A conic section is the curve you get when a plane meets a right circular cone: circle, ellipse, parabola, or hyperbola (the βdegenerateβ 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 x and y:
Ax2+Bxy+Cy2+Dx+Ey+F=0
with A,B,C not all zero. In most precalculus work B=0 (no tilted axes); then the graph is a parabola, ellipse, or hyperbola depending on the signs of A and C after completing squares.
The eccentricity e measures how βstretchedβ the conic is relative to a circle (e=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 P whose distance to the focus equals e times the perpendicular distance to the directrix. Then 0<e<1 gives an ellipse, e=1 a parabola, and e>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=0. Since circles are extensively talked about in other sections, I will not go in detail about them.
The latus rectum is the chord through the focus perpendicular to the axis of symmetry, with a length of β£4pβ£ (same as the absolute coefficient in the standard forms above). It should be parallel to the directrix.
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 d. Define the focal ratio as dpβ. This is what the f-stops are defined as in photography.
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 donβt really get a special name. The semi-major and semi-minor axes are defined as half of their respective axes.
If the denominators are equal (a=b), the ellipse is a circle of radius a.
Proof (Standard equation of an ellipse, horizontal major axis). Place the foci on the x-axis at F1β=(βc,0) and F2β=(c,0) with 0<c<a. The ellipse is the set of points P=(x,y) such that the sum of distances to the foci is the constant 2a:
(x+c)2+y2β+(xβc)2+y2β=2a.
Write r1β=(x+c)2+y2β and r2β=(xβc)2+y2β, so r1β+r2β=2a. Isolate r1β=2aβr2β and square (both sides are nonnegative):
(x+c)2+y2=4a2β4ar2β+(xβc)2+y2.
Expand and cancel x2, y2, and c2:
4cx=4a2β4ar2ββΉar2β=a2βcx.
Since r2ββ₯0 and (one can show) β£cxβ£β€a2 on the ellipse, the right-hand side is nonnegative, so we may square again:
Define b2=a2βc2>0. Then b2x2+a2y2=a2b2. Divide by a2b2:
a2x2β+b2y2β=1.
Thus the two-focus definition yields the standard equation with c2=a2βb2. Translating the center to (h,k) replaces x by xβh and y by yβk, giving a2(xβh)2β+b2(yβk)2β=1.
For a vertical major axis, the same algebra applies after swapping the roles of x and y (foci on the vertical line through the center), which produces b2(xβh)2β+a2(yβk)2β=1 with a>b and again c2=a2βb2.
the foci are (Β±c,0), where c2=a2βb2, and the eccentricity is
e=acβ.
The directrices are
x=Β±eaβ.
Since e=acβ, this can also be written as
x=Β±ca2β.
For a vertical ellipse,
b2x2β+a2y2β=1,
the directrices are
y=Β±eaβ=Β±ca2β.
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.
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 Museumβs βWhispering Room,β 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 β or 0). The transverse axis passes through the vertices.
Horizontal transverse axis (opens left/right, center (h,k))
The conjugate hyperbola swaps the roles of the terms (e.g. a2y2ββb2x2β=1 vs a2x2ββb2y2β=1) and shares the same asymptote rectangle but different vertices and branches.
Fix a point F (focus), a line β (directrix), and a number e>0 (eccentricity). The corresponding conic is the locus of points P such that
PF=eβ d(P,β),
where PF is the distance from P to F and d(P,β) is the perpendicular distance from P to β.
e=1: parabola.
0<e<1: ellipse.
e>1: hyperbola.
(The case e=0 would force PF=0 for every point on the directrix in a naive reading; the circle is usually treated via the two-focus definition or as a=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).
The number e controls how strongly the point is pulled toward the focus compared with the directrix.
If e=1, the point must stay equally far from the focus and directrix, producing a parabola.
If 0<e<1, the point is closer to the focus than the directrix distance would be, which creates a bounded curve: an ellipse.
If e>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:
d(P,β)PFβ=e.
This ratio is constant for every point P on the conic.
For an ellipse or hyperbola centered at the origin with a horizontal major/transverse axis:
e=acβ.
This is the same eccentricity from the standard equations. The value of c measures how far each focus is from the center, and a 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,
so the directrices
x=Β±eaβ
lie outside the ellipse.
For a hyperbola,
e>1,c>a,
so the directrices
x=Β±eaβ
lie between the two vertices.
For vertical conics, replace x=Β±eaβ with
y=Β±eaβ.
