Conic Sections

Slice a cone with a plane and, depending only on the angle of the cut, you get a circle, an ellipse, a parabola, or a hyperbola — four curves that look wildly different on paper but are secretly one family, born from the same solid. The ancient Greek geometer Apollonius named two of them, parabola and hyperbola, more than two thousand years ago, and the family has never lost its usefulness: planets trace ellipses around the Sun, thrown balls and reflector dishes trace parabolas, and antennas and flashlight mirrors are shaped from these same curves. This chapter builds each curve from a clean point-set definition rather than from cutting cones, then hunts for the simplest possible equation in Cartesian coordinates. The method is the same every time. Fix one or two special points, a focus or a pair of foci, and sometimes a line, a directrix. Describe the curve as the set of points obeying one geometric rule about distances to those points. Place the coordinate axes cleverly so the algebra collapses to something short, and derive the equation using nothing more than the distance formula and patient squaring. A circle is the set of points at a fixed distance from a centre. A parabola balances distance to a point against distance to a line. An ellipse fixes the sum of two distances; a hyperbola fixes their difference. Four definitions, four short derivations, four standard equations, and one number, the eccentricity, that secretly measures how un-circular each curve is. By the end you should be able to go in either direction: given a geometric description such as a focus, a vertex, a directrix, or an eccentricity, write down the equation, and given an equation, read off every geometric feature, the centre, foci, vertices, axes, eccentricity and latus rectum, at a glance. That two-way fluency is exactly what CBSE boards and JEE or NEET test, often within the same question.

Key takeaways
  • A conic section is the curve formed when a plane cuts a double napped right circular cone; the angle of the cut determines whether the section is a circle, ellipse, parabola or hyperbola.
  • A circle is the set of points at a fixed distance r, the radius, from a fixed centre (h, k); its equation is (x−h)2+(y−k)2=r2(x-h)^2+(y-k)^2=r^2.
  • A parabola is the set of points equidistant from a fixed focus and a fixed directrix; the standard form y2=4axy^2=4ax has focus (a,0)(a,0), directrix x=−ax=-a, and latus rectum of length 4a4a.
  • An ellipse is the set of points whose distances from two foci add to a constant 2a2a; the standard form x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1 (with a>ba\gt b) satisfies a2=b2+c2a^2=b^2+c^2, eccentricity e=c/a<1e=c/a\lt 1.
  • A hyperbola is the set of points whose distances from two foci differ by a constant 2a2a; the standard form x2a2−y2b2=1\frac{x^2}{a^2}-\frac{y^2}{b^2}=1 satisfies b2=c2−a2b^2=c^2-a^2, eccentricity e=c/a>1e=c/a\gt 1.
  • Latus rectum length is 4a4a for a parabola but 2b2/a2b^2/a for both the ellipse and the hyperbola, a formula pair students frequently mix up.
  • Eccentricity is the single number that classifies every conic: e=0e=0 is a circle (the limiting ellipse), 0<e<10\lt e\lt 1 an ellipse, e=1e=1 a parabola, e>1e\gt 1 a hyperbola.
  • When the intersecting plane passes through the vertex of the cone, the section degenerates to a point, a straight line, or a pair of intersecting lines.
  • Which axis of an ellipse is the major axis is decided by comparing the two denominators, never by which variable is squared first.
  • Key idea: every conic section is the locus of points satisfying one distance rule about a focus (or foci) and, for the parabola, a directrix, and placing the coordinate axes along the curve's own symmetry turns that geometric rule into one of four short standard equations.
The core insight

A conic section is the locus of points obeying a single distance rule involving a focus (or a pair of foci) and, for the parabola, a directrix; choosing axes along the curve's symmetry turns that rule into one of exactly four standard algebraic equations, distinguished by the eccentricity e=0e=0, 0<e<10\lt e\lt 1, e=1e=1 and e>1e\gt 1 for the circle, ellipse, parabola and hyperbola respectively.

What this chapter covers

This chapter opens with conic sections as slices of a cone: the vertex, axis and generators of a double napped cone, the angle conditions that produce a circle, ellipse, parabola or hyperbola, and the degenerate cases when the cutting plane passes through the vertex. It then treats each curve in turn purely as a locus in the plane, with no cones required. The circle is defined by a fixed distance from a centre. The parabola is defined by equal distances to a focus and a directrix, giving four standard orientations and the latus rectum. The ellipse and hyperbola are defined by a fixed sum, respectively difference, of distances to two foci, each with its own standard equation, eccentricity, and latus rectum. Three full derivations rebuild the standard equations from their locus definitions, three worked examples show the geometry-to-equation and equation-to-geometry conversions in both directions, and the chapter closes with eccentricity as the single number that unifies all four curves.

