When a plane cuts a double cone at different angles, the curves produced are the conic sections: the circle, the parabola, the ellipse, and the hyperbola. These curves appear constantly in nature and technology: planetary orbits are ellipses, projectiles follow parabolas, and the path of light in a reflecting telescope is governed by the parabola.
This chapter defines each conic as a locus of points satisfying a geometric property, derives its standard equation, and studies its key features. It begins with circles, then the parabola with its focus and directrix, then the ellipse and the hyperbola, each described by standard equations and their important parameters such as focus, eccentricity, latus rectum, and asymptotes.
Conic sections unify algebra and geometry in a beautiful way. Their equations encode precise geometric information, and their properties have direct applications in astronomy, optics, architecture, and engineering. This chapter provides the essential analytic geometry background needed for further study of curves in higher mathematics.
A circle is the set of all points in a plane that are at a fixed distance from a fixed point. The fixed point is the centre and the fixed distance is the radius.
A circle with centre (h, k) and radius r has equation:
(x - h)^2 + (y - k)^2 = r^2
If the centre is the origin, the equation simplifies to x^2 + y^2 = r^2.
The general equation of a circle is:
x^2 + y^2 + 2gx + 2fy + c = 0
Its centre is (-g, -f) and radius is sqrt(g^2 + f^2 - c). The circle is real only when g^2 + f^2 - c > 0.
A parabola is the set of all points in a plane that are equidistant from a fixed line (the directrix) and a fixed point (the focus) not on the line.
For a parabola with vertex at the origin:
The eccentricity e of a conic measures how much it deviates from a circle. For a parabola, e = 1.
An ellipse is the set of all points in a plane such that the sum of the distances to two fixed points (the foci) is constant.
For the ellipse with centre at the origin and major axis along the x-axis:
x^2/a^2 + y^2/b^2 = 1, with a > b
where: - The foci are at (+/- c, 0), with c^2 = a^2 - b^2. - The vertices are at (+/- a, 0). - The eccentricity is e = c/a, with 0 < e < 1. - The length of the major axis is 2a and the minor axis is 2b. - The latus rectum has length 2b^2/a.
If the major axis is along the y-axis, a and b swap roles and the equation becomes x^2/b^2 + y^2/a^2 = 1.
A hyperbola is the set of all points in a plane such that the difference of the distances to two fixed points (the foci) is constant.
For the hyperbola with centre at the origin and transverse axis along the x-axis:
x^2/a^2 - y^2/b^2 = 1
where: - The foci are at (+/- c, 0), with c^2 = a^2 + b^2. - The vertices are at (+/- a, 0). - The eccentricity is e = c/a, with e > 1. - The length of the transverse axis is 2a and the conjugate axis is 2b. - The latus rectum has length 2b^2/a. - The equations of the asymptotes are y = +/- (b/a)x.
The eccentricity e determines the type of conic:
The equation of a conic in general second degree form is Ax^2 + By^2 + Cxy + Dx + Ey + F = 0, and its type can be identified from its coefficients.
| Conic | Standard Equation | Eccentricity | Foci | Latus rectum |
|---|---|---|---|---|
| Circle | x^2 + y^2 = r^2 | 0 | Centre only | - |
| Parabola | y^2 = 4ax | 1 | (a, 0) | 4a |
| Ellipse | x^2/a^2 + y^2/b^2 = 1 | c/a (0 < e < 1) | (+/- c, 0) | 2b^2/a |
| Hyperbola | x^2/a^2 - y^2/b^2 = 1 | c/a (e > 1) | (+/- c, 0) | 2b^2/a |
| Conic | Relation | Key points |
|---|---|---|
| Ellipse | c^2 = a^2 - b^2 | a > b, c < a |
| Hyperbola | c^2 = a^2 + b^2 | c > a |
| Parabola | latus rectum = 4a | e = 1 |
| Circle | radius = r | e = 0 |
Conic sections reveal how a single family of curves arises from slicing a double cone, unifying the circle, parabola, ellipse, and hyperbola under the common language of eccentricity. Each conic has a precise algebraic equation that encodes its geometric structure, from the focus and directrix of the parabola to the foci, axes, and asymptotes of the ellipse and hyperbola. These curves model planetary motion, projectile paths, and light reflection, making them central to physics and astronomy. Mastery of the standard equations and their parameters prepares students for further analytic geometry and calculus, where conics reappear in the study of curves, tangents, and quadratic surfaces.