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Precalculus: An Investigation of Functions, by David Lippman and Melonie Rasmussen, licensed under CC BY-SA 4.0. Read the original free This shelf’s study material is shared under the same license (CC BY-SA 4.0).
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Chapter 13 · pp. 589–650
Chapter 9: Conics
A conic section is a curve made when a plane slices a cone. This chapter studies the ellipse, hyperbola and parabola. It covers their definitions, their equations (including shifted ones), and uses such as bridges, planetary orbits, ship navigation and reflectors. It also covers solving non-linear systems and describing conics in polar form with eccentricity.
Conic sections and the ellipse
Imagine a double cone cut by a flat plane. The edge of the cut is a conic section. If the plane is perpendicular to the cone's axis, the cut is a circle. If the plane is tilted a little, the cut is an oval called an ellipse. Other tilts give parabolas and hyperbolas (p. 589).
An ellipse can be drawn with two thumbtacks, a loop of string and a pencil. The tacks are the two fixed points, called the foci. The string length never changes, so the pencil traces every point whose distances to the two foci add to the same constant. In symbols, for a point Q on the ellipse, d(Q,F1)+d(Q,F2)=k (p. 590).
Vocabulary of an ellipse
The major axis is the line through the two foci. The points where it meets the ellipse are the vertices. The distance between the vertices is the major axis length. The center is the midpoint of the vertices, which is also the midpoint of the foci.
The minor axis passes through the center at right angles to the major axis. It meets the ellipse at the minor axis endpoints, also called co-vertices. The distance between them is the minor axis length. (p. 590)
Which axis is major depends on how the ellipse is turned. Foci on the x-axis mean a horizontal major axis. Foci on the y-axis mean a vertical one. The major axis is always the longer axis, and the vertices always lie on it (p. 590).
The constant sum k equals 2a, the major axis length. To see why, take the vertex (a,0). It is a−c from one focus and a+c from the other. Those distances add to 2a (p. 591).
Ellipses centered at the origin
When the major axis is horizontal and a>b>0, the equation is
a2x2+b2y2=1.
The vertices are (±a,0) and the co-vertices are (0,±b). For example, 25x2+9y2=1 has vertices (±5,0) and co-vertices (0,±3) (p. 592).
When the major axis is vertical, the larger denominator goes under y:
b2x2+a2y2=1.
Now the vertices are (0,±a) and the co-vertices are (±b,0). For x2+9y2=1, we have a=3 and b=1 (p. 592).
Reading features from an equation. Divide so the right side is 1, compare the denominators, then take square roots. For x2+9y2=9, dividing by 9 gives 9x2+1y2=1. The x denominator is larger, so the major axis is horizontal, with a=3 and b=1. The major axis length is 2a=6 and the minor axis length is 2b=2 (p. 593).
Writing an equation from axis lengths or a graph. Halve each axis length to get a and b, and put a2 under the variable of the major axis. A horizontal major axis of length 28 and a minor axis of length 16 give a=14 and b=8. The equation is 196x2+64y2=1. On a graph, read the vertices and co-vertices to get the same two numbers (p. 594).
Ellipses centered at (h,k)
Shifting the ellipse h units right and k units up means replacing x with x−h and y with y−k:
Horizontal ellipses have vertices (h±a,k). Vertical ones have vertices (h,k±a). The co-vertices use ±b in the other direction (p. 595).
Standard form from a general equation. Group the x terms and the y terms, complete the square for each, and divide so the right side is 1. Take x2+2x+4y2−24y=−32. Adding 1 completes the x square. For the y terms, factor out 4 first: 4(y2−6y). Completing the square needs 9 inside, which adds 4⋅9=36 to the equation. The result is (x+1)2+4(y−3)2=4. Dividing by 4 gives 4(x+1)2+1(y−3)2=1. The center is (−1,3), a=2 and b=1 (p. 596).
