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Unit 12: Conic Sections

AP Precalc cheatsheet

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A conic section is the curve you get when a plane meets a right circular cone: circle, ellipse, parabola, or hyperbola (the β€œdegenerate” cases: point, line, pair of lines show up when the plane passes through the vertex in special ways and will not be talked about here).

In a rectangular coordinate system, any conic can be written as a degree-two equation in xx and yy:

Ax2+Bxy+Cy2+Dx+Ey+F=0Ax^{2} + Bxy + Cy^{2} + Dx + Ey + F = 0

with A,B,CA,B,C not all zero. In most precalculus work B=0B = 0 (no tilted axes); then the graph is a parabola, ellipse, or hyperbola depending on the signs of AA and CC after completing squares.

The eccentricity ee measures how β€œstretched” the conic is relative to a circle (e=0e = 0). Another method of defining conics is using a focus and directrix: fix a focus and a directrix (a line); the conic is the set of points PP whose distance to the focus equals ee times the perpendicular distance to the directrix. Then 0<e<10 < e < 1 gives an ellipse, e=1e = 1 a parabola, and e>1e > 1 a hyperbola. We will prove the focus-directrix property in a later section.


One of the more simpler conic sections is the circle. A circle is defined as the set of points equidistant from a fixed focus. For a circle, e=0e = 0. Since circles are extensively talked about in other sections, I will not go in detail about them.


A parabola is defined as the set of points equidistant from a fixed focus and a fixed directrix (a line). For a parabola, e=1e = 1.

Standard forms (vertex at , axis parallel to a coordinate axis)

Section titled β€œStandard forms (vertex at (h,k), axis parallel to a coordinate axis)”

Opening up or down (vertical axis):

(xβˆ’h)2=4p(yβˆ’k)(x - h)^{2} = 4p(y - k)
  • Vertex: (h,k)(h,k).
  • Focus: (h, k+p)(h,\, k + p).
  • Directrix: y=kβˆ’py = k - p.
  • If p>0p > 0, opens upward; if p<0p < 0, opens downward.

Opening left or right (horizontal axis):

(yβˆ’k)2=4p(xβˆ’h)(y - k)^{2} = 4p(x - h)
  • Vertex: (h,k)(h,k).
  • Focus: (h+p, k)(h + p,\, k).
  • Directrix: x=hβˆ’px = h - p.
  • If p>0p > 0, opens to the right; if p<0p < 0, opens to the left.

The quantity ∣4p∣\lvert 4p\rvert controls how β€œwide” the parabola is: larger ∣p∣\lvert p\rvert means a more gradual curve.

Proof (Standard equation of a vertical parabola). Suppose the vertex is (h,k)(h,k), the focus is (h,k+p)(h,k+p), and the directrix is

y=kβˆ’p.y=k-p.

Let P=(x,y)P=(x,y) be a point on the parabola. By definition,

PF=d(P,directrix).PF=d(P,\text{directrix}).

The distance to the focus is

PF=(xβˆ’h)2+(yβˆ’(k+p))2.PF=\sqrt{(x-h)^2+(y-(k+p))^2}.

The perpendicular distance to the directrix is

∣yβˆ’(kβˆ’p)∣.\lvert y-(k-p)\rvert.

For points on the parabola, squaring both sides gives

(xβˆ’h)2+(yβˆ’kβˆ’p)2=(yβˆ’k+p)2.(x-h)^2+(y-k-p)^2=(y-k+p)^2.

Expand the two squared terms involving yy:

(xβˆ’h)2+(yβˆ’k)2βˆ’2p(yβˆ’k)+p2=(yβˆ’k)2+2p(yβˆ’k)+p2.(x-h)^2+(y-k)^2-2p(y-k)+p^2=(y-k)^2+2p(y-k)+p^2.

Cancel common terms:

(xβˆ’h)2=4p(yβˆ’k).(x-h)^2=4p(y-k).

This gives the standard form for a vertical parabola.

The latus rectum is the chord through the focus perpendicular to the axis of symmetry, with a length of ∣4p∣\lvert 4p\rvert (same as the absolute coefficient in the standard forms above). It should be parallel to the directrix.

For

(xβˆ’h)2=4p(yβˆ’k),(x-h)^2=4p(y-k),

the latus rectum endpoints are

(hβˆ’2p,k+p)(h-2p,k+p)

and

(h+2p,k+p).(h+2p,k+p).

For

(yβˆ’k)2=4p(xβˆ’h),(y-k)^2=4p(x-h),

the latus rectum endpoints are

(h+p,kβˆ’2p)(h+p,k-2p)

and

(h+p,k+2p).(h+p,k+2p).
xydirectrixvertex(h;k)focus(h;k+p)latusrectumpp(xΒ‘h)2=4p(yΒ‘k)

Example. For

x2=16y,x^2=16y,

compare with

(xβˆ’h)2=4p(yβˆ’k).(x-h)^2=4p(y-k).

Here h=0h=0, k=0k=0, and 4p=164p=16, so p=4p=4. Therefore:

  • Vertex: (0,0)(0,0).
  • Focus: (0,4)(0,4).
  • Directrix: y=βˆ’4y=-4.
  • Focal width: 1616.
  • Latus rectum endpoints: (βˆ’8,4)(-8,4) and (8,4)(8,4).

For a parabola, any ray starting from the focus and reflecting off of the surface of the parabola will always be perpendicular to the latus rectum (the converse is true as well)! This makes parabolas especially useful for things like flashlights and mirrors.

Extension. Prove the theorem stated above is true. One theorem you make find useful is the Law of Reflection: A ray reflecting off the surface will have the same angle of reflection as angle of incidence.

