t),z=z(t)forΒ a≀t≀b
The graph of these equations is a curve traced out in coordinate space as the parameter varies over its domain.

Concept Explanation

Unlike traditional functions where yyy is directly dependent on xxx (e.g. y=f(x)y = f(x)y=f(x)), parametric equations define both xxx and yyy independently based on the parameter ttt. This is highly useful for describing trajectories of moving objects, as it records not only the path itself but also when the object occupies each position, and in which direction it is moving.


Evaluating and Graphing Parametric Curves

To graph a parametric curve manually:

  1. Create a table of values: Choose sequential values of the parameter ttt in its domain.
  2. Calculate coordinates: For each ttt, calculate the corresponding values for x(t)x(t)x(t) and y(t)y(t)y(t).
  3. Plot the points: Plot the resulting coordinate pairs (x,y)(x,y)(x,y) in order of increasing ttt.
  4. Indicate orientation: Draw arrows along the curve to show the direction of motion as ttt increases.

Eliminating the Parameter (Converting to Cartesian)

Sometimes it is useful to rewrite a parametric curve in standard Cartesian coordinates (x,y)(x,y)(x,y) to see its geometric shape. To "eliminate the parameter":

  • Method 1 (Substitution): Solve one of the equations for ttt (e.g. t=xβˆ’x0at = \frac{x - x_0}{a}t=axβˆ’x0​​), and substitute this expression into the other equations. This works well for linear and simple polynomial paths.
  • Method 2 (Trig Identities): If the equations involve sine and cosine, isolate the trig functions and use the Pythagorean identity cos⁑2t+sin⁑2t=1\cos^2 t + \sin^2 t = 1cos2t+sin2t=1.
    • Example: xr=cos⁑t\frac{x}{r} = \cos trx​=cost and yr=sin⁑tβ€…β€ŠβŸΉβ€…β€Š(xr)2+(yr)2=cos⁑2t+sin⁑2t=1β€…β€ŠβŸΉβ€…β€Šx2+y2=r2\frac{y}{r} = \sin t \implies \left(\frac{x}{r}\right)^2 + \left(\frac{y}{r}\right)^2 = \cos^2 t + \sin^2 t = 1 \implies x^2 + y^2 = r^2ry​=sint⟹(rx​)2+(ry​)2=cos2t+sin2t=1⟹x2+y2=r2 (a circle of radius rrr).

Why We Use It in Multivariable Calculus (Calculus III)

Parametric functions are the fundamental building blocks of spatial geometry and vector calculus:

1. Vector-Valued Functions

A curve in 3D space is described as a single vector-valued function r⃗(t)\vec{r}(t)r(t) whose component scalar functions are the parametric equations of the curve:

rβƒ—(t)=⟨x(t),y(t),z(t)⟩\vec{r}(t) = \langle x(t), y(t), z(t) \rangler(t)=⟨x(t),y(t),z(t)⟩
Taking derivatives and integrals of r⃗(t)\vec{r}(t)r(t) gives velocity, acceleration, and arc lengths.

2. Parameterization for Line Integrals

To evaluate a line integral ∫Cf(x,y,z) ds\int_C f(x,y,z) \, ds∫C​f(x,y,z)ds or calculate work done by a force field along a path CCC, ∫CFβƒ—β‹…drβƒ—\int_C \vec{F} \cdot d\vec{r}∫C​Fβ‹…dr, you must first parameterize the path CCC. Parameterizing expresses xxx, yyy, and zzz in terms of a single variable ttt, converting a complex multidimensional path integral into a simple single-variable integral in terms of ttt:

∫CFβƒ—β‹…drβƒ—=∫abFβƒ—(rβƒ—(t))β‹…rβƒ—β€²(t) dt\int_C \vec{F} \cdot d\vec{r} = \int_a^b \vec{F}(\vec{r}(t)) \cdot \vec{r}'(t) \, dt∫C​Fβ‹…dr=∫ab​F(r(t))β‹…rβ€²(t)dt


Example Problems

Example Problem 1: Circular Motion & Eliminating Parameter

Graph and find the Cartesian equation for the parametric equations:

x(t)=3cos⁑t,y(t)=3sin⁑tforΒ 0≀t≀2Ο€x(t) = 3\cos t, \quad y(t) = 3\sin t \quad \text{for } 0 \leq t \leq 2\pix(t)=3cost,y(t)=3sintforΒ 0≀t≀2Ο€

Solution

Step 1: Evaluate points for key parameter values Construct a table of values:

ttt x(t)=3cos⁑tx(t) = 3\cos tx(t)=3cost y(t)=3sin⁑ty(t) = 3\sin ty(t)=3sint Point (x,y)(x,y)(x,y)
000 3cos⁑(0)=33\cos(0) = 33cos(0)=3 3sin⁑(0)=03\sin(0) = 03sin(0)=0 (3,0)(3,0)(3,0)
Ο€/2\pi/2Ο€/2 3cos⁑(Ο€/2)=03\cos(\pi/2) = 03cos(Ο€/2)=0 3sin⁑(Ο€/2)=33\sin(\pi/2) = 33sin(Ο€/2)=3 (0,3)(0,3)(0,3)
Ο€\piΟ€ 3cos⁑(Ο€)=βˆ’33\cos(\pi) = -33cos(Ο€)=βˆ’3 3sin⁑(Ο€)=03\sin(\pi) = 03sin(Ο€)=0 (βˆ’3,0)(-3,0)(βˆ’3,0)
3Ο€/23\pi/23Ο€/2 3cos⁑(3Ο€/2)=03\cos(3\pi/2) = 03cos(3Ο€/2)=0 3sin⁑(3Ο€/2)=βˆ’33\sin(3\pi/2) = -33sin(3Ο€/2)=βˆ’3 (0,βˆ’3)(0,-3)(0,βˆ’3)
2Ο€2\pi2Ο€ 3cos⁑(2Ο€)=33\cos(2\pi) = 33cos(2Ο€)=3 3sin⁑(2Ο€)=03\sin(2\pi) = 03sin(2Ο€)=0 (3,0)(3,0)(3,0)

Plotting these points in order shows a circle of radius 333. The orientation is counterclockwise (starting at (3,0)(3,0)(3,0), moving up to (0,3)(0,3)(0,3), then left to (βˆ’3,0)(-3,0)(βˆ’3,0), etc.).