Equation from a center, a vertex and another point. Suppose the center is (−2,1) and a vertex is (−2,4). The x-values match, so the major axis is vertical, and a=4−1=3. Substitute the point (0,1) into b2(x+2)2+9(y−1)2=1. This gives b24=1, so b=2 (p. 597).
Bridge arch. A half-ellipse arch over a 50 ft river that rises 20 ft is modeled by placing the center at the middle of the river, with the river as the major axis. Then a=25, b=20, and 625x2+400y2=1. At x=15, y2=400(1−625225)=256, so the arch is 16 ft high there (p. 598). If the roadway is 4 ft above the top of the arch, it is 24 ft above the river. The gap between road and arch at that spot is 24−16=8 ft.
Foci of an ellipse
The distance c from the center to each focus satisfies
b2=a2−c2,soc2=a2−b2.
The foci lie inside the ellipse, so c<a (p. 599). This looks like the Pythagorean Theorem, but it is not that theorem, and you cannot find c by adding a2 and b2. Adding the squares is the pattern for hyperbolas, whose foci lie beyond the vertices (pp. 599, 607).
Whispering chamber. The elliptical hall is 96 ft long and 46 ft wide, so a=48 and b=23. Then c=482−232=1775≈42 ft. Two people at the foci stand about 2(42)=84 ft apart, each about 48−42=6 ft from the end wall (p. 599).
Foci when the center is not the origin. Find the center, compute c=a2−b2, and move c units from the center along the major axis. In 4(x−2)2+29(y+3)2=1, the larger denominator is under y, so the ellipse is vertical. Here a2=29 and b2=4, so c=25=5. The center is (2,−3), so the foci are (2,−3±5), which are (2,−8) and (2,2) (p. 599).
Equation from the foci and the major axis length. Follow these steps:
Take the center as the midpoint of the foci.
Take a as half the major axis length.
Take c as half the distance between the foci.
Compute b2=a2−c2.
Foci (−1,4) and (3,4) give center (1,4), a horizontal ellipse, and c=2. A major axis of 10 gives a=5. So b2=25−4=21, and the equation is 25(x−1)2+21(y−4)2=1 (p. 600).
Planetary orbits
Kepler's first law says each planet moves in an ellipse with the sun at one focus. The orbits are only approximately elliptical, because bodies tug on one another. The aphelion is the planet's greatest distance from the sun, and the perihelion is its smallest. Their sum is the major axis length (p. 600).
For Mercury, the aphelion is 35.98 million miles and the perihelion is 28.58 million miles. Then 2a=64.56, so a=32.28. The perihelion is the distance from the sun (a focus) to the nearest vertex, so it equals a−c. This gives c=32.28−28.58=3.7. Then b2=32.282−3.72≈1028.3, and with the center at the origin the orbit is
1041.98x2+1028.31y2=1.
The values of a2 and b2 are nearly equal, so Mercury's orbit is close to a circle (p. 601).
Defining a hyperbola
A hyperbola is the next conic after the ellipse. It comes from slicing a double cone with a plane steep enough to cut both halves (pp. 607–608). The definition is a close cousin of the ellipse rule. For an ellipse, the distances to two foci add to a constant. For a hyperbola, the absolute value of the difference of the distances to the foci F1 and F2 is a constant k:
∣d(Q,F1)−d(Q,F2)∣=k
(pp. 607–608)
Vocabulary to know (p. 608):
The transverse axis is the line through the foci.
The vertices are the points where the curve crosses the transverse axis.
The center is the midpoint of the vertices, which is also the midpoint of the foci.
The conjugate axis is the other axis of symmetry through the center.
The two separate pieces of the curve are branches, and the curve has two asymptotes.
To find where the constant comes from, put a vertex (a,0) into the definition with foci (±c,0). The distances to the foci are c−a and c+a, and they differ by 2a. So k=2a, the length of the transverse axis (p. 609). Use this whenever a problem gives you a difference in distances directly.
Standard equations centered at the origin
Setting up the distance condition and simplifying (with b2=c2−a2) gives the standard forms (pp. 609–611):
Opens horizontally: a2x2−b2y2=1, with vertices (±a,0).
