Ellipse standard equation

Take a piece of string, pin its two ends to a board at two fixed points, and trace a pencil around while keeping the string taut. The curve you draw is an ellipse — the set of every point whose distances from those two pins always add up to the same total, the length of the string. Those pins are the ellipse's foci, and that single constant-sum property is enough to generate the whole shape, from planetary orbits to the elliptical arches used in architecture. Turning that string-and-pins picture into algebra is the goal of this section. Starting from the definition PF1+PF2=2aPF_1 + PF_2 = 2a, we place the foci symmetrically on the xx-axis, write the sum-of-distances condition in coordinates, and simplify by squaring twice until the messy square roots collapse into the clean standard form x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1. Along the way we meet the relation c2=a2−b2c^2 = a^2 - b^2 linking the semi-major axis aa, the semi-minor axis bb, and the focal distance cc, and we learn to read off an ellipse's foci, vertices, and axis lengths directly from its equation — skills tested repeatedly in CBSE Class 11 coordinate geometry.

The core insight

An ellipse is the locus of points whose distances from two fixed foci sum to a constant 2a2a, and squaring the coordinate form of that condition twice yields the standard equation x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 with c2=a2−b2c^2=a^2-b^2 tying the foci to the axes.

The core idea

The defining property. An ellipse is the locus of a point P(x,y)P(x,y) such that the sum of its distances from two fixed points F1F_1 and F2F_2, the foci, stays constant. Call that constant sum 2a2a, where 2a2a must be greater than the distance between the foci for the locus to be a real, closed curve rather than empty.

Placing coordinates conveniently. Put the centre of the ellipse at the origin and the foci on the xx-axis at F1(−c,0)F_1(-c,0) and F2(c,0)F_2(c,0), symmetric about the origin. This symmetry is a choice, not a law of nature — it is what turns the algebra into something manageable. For any point P(x,y)P(x,y) on the locus:

(x+c)2+y2+(x−c)2+y2=2a.\sqrt{(x+c)^2+y^2} + \sqrt{(x-c)^2+y^2} = 2a.

where: x,yx, y are the coordinates of a general point on the ellipse, cc is the distance from the centre to each focus, and 2a2a is the constant sum of distances fixed by the string length.

From two square roots to one clean equation. Isolating one radical and squaring twice, as carried out in full in the derivation below, eliminates both square roots and leaves an equation in x2x^2 and y2y^2 alone. Writing b2=a2−c2b^2 = a^2 - c^2 (valid since a>ca>c for a real ellipse) turns that equation into the standard form

x2a2+y2b2=1,a>b>0.\frac{x^2}{a^2}+\frac{y^2}{b^2}=1, \qquad a>b>0.

where: aa is the semi-major axis length, bb is the semi-minor axis length, and the constraint a>ba>b is a labelling convention — whichever axis is longer is always called aa, regardless of whether it lies along xx or yy.

Reading off the parts. For x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 with a>ba>b: the major axis lies along the xx-axis with length 2a2a and vertices (±a,0)(\pm a,0); the minor axis lies along the yy-axis with length 2b2b and endpoints (0,±b)(0,\pm b); and the foci sit at (±c,0)(\pm c,0) with c=a2−b2c=\sqrt{a^2-b^2}. If instead b>ab>a, every role of xx and yy swaps: the major axis runs along the yy-axis, vertices are (0,±b)(0,\pm b), and foci are (0,±c)(0,\pm c) with c=b2−a2c=\sqrt{b^2-a^2}.

Figure
Ellipse with centre origin foci at plus minus c and vertices at plus minus a on the x axis and minor axis endpoints at plus minus b on the y axis
Ellipse: sum of distances to the two foci is constant F1 minus c 0 F2 c 0 vertex minus a 0 vertex a 0 0 b 0 minus b P x y PF1 plus PF2 equals 2a for every point P on the curve
Derivation ADeriving the standard equation from the two-foci definition

Starting from the coordinate statement of the sum-of-distances property, (x+c)2+y2+(x−c)2+y2=2a\sqrt{(x+c)^2+y^2}+\sqrt{(x-c)^2+y^2}=2a, carry out the algebra of isolating and squaring each square root in turn so that the two radicals cancel out and only a polynomial relation between x2x^2, y2y^2, aa, and cc remains, then substitute b2=a2−c2b^2=a^2-c^2 to reach the boxed standard form used throughout this section.

Step 1. Isolate one radical: (x+c)2+y2=2a−(x−c)2+y2\sqrt{(x+c)^2+y^2} = 2a-\sqrt{(x-c)^2+y^2}.

Step 2. Square both sides. The left side becomes (x+c)2+y2(x+c)^2+y^2, and the right side becomes 4a2−4a(x−c)2+y2+(x−c)2+y24a^2 - 4a\sqrt{(x-c)^2+y^2} + (x-c)^2+y^2. The terms x2+y2+c2x^2+y^2+c^2 appear on both sides and cancel, along with the ±2cx\pm 2cx terms combining, leaving 4cx−4a2=−4a(x−c)2+y24cx - 4a^2 = -4a\sqrt{(x-c)^2+y^2}, which simplifies to a(x−c)2+y2=a2−cxa\sqrt{(x-c)^2+y^2} = a^2 - cx.