The core ideas

Conic sections as slices of a cone

Take a fixed vertical line ll and a second line mm that meets it at a fixed point VV, inclined to it at a constant angle α\alpha. Rotating mm about ll while keeping α\alpha fixed sweeps out a double napped right circular cone: VV is the vertex, ll is the axis, mm in any of its positions is a generator, and the vertex separates the surface into two nappes extending indefinitely in both directions. A conic section is simply the curve obtained by intersecting this cone with a plane, and which curve you get depends only on the angle β\beta that the plane makes with the axis. When the plane cuts a nappe away from the vertex, four things can happen. If β=90∘\beta=90^\circ the plane is perpendicular to the axis and the section is a circle. If α<β<90∘\alpha\lt \beta\lt 90^\circ the section is an ellipse. If β=α\beta=\alpha, so the plane is parallel to a generator, the section is a parabola. If 0≤β<α0\le\beta\lt \alpha the plane is steep enough to cut through both nappes, and the section is a hyperbola, appearing as two separate branches. If instead the plane passes through the vertex itself, the same four angle ranges give degenerate conics: a single point (when α<β≤90∘\alpha\lt \beta\le90^\circ), a single straight line lying along a generator (when β=α\beta=\alpha, the degenerate parabola), or a pair of intersecting straight lines (when 0≤β<α0\le\beta\lt \alpha, the degenerate hyperbola).

Figure
Four schematic double napped cones each sliced by a plane at a different angle producing a circle an ellipse a parabola and a hyperbola with the vertex V and axis l marked in every panel
The four conics as plane sections of a double napped cone V V V V circle beta = 90 degrees ellipse alpha less than beta less than 90 parabola beta equals alpha hyperbola beta less than alpha both nappes If the plane passes through the vertex V itself, the section degenerates to a point, a line, or a pair of intersecting lines. alpha is the half angle of the cone between axis l and any generator m; beta is the angle the cutting plane makes with axis l.

The circle

A circle is the set of all points in a plane equidistant from a fixed point. The fixed point is the centre and the constant distance is the radius rr. If the centre is C(h,k)C(h,k) and P(x,y)P(x,y) is any point on the circle, the defining condition ∣CP∣=r|CP|=r becomes, by the distance formula, the standard equation

(x−h)2+(y−k)2=r2.(1)(x-h)^2+(y-k)^2=r^2. \qquad (1)

where: (h,k)(h,k) is the centre and r>0r\gt 0 is the radius; when the centre is the origin this collapses to the simplest form x2+y2=r2x^2+y^2=r^2. Expanding equation (1) always produces a general equation of the form x2+y2+2gx+2fy+c=0x^2+y^2+2gx+2fy+c=0, and reversing that expansion by completing the square recovers centre (−g,−f)(-g,-f) and radius r=g2+f2−cr=\sqrt{g^2+f^2-c}, which is real only when g2+f2−c≥0g^2+f^2-c\ge0. This general form is how a circle usually appears disguised in a problem, and completing the square is always the way back to equation (1).

The parabola

A parabola is the set of all points in a plane equidistant from a fixed line, the directrix, and a fixed point not on that line, the focus. The line through the focus perpendicular to the directrix is the axis of the parabola, and the point where the parabola meets its axis is the vertex. Placing the vertex at the origin with the focus at (a,0)(a,0), a>0a\gt 0, and the directrix as the line x=−ax=-a gives the simplest orientation, whose equation is derived in full below:

y2=4ax.(2)y^2=4ax. \qquad (2)

where: a>0a\gt 0 is the distance from vertex to focus, equal to half the distance from focus to directrix. The three remaining orientations follow from reflecting this construction: y2=−4axy^2=-4ax opens to the left with focus (−a,0)(-a,0) and directrix x=ax=a; x2=4ayx^2=4ay opens upward with focus (0,a)(0,a) and directrix y=−ay=-a; x2=−4ayx^2=-4ay opens downward with focus (0,−a)(0,-a) and directrix y=ay=a. In every case, whichever variable appears squared fixes the axis of symmetry (a y2y^2 term means the axis is the x-axis, an x2x^2 term means the axis is the y-axis), and the sign of the linear term fixes the direction the curve opens. The latus rectum is the chord through the focus perpendicular to the axis, with endpoints on the curve; substituting x=ax=a into equation (2) gives y=±2ay=\pm2a, so the length of the latus rectum is 4a4a.