It is often helpful to rewrite the directrix location as
eaβ=ca2β,
since e=acβ. Thus:
Conic orientation
Foci
Directrices
Horizontal ellipse
(hΒ±c,k)
x=hΒ±ca2β
Vertical ellipse
(h,kΒ±c)
y=kΒ±ca2β
Horizontal hyperbola
(hΒ±c,k)
x=hΒ±ca2β
Vertical hyperbola
(h,kΒ±c)
y=kΒ±ca2β
The formula is the same, but the location feels different:
for ellipses, c<a, so ca2β>a and the directrices are outside the ellipse;
for hyperbolas, c>a, so ca2β<a and the directrices lie between the vertices.
Example. Find the directrices of
25(y+1)2ββ9(xβ2)2β=1.
This is a vertical hyperbola with center
(h,k)=(2,β1).
Since the positive term is the y term,
a2=25,b2=9.
For a hyperbola,
c2=a2+b2=25+9=34,
so
c=34β.
The directrices are vertical-orientation directrices:
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), directrix x=4, and eccentricity e=21β.
For a point P=(x,y), the distance to the focus is
PF=x2+y2β.
The distance to the directrix x=4 is
d(P,β)=β£xβ4β£.
For points on the side of the directrix containing the focus, this is 4βx. Since e=21β,
x2+y2β=21β(4βx).
Square both sides:
x2+y2=41β(4βx)2.
Multiply by 4:
4x2+4y2=x2β8x+16.
Rearrange:
3x2+8x+4y2=16.
Complete the square in x:
3(x2+38βx)+4y2=16.
Since
x2+38βx=(x+34β)2β916β,
we get
3(x+34β)2β316β+4y2=16.
Thus
3(x+34β)2+4y2=364β.
Divide by 364β:
964β(x+34β)2β+316βy2β=1.
Since 0<e<1, it makes sense that the result is an ellipse.
Example. Find the foci, eccentricity, and directrices of
9x2+16y2=144.
Write in standard form:
16x2β+9y2β=1.
This is a horizontal ellipse with
a=4,b=3.
Then
c2=a2βb2=16β9=7,
so
c=7β.
The foci are
(Β±7β,0).
The eccentricity is
e=acβ=47ββ.
The directrices are
x=Β±eaβ=Β±7β/44β=Β±7β16β.
Proof (Focus-directrix property). We show that in rectangular coordinates the locus PF=ed(P,β) is always a parabola, ellipse, or hyperbola according to e. Take e>0 and place the focus at the origin and the directrix as the vertical line x=βd with d>0, so the focus lies to the right of the directrix. For any point P=(x,y) on the same side of the directrix as the focus (so that the foot of the perpendicular has x-coordinate βd and x>βd), the perpendicular distance is
d(P,β)=x+d.
The defining relation is
x2+y2β=e(x+d).
Because the left side is nonnegative, every point on the locus satisfies x+dβ₯0. Square both sides:
x2+y2=e2(x+d)2=e2x2+2e2dx+e2d2.
Rearrange:
(1βe2)x2β2e2dx+y2=e2d2.
Case e=1. Then this equation becomes
β2dx+y2=d2βΉy2=2d(x+2dβ),
the equation of a parabola opening to the right with vertex at (β2dβ,0).
Case 1: 0<e<1. Then 1βe2>0. Divide the rearranged equation by 1βe2 and complete the square in x:
(xβ1βe2e2dβ)2+1βe2y2β=(1βe2)2e2d2β.
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 x-axis).
Case 2: e>1. Then 1βe2<0. Multiply the rearranged equation by β1 and write
(e2β1)x2+2e2dxβy2=βe2d2.
Complete the square in x:
(e2β1)(x+e2β1e2dβ)2βy2=e2β1e2d2β,
which is the equation of a hyperbola (difference of squared terms with opposite signs).
Thus the focusβdirectrix condition with fixed e>0 produces exactly one nondegenerate conic type in each case e=1, 0<e<1, and e>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) and align the directrix perpendicular to the polar axis. With eccentricity eβ₯0 and distance to directrix (from focus) d, polar conics usually have the form
r=1Β±ecosΞΈedβ
or
r=1Β±esinΞΈedβ.
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 ed is sometimes called the semi-latus rectum of the conic. It is often written as p or β in other texts. To avoid confusing it with the parabola parameter p from earlier, we will usually keep it as ed here.
Here:
e is the eccentricity.
d is the distance from the focus to the directrix.
ed is the numerator.