Step 3. Square once more: a2[(x−c)2+y2]=(a2−cx)2a^2\big[(x-c)^2+y^2\big] = (a^2-cx)^2. Expanding both sides gives a2x2−2a2cx+a2c2+a2y2=a4−2a2cx+c2x2a^2x^2 - 2a^2cx + a^2c^2 + a^2y^2 = a^4 - 2a^2cx + c^2x^2. The −2a2cx-2a^2cx terms cancel from each side, leaving a2x2−c2x2+a2y2=a4−a2c2a^2x^2 - c^2x^2 + a^2y^2 = a^4 - a^2c^2, i.e. (a2−c2)x2+a2y2=a2(a2−c2)(a^2-c^2)x^2 + a^2y^2 = a^2(a^2-c^2).

Step 4. Divide both sides by a2(a2−c2)a^2(a^2-c^2) to get x2a2+y2a2−c2=1\dfrac{x^2}{a^2} + \dfrac{y^2}{a^2-c^2} = 1. Since a>ca>c for a genuine ellipse, a2−c2a^2-c^2 is a positive quantity; define b2=a2−c2b^2 = a^2 - c^2 so that b<ab<a.

Step 5. Substituting gives the standard equation x2a2+y2b2=1\boxed{\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1}, and rearranging the definition of b2b^2 gives the key relation used throughout this topic, c2=a2−b2c^2 = a^2 - b^2, i.e. c=a2−b2c=\sqrt{a^2-b^2}.

Worked example

Problem. Find the equation of the ellipse with foci (±4,0)(\pm 4,0) and vertices (±5,0)(\pm 5,0), then verify the sum-of-distances property at a vertex.

Step 1. The vertices are at (±a,0)(\pm a, 0), so a=5a = 5 and a2=25a^2 = 25.

Step 2. The foci are at (±c,0)(\pm c, 0), so c=4c = 4.

Step 3. Using b2=a2−c2=25−16=9b^2 = a^2 - c^2 = 25 - 16 = 9.

Step 4. Substitute a2=25a^2=25 and b2=9b^2=9 into the standard form to get the equation of the ellipse: x225+y29=1\boxed{\dfrac{x^2}{25}+\dfrac{y^2}{9}=1}.

Step 5 (verification). At the vertex (5,0)(5,0), the distance to focus (4,0)(4,0) is 11 and the distance to focus (−4,0)(-4,0) is 99, and their sum is 1+9=10=2a1+9=10=2a, confirming a=5a=5 as required by the defining property.

Competitive stretch

Reverse the labelling: for x216+y225=1\dfrac{x^2}{16}+\dfrac{y^2}{25}=1, compare denominators — 25>1625>16, so the major axis is along the yy-axis, giving a2=25a^2=25, b2=16b^2=16, a=5a=5, b=4b=4, and c=a2−b2=9=3c=\sqrt{a^2-b^2}=\sqrt{9}=3. The foci are at (0,±3)(0,\pm 3) and the vertices at (0,±5)(0,\pm 5), with major axis length 2a=102a=10 and minor axis length 2b=82b=8 — a reminder that aa always names the semi-major axis, whichever coordinate it multiplies.

Common traps

  • Assuming the larger denominator always sits under x2x^2 — it does not; compare the two denominators and call the larger one a2a^2, whichever axis it belongs to.
  • Confusing the ellipse relation c2=a2−b2c^2=a^2-b^2 with the hyperbola's c2=a2+b2c^2=a^2+b^2 — the minus sign here reflects that c<ac<a for a real ellipse.
  • Treating a>b>0a>b>0 as meaning "x2x^2's denominator is bigger" rather than a naming convention for whichever axis is longer.
  • Forgetting to take the positive square root when solving c=a2−b2c=\sqrt{a^2-b^2}, or mixing up which of aa, bb, cc was given in a problem.

Ask the tutor: want to see how this same squaring method changes when the foci are placed on the y-axis instead, or how eccentricity connects back to aa, bb, cc?

Why do we place the foci on the x-axis instead of somewhere general

Placing the foci symmetrically on the xx-axis at (±c,0)(\pm c,0) is purely a convenience of coordinate choice, not a restriction on ellipses in general. Any ellipse can be moved and rotated so its centre sits at the origin and its axes align with the coordinate axes; doing so turns the algebra of the derivation into a manageable sequence of squarings. An ellipse centred elsewhere or tilted would have the same shape but a messier equation, which is why the standard, axis-aligned form is the one CBSE Class 11 focuses on.

How do I quickly tell whether the major axis is along x or y just by looking at the equation

Compare the two denominators in x2p+y2q=1\dfrac{x^2}{p}+\dfrac{y^2}{q}=1. Whichever denominator is larger names a2a^2, and the major axis runs along that variable's axis. If p>qp>q, the major axis is along xx and foci are at (±c,0)(\pm c,0); if q>pq>p, the major axis is along yy and foci are at (0,±c)(0,\pm c). Either way, c=(larger denominator)−(smaller denominator)c=\sqrt{(\text{larger denominator})-(\text{smaller denominator})}.

Is the relation c squared equals a squared minus b squared always true for any ellipse

Yes, for every ellipse in standard position this relation holds, because it comes directly from the substitution b2=a2−c2b^2=a^2-c^2 made during the derivation, and aa is always defined as the semi-major axis while bb is the semi-minor axis. It is worth memorising alongside the standard equation itself, since most problems give you two of aa, bb, cc and expect you to find the third using this exact relation.

Before this

Where this leads