The ellipse

An ellipse is the set of all points in a plane the sum of whose distances from two fixed points, the foci, is a constant. The midpoint of the segment joining the foci is the centre; the line through the foci is the major axis, and the perpendicular line through the centre is the minor axis. Writing the length of the major axis as 2a2a, the minor axis as 2b2b, and the distance between the foci as 2c2c, a point PP at the end of the major axis gives sum of distances (c+a)+(a−c)=2a(c+a)+(a-c)=2a, while a point QQ at the end of the minor axis gives sum of distances 2b2+c22\sqrt{b^2+c^2}; equating these two expressions for the same constant, 2b2+c2=2a2\sqrt{b^2+c^2}=2a, yields the fundamental relation of the ellipse:

a2=b2+c2,soc=a2−b2.(3)a^2=b^2+c^2, \qquad\text{so}\qquad c=\sqrt{a^2-b^2}. \qquad (3)

where: aa is the semi-major axis, bb the semi-minor axis, and cc the centre-to-focus distance, with aa always the largest of the three. Placing the centre at the origin with foci on the x-axis at (±c,0)(\pm c,0) gives the standard equation, derived in full below,

x2a2+y2b2=1,a>b>0.(4)\frac{x^2}{a^2}+\frac{y^2}{b^2}=1, \qquad a\gt b\gt 0. \qquad (4)

where: the major axis lies along whichever coordinate axis carries the larger denominator, regardless of whether that denominator sits under x2x^2 or y2y^2; swapping the roles of a2a^2 and b2b^2 gives the equation x2b2+y2a2=1\frac{x^2}{b^2}+\frac{y^2}{a^2}=1 for foci on the y-axis. The eccentricity is e=c/ae=c/a, always strictly between 00 and 11 because a>ca\gt c, and the latus rectum, the focal chord perpendicular to the major axis, has length 2b2/a2b^2/a.

The hyperbola

A hyperbola is the set of all points in a plane the difference of whose distances from two fixed foci is a constant, where difference always means the farther distance minus the nearer one. The line through the foci is the transverse axis and the perpendicular line through the centre is the conjugate axis; the curve meets the transverse axis at two vertices, a distance 2a2a apart, while the foci are a distance 2c2c apart with c>ac\gt a. Unlike the ellipse, the defining quantity bb is introduced by the opposite subtraction,

b2=c2−a2.(5)b^2=c^2-a^2. \qquad (5)

where: 2b2b is the length of the conjugate axis, and because c>ac\gt a always, b2b^2 is automatically positive with no restriction relating bb to aa; a hyperbola with a=ba=b is called equilateral, with eccentricity e=2e=\sqrt2. With foci on the x-axis at (±c,0)(\pm c,0), the standard equation, derived in full below, is

x2a2−y2b2=1.(6)\frac{x^2}{a^2}-\frac{y^2}{b^2}=1. \qquad (6)

where: the transverse axis lies along whichever coordinate axis carries the positive squared term; the mirror form y2a2−x2b2=1\frac{y^2}{a^2}-\frac{x^2}{b^2}=1 has its transverse axis on the y-axis. Because x2/a2=1+y2/b2≥1x^2/a^2=1+y^2/b^2\ge1, every point satisfies x≤−ax\le-a or x≥ax\ge a, so the curve never enters the strip between the lines x=−ax=-a and x=ax=a. The eccentricity e=c/ae=c/a is always strictly greater than 11, and the latus rectum again has length 2b2/a2b^2/a.

Eccentricity: one number that classifies every conic

Eccentricity is the ratio ee of the distance from the centre to a focus and the distance from the centre to a vertex, and for the parabola, ellipse and hyperbola it also equals the constant ratio of a point's distance from the focus to its distance from the corresponding directrix, SP=e⋅PMSP=e\cdot PM. As ee increases from 00, the family of conics sweeps through every shape: e=0e=0 is the circle, the limiting case of an ellipse in which the two foci merge into a single centre and a=b=ra=b=r (its directrix having receded to infinity); 0<e<10\lt e\lt 1 gives every ellipse in between; e=1e=1 is exactly the parabola, the balance point where distance to focus equals distance to directrix outright; and e>1e\gt 1 gives every hyperbola, growing ever flatter and more open as ee increases further. This one number is the fastest way to identify a conic without even solving for its other features.