Opens vertically: a2y2−b2x2=1, with vertices (0,±a).
The opening direction depends on which squared term is positive. It does not depend on which denominator is bigger. In both forms, a2 sits under the positive term.
The asymptotes are y=±abx for a horizontal hyperbola and y=±bax for a vertical one (pp. 610–611). The reasoning: solve the horizontal form for y to get y=±abx1−x2a2. When ∣x∣ is very large, x2a2 is nearly 0, so the root is nearly 1. The branches therefore hug the lines y=±abx (p. 610).
Sketching a hyperbola
Put the equation in standard form and read a and b.
Draw the central rectangle. Its sides are parallel to the axes and pass through the vertices and co-vertices.
Draw the rectangle's diagonals, extended. These are the asymptotes.
Start each branch at a vertex and curve it outward toward the asymptotes.
Example: y2−4x2=4. Divide by 4 to get 4y2−x2=1. The y2 term is positive, so the hyperbola opens vertically. Here a=2 and b=1. The vertices are (0,±2), the transverse axis has length 4, and the rectangle has corners (±1,±2). The asymptotes are y=±2x (pp. 608, 611–612).
Writing equations at the origin
From vertices and an asymptote. Vertices (±6,0) mean a horizontal hyperbola with a=6. The asymptote y=34x has slope ab=34, so b=8. The equation is 36x2−64y2=1. For a vertical hyperbola, the slope is ba instead, so be careful about which ratio to use (p. 613).
From vertices and a point. Vertices (0,±9) give a vertical form with a=9. Substitute the point (8,15) into 81y2−b2x2=1 to get 81225−b264=1. Then b264=916, so b2=36. The equation is 81y2−36x2=1 (p. 613).
Hyperbolas centered at (h,k)
Shifting the center to (h,k) gives (p. 614):
Horizontal: a2(x−h)2−b2(y−k)2=1. The vertices are (h±a,k), and the asymptotes are y−k=±ab(x−h).
Vertical: a2(y−k)2−b2(x−h)2=1. The vertices are (h,k±a), and the asymptotes are y−k=±ba(x−h).
The rectangle corners are (h±a,k±b) in the horizontal case.
Reading a graph. If the asymptotes cross at (2,3) and the vertices are (2,2) and (2,4), the hyperbola is vertical with a=1. If the rectangle reaches from x=−1 to x=5, then b=3. The equation is 1(y−3)2−9(x−2)2=1 (p. 615).
General form to standard form. Group the x terms and y terms, and complete the square for each. Take care with the minus sign in front of the y part, because the number you add inside the parentheses gets multiplied by a negative. For 9x2+18x−4y2+16y=43:
9(x+1)2−4(y−2)2=36⇒4(x+1)2−9(y−2)2=1
The center is (−1,2), with a=2 and b=3. It opens horizontally, with vertices (−3,2) and (1,2) (pp. 615–616).
Vertices and an asymptote, center not at the origin. Vertices (−2,−5) and (−2,7) share an x-value, so the hyperbola is vertical. The center is their midpoint, (−2,1), and a=6. The asymptote slope 23 equals ba, so b=4. The equation is 36(y−1)2−16(x+2)2=1 (pp. 616–617).
Foci of a hyperbola
The distance c from the center to each focus satisfies
b2=c2−a2,soc2=a2+b2.
This is not the Pythagorean Theorem, and it is not the ellipse rule b2=a2−c2 either. The difference makes sense geometrically. Ellipse foci lie inside the curve, before the vertices, so c<a. Hyperbola foci lie beyond the vertices, so c>a (p. 617).
Example: for 4(y+1)2−5(x−3)2=1, the center is (3,−1) and the hyperbola is vertical. Then c=4+5=3, and the foci are (3,−1±3), which are (3,−4) and (3,2) (p. 618).