In photography, lenses are made up of portions of parabolas. Suppose you have a chord (parallel to the directrix) with half-length dd. Define the focal ratio as pd\frac{p}{d}. This is what the ff-stops are defined as in photography.


An ellipse is defined as the set of points the sum of whose distances to two fixed foci is constant (greater than the distance between the foci).

xymajoraxisminoraxiscenterF1F2vertexvertexPF1+PF2isconstantforeverypointPontheellipse

In an ellipse, the major axis is always defined as the longer axis, while the minor axis is defined as the shorter axis. The vertices of a ellipse are always defined as the endpoints of the major axis. The endpoints of the minor axis don’t really get a special name. The semi-major and semi-minor axes are defined as half of their respective axes.

(xβˆ’h)2a2+(yβˆ’k)2b2=1,a>b>0\frac{(x - h)^{2}}{a^{2}} + \frac{(y - k)^{2}}{b^{2}} = 1, \qquad a > b > 0
  • Center: (h,k)(h,k).
  • Vertices (ends of major axis): (hΒ±a, k)(h \pm a,\, k).
  • Co-vertices (ends of minor axis): (h, kΒ±b)(h,\, k \pm b).
  • Foci: (hΒ±c, k)(h \pm c,\, k) where c2=a2βˆ’b2c^{2} = a^{2} - b^{2}.
  • Major axis length 2a2a, minor axis length 2b2b.
  • Eccentricity: e=ca\displaystyle e = \frac{c}{a} with 0<e<10 < e < 1.
(xβˆ’h)2b2+(yβˆ’k)2a2=1,a>b>0\frac{(x - h)^{2}}{b^{2}} + \frac{(y - k)^{2}}{a^{2}} = 1, \qquad a > b > 0
  • Vertices: (h, kΒ±a)(h,\, k \pm a); co-vertices: (hΒ±b, k)(h \pm b,\, k).
  • Foci: (h, kΒ±c)(h,\, k \pm c) with c2=a2βˆ’b2c^{2} = a^{2} - b^{2}.

If the denominators are equal (a=ba = b), the ellipse is a circle of radius aa.

Proof (Standard equation of an ellipse, horizontal major axis). Place the foci on the xx-axis at F1=(βˆ’c,0)F_{1} = (-c,0) and F2=(c,0)F_{2} = (c,0) with 0<c<a0 < c < a. The ellipse is the set of points P=(x,y)P = (x,y) such that the sum of distances to the foci is the constant 2a2a:

(x+c)2+y2+(xβˆ’c)2+y2=2a.\sqrt{(x+c)^{2} + y^{2}} + \sqrt{(x-c)^{2} + y^{2}} = 2a.

Write r1=(x+c)2+y2r_{1} = \sqrt{(x+c)^{2} + y^{2}} and r2=(xβˆ’c)2+y2r_{2} = \sqrt{(x-c)^{2} + y^{2}}, so r1+r2=2ar_{1} + r_{2} = 2a. Isolate r1=2aβˆ’r2r_{1} = 2a - r_{2} and square (both sides are nonnegative):

(x+c)2+y2=4a2βˆ’4ar2+(xβˆ’c)2+y2.(x+c)^{2} + y^{2} = 4a^{2} - 4a r_{2} + (x-c)^{2} + y^{2}.

Expand and cancel x2x^{2}, y2y^{2}, and c2c^{2}:

4cx=4a2βˆ’4ar2⟹ar2=a2βˆ’cx.4cx = 4a^{2} - 4a r_{2} \quad\Longrightarrow\quad a r_{2} = a^{2} - cx.

Since r2β‰₯0r_{2} \ge 0 and (one can show) ∣cxβˆ£β‰€a2\lvert cx\rvert \le a^{2} on the ellipse, the right-hand side is nonnegative, so we may square again:

a2((xβˆ’c)2+y2)=(a2βˆ’cx)2.a^{2}\bigl((x-c)^{2} + y^{2}\bigr) = (a^{2} - cx)^{2}.

Multiply out:

a2x2βˆ’2a2cx+a2c2+a2y2=a4βˆ’2a2cx+c2x2.a^{2}x^{2} - 2a^{2}cx + a^{2}c^{2} + a^{2}y^{2} = a^{4} - 2a^{2}cx + c^{2}x^{2}.

Cancel βˆ’2a2cx-2a^{2}cx and rearrange:

a2x2βˆ’c2x2+a2y2=a4βˆ’a2c2⟹(a2βˆ’c2)x2+a2y2=a2(a2βˆ’c2).a^{2}x^{2} - c^{2}x^{2} + a^{2}y^{2} = a^{4} - a^{2}c^{2} \quad\Longrightarrow\quad (a^{2} - c^{2})x^{2} + a^{2}y^{2} = a^{2}(a^{2} - c^{2}).

Define b2=a2βˆ’c2>0b^{2} = a^{2} - c^{2} > 0. Then b2x2+a2y2=a2b2b^{2}x^{2} + a^{2}y^{2} = a^{2}b^{2}. Divide by a2b2a^{2}b^{2}:

x2a2+y2b2=1.\frac{x^{2}}{a^{2}} + \frac{y^{2}}{b^{2}} = 1.

Thus the two-focus definition yields the standard equation with c2=a2βˆ’b2c^{2} = a^{2} - b^{2}. Translating the center to (h,k)(h,k) replaces xx by xβˆ’hx-h and yy by yβˆ’ky-k, giving (xβˆ’h)2a2+(yβˆ’k)2b2=1\dfrac{(x-h)^{2}}{a^{2}} + \dfrac{(y-k)^{2}}{b^{2}} = 1.

