Polar Coordinates

A point named by a distance and an angle.

A distance and an angle

Cartesian coordinates name a point by how far across and how far up it is. Polar coordinates name it by how far it is from a fixed point, and in which direction.

The fixed point is the pole, O, at the origin, and the directions are measured from the initial line, the positive x-axis. A point P has polar coordinates (r, θ): r is the distance OP, and θ is the angle turned counterclockwise from the initial line to OP, in radians.

For example, the point 2 from O in the direction π/3, which is 60° above the initial line, has r = 2 and θ = π/3.

xyr = 2

The point r = 2, θ = π/3. It lies on the dashed circle of radius 2 about the pole, where the arrow from the pole at π/3 above the initial line meets it. Straight below it, at (1, 0), is the foot of the right triangle whose legs are its x and y.

From polar to Cartesian

Drop a perpendicular from P to the x-axis. That makes a right triangle with hypotenuse r and angle θ at the pole. The horizontal leg is adjacent to θ and the vertical leg is opposite, so x = r cos θ and y = r sin θ.

For r = 2 and θ = π/3, x = 2 × ½ = 1 and y = 2 × √3/2 = √3, so the point is (1, √3).

The same formulas work in every quadrant, because cos θ and sin θ carry the signs. For r = 4 and θ = 5π/6, x = 4 cos 5π/6 = −2√3 ≈ −3.46 and y = 4 sin 5π/6 = 2, a point up and to the left.

From Cartesian to polar

Going back, r is the hypotenuse, so Pythagoras gives r = √(x² + y²). The angle satisfies tan θ = y/x.

The tangent repeats every half turn, so two directions share each value of tan θ. A calculator’s inverse tangent only returns angles between −π/2 and π/2, which point to the right of the y-axis. So find the quadrant first, then correct the angle.

Take (−3, 4). It is r = √(9 + 16) = 5 from the pole. The inverse tangent of 4/(−3) gives −0.927, which points down and to the right, but (−3, 4) is up and to the left, in the second quadrant. The acute angle with tangent 4/3 is 0.927, so θ = π − 0.927 ≈ 2.214. Check: 5 cos 2.214 = −3 and 5 sin 2.214 = 4.

Taking θ between 0 and 2π, the other quadrants work the same way. (−3, −4), in the third quadrant, has θ = π + 0.927 ≈ 4.069, and (3, −4), in the fourth, has θ = 2π − 0.927 ≈ 5.356. Some books take θ between −π and π instead; then (3, −4) has θ ≈ −0.927.

xyr = 5

The arrow runs from the pole to (−3, 4), 5 long at the angle 2.214. The hollow point is (3, −4), where the inverse tangent’s angle −0.927 would put a point 5 from the pole: the same tangent, the opposite direction.

There and back

r = 2 at θ = π/3 is the point (2 cos(π/3), 2 sin(π/3)) = (1, √3). Going back, r = √(1 + 3) = 2, and tan θ = √3. The point is in the first quadrant, so θ = π/3, and the round trip returns the same pair.

A point has more than one polar name. Adding 2π to θ turns the direction a full turn and back to where it was, so (2, π/3) and (2, 7π/3) are the same point. The pole itself has r = 0, and any θ names it.

Equations in polar form

A curve’s equation converts the same way. The circle x² + y² = 9 becomes r² = 9, that is r = 3: every point is 3 from the pole.

The circle x² + y² = 6x passes through the pole. Substituting gives r² = 6r cos θ, and dividing by r gives r = 6 cos θ. The distance from the pole now depends on the direction: 6 along the initial line, and 0 at θ = π/2.

The usual mistakes

Swapping the legs. x = r cos θ and y = r sin θ: the cosine goes with the leg next to the angle.

Trusting the inverse tangent in every quadrant. It gives −0.927 for both (−3, 4) and (3, −4), so the quadrant has to be checked.

Leaving out the square root. x² + y² is r², not r: for (3, 4) it is 25, while r = 5.

Adding the legs. 3 + 4 = 7 is longer than the distance 5, because a straight line is the shortest way.

A dish antenna

In the application below, the cross-section of a dish antenna is given from its receiver as r = 1.2/(1 − cos θ). Multiplying out gives r − r cos θ = 1.2. Replacing r cos θ by x leaves r = x + 1.2, and squaring with r² = x² + y² turns it into a Cartesian equation.

