Circle (Standard Equation)

A circle is one of the four classical conic sections, formed when a plane intersects a right circular cone parallel to the base. In coordinate geometry, a circle is defined as the set of all points in a plane that are equidistant from a fixed point called the center. This fixed distance is called the radius. Because this definition is purely about distance, the equation of a circle follows directly from the distance formula, making it one of the most elegant connections between geometry and algebra. The standard equation of a circle with center (h, k) and radius r is (x − h)² + (y − k)² = r². When the center is at the origin, this simplifies to x² + y² = r². These equations allow us to identify a circle's properties instantly, graph it precisely, and solve geometric problems involving tangent lines, chords, and intersections with other curves. Understanding the circle equation is foundational to analytic geometry and appears throughout calculus, physics, and engineering. Circles differ from other conics — parabolas, ellipses, and hyperbolas — because they have a single eccentricity value of exactly 0, meaning every point on the curve is the same distance from the center. This special symmetry makes circles the basis for trigonometry, polar coordinates, and the study of periodic motion. Mastering the standard circle equation prepares you for all these advanced topics.

Key takeaways
  • Start with the Definition of a Circle
  • Apply the Distance Formula
  • Square Both Sides to Get Standard Form
  • Identify Center and Radius from the Equation
  • Convert General Form to Standard Form by Completing the Square
  • Key Properties of a Circle

Start with the Definition of a Circle

A circle is the set of all points P(x, y) whose distance from a fixed center C(h, k) equals the radius r. This means every point on the circle satisfies: distance from P to C = r.

Apply the Distance Formula

The distance between point P(x, y) and center C(h, k) is given by the distance formula: d = √((x − h)² + (y − k)²). Setting this equal to r gives: √((x − h)² + (y − k)²) = r.

Square Both Sides to Get Standard Form

Squaring both sides eliminates the square root: (x − h)² + (y − k)² = r². This is the standard equation of a circle. Since r > 0, squaring introduces no extraneous issues. The equation only holds for r > 0; if the right side were 0, it would represent just the single point (h, k), and a negative right side gives no real graph.

Identify Center and Radius from the Equation

Given (x − h)² + (y − k)² = r², read the center as (h, k) — note the sign change from the equation — and the radius as r = √(right-hand side). For example, (x − 3)² + (y + 2)² = 25 has center (3, −2) and radius r = √25 = 5. Be careful: (y + 2)² = (y − (−2))², so the y-coordinate of the center is −2, not +2.

Convert General Form to Standard Form by Completing the Square

A circle's equation is sometimes given in general form: x² + y² + Dx + Ey + F = 0. To convert, group x-terms and y-terms, then complete the square for each variable. For x² + Dx, add (D/2)² to both sides; for y² + Ey, add (E/2)² to both sides. The result is (x + D/2)² + (y + E/2)² = (D/2)² + (E/2)² − F. The circle is real when the right side is positive, a point when zero, and imaginary when negative.

Key Properties of a Circle

From the standard equation, several properties follow immediately. The diameter is d = 2r. The circumference is C = 2πr and the area is A = πr². The circle is symmetric about every line passing through its center. The x-intercepts are found by setting y = 0 and solving; similarly for y-intercepts. A tangent line at any point on the circle is perpendicular to the radius drawn to that point, a fact used extensively in circle geometry problems.

The Key Equation

(x−h)2+(y−k)2=r2(x - h)^2 + (y - k)^2 = r^2
  • x,\, y — Coordinates of a point on the circle (none (dimensionless coordinates)): Any point satisfying the equation lies exactly on the circle.
  • h — x-coordinate of the center (none): The horizontal position of the circle's center; appears as (x − h), so a positive h shifts the circle right.
  • k — y-coordinate of the center (none): The vertical position of the circle's center; appears as (y − k), so a positive k shifts the circle up.
  • r — Radius (length units): The constant distance from the center to every point on the circle; must be positive (r > 0).

Worked Example

Problem. The equation x² + y² − 6x + 4y − 3 = 0 is given. (a) Write this equation in standard form. (b) Identify the center and radius. (c) Find the x-intercepts of the circle.

(x−3)2+(y+2)2=16;C=(3,−2),  r=4;x-intercepts: x=3±23(x-3)^2 + (y+2)^2 = 16;\quad C=(3,-2),\; r=4;\quad x\text{-intercepts: } x = 3 \pm 2\sqrt{3}

Answer. Standard form: (x − 3)² + (y + 2)² = 16; Center: (3, −2); Radius: 4; x-intercepts: (3 ± 2√3, 0)

Figure
Diagram
xy12-1-212-1-2h=2, k=1r(h, k)(x−h)²+(y−k)²=r²P(x, y) — any point on circleP(x,y)
Origins · 1 minRené Descartes and how this was discovered
RD
René Descartes
1596–1650 · French

Descartes invented the Cartesian coordinate system, published in his 1637 work 'La Géométrie' (an appendix to his Discourse on the Method). By assigning numerical coordinates to points in a plane, he created the bridge between algebra and geometry that makes the circle equation — and all of analytic geometry — possible. His insight that every geometric curve can be described by an algebraic equation was revolutionary and forms the foundation of all coordinate geometry studied today. Descartes reportedly developed his ideas about coordinates while lying in bed watching a fly on the ceiling, wondering how to describe its exact position — a perfect origin story for a system built on locating points in a plane!

  • Distance Formula — The standard circle equation is derived directly from the distance formula; understanding d = √((x₂−x₁)² + (y₂−y₁)²) is essential to deriving and interpreting (x−h)²+(y−k)²=r².
  • Completing the Square — Converting a circle's general form (x²+y²+Dx+Ey+F=0) to standard form requires completing the square for both x and y terms.
  • Ellipse (Standard Equation) — An ellipse generalizes the circle: when the two denominators in (x−h)²/a² + (y−k)²/b² = 1 are equal (a = b = r), the ellipse becomes a circle.
  • Unit Circle — The unit circle is the special case x²+y²=1 (center at origin, radius 1) and is the foundation of trigonometry, defining sine and cosine as coordinates of points on this circle.
  • Midpoint Formula — The midpoint formula is used in circle problems to find centers from endpoints of diameters, since the center is the midpoint of any diameter.