Ellipse latus rectum

Every ellipse has a favourite chord: the one that passes through a focus and stands perpendicular to the major axis. This is the latus rectum, and it answers a very concrete question — how "wide" is the ellipse right where the foci sit? Unlike the vertices, where the curve is at its widest along the major axis, the latus rectum measures the curve's narrowest cross-section through a focus, and that width turns out to have a remarkably clean formula: 2b2a\dfrac{2b^2}{a}. This section sits inside Conic Sections, Unit III (Coordinate Geometry) of CBSE Class 11 Mathematics, as one of the standard "simple properties" of the ellipse alongside its equation, axes, and eccentricity. You are expected to derive the length, compute it from a given ellipse, and go the other way — recover bb and ee from a known latus rectum. The idea also quietly connects the ellipse's shape to how flattened it is: a longer latus rectum means a rounder ellipse, a shorter one means a more elongated ellipse.

The core insight

The latus rectum is the focal chord perpendicular to the major axis, and for x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 its length is always 2b2a\dfrac{2b^2}{a}, equivalently 2a(1−e2)2a(1-e^2).

The core idea

What the latus rectum is. Take the standard ellipse x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 with a>b>0a>b>0, foci at (±c,0)(\pm c,0) where c=a2−b2c=\sqrt{a^2-b^2}. Draw the vertical line through one focus — say x=cx=c — and mark where it cuts the ellipse. That chord, perpendicular to the major axis and passing through the focus, is the latus rectum. Because the ellipse is symmetric about the xx-axis, this chord is automatically bisected by the axis, and because the ellipse is also symmetric about the yy-axis, the chord through the other focus (−c,0)(-c,0) has exactly the same length.

Why its length depends only on aa and bb. Substituting x=cx=c into the ellipse equation isolates the yy-values at that vertical slice:

c2a2+y2b2=1.\frac{c^2}{a^2}+\frac{y^2}{b^2}=1.

where: aa is the semi-major axis, bb is the semi-minor axis, and c=a2−b2c=\sqrt{a^2-b^2} is the distance from the centre to a focus. Solving for yy and using a2−c2=b2a^2-c^2=b^2 gives y=±b2ay=\pm\dfrac{b^2}{a} (worked in full below), so the two endpoints straddle the axis symmetrically and the chord length is twice that value.

The result, and how to read it. The length of the latus rectum is

L=2b2a.L=\frac{2b^2}{a}.

where: LL is the latus rectum length, b2b^2 the square of the semi-minor axis, aa the semi-major axis. Since b<ab<a for any non-circular ellipse, L=2b2a<2bL=\dfrac{2b^2}{a}<2b — the latus rectum is always shorter than the minor axis, and it always lies strictly between 00 and 2a2a. A more flattened ellipse (larger eccentricity, smaller bb relative to aa) has a shorter latus rectum, matching the intuition that an elongated ellipse pinches in sharply near its foci.

Figure
An ellipse with its major and minor axes marked and the latus rectum drawn as a vertical chord through the right focus, with its two endpoints labelled at height plus or minus b squared over a
Latus rectum: the focal chord perpendicular to the major axis O F(c, 0) F'(-c, 0) (c, b²/a) (c, -b²/a) (a, 0) (-a, 0) (0, b) Length of latus rectum L = 2b²/a

In terms of eccentricity. Since b2=a2(1−e2)b^2=a^2(1-e^2), the same length can be written as

L=2a(1−e2).L=2a(1-e^2).

where: ee is the eccentricity of the ellipse. This form is handy when a problem states ee directly, letting you skip finding b2b^2 first. Because the two latus recta (through each focus) are mirror images across the centre, both share this one value of LL.

How LL tracks the ellipse's shape. Think of ee sweeping from 00 (a circle) toward 11 (an increasingly stretched ellipse) while aa stays fixed. At e=0e=0, L=2a(1−0)=2aL=2a(1-0)=2a, matching the fact that a circle's "latus rectum" through its centre would simply be a diameter. As ee grows, the factor (1−e2)(1-e^2) shrinks, so LL steadily falls — the chord through the focus gets pinched narrower the more elongated the ellipse becomes. This single formula therefore packages two separate facts you already know (the axis lengths and the eccentricity) into one number that tells you, at a glance, how "fat" or "thin" the ellipse is near its foci, which is why textbooks group it with eccentricity as one of the ellipse's basic descriptive properties rather than treating it as an isolated curiosity.

Worked example

Problem. Find the length of the latus rectum of the ellipse x236+y216=1\dfrac{x^2}{36}+\dfrac{y^2}{16}=1, and verify the answer using eccentricity.

Step 1. Identify a2a^2 and b2b^2. The larger denominator sits under x2x^2, so a2=36⇒a=6a^2=36 \Rightarrow a=6, and b2=16b^2=16.

Step 2. Apply the formula. L=2b2a=2×166=326=163L=\dfrac{2b^2}{a}=\dfrac{2\times16}{6}=\dfrac{32}{6}=\dfrac{16}{3}.

Step 3. Cross-check via eccentricity. c2=a2−b2=36−16=20c^2=a^2-b^2=36-16=20, so e2=c2a2=2036=59e^2=\dfrac{c^2}{a^2}=\dfrac{20}{36}=\dfrac{5}{9}. Then 2a(1−e2)=2(6)(1−59)=12×49=489=1632a(1-e^2)=2(6)\left(1-\dfrac{5}{9}\right)=12\times\dfrac{4}{9}=\dfrac{48}{9}=\dfrac{16}{3} — matching Step 2 exactly.

Answer: the latus rectum has length 163\boxed{\dfrac{16}{3}}.