The denominator tells which direction the directrix lies.
cosΞΈ means the directrix is vertical, since x=rcosΞΈ.
sinΞΈ means the directrix is horizontal, since y=rsinΞΈ.
The sign tells which side the directrix is on:
1+ecosΞΈ pairs with x=d,
1βecosΞΈ pairs with x=βd,
1+esinΞΈ pairs with y=d,
1βesinΞΈ pairs with y=βd.
For different types of e:
e=1: one unbounded branch (parabola opening toward the directrix side that makes the denominator able to go to 0).
e<1: bounded curve (ellipse), with a focus at the origin (which focus depends on the sign of d).
e>1: two branches (hyperbola); values of ΞΈ that make 1+ecosΞΈ=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 d.
For equations involving cosΞΈ, the easiest points to check are usually along the polar axis:
ΞΈ=0,ΞΈ=Ο.
For
r=1+ecosΞΈedβ,
these give
r(0)=1+eedβ,r(Ο)=1βeedβ.
If 0<e<1, both values are finite and positive, so they give the two vertices of the ellipse on the horizontal axis. If e=1, then r(Ο) is undefined, which matches the unbounded side of a parabola. If e>1, the denominator can become zero for some angle, which produces asymptotic directions for a hyperbola.
For equations involving sinΞΈ, check
ΞΈ=2Οβ,ΞΈ=23Οβ.
These are the positive and negative vertical directions.
Example. Find the eccentricity, directrix, and vertices of
r=1+21βcosΞΈ6β.
This is already in the form
r=1+ecosΞΈedβ.
Thus
e=21β.
Since 0<e<1, the conic is an ellipse. The numerator is ed=6, so
d=1/26β=12.
Because the denominator is 1+ecosΞΈ, the directrix is
x=12.
To find the horizontal vertices, use ΞΈ=0 and ΞΈ=Ο:
r(0)=1+21β6β=4,
and
r(Ο)=1β21β6β=12.
So the vertices in polar form are
(4,0)Β andΒ (12,Ο).
In rectangular coordinates, these points are
(4,0)Β andΒ (β12,0).
Proof (Polar conic formula). Put the focus at the pole and let the directrix be
x=d.
For a point P=(r,ΞΈ), the distance to the focus is
PF=r.
Since
x=rcosΞΈ,
the horizontal distance from P to the directrix is
dβrcosΞΈ.
Using the focus-directrix definition,
d(P,β)PFβ=e,
we get
dβrcosΞΈrβ=e.
Solve for r:
r=e(dβrcosΞΈ).
So
r=edβercosΞΈ.
Move the r terms together:
r(1+ecosΞΈ)=ed.
Thus,
r=1+ecosΞΈedβ.
Depending on which side the directrix is on and whether it is horizontal or vertical, the sign and trig function change.
Complete the square for 4x2+9y2β24x+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.
Complete the square:
4x2+9y2β24x+36y+36=04(x2β6x)+9(y2+4y)+36=0.
Then
4((xβ3)2β9)+9((y+2)2β4)+36=0.
Simplify:
4(xβ3)2+9(y+2)2=36.
Divide by 36:
9(xβ3)2β+4(y+2)2β=1.
This is an ellipse centered at (3,β2) with horizontal major axis. Here a2=9, b2=4, so a=3 and b=2. Also
c2=a2βb2=9β4=5,
so c=5β and e=acβ=35ββ.
Thus
9(xβ3)2β+4(y+2)2β=1β
with center (3,β2)β, vertices (0,β2),(6,β2)β, co-vertices (3,β4),(3,0)β, foci (3β5β,β2),(3+5β,β2)β, eccentricity 35βββ, major axis length 6β, and minor axis length 4β.
The graph of the conic is displayed below:
Find the equation of the parabola whose focus is (5,β2) and whose directrix is x=β1. Give the vertex, value of p, axis of symmetry, and latus rectum endpoints.
The focus is (5,β2) and the directrix is x=β1, so the parabola opens horizontally. The vertex is halfway between the focus and directrix along the horizontal axis:
(25+(β1)β,β2)=(2,β2).
Thus h=2 and k=β2. Since the focus is (h+p,k)=(5,β2),
p=3.
Use the horizontal parabola form
(yβk)2=4p(xβh).
So
(y+2)2=12(xβ2)β.
The axis of symmetry is y=β2β. The latus rectum is vertical through the focus. Its length is β£4pβ£=12, so its endpoints are 6 units above and below the focus:
(5,4)Β andΒ (5,β8)β.
