The Hyperbola
Stretch a rubber band around two pins and trace the curve that keeps the sum of the two
distances fixed and you get an
ellipse. The
hyperbola is its rebellious twin: instead of the sum of the distances to two
special points, it keeps the difference fixed. Same two points — the
foci — but a mirror-image rule, and a wildly different shape.
A hyperbola is every point (x, y) for which the
distances to two fixed foci F_1 and F_2
differ by a constant amount, written 2a:
\left| \, PF_1 - PF_2 \, \right| = 2a.
Because a difference can be positive or negative, this rule carves out two separate
curves — the two branches, one hugging each focus. That is the hyperbola's
signature: it comes in a matched pair that open away from each other and race off toward
infinity.
The standard equation
Put the two foci on the x-axis, symmetric about the origin, and the
"constant difference" rule tidies up into a single clean equation:
\frac{x^2}{a^2} - \frac{y^2}{b^2} = 1.
The minus sign is everything — swap it for a plus and you would be back at an ellipse. Reading
this equation gives you the whole figure at a glance:
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the vertices — where each branch turns around — sit at
(\pm a, 0) (set y = 0 and solve);
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the foci sit at (\pm c, 0), where
c comes from
c^2 = a^2 + b^2 — note the plus;
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the segment between the vertices, length 2a, is the
transverse axis; the perpendicular segment of length
2b is the conjugate axis.
The letter under the positive term is a, and it always points
along the axis the curve opens toward. Here x^2 is positive, so the
branches open left and right.
Meet the asymptotes
Follow a branch far enough from the centre and it flattens against a pair of straight lines it
never quite touches — the asymptotes. For
\dfrac{x^2}{a^2} - \dfrac{y^2}{b^2} = 1 they are the two lines
y = \pm \frac{b}{a}\, x.
They are the single most useful sketching aid you own: draw the box
a wide and b tall around the centre, run
the diagonals out to infinity, and the branches slot neatly inside, kissing the diagonals as they
go. Step through the figure below to watch the branches, vertices, asymptotes and foci appear one
layer at a time.
Worked examples
1 · Read off everything from
\dfrac{x^2}{9} - \dfrac{y^2}{16} = 1.
Match it to \dfrac{x^2}{a^2} - \dfrac{y^2}{b^2} = 1. The number under
x^2 is a^2 = 9, so
a = 3; the number under y^2 is
b^2 = 16, so b = 4. Now use the
plus relation:
c^2 = a^2 + b^2 = 9 + 16 = 25 \;\Rightarrow\; c = 5.
So the vertices are (\pm 3, 0), the
foci are (\pm 5, 0), the asymptotes
are y = \pm \frac{4}{3} x, and the eccentricity is
e = \frac{c}{a} = \frac{5}{3} \approx 1.67 \; (> 1).
2 · Asymptotes and foci of
\dfrac{x^2}{4} - \dfrac{y^2}{9} = 1.
Here a^2 = 4 and b^2 = 9, so
a = 2 and b = 3. The asymptotes are
y = \pm \frac{b}{a} x = \pm \frac{3}{2} x. For the foci,
c^2 = a^2 + b^2 = 4 + 9 = 13 \;\Rightarrow\; c = \sqrt{13} \approx 3.61,
so the foci are (\pm \sqrt{13},\, 0). The c
need not be a whole number — only c^2 has to be.
-
Locus rule: the set of points whose distances to two foci have a constant
difference, \left| PF_1 - PF_2 \right| = 2a.
-
Standard form (opens left/right):
\dfrac{x^2}{a^2} - \dfrac{y^2}{b^2} = 1, with vertices
(\pm a, 0) and foci (\pm c, 0).
-
Focal relation: c^2 = a^2 + b^2 — a
plus, so c > a always.
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Asymptotes: y = \pm \dfrac{b}{a} x.
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Eccentricity: e = \dfrac{c}{a} > 1 (an ellipse
has e < 1; a parabola, exactly 1).
Other flavours
Swap the roles of x and y and the
hyperbola stands up on end:
\frac{y^2}{a^2} - \frac{x^2}{b^2} = 1
now has the y^2 term positive, so it opens up and down,
with vertices at (0, \pm a) and foci at
(0, \pm c). The rule for which way it opens is always the same: whichever
variable sits over the positive term is the axis it opens along.
There is also the friendly rectangular hyperbola
xy = k — the graph of inverse proportion,
y = k/x. Its two branches live in opposite quadrants and its asymptotes
are simply the x- and y-axes. It is the same
curve, just rotated 45^\circ.
Here is the beautiful part: the "constant difference of distances" rule is not just geometry — it
is how navigation systems find you. Two radio stations broadcast synchronised pulses. A
receiver can't measure how far it is from each station, but it can measure the
difference in arrival times — and time difference means distance difference. A
fixed distance difference is exactly the locus of a hyperbola with the two stations as foci, so
your receiver knows it lies somewhere on one specific hyperbola.
Add a second pair of stations and you get a second hyperbola; where the two curves cross is your
position. This was the whole idea behind LORAN (Long Range Navigation), which
guided ships and aircraft for decades, and the same time-difference-of-arrival trick still helps
modern GPS and mobile-phone location work. Every time a system turns "how much
later did this signal arrive" into "where am I," a hyperbola is quietly doing the maths.
You have probably seen the shape without noticing, too: the curved edge of the shadow a lampshade
throws on a wall, and the graceful waist of a power-station cooling tower, are
both hyperbolas.
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The focal relation uses a PLUS. For a hyperbola
c^2 = a^2 + b^2 — the opposite of the ellipse, where
c^2 = a^2 - b^2. Because of the plus, c is
always bigger than a, so the foci sit outside the
vertices, and the eccentricity e = c/a is always
greater than 1. If you ever get c < a, you have
used the ellipse formula by mistake.
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a lives under the POSITIVE term. In a hyperbola
a is not the bigger denominator — it is whichever
denominator sits under the positive term, and that term decides the opening
direction. In \frac{x^2}{9} - \frac{y^2}{16} = 1 the
x^2 is positive, so a^2 = 9 and it opens
left/right — even though 16 > 9. Don't reflexively
pick the larger number for a^2 the way you do for an ellipse.
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Asymptote slope is \frac{b}{a}, not
\frac{a}{b}. Rise over run:
b is the height of the box, a its
half-width, so the diagonals climb b/a.