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🍬Honors Algebra II Unit 12 Review

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12.3 Polar Coordinates and Complex Numbers in Trigonometric Form

12.3 Polar Coordinates and Complex Numbers in Trigonometric Form

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
🍬Honors Algebra II
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Rectangular vs Polar Coordinates

Rectangular coordinates (x,y)(x, y) describe a point using horizontal and vertical distances from the origin. Polar coordinates (r,θ)(r, \theta) describe the same point using a distance rr from the origin and an angle θ\theta measured from the positive xx-axis. Both systems locate the same points; they just use different measurements to get there.

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Converting Between Coordinate Systems

Polar to rectangular is the more straightforward direction:

x=rcosθy=rsinθx = r\cos\theta \qquad y = r\sin\theta

Example: Convert (3,π6)(3, \frac{\pi}{6}) from polar to rectangular. x=3cosπ6=332=332x = 3\cos\frac{\pi}{6} = 3 \cdot \frac{\sqrt{3}}{2} = \frac{3\sqrt{3}}{2} y=3sinπ6=312=32y = 3\sin\frac{\pi}{6} = 3 \cdot \frac{1}{2} = \frac{3}{2} So the rectangular form is (332,  32)\left(\frac{3\sqrt{3}}{2},\; \frac{3}{2}\right).

Rectangular to polar requires more care:

r=x2+y2θ=tan1 ⁣(yx)r = \sqrt{x^2 + y^2} \qquad \theta = \tan^{-1}\!\left(\frac{y}{x}\right)

The catch with θ\theta: your calculator's tan1\tan^{-1} only returns values in (π2,π2)\left(-\frac{\pi}{2}, \frac{\pi}{2}\right), which covers Quadrants I and IV. If the point is in Quadrant II or III (meaning x<0x < 0), you need to add π\pi to the calculator result to get the correct angle.

One more detail: the origin (0,0)(0, 0) in rectangular corresponds to r=0r = 0 in polar, but the angle θ\theta is undefined there since there's no unique direction from the origin to itself.

Comparing Coordinate Systems

  • Rectangular coordinates work well for grid-like settings (maps, standard graphs, linear equations).
  • Polar coordinates shine when a problem involves distance and direction from a central point (radar, circular motion, navigation).
  • Some equations simplify dramatically in polar form. A circle centered at the origin is x2+y2=a2x^2 + y^2 = a^2 in rectangular but just r=ar = a in polar.

Graphing Polar Equations

Converting Between Coordinate Systems, Converting Between Polar Coordinates to Rectangular Coordinates | Precalculus II

Plotting Points and Curves

Polar equations have the form r=f(θ)r = f(\theta). To graph one:

  1. Build a table of θ\theta values, usually from 00 to 2π2\pi (choose increments like π6\frac{\pi}{6} or 30°30°).
  2. Calculate the corresponding rr for each θ\theta.
  3. Plot each point (r,θ)(r, \theta) on polar graph paper (or by converting to rectangular).
  4. Connect the points with a smooth curve.

For example, to graph r=2sin(3θ)r = 2\sin(3\theta), you'd evaluate rr at θ=0°,30°,60°,,330°\theta = 0°, 30°, 60°, \ldots, 330°. This particular equation produces a rose curve with 3 petals.

Common polar curves you should recognize:

  • Circles: r=ar = a (centered at origin) or r=acosθr = a\cos\theta / r=asinθr = a\sin\theta (passing through origin)
  • Cardioids: r=a(1+cosθ)r = a(1 + \cos\theta) — heart-shaped, with a cusp at the origin
  • Limaçons: r=a+bcosθr = a + b\cos\theta — may have an inner loop if b>ab > a
  • Rose curves: r=acos(nθ)r = a\cos(n\theta)nn petals if nn is odd, 2n2n petals if nn is even

Identifying Symmetry

Testing for symmetry saves you work when graphing because you only need to plot part of the curve and reflect the rest.

  • Symmetry about the polar axis (horizontal axis): Replace θ\theta with θ-\theta. If the equation is unchanged, the curve is symmetric about the polar axis.
  • Symmetry about the origin: Replace rr with r-r (or equivalently, replace θ\theta with θ+π\theta + \pi). If the equation is unchanged, the curve is symmetric about the origin.
  • Symmetry about the line θ=π2\theta = \frac{\pi}{2} (vertical axis): Replace θ\theta with πθ\pi - \theta. If the equation is unchanged, the curve has vertical symmetry.

Note: an equation like r=1cosθr = \frac{1}{\cos\theta} is actually the vertical line x=1x = 1 in rectangular form. It's undefined at θ=π2\theta = \frac{\pi}{2} and θ=3π2\theta = \frac{3\pi}{2} because cosθ=0\cos\theta = 0 there, producing vertical asymptotes in the polar graph.

Complex Numbers in Trigonometric Form

Converting Between Coordinate Systems, Identify and Graph Polar Equations by Converting to Rectangular Equations | Precalculus II

Representing Complex Numbers

Any complex number z=a+biz = a + bi can be rewritten in trigonometric (polar) form:

z=r(cosθ+isinθ)z = r(\cos\theta + i\sin\theta)

Here rr is the modulus (the distance from the origin to the point (a,b)(a, b) on the complex plane) and θ\theta is the argument (the angle from the positive real axis).