From foci and vertices. Foci (5,−8) and (−3,−8) and vertices (4,−8) and (−2,−8) give center (1,−8). The distance to a vertex is a=3, and the distance to a focus is c=4. So b2=16−9=7, and the equation is 9(x−1)2−7(y+8)2=1 (p. 618).
Application: LORAN
Before GPS, LORAN located ships using two radio stations that sent signals at the same moment. The ship measured the difference in arrival times and converted it to a difference in distance. That put the ship on a hyperbola with the two stations as foci. A second pair of stations gave a second hyperbola, and the ship lay where the two hyperbolas crossed (p. 619).
Example: stations 150 km apart, signals travel at 300,000 km/s, and one signal arrives 0.0003 s before the other. The distance difference is 300,000×0.0003=90 km. Since this equals 2a, a=45. Half the station distance gives c=75. Then b2=752−452=3600. With the center at the origin and stations at (±75,0), the hyperbola is
2025x2−3600y2=1
(p. 619).
The Parabola as a Conic
A parabola is the curve you get when a plane cuts a cone while running parallel to the cone's side. It can also be defined by distances. Pick a fixed point, the focus, and a fixed line, the directrix. The parabola is every point that is the same distance from the focus as from the directrix (p. 627).
Vocabulary:
The axis of symmetry runs through the focus and is perpendicular to the directrix.
The vertex is where the parabola crosses its axis. It sits exactly halfway between the focus and the directrix.
The focal lengthp is the distance from the vertex to the focus (p. 627).
With the vertex at the origin and the focus at (0,p), the directrix is y=−p (p. 627).
Equations with Vertex at the Origin
To get the equation, let (x,y) be any point on the parabola. Set its distance to the focus equal to its distance to the directrix:
x2+(y−p)2=y+p
Square both sides and expand. The y2 and p2 terms cancel, leaving
x2=4py
(p. 628). Dividing by 4p gives y=4p1x2. So this is just y=x2 stretched or compressed vertically by the factor 4p1 (p. 628).
A parabola with a horizontal axis has focus (p,0) and a vertical directrix. Its equation is y2=4px (p. 628).
The sign of p tells you which way the parabola opens:
For x2=4py: p>0 opens up, p<0 opens down.
For y2=4px: p>0 opens right, p<0 opens left (p. 628).
Example. A parabola has vertex (0,0) and focus (0,−2). The focus is on the y-axis, so the axis is vertical and the form is x2=4py. Here p=−2, so x2=4(−2)y, or x2=−8y. It opens down (p. 628).
Vertex at (h,k)
Shifting the parabola h units right and k units up gives two standard forms (p. 629):
Vertical axis
Horizontal axis
Equation
(x−h)2=4p(y−k)
(y−k)2=4p(x−h)
Axis of symmetry
x=h
y=k
Focus
(h,k+p)
(h+p,k)
Directrix
y=k−p
x=h−p
Finding the focus and directrix from a quadratic. Isolate the squared factor so the equation matches the standard form. For y=8(x−1)2+2:
Subtract 2: y−2=8(x−1)2.
Divide by 8: (x−1)2=81(y−2).
Match 4p=81, so p=321.
The vertex is (1,2) and the axis is x=1. The focus is (1,2+321), which is (1,2321). The directrix is y=2−321=13231 (p. 630).
Writing an equation from the vertex and focus. Say the vertex is (1,5) and the focus is (3,5). Both points lie on y=5, so that is the axis and the parabola is horizontal. Then h=1, k=5, and p=3−1=2. Substitute into (y−k)2=4p(x−h):
(y−5)2=8(x−1)
(pp. 630–631). Keep the sign of p. If the focus were below a vertex of (−2,3) at (−2,2), then p=2−3=−1 and the parabola would open down.
Reflection and Applications
A parabola has a reflection property. A ray leaving the focus bounces off the curve and travels parallel to the axis of symmetry. Run in reverse, parallel incoming rays all bounce to the focus (p. 631). Flashlight and headlight reflectors use the first direction to make a straight beam. Satellite dishes, radio telescopes, and solar cookers use the second direction to collect energy at one point (p. 631).
