Polar coordinates represent a point by its distance from the origin (r) and the angle from the positive x-axis (theta), rather than by horizontal and vertical distances (x, y). The conversion formulas are x = r*cos(theta), y = r*sin(theta), r^2 = x^2 + y^2, tan(theta) = y/x. Polar coordinates are the natural choice for problems with circular or rotational symmetry.
Plot points in polar coordinates, including negative r values. Practice converting points and equations between rectangular and polar forms. Convert familiar curves (circles, lines) to polar form to build intuition.
The rectangular coordinate system you know from algebra locates points by measuring how far left/right (x) and up/down (y) to travel from the origin. Polar coordinates ask a different question: how far away is the point (r), and in what direction (θ)? For a point directly to the right of the origin at distance 5, you would write (5, 0°). Directly up at distance 5 is (5, 90°) or (5, π/2). This way of thinking turns out to be far more natural for anything involving circles or rotation.
The conversion formulas follow directly from right-triangle trigonometry, which you already know. If you draw the segment from the origin to the point (r, θ), it forms the hypotenuse of a right triangle. The horizontal leg has length r·cos(θ) — that is the x-coordinate. The vertical leg has length r·sin(θ) — that is the y-coordinate. Going the other direction: r = √(x² + y²) (the Pythagorean theorem) and tan(θ) = y/x. These four formulas let you move freely between the two systems.
One feature of polar coordinates surprises many students: the same physical point can be written in infinitely many ways. The point (3, π/4) is identical to (3, π/4 + 2π), since adding a full rotation lands you back in the same direction. It is also identical to (-3, π/4 + π), because a negative r means "go the opposite direction." This non-uniqueness is not a flaw — it is a reflection of how angles and rotations work. But it does mean you must be careful when checking whether two polar expressions represent the same point.
The power of polar coordinates becomes clear when you try to write the equations of certain curves. The circle x² + y² = 25 is a compact equation in rectangular form, but it becomes r = 5 in polar form — just a constant. A spiral that grows with each rotation is r = θ, which would be nearly impossible to express in x and y. Curves like rose petals and cardioids, which are nightmarishly complicated in rectangular form, reduce to elegant formulas in polar form. The coordinate system you choose is a tool, and polar coordinates are the right tool whenever the geometry has rotational symmetry.