The conversion formulas are the same as rectangular-to-polar:

r=a2+b2θ=tan1 ⁣(ba) (with quadrant adjustments)r = \sqrt{a^2 + b^2} \qquad \theta = \tan^{-1}\!\left(\frac{b}{a}\right) \text{ (with quadrant adjustments)}

Example: Convert 3+4i3 + 4i to trigonometric form. r=9+16=5r = \sqrt{9 + 16} = 5 θ=tan1 ⁣(43)53.13°\theta = \tan^{-1}\!\left(\frac{4}{3}\right) \approx 53.13° Since a>0a > 0 and b>0b > 0 (Quadrant I), no adjustment is needed. Trigonometric form: 5(cos53.13°+isin53.13°)5(\cos 53.13° + i\sin 53.13°)

You may also see the shorthand cis notation: r  cis  θ=r(cosθ+isinθ)r\;\text{cis}\;\theta = r(\cos\theta + i\sin\theta).

Euler's formula provides yet another equivalent form: eiθ=cosθ+isinθe^{i\theta} = \cos\theta + i\sin\theta, so z=reiθz = re^{i\theta}. This is useful for understanding why multiplication and division rules work the way they do.

Geometric Interpretation

On the complex plane, the modulus rr tells you how far the number is from the origin, and the argument θ\theta tells you the direction. For instance, 2(cosπ3+isinπ3)2(\cos\frac{\pi}{3} + i\sin\frac{\pi}{3}) sits 2 units from the origin at a 60°60° angle. This geometric view makes operations like multiplication and finding roots much more intuitive.

Operations on Complex Numbers

Multiplication and Division

Trigonometric form turns multiplication and division into simple arithmetic on the moduli and arguments.

Multiplication: Multiply the moduli, add the arguments.

r1(cis  θ1)r2(cis  θ2)=r1r2  cis(θ1+θ2)r_1(\text{cis}\;\theta_1) \cdot r_2(\text{cis}\;\theta_2) = r_1 r_2\;\text{cis}(\theta_1 + \theta_2)

Example: (2  cis  π3)(3  cis  π4)=6  cis  7π12(2\;\text{cis}\;\frac{\pi}{3})(3\;\text{cis}\;\frac{\pi}{4}) = 6\;\text{cis}\;\frac{7\pi}{12}

Division: Divide the moduli, subtract the arguments.

r1(cis  θ1)r2(cis  θ2)=r1r2  cis(θ1θ2)\frac{r_1(\text{cis}\;\theta_1)}{r_2(\text{cis}\;\theta_2)} = \frac{r_1}{r_2}\;\text{cis}(\theta_1 - \theta_2)

Example: 6  cis  2π32  cis  π6=3  cis  π2\frac{6\;\text{cis}\;\frac{2\pi}{3}}{2\;\text{cis}\;\frac{\pi}{6}} = 3\;\text{cis}\;\frac{\pi}{2}

If your resulting angle falls outside [0,2π)[0, 2\pi), add or subtract 2π2\pi to bring it back into the principal range.

Powers and Roots (De Moivre's Theorem)

De Moivre's Theorem is the key result here. For any complex number z=r(cosθ+isinθ)z = r(\cos\theta + i\sin\theta) and positive integer nn:

zn=rn(cos(nθ)+isin(nθ))z^n = r^n(\cos(n\theta) + i\sin(n\theta))

You raise the modulus to the nnth power and multiply the argument by nn. This is far faster than multiplying zz by itself nn times in rectangular form.

Example: [2(cosπ6+isinπ6)]5=25(cos5π6+isin5π6)=32(cos5π6+isin5π6)\left[2\left(\cos\frac{\pi}{6} + i\sin\frac{\pi}{6}\right)\right]^5 = 2^5\left(\cos\frac{5\pi}{6} + i\sin\frac{5\pi}{6}\right) = 32\left(\cos\frac{5\pi}{6} + i\sin\frac{5\pi}{6}\right)

Finding nnth roots uses the same theorem in reverse. The nnth roots of z=r(cosθ+isinθ)z = r(\cos\theta + i\sin\theta) are:

zk=rn(cosθ+2kπn+isinθ+2kπn),k=0,1,2,,n1z_k = \sqrt[n]{r}\left(\cos\frac{\theta + 2k\pi}{n} + i\sin\frac{\theta + 2k\pi}{n}\right), \quad k = 0, 1, 2, \ldots, n-1

This gives exactly nn distinct roots, evenly spaced around a circle of radius rn\sqrt[n]{r}.

Steps to find nnth roots:

  1. Write the complex number in trigonometric form r(cosθ+isinθ)r(\cos\theta + i\sin\theta).
  2. Compute rn\sqrt[n]{r} for the new modulus.
  3. For k=0k = 0, the first root has argument θn\frac{\theta}{n}.
  4. Each successive root (k=1,2,k = 1, 2, \ldots) adds 2πn\frac{2\pi}{n} to the argument.

Example: Find the cube roots of 8(cos2π3+isin2π3)8(\cos\frac{2\pi}{3} + i\sin\frac{2\pi}{3}).

  • New modulus: 83=2\sqrt[3]{8} = 2
  • k=0k = 0: 2(cos2π9+isin2π9)2(\cos\frac{2\pi}{9} + i\sin\frac{2\pi}{9})
  • k=1k = 1: 2(cos8π9+isin8π9)2(\cos\frac{8\pi}{9} + i\sin\frac{8\pi}{9})
  • k=2k = 2: 2(cos14π9+isin14π9)2(\cos\frac{14\pi}{9} + i\sin\frac{14\pi}{9})

These three roots are equally spaced at 2π3\frac{2\pi}{3} apart on a circle of radius 2.

The geometric spacing of roots is a useful check: if your roots aren't evenly distributed around the circle, something went wrong in the calculation.

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