For a vertical major axis, the same algebra applies after swapping the roles of xx and yy (foci on the vertical line through the center), which produces (xβˆ’h)2b2+(yβˆ’k)2a2=1\dfrac{(x-h)^{2}}{b^{2}} + \dfrac{(y-k)^{2}}{a^{2}} = 1 with a>ba > b and again c2=a2βˆ’b2c^{2} = a^{2} - b^{2}.

The sum of the distances from any point on the ellipse to the two foci is always

2a.2a.

This is why aa is the semi-major axis.

Example. Graph and identify the key features of

x29+y24=1.\frac{x^2}{9}+\frac{y^2}{4}=1.

The center is

(0,0).(0,0).

Since 9>49>4, the major axis is horizontal. Thus,

a2=9,b2=4,a^2=9,\qquad b^2=4,

so

a=3,b=2.a=3,\qquad b=2.

The vertices are

(Β±3,0),(\pm3,0),

and the co-vertices are

(0,Β±2).(0,\pm2).

Find cc:

c2=a2βˆ’b2=9βˆ’4=5.c^2=a^2-b^2=9-4=5.

So

c=5,c=\sqrt5,

and the foci are

(βˆ’5,0)(-\sqrt5,0)

and

(5,0).(\sqrt5,0).

The eccentricity is

e=ca=53.e=\frac{c}{a}=\frac{\sqrt5}{3}.
Β‘3Β‘2Β‘1123Β‘2Β‘112xy

For a horizontal ellipse centered at the origin,

x2a2+y2b2=1,a>b,\frac{x^2}{a^2}+\frac{y^2}{b^2}=1,\qquad a>b,

the foci are (Β±c,0)(\pm c,0), where c2=a2βˆ’b2c^2=a^2-b^2, and the eccentricity is

e=ca.e=\frac ca.

The directrices are

x=Β±ae.x=\pm\frac{a}{e}.

Since e=cae=\frac ca, this can also be written as

x=Β±a2c.x=\pm\frac{a^2}{c}.

For a vertical ellipse,

x2b2+y2a2=1,\frac{x^2}{b^2}+\frac{y^2}{a^2}=1,

the directrices are

y=Β±ae=Β±a2c.y=\pm\frac{a}{e}=\pm\frac{a^2}{c}.

Each focus has its own directrix. The right focus pairs with the right directrix, the left focus pairs with the left directrix, and similarly for vertical ellipses. These directrices will come in handy later in the Focus-Directrix section.

Β‘5Β‘4Β‘3Β‘2Β‘112345Β‘2Β‘112xy

Most planets orbit in ellipses! Johannes Kepler discovered the planets in our solar system did not orbit in a perfect circle (as previously believed), but orbited in ellipses! His three laws of planetary motion revolutionized astrophysics, and all of the physics are based on the properties of ellipses!

In addition, like a parabola, ellipses have cool reflective properties. If you start at one foci and point a ray and bounce it off of the ellipse, you will always pass through the other foci! The Griffin Museum’s β€œWhispering Room,” is based on this principle, where if you stand at one foci you can whisper something that can only be heard by a person standing at the other foci.


A hyperbola is defined as the set of points the absolute difference of whose distances to two foci is constant (less than the distance between the foci).

In a hyperbola, the transverse axis is always defined as the axis that passes through the the hyperbola (perpendicualr to the directrix), while the conjugate axis is always defined as the other axis. The vertices of a hyperbola are the relative extrema (basically the points with slope of ∞\infty or 00). The transverse axis passes through the vertices.

Horizontal transverse axis (opens left/right, center )

Section titled β€œHorizontal transverse axis (opens left/right, center (h,k))”
(xβˆ’h)2a2βˆ’(yβˆ’k)2b2=1\frac{(x - h)^{2}}{a^{2}} - \frac{(y - k)^{2}}{b^{2}} = 1
  • Center: (h,k)(h,k).
  • Vertices: (hΒ±a, k)(h \pm a,\, k).
  • Foci: (hΒ±c, k)(h \pm c,\, k) where c2=a2+b2c^{2} = a^{2} + b^{2}.
  • Asymptotes (useful for sketching):
yβˆ’k=Β±ba(xβˆ’h)y - k = \pm \frac{b}{a}(x - h) (yβˆ’k)2a2βˆ’(xβˆ’h)2b2=1\frac{(y - k)^{2}}{a^{2}} - \frac{(x - h)^{2}}{b^{2}} = 1
  • Vertices: (h, kΒ±a)(h,\, k \pm a).
  • Foci: (h, kΒ±c)(h,\, k \pm c) with c2=a2+b2c^{2} = a^{2} + b^{2}.
  • Asymptotes:
yβˆ’k=Β±ab(xβˆ’h)y - k = \pm \frac{a}{b}(x - h)

Eccentricity: e=ca>1\displaystyle e = \frac{c}{a} > 1.

The conjugate hyperbola swaps the roles of the terms (e.g. y2a2βˆ’x2b2=1\frac{y^{2}}{a^{2}} - \frac{x^{2}}{b^{2}} = 1 vs x2a2βˆ’y2b2=1\frac{x^{2}}{a^{2}} - \frac{y^{2}}{b^{2}} = 1) and shares the same asymptote rectangle but different vertices and branches.

xy

For a horizontal hyperbola,

(xβˆ’h)2a2βˆ’(yβˆ’k)2b2=1,\frac{(x-h)^2}{a^2}-\frac{(y-k)^2}{b^2}=1,

the asymptotes have slope

Β±ba.\pm\frac ba.

For a vertical hyperbola,

(yβˆ’k)2a2βˆ’(xβˆ’h)2b2=1,\frac{(y-k)^2}{a^2}-\frac{(x-h)^2}{b^2}=1,

the asymptotes have slope

Β±ab.\pm\frac ab.