Figure
An ellipse with semi major axis five semi minor axis three and foci at plus or minus four on the x axis showing the vertices the minor axis endpoints a focal chord latus rectum and a point P whose distances to the two foci sum to ten
Anatomy of the ellipse x squared over 25 plus y squared over 9 equals 1 F1 (-4, 0) F2 (4, 0) A (-5, 0) A prime (5, 0) B (0, 3) B prime (0, -3) O P PF1 + PF2 = 2a = 10 latus rectum = 2b squared over a = 18 / 5 a = 5 b = 3 c = 4 eccentricity e = c / a = 4 / 5
Figure
Four standard parabolas in a two by two grid opening right left up and down each showing the vertex the focus the directrix and its equation
The four standard orientations of a parabola F (a, 0) directrix x = -a V y squared = 4ax, opens right F (-a, 0) directrix x = a V y squared = -4ax, opens left F (0, a) directrix y = -a V x squared = 4ay, opens up F (0, -a) directrix y = a V x squared = -4ay, opens down
Derivation AStandard equation of a parabola

The goal here is to convert the pure geometric definition of a parabola, equal distance from a fixed focus and a fixed directrix, into a Cartesian equation, and to do it in the coordinate system that makes the algebra shortest: axes chosen along the parabola's own axis of symmetry rather than left in some arbitrary orientation. We derive the case with focus to the right of the origin and directrix to the left, then read off the other three orientations by symmetry without repeating the algebra.

Step 1. Set up coordinates. Let FF be the focus and ll the directrix, and let MM be the foot of the perpendicular from FF to ll. Let OO bisect FMFM; by the very definition of the parabola, OO is equidistant from FF and ll, so OO itself lies on the curve and is its vertex. Take OO as the origin, the ray OFOF as the positive x-axis, and the perpendicular through OO as the y-axis. If the distance from directrix to focus is taken as 2a2a, the focus is F(a,0)F(a,0) and the directrix is the line x=−ax=-a.

Step 2. Translate the defining rule into distances. Let P(x,y)P(x,y) be any point on the parabola and let BB be the foot of the perpendicular from PP to the directrix, so B=(−a,y)B=(-a,y). The defining property is PF=PBPF=PB. By the distance formula, PF=(x−a)2+y2PF=\sqrt{(x-a)^2+y^2} and PB=(x+a)2PB=\sqrt{(x+a)^2}.

Step 3. Square and simplify. Setting PF=PBPF=PB and squaring both sides removes the radicals: (x−a)2+y2=(x+a)2(x-a)^2+y^2=(x+a)^2. Expanding, x2−2ax+a2+y2=x2+2ax+a2x^2-2ax+a^2+y^2=x^2+2ax+a^2, and the x2x^2 and a2a^2 terms cancel from both sides, leaving y2=4axy^2=4ax, with a>0a\gt 0. Every point on the parabola therefore satisfies this equation.

Step 4. Confirm the converse. For the equation to describe exactly the same set of points as the geometric definition, any point satisfying y2=4axy^2=4ax must also satisfy PF=PBPF=PB. Substituting y2=4axy^2=4ax into PFPF gives PF=(x−a)2+4ax=x2+2ax+a2=(x+a)2=PBPF=\sqrt{(x-a)^2+4ax}=\sqrt{x^2+2ax+a^2}=\sqrt{(x+a)^2}=PB, since x≥0x\ge0 for points on the curve, making x+a>0x+a\gt 0. So the equation and the geometric definition describe exactly the same locus, and y2=4axy^2=4ax is the standard equation of the parabola with vertex at the origin, focus (a,0)(a,0), and directrix x=−ax=-a. Reflecting the construction across the axes or exchanging the roles of xx and yy gives, without repeating the algebra, the other three standard forms y2=−4axy^2=-4ax, x2=4ayx^2=4ay and x2=−4ayx^2=-4ay. Verified: substituting x=y2/4ax=y^2/4a back into PF−PBPF-PB gives zero identically, and setting x=ax=a in y2=4axy^2=4ax gives the latus-rectum endpoints y=±2ay=\pm2a, a chord of length 4a4a, matching the definition of the latus rectum as the focal chord perpendicular to the axis.

Go deeper · Derivation B · 2 minStandard equation of an ellipse
Derivation BStandard equation of an ellipse

The task is to convert the two-focus, sum-of-distances definition of an ellipse into a Cartesian equation, again by choosing axes along the curve's own symmetry so the two square roots that the distance formula produces can be cleared systematically. The derivation needs two rounds of squaring, because two separate radicals appear, and the whole trick is organising the algebra so each squaring removes exactly one radical rather than tangling both together.

Step 1. Set up coordinates and the defining sum. Let F1F_1 and F2F_2 be the foci and OO their midpoint. Take OO as the origin and the ray from OO through F2F_2 as the positive x-axis, so F1=(−c,0)F_1=(-c,0) and F2=(c,0)F_2=(c,0). Let P(x,y)P(x,y) be a point on the ellipse with PF1+PF2=2aPF_1+PF_2=2a, a fixed constant greater than 2c2c.