Example: solar cooker. A dish is 16 in. across and 4 in. deep. Put the vertex at the origin, so a rim point is (8,4). Use x2=4py:
82=4p(4)⇒64=16p⇒p=4
The food belongs 4 in. above the vertex (p. 631). The same method for a 100 m wide, 20 m deep telescope uses the point (50,20). It gives 2500=80p, so p=31.25 m (p. 631).
Solving Non-Linear Systems
To find where two curves cross, solve their equations together. Substitution and elimination both still work (p. 632).
Substitution. Find the intersection of 4x2+25y2=1 and x2+y2=9.
Clear fractions in the ellipse by multiplying by 100: 25x2+4y2=100.
Solve the circle for x2 (not for x): x2=9−y2.
Substitute: 25(9−y2)+4y2=100, so −21y2=−125 and y2=21125.
Back-substitute: x2=9−21125=2164.
Each square root has a plus and a minus, so x=±218 and y=±2155. That gives four intersection points (p. 632).
Elimination. Multiply the circle by −4 to get −4x2−4y2=−36. Add it to 25x2+4y2=100. The y2 terms cancel, leaving 21x2=64, the same x-values as before (p. 633).
A quadratic in disguise. Substitute y=2x2 into 4y2−9x2=1. This gives x4−9x2=1, or
9x4−x2−9=0
Only even powers appear, so let u=x2. Then 9u2−u−9=0 and the quadratic formula gives u=181±325. Since u=x2 cannot be negative, discard the minus root. Then u≈1.057, so x≈±1.028. Then y=2x2≈2.114. The curves meet at about (1.028,2.114) and (−1.028,2.114) (p. 633).
Locating a Ship with Two Hyperbolas
Each pair of LORAN stations gives one hyperbola, and the ship lies on both. In the example, the first pair gives 2025x2−3600y2=1. A second pair 200 km farther south gives 225x2−2275(y+200)2=1 (pp. 634–635).
Solve each equation for x2:
x2=2025+169y2x2=225+919(y+200)2
Set them equal and simplify. This gives the quadratic 75y2−6400y−348800=0, with roots y≈123.11 km and y≈−37.78 km (p. 635).
Putting each y back into a hyperbola gives x≈±102.71 for the first root and x≈±53.18 for the second. That makes four candidate positions. Two lie on land, so they are discarded. Navigators use other methods to choose between the remaining two (p. 635). In general, intersecting curves can give several solutions, and the real-world setting decides which one is correct.
One definition for all conics
Earlier sections defined each conic in its own way. A single rule covers ellipses, parabolas and hyperbolas. Put a focus F at the origin and draw a line L, the directrix, at x=±p or y=±p. A conic is the set of points Q where the ratio of the distance to the focus over the distance to the directrix is a constant e:
d(Q,L)d(Q,F)=e,e>0
The constant e is the eccentricity. (p. 640)
Watch out: this e is not the number 2.71828… from exponential functions. Here it only names a distance ratio, and it can be any positive number, such as 0.5 or 3. (p. 640)
The polar equation of a conic
Write Q in polar form as (rcosθ,rsinθ). Take the directrix y=−p. The distance from Q to the focus is just r. The distance from Q to the line is p+rsinθ. So the rule becomes p+rsinθr=e. Solving for r:
Clear the fraction: r=e(p+rsinθ).
Gather the r terms: r−ersinθ=ep.
Factor: r(1−esinθ)=ep, so r=1−esinθep. (pp. 640–641)
The other three directrix positions work the same way:
Horizontal directrix y=±p: r=1±esinθep.
Vertical directrix x=±p: r=1±ecosθep.
The sign matches the side of the origin the directrix is on. A plus sign means the directrix is at a positive value (y=p or x=p). A minus sign means it is at a negative value (y=−p or x=−p). (pp. 640–641, 644)
Writing a polar equation from e and the directrix
Pick sine for a horizontal directrix or cosine for a vertical one.