Example. Graph and identify the key features of

x29βˆ’y24=1.\frac{x^2}{9}-\frac{y^2}{4}=1.

The center is (0,0)(0,0). The positive term is the xx-term, so the hyperbola opens left and right.

Here

a2=9,b2=4,a^2=9,\qquad b^2=4,

so

a=3,b=2.a=3,\qquad b=2.

The vertices are

(Β±3,0).(\pm3,0).

The asymptotes are

y=Β±23x.y=\pm\frac23x.

For the foci,

c2=a2+b2=9+4=13,c^2=a^2+b^2=9+4=13,

so

c=13.c=\sqrt{13}.

The foci are

(Β±13,0),(\pm\sqrt{13},0),

and the eccentricity is

e=ca=133.e=\frac ca=\frac{\sqrt{13}}{3}.
Β‘6Β‘4Β‘2246Β‘4Β‘224xy

For a horizontal hyperbola centered at the origin,

x2a2βˆ’y2b2=1,\frac{x^2}{a^2}-\frac{y^2}{b^2}=1,

the foci are (Β±c,0)(\pm c,0), where

c2=a2+b2.c^2=a^2+b^2.

The eccentricity is

e=ca>1.e=\frac ca>1.

The directrices are

x=Β±ae=Β±a2c.x=\pm\frac ae=\pm\frac{a^2}{c}.

For a vertical hyperbola,

y2a2βˆ’x2b2=1,\frac{y^2}{a^2}-\frac{x^2}{b^2}=1,

the directrices are

y=Β±ae=Β±a2c.y=\pm\frac ae=\pm\frac{a^2}{c}.

Unlike ellipses, the directrices of a hyperbola lie between the vertices:

ae<a<c.\frac ae<a<c.
Β‘5Β‘4Β‘3Β‘2Β‘112345Β‘4Β‘224xy

Extension. Prove the standard formula for a hyperbola. This procedure should be similar to the procedure for deriving the equation for an ellipse.


Fix a point FF (focus), a line β„“\ell (directrix), and a number e>0e > 0 (eccentricity). The corresponding conic is the locus of points PP such that

PF=eβ‹…d(P,β„“),PF = e \cdot d(P,\ell),

where PFPF is the distance from PP to FF and d(P,β„“)d(P,\ell) is the perpendicular distance from PP to β„“\ell.

  • e=1e = 1: parabola.
  • 0<e<10 < e < 1: ellipse.
  • e>1e > 1: hyperbola.

(The case e=0e = 0 would force PF=0PF = 0 for every point on the directrix in a naive reading; the circle is usually treated via the two-focus definition or as a=ba = b in the ellipse equation.)

For parabolas, this matches the equal-distance definition to focus and directrix. For ellipses and hyperbolas, the same relation holds once focus and directrix are chosen consistently (a second focus appears from symmetry in the standard pictures).

The focus-directrix definition is useful because it gives one unified way to describe all three major conics. Instead of memorizing ellipse, parabola, and hyperbola as completely separate objects, you can think of them as different responses to the same rule:

distanceΒ toΒ focus=e(distanceΒ toΒ directrix).\text{distance to focus}=e(\text{distance to directrix}).

The number ee controls how strongly the point is pulled toward the focus compared with the directrix.

  • If e=1e=1, the point must stay equally far from the focus and directrix, producing a parabola.
  • If 0<e<10<e<1, the point is closer to the focus than the directrix distance would be, which creates a bounded curve: an ellipse.
  • If e>1e>1, the focus distance is larger than the directrix distance, which creates an unbounded curve: a hyperbola.

For ellipses and hyperbolas, there are two foci and two directrices. Each focus pairs with the directrix on the same side of the center. For a horizontal ellipse, the right focus pairs with the right directrix and the left focus pairs with the left directrix. The same idea works for a horizontal hyperbola.

The focus-directrix definition can be written as a ratio:

PFd(P,β„“)=e.\frac{PF}{d(P,\ell)}=e.

This ratio is constant for every point PP on the conic.

For an ellipse or hyperbola centered at the origin with a horizontal major/transverse axis:

e=ca.e=\frac ca.

This is the same eccentricity from the standard equations. The value of cc measures how far each focus is from the center, and aa measures how far each vertex is from the center. So eccentricity compares the focus distance to the vertex distance.

For an ellipse,

0<e<1,c<a,0<e<1,\qquad c<a,

so the directrices

x=Β±aex=\pm\frac ae

lie outside the ellipse.

For a hyperbola,

e>1,c>a,e>1,\qquad c>a,

so the directrices

x=Β±aex=\pm\frac ae

lie between the two vertices.

For vertical conics, replace x=Β±aex=\pm\frac ae with

y=Β±ae.y=\pm\frac ae.

It is often helpful to rewrite the directrix location as

ae=a2c,\frac ae=\frac{a^2}{c},

since e=cae=\frac ca. Thus:

Conic orientationFociDirectrices
Horizontal ellipse(hΒ±c,k)(h\pm c,k)x=hΒ±a2cx=h\pm \dfrac{a^2}{c}
Vertical ellipse(h,kΒ±c)(h,k\pm c)y=kΒ±a2cy=k\pm \dfrac{a^2}{c}
Horizontal hyperbola(hΒ±c,k)(h\pm c,k)x=hΒ±a2cx=h\pm \dfrac{a^2}{c}
Vertical hyperbola(h,kΒ±c)(h,k\pm c)y=kΒ±a2cy=k\pm \dfrac{a^2}{c}

The formula is the same, but the location feels different:

  • for ellipses, c<ac<a, so a2c>a\dfrac{a^2}{c}>a and the directrices are outside the ellipse;
  • for hyperbolas, c>ac>a, so a2c<a\dfrac{a^2}{c}<a and the directrices lie between the vertices.