Worked example: A Dish Antenna Described From Its Receiver: The Shape in Cartesian Form, and the Width and Depth of the Dish

Question In a cross-section through its axis, the reflector of a dish antenna follows the curve r = 1.21 − cos θ meters. The pole is at the receiver, which is held in front of the dish, and the initial line runs from the receiver along the axis, away from the dish and toward the satellite; θ is in radians measured counterclockwise from it. (a) Write the curve as a Cartesian equation, and find how far the center of the dish is behind the receiver. (b) The rim of the dish lies where θ = 2π3 and where θ = 4π3. How wide is the dish across its rim, and how deep is it, from the plane of the rim to its center?

  1. 1.Multiplying out, r − rcos θ = 1.2. Since rcos θ = x, this is r = x + 1.2, and since r2 = x2 + y2, squaring both sides gives x2 + y2 = x2 + 2.4x + 1.44.

    satellitereceiverr − r cos θ = 1.2, so r = x + 1.2
    satellitereceiverr − r cos θ = 1.2, so r = x + 1.2
    Multiplying out, r − rcos θ = 1.2; with rcos θ = x this is r = x + 1.2, and r2 = x2 + y2.
  2. 2.(a) The x2 terms cancel, leaving y2 = 2.4x + 1.44 = 2.4(x + 0.6), a parabola whose axis is the initial line. Its vertex, the center of the dish, is where y = 0: x = −0.6, so the center of the dish is 0.6 meters behind the receiver. The polar equation agrees: at θ = π, r = 1.22 = 0.6.

    satellitereceiver0.6 mr − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behind
    satellitereceiver0.6 mr − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behind
    (a) Squaring, y2 = 2.4x + 1.44 = 2.4(x + 0.6): a parabola with its vertex, the center of the dish, 0.6 meters behind the receiver.
  3. 3.At the rim, θ = 2π3 and cos θ = −12, so r = 1.21.5 = 0.8 meters. In Cartesian coordinates that point is x = 0.8cos 2π3 = −0.4 and y = 0.8sin 2π3 = 0.4√3, and by symmetry the rim point at θ = 4π3 is (−0.4, −0.4√3).

    satellitereceiver0.6 mr = 0.8r − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behindrim: r = 1.2/1.5 = 0.8, x = −0.4, y = 0.4√3
    satellitereceiver0.6 mr = 0.8r − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behindrim: r = 1.2/1.5 = 0.8, x = −0.4, y = 0.4√3
    At the rim, r = 1.21 + 0.5 = 0.8, so the rim is at x = −0.4, y = ± 0.4√3.
  4. 4.(b) The dish is 2 × 0.4√3 = 0.8√3 ≈ 1.39 meters wide across its rim. The rim lies in the plane x = −0.4 and the center at x = −0.6, so the dish is 0.6 − 0.4 = 0.2 meters deep. Check: the rim point satisfies the Cartesian equation, since (0.4√3)2 = 0.48 and 2.4(−0.4 + 0.6) = 0.48.

    satellitereceiver0.6 mr = 0.81.39 m0.2 m deepr − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behindrim: r = 1.2/1.5 = 0.8, x = −0.4, y = 0.4√3(b) width 2 × 0.693 = 1.39 mdepth 0.6 − 0.4 = 0.2 m
    satellitereceiver0.6 mr = 0.81.39 m0.2 m deepr − r cos θ = 1.2, so r = x + 1.2(a) y2= 2.4(x + 0.6): center 0.6 m behindrim: r = 1.2/1.5 = 0.8, x = −0.4, y = 0.4√3(b) width 2 × 0.693 = 1.39 mdepth 0.6 − 0.4 = 0.2 m
    (b) The dish is 0.8√3 ≈ 1.39 meters wide and 0.6 − 0.4 = 0.2 meters deep.

Answer: (a) y² = 2.4(x + 0.6), a parabola, and the center of the dish is 0.6 meters behind the receiver; (b) the dish is 0.8√3 ≈ 1.39 meters wide and 0.2 meters deep

Common mistakes

  • Squaring r − rcos θ = 1.2 as it stands. That gives x2 + y2 − 2x√x2 + y2 + x2 = 1.44, which still holds a root. Moving rcos θ across first leaves r = x + 1.2, and one squaring then removes the root.
  • Taking cos 2π3 as +12 and getting r = 1.20.5 = 2.4 meters at the rim. The angle 2π3 lies in the second quadrant, where the cosine is negative, so the denominator is 1 + 12 and the rim is 0.8 meters from the receiver.

More polar curves problems, worked step by step →

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