Step 2: Eliminate the parameter Isolate the trigonometric terms:

x3=cos⁑tandy3=sin⁑t\frac{x}{3} = \cos t \quad \text{and} \quad \frac{y}{3} = \sin t3x​=costand3y​=sint

Use the identity cos⁑2t+sin⁑2t=1\cos^2 t + \sin^2 t = 1cos2t+sin2t=1:

(x3)2+(y3)2=1β€…β€ŠβŸΉβ€…β€Šx29+y29=1β€…β€ŠβŸΉβ€…β€Šx2+y2=9\left(\frac{x}{3}\right)^2 + \left(\frac{y}{3}\right)^2 = 1 \implies \frac{x^2}{9} + \frac{y^2}{9} = 1 \implies x^2 + y^2 = 9(3x​)2+(3y​)2=1⟹9x2​+9y2​=1⟹x2+y2=9

The Cartesian equation is x2+y2=9x^2 + y^2 = 9x2+y2=9, which represents a circle centered at the origin with radius 333.

Example Problem 2: 3D Line Segment Parameterization

Find parametric equations for the 3D line segment starting at the point P(1,2,βˆ’1)P(1, 2, -1)P(1,2,βˆ’1) and ending at the point Q(3,5,2)Q(3, 5, 2)Q(3,5,2) for the domain 0≀t≀10 \leq t \leq 10≀t≀1.

Solution

Step 1: Find the direction vector (v⃗\vec{v}v) The vector v⃗\vec{v}v points from the start point PPP to the end point QQQ:

vβƒ—=PQβ†’=⟨Qxβˆ’Px,Qyβˆ’Py,Qzβˆ’Pz⟩\vec{v} = \overrightarrow{PQ} = \langle Q_x - P_x, Q_y - P_y, Q_z - P_z \ranglev=PQ​=⟨Qxβ€‹βˆ’Px​,Qyβ€‹βˆ’Py​,Qzβ€‹βˆ’Pzβ€‹βŸ©
vβƒ—=⟨3βˆ’1,5βˆ’2,2βˆ’(βˆ’1)⟩=⟨2,3,3⟩\vec{v} = \langle 3 - 1, 5 - 2, 2 - (-1) \rangle = \langle 2, 3, 3 \ranglev=⟨3βˆ’1,5βˆ’2,2βˆ’(βˆ’1)⟩=⟨2,3,3⟩

Step 2: Set up the vector equation of the line segment The vector equation is rβƒ—(t)=rβƒ—0+tvβƒ—\vec{r}(t) = \vec{r}_0 + t\vec{v}r(t)=r0​+tv where rβƒ—0=⟨1,2,βˆ’1⟩\vec{r}_0 = \langle 1, 2, -1 \rangler0​=⟨1,2,βˆ’1⟩ is the starting point:

rβƒ—(t)=⟨1,2,βˆ’1⟩+t⟨2,3,3⟩\vec{r}(t) = \langle 1, 2, -1 \rangle + t\langle 2, 3, 3 \rangler(t)=⟨1,2,βˆ’1⟩+t⟨2,3,3⟩

Step 3: Extract component parametric equations

x(t)=1+2t,y(t)=2+3t,z(t)=βˆ’1+3tforΒ 0≀t≀1x(t) = 1 + 2t, \quad y(t) = 2 + 3t, \quad z(t) = -1 + 3t \quad \text{for } 0 \leq t \leq 1x(t)=1+2t,y(t)=2+3t,z(t)=βˆ’1+3tforΒ 0≀t≀1

Step 4: Verify boundary conditions

  • At t=0t = 0t=0: x(0)=1,y(0)=2,z(0)=βˆ’1β€…β€ŠβŸΉβ€…β€Šx(0)=1, y(0)=2, z(0)=-1 \impliesx(0)=1,y(0)=2,z(0)=βˆ’1⟹ point is (1,2,βˆ’1)(1, 2, -1)(1,2,βˆ’1) (Start point PPP)
  • At t=1t = 1t=1: x(1)=3,y(1)=5,z(1)=2β€…β€ŠβŸΉβ€…β€Šx(1)=3, y(1)=5, z(1)=2 \impliesx(1)=3,y(1)=5,z(1)=2⟹ point is (3,5,2)(3, 5, 2)(3,5,2) (End point QQQ)

The parametric equations are x(t)=1+2tx(t) = 1 + 2tx(t)=1+2t, y(t)=2+3ty(t) = 2 + 3ty(t)=2+3t, z(t)=βˆ’1+3tz(t) = -1 + 3tz(t)=βˆ’1+3t for 0≀t≀10 \leq t \leq 10≀t≀1.


Connections & References

  • Parent Concepts: Calculus Foundations
  • Related Concepts: Solving Right Triangles, Line Integrals
  • Course Links: Calc-3 Discussion 01