Step 2. Write the distances and isolate one radical. By the distance formula, (x+c)2+y2+(x−c)2+y2=2a\sqrt{(x+c)^2+y^2}+\sqrt{(x-c)^2+y^2}=2a. Moving the second radical to the right gives (x+c)2+y2=2a−(x−c)2+y2\sqrt{(x+c)^2+y^2}=2a-\sqrt{(x-c)^2+y^2}, ready for the first squaring.

Step 3. Square once. Squaring both sides gives (x+c)2+y2=4a2−4a(x−c)2+y2+(x−c)2+y2(x+c)^2+y^2=4a^2-4a\sqrt{(x-c)^2+y^2}+(x-c)^2+y^2. The y2y^2 terms cancel, and since (x+c)2−(x−c)2=4cx(x+c)^2-(x-c)^2=4cx, collecting terms and dividing by 4a4a reduces this to a single remaining radical: (x−c)2+y2=a−cax\sqrt{(x-c)^2+y^2}=a-\frac{c}{a}x.

Step 4. Square again and use c2=a2−b2c^2=a^2-b^2. Squaring once more, (x−c)2+y2=a2−2cx+c2a2x2(x-c)^2+y^2=a^2-2cx+\frac{c^2}{a^2}x^2. Expanding the left side and cancelling the common −2cx-2cx term from both sides, then multiplying through by a2a^2 and collecting the x2x^2 terms, leaves x2(a2−c2)+a2y2=a2(a2−c2)x^2(a^2-c^2)+a^2y^2=a^2(a^2-c^2). Writing b2=a2−c2b^2=a^2-c^2, a positive quantity because 2a>2c2a\gt 2c, and dividing throughout by a2b2a^2b^2 gives x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1.

Step 5. Confirm the converse. Substituting back, a point satisfying x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1 gives PF1=a+caxPF_1=a+\frac{c}{a}x and PF2=a−caxPF_2=a-\frac{c}{a}x, each obtained by the same simplification using b2=a2−c2b^2=a^2-c^2 inside the square root. Adding these two expressions cancels the cax\frac{c}{a}x terms exactly, returning PF1+PF2=2aPF_1+PF_2=2a. The two-way equivalence therefore holds, and x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1, with a>b>0a\gt b\gt 0 and c2=a2−b2c^2=a^2-b^2, is the standard equation of the ellipse with foci (±c,0)(\pm c,0). The mirror construction with foci on the y-axis gives x2b2+y2a2=1\frac{x^2}{b^2}+\frac{y^2}{a^2}=1 by exactly the same steps with xx and yy exchanged. Verified: adding the back-substituted PF1PF_1 and PF2PF_2 gives exactly 2a2a with no leftover terms, and setting x=cx=c recovers the latus-rectum half-length l=b2/al=b^2/a, matching the length 2b2/a2b^2/a derived independently in the core-ideas section.

Go deeper · Derivation C · 2 minStandard equation of a hyperbola
Derivation CStandard equation of a hyperbola

The goal is to run the same distance-formula method used for the ellipse, but now with a difference of distances fixed instead of a sum, and to show precisely where the algebra forks away from the ellipse case, producing the opposite sign in front of y2y^2 and the opposite relation between aa, bb and cc. As with the ellipse, two squarings are needed to clear two radicals in turn.

Step 1. Set up coordinates and the defining difference. With foci F1(−c,0)F_1(-c,0) and F2(c,0)F_2(c,0) as before, let P(x,y)P(x,y) be a point on the branch nearer F2F_2, satisfying PF1−PF2=2aPF_1-PF_2=2a (the farther distance minus the nearer one).

Step 2. Write the distances and isolate one radical. (x+c)2+y2−(x−c)2+y2=2a\sqrt{(x+c)^2+y^2}-\sqrt{(x-c)^2+y^2}=2a, so (x+c)2+y2=2a+(x−c)2+y2\sqrt{(x+c)^2+y^2}=2a+\sqrt{(x-c)^2+y^2}.

Step 3. Square once. (x+c)2+y2=4a2+4a(x−c)2+y2+(x−c)2+y2(x+c)^2+y^2=4a^2+4a\sqrt{(x-c)^2+y^2}+(x-c)^2+y^2. As before, the y2y^2 terms cancel and (x+c)2−(x−c)2=4cx(x+c)^2-(x-c)^2=4cx; collecting terms and dividing by 4a4a gives (x−c)2+y2=cax−a\sqrt{(x-c)^2+y^2}=\frac{c}{a}x-a, the same shape as the ellipse's Step 3 but with the sign of aa flipped.

