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NDA Maths · Conics

Ellipse — Foci, Eccentricity & Focal Distances

An ellipse is the set of points whose two focal distances add to a constant 2a; its standard form x²/a² + y²/b² = 1 gives the axes, and c² = a² − b² locates the foci and the eccentricity.

Why this matters

The chapter's largest pocket (14 PYQs). Most questions are direct reads — distance between foci, eccentricity, the constant focal sum — or building the equation from given foci/eccentricity/latus rectum. The one judgement call is which axis is major.

Test yourself — a quick 18-question Conics recall quiz, instant score.

Concept 1 of 3: Standard Form, Foci & Eccentricity

Read the standard form to get a and b; the larger denominator sits under the major axis. The foci lie on the major axis a distance c from the centre, where c² = a² − b², and the eccentricity is c/a.

Definition

For x2a2+y2b2=1\dfrac{x^2}{a^2} + \dfrac{y^2}{b^2} = 1 with a>ba > b (major axis along xx):

  • Foci: (±c,0)(\pm c, 0) with c2=a2−b2c^2 = a^2 - b^2; distance between foci =2c= 2c.
  • Eccentricity: e=ca=1−b2a2e = \dfrac{c}{a} = \sqrt{1 - \dfrac{b^2}{a^2}} (0<e<10 < e < 1).
  • Major axis is along the variable with the LARGER denominator. If b>ab > a, swap roles: the major axis is along yy, foci at (0,±c)(0, \pm c).
  • Parametric point: (acos⁡θ, bsin⁡θ)(a\cos\theta,\ b\sin\theta) — eliminate θ\theta with cos⁡2θ+sin⁡2θ=1\cos^2\theta+\sin^2\theta=1 to recover the Cartesian equation, e.g. (3cos⁡θ, 5sin⁡θ)(3\cos\theta,\,5\sin\theta) lies on x29+y225=1\tfrac{x^2}{9}+\tfrac{y^2}{25}=1, major axis along yy.
  • A right angle at a focus — the perpendicularity test: two segments from a focus SS to points P,QP,Q are perpendicular iff SP⃗⋅SQ⃗=0\vec{SP}\cdot\vec{SQ}=0 (equivalently the slopes multiply to −1-1). Standard result: if the ends of the minor axis (0,±b)(0,\pm b) subtend 90°90° at a focus (ae,0)(ae,0), then a2e2−b2=0⇒b=c⇒a2=2b2a^2e^2-b^2=0\Rightarrow b=c\Rightarrow a^2=2b^2, so e=12e=\tfrac{1}{\sqrt2} — two separate PYQs ask for exactly this number. If the ends of the LATUS RECTUM subtend 90°90° at the centre, then b2a=c\tfrac{b^2}{a}=c, giving e2+e−1=0e^2+e-1=0, e=5−12e=\tfrac{\sqrt5-1}{2}.

Foci & eccentricity

c2=a2−b2,e=cac^2 = a^2 - b^2, \qquad e = \dfrac{c}{a}
F₁(−c,0)F₂(c,0)PabPF₁ + PF₂ = 2a · c² = a² − b²

Worked example

Find the eccentricity of x225+y29=1\dfrac{x^2}{25} + \dfrac{y^2}{9} = 1.

The same idea in a real exam question:

NDA · Apr 2022 · Q85Moderate

Example 1 · Conics · Ellipse — Foci, Eccentricity, and Focal Distances

What is the distance between the foci of the ellipse x2+2y2=1x^2+2y^2=1?

Major axis = larger denominator

If the bigger number is under y2y^2, the major axis is vertical and the foci are on the y-axis — and c2=(larger)−(smaller)c^2 = (\text{larger}) - (\text{smaller}) always. Assuming xx is the major axis when b>ab>a puts the foci in the wrong place.

Concept 2 of 3: The Sum of Focal Distances

The ellipse's defining property is that the two distances from any point to the two foci always add to the same value — the length of the major axis, 2a. That single fact answers a whole class of questions without coordinates.

Definition

For any point PP on the ellipse with foci F1,F2F_1, F_2:

PF1+PF2=2a(the major-axis length).PF_1 + PF_2 = 2a \quad (\text{the major-axis length}).