Example. Find the directrices of

(y+1)225βˆ’(xβˆ’2)29=1.\frac{(y+1)^2}{25}-\frac{(x-2)^2}{9}=1.

This is a vertical hyperbola with center

(h,k)=(2,βˆ’1).(h,k)=(2,-1).

Since the positive term is the yy term,

a2=25,b2=9.a^2=25,\qquad b^2=9.

For a hyperbola,

c2=a2+b2=25+9=34,c^2=a^2+b^2=25+9=34,

so

c=34.c=\sqrt{34}.

The directrices are vertical-orientation directrices:

y=kΒ±a2c.y=k\pm\frac{a^2}{c}.

Therefore

y=βˆ’1Β±2534.y=-1\pm\frac{25}{\sqrt{34}}.

When a problem gives a focus, a directrix, and eccentricity, start from the definition instead of trying to guess the standard form immediately.

Example. Find the conic with focus (0,0)(0,0), directrix x=4x=4, and eccentricity e=12e=\frac12.

For a point P=(x,y)P=(x,y), the distance to the focus is

PF=x2+y2.PF=\sqrt{x^2+y^2}.

The distance to the directrix x=4x=4 is

d(P,β„“)=∣xβˆ’4∣.d(P,\ell)=\lvert x-4\rvert.

For points on the side of the directrix containing the focus, this is 4βˆ’x4-x. Since e=12e=\frac12,

x2+y2=12(4βˆ’x).\sqrt{x^2+y^2}=\frac12(4-x).

Square both sides:

x2+y2=14(4βˆ’x)2.x^2+y^2=\frac14(4-x)^2.

Multiply by 44:

4x2+4y2=x2βˆ’8x+16.4x^2+4y^2=x^2-8x+16.

Rearrange:

3x2+8x+4y2=16.3x^2+8x+4y^2=16.

Complete the square in xx:

3(x2+83x)+4y2=16.3\left(x^2+\frac83x\right)+4y^2=16.

Since

x2+83x=(x+43)2βˆ’169,x^2+\frac83x=\left(x+\frac43\right)^2-\frac{16}{9},

we get

3(x+43)2βˆ’163+4y2=16.3\left(x+\frac43\right)^2-\frac{16}{3}+4y^2=16.

Thus

3(x+43)2+4y2=643.3\left(x+\frac43\right)^2+4y^2=\frac{64}{3}.

Divide by 643\frac{64}{3}:

(x+43)2649+y2163=1.\frac{\left(x+\frac43\right)^2}{\frac{64}{9}}+\frac{y^2}{\frac{16}{3}}=1.

Since 0<e<10<e<1, it makes sense that the result is an ellipse.

Example. Find the foci, eccentricity, and directrices of

9x2+16y2=144.9x^2+16y^2=144.

Write in standard form:

x216+y29=1.\frac{x^2}{16}+\frac{y^2}{9}=1.

This is a horizontal ellipse with

a=4,b=3.a=4,\qquad b=3.

Then

c2=a2βˆ’b2=16βˆ’9=7,c^2=a^2-b^2=16-9=7,

so

c=7.c=\sqrt7.

The foci are

(Β±7,0).(\pm\sqrt7,0).

The eccentricity is

e=ca=74.e=\frac ca=\frac{\sqrt7}{4}.

The directrices are

x=Β±ae=Β±47/4=Β±167.x=\pm\frac ae =\pm\frac{4}{\sqrt7/4} =\pm\frac{16}{\sqrt7}.

Proof (Focus-directrix property). We show that in rectangular coordinates the locus PF=e d(P,β„“)PF = e\,d(P,\ell) is always a parabola, ellipse, or hyperbola according to ee. Take e>0e > 0 and place the focus at the origin and the directrix as the vertical line x=βˆ’dx = -d with d>0d > 0, so the focus lies to the right of the directrix. For any point P=(x,y)P = (x,y) on the same side of the directrix as the focus (so that the foot of the perpendicular has xx-coordinate βˆ’d-d and x>βˆ’dx > -d), the perpendicular distance is

d(P,β„“)=x+d.d(P,\ell) = x + d.

The defining relation is

x2+y2=e(x+d).\sqrt{x^{2} + y^{2}} = e(x + d).

Because the left side is nonnegative, every point on the locus satisfies x+dβ‰₯0x + d \ge 0. Square both sides:

x2+y2=e2(x+d)2=e2x2+2e2d x+e2d2.x^{2} + y^{2} = e^{2}(x + d)^{2} = e^{2}x^{2} + 2e^{2}d\,x + e^{2}d^{2}.

Rearrange:

(1βˆ’e2)x2βˆ’2e2d x+y2=e2d2.(1 - e^{2})x^{2} - 2e^{2}d\,x + y^{2} = e^{2}d^{2}.

Case e=1e = 1. Then this equation becomes

βˆ’2d x+y2=d2⟹y2=2d(x+d2),-2d\,x + y^{2} = d^{2} \quad\Longrightarrow\quad y^{2} = 2d\left(x + \frac{d}{2}\right),

the equation of a parabola opening to the right with vertex at (βˆ’d2, 0)\left(-\frac{d}{2},\,0\right).

Case 1: 0<e<10 < e < 1. Then 1βˆ’e2>01 - e^{2} > 0. Divide the rearranged equation by 1βˆ’e21 - e^{2} and complete the square in xx:

(xβˆ’e2d1βˆ’e2)2+y21βˆ’e2=e2d2(1βˆ’e2)2.\left(x - \frac{e^{2}d}{1 - e^{2}}\right)^{2} + \frac{y^{2}}{1 - e^{2}} = \frac{e^{2}d^{2}}{(1 - e^{2})^{2}}.