Step 4. Square again and use b2=c2−a2b^2=c^2-a^2. Squaring gives (x−c)2+y2=c2a2x2−2cx+a2(x-c)^2+y^2=\frac{c^2}{a^2}x^2-2cx+a^2. Expanding the left side and cancelling the common −2cx-2cx term, then multiplying through by a2a^2 and collecting the x2x^2 terms, leaves x2(c2−a2)−a2y2=a2(c2−a2)x^2(c^2-a^2)-a^2y^2=a^2(c^2-a^2). Writing b2=c2−a2b^2=c^2-a^2, positive since c>ac\gt a for a hyperbola, and dividing by a2b2a^2b^2 gives x2a2−y2b2=1\frac{x^2}{a^2}-\frac{y^2}{b^2}=1.

Step 5. Confirm the converse and note the sign flip against the ellipse. Back-substitution gives PF1=a+caxPF_1=a+\frac{c}{a}x and PF2=cax−aPF_2=\frac{c}{a}x-a for points with x≥ax\ge a, so PF1−PF2=2aPF_1-PF_2=2a exactly; a symmetric argument on the branch with x≤−ax\le-a gives PF2−PF1=2aPF_2-PF_1=2a, matching the farther-minus-nearer convention on that branch too. So x2a2−y2b2=1\frac{x^2}{a^2}-\frac{y^2}{b^2}=1, with b2=c2−a2b^2=c^2-a^2, is the standard hyperbola with foci (±c,0)(\pm c,0). Contrast this directly with the ellipse: there b2=a2−c2b^2=a^2-c^2, subtracting the focal distance from the semi-major axis, while here b2=c2−a2b^2=c^2-a^2, subtracting the semi-transverse axis from the focal distance. That reversal is exactly why the two curves look so different, and why the ellipse's bb is always smaller than aa while the hyperbola's bb carries no such restriction at all. Verified: on the branch x≥ax\ge a, PF1−PF2=(a+cax)−(cax−a)=2aPF_1-PF_2=\left(a+\frac{c}{a}x\right)-\left(\frac{c}{a}x-a\right)=2a identically, independent of xx, and setting x=cx=c recovers the latus-rectum half-length b2/ab^2/a, matching 2b2/a2b^2/a used in the core-ideas section.

Worked examples

Board level - centre and radius of a circle from the general equation

Find the centre and radius of the circle x2+y2+8x+10y−8=0x^2+y^2+8x+10y-8=0, and verify using the general-form shortcut.

Step 1. Group and complete the square. Rewrite as (x2+8x)+(y2+10y)=8(x^2+8x)+(y^2+10y)=8. Completing the square in each bracket, (x2+8x+16)+(y2+10y+25)=8+16+25(x^2+8x+16)+(y^2+10y+25)=8+16+25, which is (x+4)2+(y+5)2=49(x+4)^2+(y+5)^2=49.

Step 2. Read off the centre and radius. Comparing with (x−h)2+(y−k)2=r2(x-h)^2+(y-k)^2=r^2, written as {x−(−4)}2+{y−(−5)}2=72\{x-(-4)\}^2+\{y-(-5)\}^2=7^2, the centre is (−4,−5)(-4,-5) and the radius is 77.

Step 3. Cross-check with the general-form shortcut. Matching x2+y2+2gx+2fy+c=0x^2+y^2+2gx+2fy+c=0 to the given equation gives 2g=82g=8 so g=4g=4, 2f=102f=10 so f=5f=5, and c=−8c=-8. The shortcut formulas centre =(−g,−f)=(-g,-f) and radius =g2+f2−c=\sqrt{g^2+f^2-c} give centre (−4,−5)(-4,-5) and radius 16+25+8=49=7\sqrt{16+25+8}=\sqrt{49}=7, matching Step 2 exactly. Answer: centre (−4,−5)(-4,-5), radius 77.

Board level - foci, vertices, axes, eccentricity and latus rectum of an ellipse

For the ellipse x225+y29=1\frac{x^2}{25}+\frac{y^2}{9}=1, find the coordinates of the foci and vertices, the lengths of the major and minor axes, the eccentricity, and the length of the latus rectum.

Step 1. Identify the major axis. The denominator under x2x^2 is 2525 and under y2y^2 is 99; since 25>925\gt 9, the major axis lies along the x-axis, so the standard form is x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1 with a2=25a^2=25, b2=9b^2=9, that is a=5a=5, b=3b=3.

Step 2. Find cc from a2=b2+c2a^2=b^2+c^2. c=a2−b2=25−9=16=4c=\sqrt{a^2-b^2}=\sqrt{25-9}=\sqrt{16}=4. The foci are (±4,0)(\pm4,0) and the vertices are (±5,0)(\pm5,0).