  • This is the locus definition: 'sum of distances from two fixed points is constant'.
  • The latus rectum has length 2b2a\dfrac{2b^2}{a}, with endpoints at (±c,±b2a)\left(\pm c, \pm \tfrac{b^2}{a}\right).
  • Each focal distance on its own: for P(x1,y1)P(x_1,y_1) on the ellipse, PF1=a+ex1PF_1=a+ex_1 and PF2=a−ex1PF_2=a-ex_1 (focus F1F_1 at (−c,0)(-c,0), F2F_2 at (c,0)(c,0)) — from the focus–directrix definition, PF=e×PF=e\times(distance to the directrix x=±a/ex=\pm a/e). They sum to 2a2a as they must, and a question that names ONE focus wants this, not the sum: on x225+y29=1\tfrac{x^2}{25}+\tfrac{y^2}{9}=1 (e=45e=\tfrac45) the point (3,125)(3,\tfrac{12}5) is 5+125=7.45+\tfrac{12}5=7.4 from one focus and 2.62.6 from the other.

Constant focal sum

PF1+PF2=2a,latus rectum=2b2aPF_1 + PF_2 = 2a, \qquad \text{latus rectum} = \dfrac{2b^2}{a}

Worked example

For the ellipse x216+y27=1\dfrac{x^2}{16} + \dfrac{y^2}{7} = 1, what is PF1+PF2PF_1 + PF_2 for any point PP?

The same idea in a real exam question:

NDA · Apr 2019 · Q53Easy

Example 2 · Conics · Ellipse — Foci, Eccentricity, and Focal Distances

The sum of the focal distances of a point on an ellipse is constant and equal to the

Constant focal sum is 2a2a (major axis), not 2b2b

PF1+PF2=2aPF_1 + PF_2 = 2a uses the SEMI-MAJOR axis aa (the larger denominator), giving the full major-axis length. Using 2b2b (the minor axis) or the value aa itself gives the wrong constant. For x216+y27=1\tfrac{x^2}{16}+\tfrac{y^2}{7}=1, a=4a=4, so the sum is 88.

Concept 3 of 3: Building the Ellipse from Given Data

Given foci, eccentricity, latus rectum, or two points, set up the relations among a, b, c and solve. The locus definition (constant focal sum) also lets you build an ellipse from a worded 'sum of distances' setup.

Definition

Translate the given data into equations in a,b,ca, b, c (using c=aec = ae, c2=a2−b2c^2 = a^2 - b^2, latus rectum =2b2/a= 2b^2/a):

  • Vertices and foci given: read aa from the vertices, cc from the foci, then b2=a2−c2b^2 = a^2 - c^2.
  • Two points given: substitute into x2A+y2B=1\tfrac{x^2}{A} + \tfrac{y^2}{B} = 1 and solve the linear system in 1A,1B\tfrac1A, \tfrac1B.
  • Position of a point (x1,y1)(x_1,y_1): inside if x12a2+y12b2<1\tfrac{x_1^2}{a^2}+\tfrac{y_1^2}{b^2} < 1, on if =1=1, outside if >1>1.
  • Area enclosed =πab= \pi a b.

Key relations

c=ae,b2=a2−c2,LR=2b2ac = ae, \quad b^2 = a^2 - c^2, \quad \text{LR} = \dfrac{2b^2}{a}

Worked example

Find the ellipse with vertices (±5,0)(\pm 5, 0) and foci (±3,0)(\pm 3, 0).

The same idea in a real exam question:

NDA · Apr 2018 · Q56Easy

Example 3 · Conics · Ellipse — Foci, Eccentricity, and Focal Distances

What is the equation of the ellipse with vertices (plus/minus 5, 0) and foci at (plus/minus 4, 0)?

Ellipse latus rectum is 2b2a\dfrac{2b^2}{a} — semi-MINOR squared over semi-major

The latus rectum is 2b2a\dfrac{2b^2}{a}: the SMALLER axis squared on top, the LARGER axis on the bottom. Flipping it to 2a2b\dfrac{2a^2}{b} makes it longer than the major axis, which is impossible for an ellipse.

Summary — formulas & gotchas at a glance

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Formulas (3)

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