Competitive stretch

An ellipse has a=10a=10 and latus rectum 12.812.8. From 2b210=12.8\dfrac{2b^2}{10}=12.8, b2=64⇒b=8b^2=64 \Rightarrow b=8; then c2=100−64=36⇒c=6c^2=100-64=36 \Rightarrow c=6, giving e=ca=0.6e=\dfrac{c}{a}=0.6. Checking with 2a(1−e2)=20(1−0.36)=20×0.64=12.82a(1-e^2)=20(1-0.36)=20\times0.64=12.8 confirms the values are consistent — a useful two-way habit for exams. Notice the pattern: whenever a problem gives you the latus rectum together with one of aa, bb, cc or ee, it has effectively handed you the whole ellipse, since any two of the five quantities aa, bb, cc, ee, LL pin down the rest through the axis-focus relation c2=a2−b2c^2=a^2-b^2 and the two latus-rectum formulas above.

Derivation ALength of the latus rectum

The goal is to show, starting only from the standard ellipse equation x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1 and the axis-focus relation c2=a2−b2c^2=a^2-b^2, that the chord through a focus (c,0)(c,0) perpendicular to the major axis has endpoints y=±b2ay=\pm\dfrac{b^2}{a} and hence total length 2b2a\dfrac{2b^2}{a}, with no assumption beyond substituting the focus's xx-coordinate into the ellipse equation and simplifying algebraically.

Step 1. Locate the focus. For the ellipse x2a2+y2b2=1\dfrac{x^2}{a^2}+\dfrac{y^2}{b^2}=1, the foci lie at (±c,0)(\pm c,0) with c=a2−b2c=\sqrt{a^2-b^2}. Take the focus F(c,0)F(c,0); the latus rectum through FF is the vertical line x=cx=c intersected with the ellipse.

Step 2. Substitute x=cx=c into the ellipse equation. This gives c2a2+y2b2=1\dfrac{c^2}{a^2}+\dfrac{y^2}{b^2}=1, so y2b2=1−c2a2=a2−c2a2\dfrac{y^2}{b^2}=1-\dfrac{c^2}{a^2}=\dfrac{a^2-c^2}{a^2}.

Step 3. Use the axis-focus relation a2−c2=b2a^2-c^2=b^2 to simplify the right-hand side to b2a2\dfrac{b^2}{a^2}. So y2b2=b2a2\dfrac{y^2}{b^2}=\dfrac{b^2}{a^2}, which gives y2=b4a2y^2=\dfrac{b^4}{a^2} and hence y=±b2ay=\pm\dfrac{b^2}{a}.

Step 4. Read off the endpoints and the length. The latus rectum through F(c,0)F(c,0) meets the ellipse at (c,b2a)\left(c,\dfrac{b^2}{a}\right) and (c,−b2a)\left(c,-\dfrac{b^2}{a}\right), so its length is the distance between these two points, L=2b2aL=\dfrac{2b^2}{a}. By symmetry the same length holds for the focus (−c,0)(-c,0).

Common traps

  • Substituting x=ax=a (the vertex) instead of x=cx=c (the focus) — the latus rectum must pass through a focus, not a vertex.
  • Confusing the ellipse formula 2b2a\dfrac{2b^2}{a} with the visually identical hyperbola formula — same expression, but check which conic's aa and bb you are using.
  • Sign or placement errors in the endpoints — they are (c,±b2a)\left(c,\pm\dfrac{b^2}{a}\right), not ±a2b\pm\dfrac{a^2}{b} or ±ba\pm\dfrac{b}{a}.
  • Re-deriving b2b^2 from scratch when eccentricity is given directly, instead of using the shortcut L=2a(1−e2)L=2a(1-e^2).
  • Misreading which denominator is a2a^2 and which is b2b^2 when the equation is not already in the form a>ba>b — always compare the two denominators first; the larger one is a2a^2.

Ask the tutor: if you want to see step by step why substituting x=cx=c into the ellipse equation lands exactly on y=±b2/ay=\pm b^2/a, or how to switch quickly between the bb-based and eccentricity-based forms, ask the AI tutor to walk through it with you.

Why is the latus rectum always shorter than the minor axis

Because L=2b2aL=\dfrac{2b^2}{a} and b<ab<a for any non-circular ellipse, multiplying both sides by ba<1\dfrac{b}{a}<1 shows 2b2a<2b\dfrac{2b^2}{a}<2b, the full minor-axis length. Geometrically, the latus rectum is measured at the focus, which sits strictly between the centre and a vertex, so the ellipse has already started narrowing there compared to its widest point along the minor axis at the centre.

Does the ellipse have one latus rectum or two

Two — one through each focus, at x=cx=c and x=−cx=-c. They have identical length 2b2a\dfrac{2b^2}{a} because the ellipse is symmetric about the centre, but their endpoints are mirror images of each other, not the same points. When a question just says "the latus rectum" without specifying a focus, it usually wants the length, which is the same either way.

How do I quickly tell whether to use 2b squared over a or 2a times 1 minus e squared

Both give the identical number, so use whichever quantities the problem hands you directly. If aa and bb are given (or easily read off the equation), use 2b2a\dfrac{2b^2}{a}. If instead aa and the eccentricity ee are given, use 2a(1−e2)2a(1-e^2) to avoid the extra step of computing b2=a2(1−e2)b^2=a^2(1-e^2) first. Both forms are worth memorising together since problems mix them freely, and a quick way to remember the link is that they must agree — if your two computations of LL disagree, you have made an arithmetic slip somewhere and should recheck c2=a2−b2c^2=a^2-b^2. The formula itself is unchanged even if the major axis is vertical (equation x2b2+y2a2=1\dfrac{x^2}{b^2}+\dfrac{y^2}{a^2}=1 with a>ba>b); only the direction of the chord changes, since aa and bb are always defined by size, not by which axis they sit on.

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