Step 3. Compute the remaining quantities. Length of major axis =2a=10=2a=10; length of minor axis =2b=6=2b=6; eccentricity e=c/a=4/5=0.8e=c/a=4/5=0.8; latus rectum =2b2/a=2(9)/5=18/5=3.6=2b^2/a=2(9)/5=18/5=3.6. Answer: foci (±4,0)(\pm4,0), vertices (±5,0)(\pm5,0), major axis 1010, minor axis 66, e=4/5e=4/5, latus rectum =18/5=18/5.

Competitive level (JEE / NEET) - hyperbola from foci and latus rectum, with an extraneous root

A hyperbola has its foci on the y-axis at (0,±12)(0,\pm12), and the length of its latus rectum is 3636. Find its equation.

Step 1. Translate the data. Foci on the y-axis at (0,±c)(0,\pm c) means c=12c=12 and the standard form is y2a2−x2b2=1\frac{y^2}{a^2}-\frac{x^2}{b^2}=1. The latus rectum formula 2b2/a=362b^2/a=36 gives b2=18ab^2=18a.

Step 2. Substitute into c2=a2+b2c^2=a^2+b^2. 144=a2+18a144=a^2+18a, that is a2+18a−144=0a^2+18a-144=0, a quadratic in aa. Solving with the quadratic formula, a=−18±324+5762=−18±9002=−18±302a=\frac{-18\pm\sqrt{324+576}}{2}=\frac{-18\pm\sqrt{900}}{2}=\frac{-18\pm30}{2}, giving a=6a=6 or a=−24a=-24.

Step 3. Reject the impossible root and finish. A length aa must be positive, so a=−24a=-24 is rejected outright; a common JEE trap is carrying both roots through to the final equation instead of discarding the negative one immediately. Taking a=6a=6 gives b2=18(6)=108b^2=18(6)=108. Answer: the equation is y236−x2108=1\frac{y^2}{36}-\frac{x^2}{108}=1, equivalently 3y2−x2=1083y^2-x^2=108. Timing note: this should take under two minutes once the latus rectum formula is remembered correctly as 2b2/a2b^2/a, not 2a2/b2a^2/b, because everything after that is one substitution and one quadratic. The real trap is arithmetic and sign discipline in the quadratic formula, plus the discipline to discard the negative root for aa on sight rather than plugging both roots back into the original relation to check.

Common traps

  • Deciding the major axis of an ellipse by which variable "comes first" instead of comparing denominators: whichever denominator is larger fixes the major axis, regardless of whether it sits under x2x^2 or y2y^2.
  • Swapping the sign convention in b2b^2 between the ellipse and the hyperbola: for an ellipse b2=a2−c2b^2=a^2-c^2, so b<ab\lt a always, but for a hyperbola b2=c2−a2b^2=c^2-a^2, so bb can be anything positive; using the wrong subtraction order gives an impossible negative square.
  • Using the parabola's latus rectum formula 4a4a for an ellipse or hyperbola, or vice versa; the correct formula for the ellipse and hyperbola alike is 2b2/a2b^2/a.
  • Forgetting the sign of the directrix relative to the focus: for y2=4axy^2=4ax opening right with focus (a,0)(a,0), a>0a\gt 0, the directrix is the line x=−ax=-a, not x=ax=a.
  • Assuming eccentricity can never exceed 11: that is true only for the ellipse (0<e<10\lt e\lt 1); a hyperbola always has e>1e\gt 1, and treating a hyperbola's ee as though it must be a proper fraction is a common slip.
  • Getting the sign of the centre backward when converting a circle's general equation x2+y2+2gx+2fy+c=0x^2+y^2+2gx+2fy+c=0 to centre-radius form: the centre is (−g,−f)(-g,-f), not (g,f)(g,f).
  • Treating the hyperbola's "difference of distances" as a signed subtraction rather than farther-minus-nearer, which can lead to a negative constant on one branch if the order is not fixed carefully.
  • Reporting r2r^2, a2a^2, b2b^2 or c2c^2 as though they were rr, aa, bb or cc themselves when substituting into eccentricity or latus rectum formulas, instead of taking the square root first.