Both denominators on the left are positive after the division, so this is the equation of an ellipse in standard position (after translation of the xx-axis).

Case 2: e>1e > 1. Then 1βˆ’e2<01 - e^{2} < 0. Multiply the rearranged equation by βˆ’1-1 and write

(e2βˆ’1)x2+2e2d xβˆ’y2=βˆ’e2d2.(e^{2} - 1)x^{2} + 2e^{2}d\,x - y^{2} = -e^{2}d^{2}.

Complete the square in xx:

(e2βˆ’1)(x+e2de2βˆ’1)2βˆ’y2=e2d2e2βˆ’1,(e^{2} - 1)\left(x + \frac{e^{2}d}{e^{2} - 1}\right)^{2} - y^{2} = \frac{e^{2}d^{2}}{e^{2} - 1},

which is the equation of a hyperbola (difference of squared terms with opposite signs).

Thus the focus–directrix condition with fixed e>0e > 0 produces exactly one nondegenerate conic type in each case e=1e = 1, 0<e<10 < e < 1, and e>1e > 1. Other placements of the focus and directrix (rotations and translations) only change coordinates, not the classification.

Much of the final algebra is not shown here and is left as practice.


Place a focus at the pole (0,0)(0,0) and align the directrix perpendicular to the polar axis. With eccentricity eβ‰₯0e \ge 0 and distance to directrix (from focus) dd, polar conics usually have the form

r=ed1±ecos⁑θr=\frac{ed}{1\pm e\cos\theta}

or

r=ed1±esin⁑θ.r=\frac{ed}{1\pm e\sin\theta}.

Polar form is especially natural for conics because the pole can be placed at a focus. In rectangular form, the center is usually the most convenient reference point. In polar form, a focus is usually the most convenient reference point.

The numerator eded is sometimes called the semi-latus rectum of the conic. It is often written as pp or β„“\ell in other texts. To avoid confusing it with the parabola parameter pp from earlier, we will usually keep it as eded here.

Here:

  • ee is the eccentricity.
  • dd is the distance from the focus to the directrix.
  • eded is the numerator.

The denominator tells which direction the directrix lies.

PolarΒ equationDirectrixr=ed1+ecos⁑θx=dr=ed1βˆ’ecos⁑θx=βˆ’dr=ed1+esin⁑θy=dr=ed1βˆ’esin⁑θy=βˆ’d\begin{array}{c|c} \text{Polar equation} & \text{Directrix}\\ \hline r=\frac{ed}{1+e\cos\theta} & x=d\\ r=\frac{ed}{1-e\cos\theta} & x=-d\\ r=\frac{ed}{1+e\sin\theta} & y=d\\ r=\frac{ed}{1-e\sin\theta} & y=-d \end{array}

The trig function tells the orientation:

  • cos⁑θ\cos\theta means the directrix is vertical, since x=rcos⁑θx=r\cos\theta.
  • sin⁑θ\sin\theta means the directrix is horizontal, since y=rsin⁑θy=r\sin\theta.

The sign tells which side the directrix is on:

  • 1+ecos⁑θ1+e\cos\theta pairs with x=dx=d,
  • 1βˆ’ecos⁑θ1-e\cos\theta pairs with x=βˆ’dx=-d,
  • 1+esin⁑θ1+e\sin\theta pairs with y=dy=d,
  • 1βˆ’esin⁑θ1-e\sin\theta pairs with y=βˆ’dy=-d.

For different types of ee:

  • e=1e = 1: one unbounded branch (parabola opening toward the directrix side that makes the denominator able to go to 00).
  • e<1e < 1: bounded curve (ellipse), with a focus at the origin (which focus depends on the sign of dd).
  • e>1e > 1: two branches (hyperbola); values of ΞΈ\theta that make 1+ecos⁑θ=01 + e\cos\theta = 0 (or the corresponding denominator in your chosen form) are asymptotic directions (no finite points). The branch closest to the origin depends on the sign of dd.

For equations involving cos⁑θ\cos\theta, the easiest points to check are usually along the polar axis:

ΞΈ=0,ΞΈ=Ο€.\theta=0,\qquad \theta=\pi.

For

r=ed1+ecos⁑θ,r=\frac{ed}{1+e\cos\theta},

these give

r(0)=ed1+e,r(Ο€)=ed1βˆ’e.r(0)=\frac{ed}{1+e}, \qquad r(\pi)=\frac{ed}{1-e}.

If 0<e<10<e<1, both values are finite and positive, so they give the two vertices of the ellipse on the horizontal axis. If e=1e=1, then r(Ο€)r(\pi) is undefined, which matches the unbounded side of a parabola. If e>1e>1, the denominator can become zero for some angle, which produces asymptotic directions for a hyperbola.

For equations involving sin⁑θ\sin\theta, check

ΞΈ=Ο€2,ΞΈ=3Ο€2.\theta=\frac{\pi}{2},\qquad \theta=\frac{3\pi}{2}.

These are the positive and negative vertical directions.

Example. Find the eccentricity, directrix, and vertices of

r=61+12cos⁑θ.r=\frac{6}{1+\frac12\cos\theta}.

This is already in the form

r=ed1+ecos⁑θ.r=\frac{ed}{1+e\cos\theta}.

Thus

e=12.e=\frac12.

Since 0<e<10<e<1, the conic is an ellipse. The numerator is ed=6ed=6, so

d=61/2=12.d=\frac{6}{1/2}=12.

Because the denominator is 1+ecos⁑θ1+e\cos\theta, the directrix is

x=12.x=12.