Pick the sign from the side of the origin the directrix is on.
Compute the numerator ep.
Example:e=3 and directrix x=2. The directrix is vertical and at positive x, so use cosine with a plus sign. Here ep=3⋅2=6, so
r=1+3cosθ6
This graphs as a hyperbola. (p. 641)
How eccentricity sets the shape
0<e<1: ellipse
e=1: parabola
e>1: hyperbola (p. 642)
Why it works (algebra). Take the directrix x=1, so r=1+ecosθe. Multiply out and use rcosθ=x and r2=x2+y2. This gives
(1−e2)x2+y2+2e2x=e2
If e<1, the x2 and y2 coefficients are both positive, which is an ellipse. If e>1, the x2 coefficient is negative, which is a hyperbola. If e=1, the x2 term vanishes, which is a parabola. (p. 642)
Why it works (intuition). Look at the denominator 1+ecosθ.
If e<1, it is always positive, so r is finite at every angle. That closed loop is an ellipse.
If e=1, it hits zero at one angle (θ=π), so r is undefined there. That matches a parabola, which has no point in the direction of its axis away from the vertex.
If e>1, it is zero at two angles and r turns negative for some angles. The positive and negative parts make two separate branches, which is a hyperbola. (p. 643)
Identifying a conic from its polar equation
Divide the top and bottom so the denominator starts with 1.
Read e as the coefficient of sinθ or cosθ.
Use the numerator ep to find p.
Use the function and sign to name the directrix.
Example A:r=3−2cosθ6. Divide by 3 to get 1−32cosθ2. Then e=32, so it is an ellipse. From ep=2, p=3. The minus sign gives directrix x=−3. (pp. 643–644)
Example B:r=1−2sinθ8 is already in standard form. Here e=2, so it is a hyperbola. From ep=8, p=4, and the directrix is y=−4. (p. 643)
Example C:r=5+5sinθ8. Divide by 5 to get 1+sinθ8/5. Then e=1, so it is a parabola, and p=58. The directrix y=58 lies above the focus, so the parabola opens downward, away from the directrix. (p. 644)
Sketching a polar ellipse
Evaluate r at θ=0,2π,π,23π and plot the points. Then use the vertices to find the center, a, c and b. Remember that the origin is one focus.
Example:r=1−0.5sinθ3. Here e=0.5, an ellipse, and ep=3 gives p=6, so the directrix is y=−6.
The points are (3,0), (0,6), (−3,0) and (0,−2).
The vertices are (0,−2) and (0,6), so the center is the midpoint (0,2) and a=4.
The focus at the origin is 2 from the center, so c=2.
Then b2=a2−c2=16−4=12.
The Cartesian equation is 12x2+16(y−2)2=1. (pp. 645–646)
Analyzing a polar hyperbola
Find the vertices on the axis. Their midpoint is the center. The distance from the center to the origin focus is c, and b2=c2−a2.
Example:r=1+2cosθ6. Here e=2, so it is a hyperbola.
At θ=0, r=2, giving (2,0). At θ=π, r=−6, which plots at (6,0).
The vertices are (2,0) and (6,0), so the center is (4,0) and a=2.
The origin focus is 4 from the center, so c=4 and b2=16−4=12.
The equation is 4(x−4)2−12y2=1.
The asymptotes are y=±3(x−4). (pp. 646–647)
Check yourself
For an ellipse with a=5 and b=3, find c. Why is b2=a2−c2 not simply the Pythagorean Theorem applied to any right triangle?
A hyperbola opens horizontally with center (2,−1), a=3 and b=4. Write its equation and the equations of its asymptotes.
A parabolic dish has vertex at the origin and passes through the rim point (4,2) on x2=4py. How do you find where to place the receiver (the focus)?
Write the polar equation of the conic with eccentricity 21 and directrix y=4. What shape is it?
A system has the equations x2+y2=25 and y=x2−5. Describe how you would solve it by substitution.