You should be able to…

  • State the point-set definition of a circle, parabola, ellipse and hyperbola, and explain how each follows from slicing a cone at a particular angle.
  • Derive the standard equation of a parabola, ellipse or hyperbola from its focus-distance definition, including checking that the converse holds.
  • Identify, from a standard equation, the centre, foci, vertices, axes, eccentricity and latus rectum of any of the four conics.
  • Correctly apply a2=b2+c2a^2=b^2+c^2 for an ellipse and b2=c2−a2b^2=c^2-a^2 for a hyperbola without mixing up the direction of the subtraction.
  • Determine the orientation of a parabola, ellipse or hyperbola, which axis it opens along or lies on, from the signs and relative sizes in its equation.
  • Convert a circle's general equation x2+y2+2gx+2fy+c=0x^2+y^2+2gx+2fy+c=0 into centre-radius form by completing the square.
  • Compute the latus rectum of any conic and know when to use 4a4a versus 2b2/a2b^2/a.
  • Set up and solve for an unknown conic's equation given geometric data such as foci, vertices, eccentricity or latus rectum length, discarding extraneous roots.
  • Explain the unifying role of eccentricity across all four conics, including the circle and the parabola as limiting and boundary cases.

Ask the tutor: Want to work through converting a messy general-form conic equation into standard form step by step, or practice a JEE-style problem that mixes two conics in one question?

Why is the rule for the major axis of an ellipse based on the size of the denominator and not on whether x squared or y squared appears first?

Because the standard forms are written so that aa is always the semi-major axis and bb the semi-minor axis, and aa is always the larger of the two. If you see x225+y29=1\frac{x^2}{25}+\frac{y^2}{9}=1, the larger denominator, 2525, sits under x2x^2, so a2=25a^2=25 and the major axis is along the x-axis; if instead you saw x29+y225=1\frac{x^2}{9}+\frac{y^2}{25}=1, the larger denominator now sits under y2y^2, so a2=25a^2=25 and the major axis is along the y-axis, even though the equation looks like the same shape at a glance. The position of the letters xx and yy tells you nothing about which axis is major; only comparing the two denominators does. This is exactly the observation NCERT itself flags, and examiners exploit it deliberately.

Why does an ellipse always have eccentricity less than 1 while a hyperbola always has eccentricity greater than 1?

Eccentricity is defined the same way for both, e=c/ae=c/a, but what cc and aa mean relative to each other differs. In an ellipse, the sum of the two focal distances is fixed at 2a2a, and by the triangle inequality that sum must exceed the distance 2c2c between the foci, so a>ca\gt c and e=c/a<1e=c/a\lt 1. In a hyperbola, the difference of the two focal distances is fixed at 2a2a, and the geometry works the opposite way: the foci sit outside the curve, farther from the centre than any vertex, forcing c>ac\gt a and hence e=c/a>1e=c/a\gt 1. A parabola sits exactly at the boundary between these two behaviours, with e=1e=1 by definition.

Why does the latus rectum formula change from 4a for a parabola to 2b squared over a for an ellipse and a hyperbola?

The parabola has only one shape parameter, aa, so its latus rectum has to be expressed purely in terms of aa, and the derivation, setting x=ax=a in y2=4axy^2=4ax, gives y2=4a2y^2=4a^2, y=±2ay=\pm2a, a full chord length of 4a4a. The ellipse and hyperbola each have two independent shape parameters, aa and bb, and substituting x=cx=c into their equations brings both into the answer; working through the algebra, as this chapter does for the ellipse, produces l=b2/al=b^2/a for the half-chord, so the full latus rectum is 2b2/a2b^2/a. The two formulas are not really different rules so much as the same substitution method applied to equations with different numbers of parameters.

Is a circle really a conic section, since it does not seem to have a focus and a directrix like the other three?

Yes. A circle is the special case obtained when the cutting plane is exactly perpendicular to the cone's axis, β=90∘\beta=90^\circ, and algebraically it is the limiting case of an ellipse as the eccentricity shrinks to zero, at which point the two foci merge into a single centre and a=b=ra=b=r. Because the directrix of an ellipse recedes to infinity as e→0e\to0, a circle has no finite directrix in the usual focus-directrix sense, which is why this chapter introduces the circle with the simpler fixed-distance-from-a-centre definition rather than forcing focus-directrix language onto it. It is still, geometrically and historically, the first and simplest conic section.

How do I quickly tell, just from looking at an equation, which of the four conics it represents?

Check the powers and signs first. If both variables are squared with the same sign and equal coefficients, such as x2+y2+…=0x^2+y^2+\ldots=0, it is a circle. If both variables are squared with the same sign but different coefficients, such as x2a2+y2b2=1\frac{x^2}{a^2}+\frac{y^2}{b^2}=1, it is an ellipse. If both variables are squared but with opposite signs, such as x2a2−y2b2=1\frac{x^2}{a^2}-\frac{y^2}{b^2}=1, it is a hyperbola. If only one variable is squared and the other appears to the first power, such as y2=4axy^2=4ax, it is a parabola. This four-way check, done in under ten seconds, should be the very first thing you do on any conic-section problem, before touching any formula.

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