To find the horizontal vertices, use ΞΈ=0\theta=0 and ΞΈ=Ο€\theta=\pi:

r(0)=61+12=4,r(0)=\frac{6}{1+\frac12}=4,

and

r(Ο€)=61βˆ’12=12.r(\pi)=\frac{6}{1-\frac12}=12.

So the vertices in polar form are

(4,0)Β andΒ (12,Ο€).(4,0)\text{ and }(12,\pi).

In rectangular coordinates, these points are

(4,0)Β andΒ (βˆ’12,0).(4,0)\text{ and }(-12,0).

Proof (Polar conic formula). Put the focus at the pole and let the directrix be

x=d.x=d.

For a point P=(r,ΞΈ)P=(r,\theta), the distance to the focus is

PF=r.PF=r.

Since

x=rcos⁑θ,x=r\cos\theta,

the horizontal distance from PP to the directrix is

dβˆ’rcos⁑θ.d-r\cos\theta.

Using the focus-directrix definition,

PFd(P,β„“)=e,\frac{PF}{d(P,\ell)}=e,

we get

rdβˆ’rcos⁑θ=e.\frac{r}{d-r\cos\theta}=e.

Solve for rr:

r=e(dβˆ’rcos⁑θ).r=e(d-r\cos\theta).

So

r=edβˆ’ercos⁑θ.r=ed-er\cos\theta.

Move the rr terms together:

r(1+ecos⁑θ)=ed.r(1+e\cos\theta)=ed.

Thus,

r=ed1+ecos⁑θ.r=\frac{ed}{1+e\cos\theta}.

Depending on which side the directrix is on and whether it is horizontal or vertical, the sign and trig function change.

Example. Identify the conic:

r=102βˆ’cos⁑θ.r=\frac{10}{2-\cos\theta}.

First factor the denominator:

r=102(1βˆ’12cos⁑θ)=51βˆ’12cos⁑θ.r=\frac{10}{2\left(1-\frac12\cos\theta\right)} =\frac{5}{1-\frac12\cos\theta}.

So

e=12.e=\frac12.

Since 0<e<10<e<1, the conic is an ellipse.

The numerator is eded:

ed=5.ed=5.

Since e=12e=\frac12,

d=10.d=10.

Because the denominator is

1βˆ’ecos⁑θ,1-e\cos\theta,

the directrix is

x=βˆ’d=βˆ’10.x=-d=-10.

Sometimes it is useful to convert a polar conic into rectangular form. Use

x=rcos⁑θ,y=rsin⁑θ,r2=x2+y2.x=r\cos\theta,\qquad y=r\sin\theta,\qquad r^2=x^2+y^2.

Example. Convert

r=41βˆ’cos⁑θr=\frac{4}{1-\cos\theta}

to rectangular form.

Multiply both sides by the denominator:

r(1βˆ’cos⁑θ)=4.r(1-\cos\theta)=4.

Distribute:

rβˆ’rcos⁑θ=4.r-r\cos\theta=4.

Since rcos⁑θ=xr\cos\theta=x,

rβˆ’x=4.r-x=4.

Thus

r=x+4.r=x+4.

Now square both sides:

r2=(x+4)2.r^2=(x+4)^2.

Use r2=x2+y2r^2=x^2+y^2:

x2+y2=x2+8x+16.x^2+y^2=x^2+8x+16.

Cancel x2x^2:

y2=8x+16=8(x+2).y^2=8x+16=8(x+2).

So

y2=8(x+2).y^2=8(x+2).

This is a parabola, which matches e=1e=1 from the original polar equation.

Example. Identify the conic:

r=123+4cos⁑θ.r=\frac{12}{3+4\cos\theta}.

Rewrite with constant term 11:

r=41+43cos⁑θ.r=\frac{4}{1+\frac43\cos\theta}.

Thus,

e=43.e=\frac43.

Since e>1e>1, the conic is a hyperbola.

The numerator is ed=4ed=4, so

d=44/3=3.d=\frac{4}{4/3}=3.

Because the denominator is

1+ecos⁑θ,1+e\cos\theta,

the directrix is

x=3.x=3.

The denominator is zero when

1+43cos⁑θ=0,1+\frac43\cos\theta=0,

so

cos⁑θ=βˆ’34.\cos\theta=-\frac34.

These angles give the asymptotic directions of the hyperbola.

Β‘8Β‘6Β‘4Β‘2246Β‘6Β‘4Β‘2246xy

Polar conics appear naturally in orbital motion because one focus is physically important. For example:

  • Planets and many moons move in elliptical orbits with the central body at one focus.
  • Some comets follow parabolic-type escape paths.
  • Objects that pass by a planet and escape can follow hyperbolic paths.

This is why polar equations with a focus at the pole are often more natural than rectangular equations for astronomy and central-force motion.

  1. Complete the square for 4x2+9y2βˆ’24x+36y+36=04x^{2}+9y^{2}-24x+36y+36=0. Write the equation in standard form and give the center, vertices, co-vertices, foci, eccentricity, and major/minor axis lengths. Graph the conic.
  1. Find the equation of the parabola whose focus is (5,βˆ’2)(5,-2) and whose directrix is x=βˆ’1x=-1. Give the vertex, value of pp, axis of symmetry, and latus rectum endpoints.
  1. Find all lines with slope βˆ’2-2 that are tangent to the parabola (xβˆ’1)2=8(y+3)(x-1)^{2}=8(y+3).
  1. An ellipse has foci (1,4)(1,4) and (1,βˆ’2)(1,-2) and passes through (5,1)(5,1). Find its standard-form equation and its eccentricity.
  1. The ellipse (x+2)236+(yβˆ’1)220=1\dfrac{(x+2)^{2}}{36}+\dfrac{(y-1)^{2}}{20}=1 has foci F1F_1 and F2F_2. If PP is the point on the ellipse with x=1x=1 and y>1y>1, find PF1PF_1 and PF2PF_2 separately.
  1. Find all real numbers mm such that the line y=mx+3y=mx+3 is tangent to the ellipse x29+y24=1\dfrac{x^{2}}{9}+\dfrac{y^{2}}{4}=1.
  1. Complete the square for 9y2βˆ’4x2βˆ’54yβˆ’16x+29=09y^{2}-4x^{2}-54y-16x+29=0. Write the equation in standard form and give the center, vertices, foci, eccentricity, and asymptotes. Graph the conic.
  1. A hyperbola has center (2,βˆ’1)(2,-1), asymptotes y+1=Β±32(xβˆ’2)y+1=\pm\dfrac{3}{2}(x-2), and one focus at (2+52,βˆ’1)(2+\sqrt{52},-1). Assuming it opens left/right, find its standard-form equation.
  1. Find all intersection points in R2\mathbb{R}^{2} of the ellipse x216+y29=1\dfrac{x^{2}}{16}+\dfrac{y^{2}}{9}=1 and the hyperbola x24βˆ’y29=1\dfrac{x^{2}}{4}-\dfrac{y^{2}}{9}=1.
  1. With focus at (0,0)(0,0), directrix x=βˆ’6x=-6, and eccentricity e=23e=\dfrac{2}{3}, derive the Cartesian equation of the conic. Write it in standard form and identify the conic type.
  1. Convert r=102βˆ’cos⁑θr=\dfrac{10}{2-\cos\theta} to a Cartesian equation. Identify the conic type, eccentricity, center, vertices, and foci.
  1. For r=123+4cos⁑θr=\dfrac{12}{3+4\cos\theta}, identify the conic type and eccentricity, then find the values of θ\theta where the denominator vanishes. Explain what those angles represent geometrically.
  1. A circle is tangent to both axes in Quadrant I and its center lies on the ellipse x225+y29=1\dfrac{x^{2}}{25}+\dfrac{y^{2}}{9}=1. Find the circle’s radius.
  1. Show that the conic Ax2+Cy2+Dx+Ey+F=0Ax^{2}+Cy^{2}+Dx+Ey+F=0 has center (h,k)(h,k) when Aβ‰ 0A\ne 0 and Cβ‰ 0C\ne 0. Derive formulas for hh and kk in terms of A,C,D,EA,C,D,E, then find the center of 5x2βˆ’3y2+20x+18yβˆ’11=05x^{2}-3y^{2}+20x+18y-11=0.
  1. For the parabola y2=4pxy^{2}=4px with p>0p>0, let a line through the focus (p,0)(p,0) have slope mβ‰ 0m\ne 0 and meet the parabola at two distinct points AA and BB. Prove that the product of the yy-coordinates of AA and BB equals βˆ’4p2-4p^{2}.
  1. (Bonus, 2026 USAPhO)

You are studying the motion of charged particles constrained to the xyxy-plane. Particle Ξ±\alpha, with charge +1Β C+1\ \mathrm{C}, is fixed at the origin.

For motion under an inverse-square central force, trajectories are conic sections with the fixed particle at a focus. In polar coordinates:

  • For an attractive interaction (ellipse),
r=r01+ecos⁑ϕ,e<1.r=\frac{r_0}{1+e\cos\phi},\qquad e<1.
  • For a repulsive interaction (hyperbola),
r=r0ecosβ‘Ο•βˆ’1,e>1.r=\frac{r_0}{e\cos\phi-1},\qquad e>1.

You have a camera that takes three snapshots of a moving particle at equal time intervals.

(A)(A) A particle Ξ²\beta, with charge βˆ’1Β C-1\ \mathrm{C}, moves under the electrostatic force of particle Ξ±\alpha. In three consecutive snapshots, its positions are

(0,βˆ’5Β m),(3Β m,0),(0,5Β m).(0,-5\ \mathrm{m}),\qquad (3\ \mathrm{m},0),\qquad (0,5\ \mathrm{m}).

Assuming the motion is governed only by the Coulomb interaction with Ξ±\alpha, determine the maximum distance that particle Ξ²\beta reaches from the origin.

(B)(B) Now particle Ξ²\beta is replaced by particle Ξ³\gamma, which has charge +2Β C+2\ \mathrm{C} and is free to move in the plane. In three consecutive snapshots, its positions are

(3Β m,βˆ’4Β m),(2Β m,0),(3Β m,4Β m).(3\ \mathrm{m},-4\ \mathrm{m}),\qquad (2\ \mathrm{m},0),\qquad (3\ \mathrm{m},4\ \mathrm{m}).

Assuming the motion is governed only by the Coulomb interaction with Ξ±\alpha, determine the angle ΞΈ\theta, measured from the positive xx-axis, of the velocity of particle Ξ³\gamma at a large time.

(C)(C) A family of particles, each identical to particle γ\gamma (that is, each has charge +2 C+2\ \mathrm{C}), approaches from infinity in the xyxy-plane. All particles have the same speed v∞v_{\infty} far from the origin and move along lines parallel to the initial asymptotic direction of particle γ\gamma from part (B)(B). The particles are injected one at a time, so they do not interact with one another.

For each trajectory, define the impact parameter BB to be the perpendicular distance between the initial straight-line path of the particle and the origin.

As a particle passes near the scattering center, its direction changes due to Coulomb repulsion. Let Ξ±\alpha denote the total deflection angle of the trajectory, i.e. the angle between the incoming and outgoing asymptotic directions.

(i)(i) Using the conic form of the trajectory, derive a formula for B(Ξ±)B(\alpha).

(ii)(ii) Using the result of part (B)(B), express B(Ξ±)B(\alpha) in terms of r0r_0.