Find all lines with slope β2 that are tangent to the parabola (xβ1)2=8(y+3).
A line with slope β2 has equation
y=β2x+b.
Substitute into the parabola
(xβ1)2=8(y+3).
Then
(xβ1)2=8(β2x+b+3).
Expand:
x2β2x+1=β16x+8b+24.
Move everything to one side:
x2+14xβ(8b+23)=0.
For the line to be tangent, this quadratic must have exactly one solution, so its discriminant is 0:
142β4(1)(β(8b+23))=0.
Thus
196+32b+92=0βΉ32b=β288βΉb=β9.
Therefore the tangent line is
y=β2xβ9β.
An ellipse has foci (1,4) and (1,β2) and passes through (5,1). Find its standard-form equation and its eccentricity.
The foci (1,4) and (1,β2) have midpoint
(h,k)=(1,24+(β2)β)=(1,1).
The foci are vertical, so the major axis is vertical. The distance from the center to either focus is
c=3.
The point (5,1) lies on the ellipse. Its distances to the foci are
(5β1)2+(1β4)2β=5
and
(5β1)2+(1β(β2))2β=5.
The sum of distances is 10, so 2a=10 and a=5. Then
b2=a2βc2=25β9=16.
Since the major axis is vertical,
16(xβ1)2β+25(yβ1)2β=1β.
The eccentricity is
e=acβ=53ββ.
The ellipse 36(x+2)2β+20(yβ1)2β=1 has foci F1β and F2β. If P is the point on the ellipse with x=1 and y>1, find PF1β and PF2β separately.
The ellipse
36(x+2)2β+20(yβ1)2β=1
has center (β2,1), a2=36, and b2=20. Therefore
c2=a2βb2=36β20=16,
so c=4. The foci are
(β2β4,1)=(β6,1)and(β2+4,1)=(2,1).
Now use x=1:
36(1+2)2β+20(yβ1)2β=1.
So
369β+20(yβ1)2β=1βΉ20(yβ1)2β=43β.
Thus
(yβ1)2=15.
Since y>1,
y=1+15β.
So P=(1,1+15β). Its distance to the right focus (2,1) is
(1β2)2+(15β)2β=16β=4.
Its distance to the left focus (β6,1) is
(1+6)2+(15β)2β=64β=8.
Therefore
PFrightβ=4andPFleftβ=8β.
Find all real numbers m such that the line y=mx+3 is tangent to the ellipse 9x2β+4y2β=1.
Substitute y=mx+3 into
9x2β+4y2β=1.
Then
9x2β+4(mx+3)2β=1.
Multiply by 36:
4x2+9(mx+3)2=36.
Expand:
4x2+9(m2x2+6mx+9)=36.
So
(4+9m2)x2+54mx+45=0.
For tangency, the discriminant must be 0:
(54m)2β4(4+9m2)(45)=0.
Simplify:
2916m2β180(4+9m2)=01296m2β720=0βΉm2=95β.
Thus
m=Β±35βββ.
Complete the square for 9y2β4x2β54yβ16x+29=0. Write the equation in standard form and give the center, vertices, foci, eccentricity, and asymptotes. Graph the conic.
Start with
9y2β4x2β54yβ16x+29=0.
Group and complete the square:
9(y2β6y)β4(x2+4x)+29=0.
Then
9((yβ3)2β9)β4((x+2)2β4)+29=0.
Simplify:
9(yβ3)2β4(x+2)2β36=0.
So
9(yβ3)2β4(x+2)2=36.
Divide by 36:
4(yβ3)2ββ9(x+2)2β=1β.
This is a vertical hyperbola. The center is (β2,3). Here a2=4, b2=9, so a=2 and b=3. Also
c2=a2+b2=4+9=13,
so c=13β and e=213ββ.
The vertices are
(β2,1)Β andΒ (β2,5)β.
The foci are
(β2,3β13β)Β andΒ (β2,3+13β)β.
The asymptotes are
yβ3=Β±32β(x+2)β.
An image of the hyperbola is shown below:
A hyperbola has center (2,β1), asymptotes y+1=Β±23β(xβ2), and one focus at (2+52β,β1). Assuming it opens left/right, find its standard-form equation.
A horizontal hyperbola centered at (2,β1) has form
a2(xβ2)2ββb2(y+1)2β=1.
Its asymptotes are
y+1=Β±abβ(xβ2).
We are given slope 23β, so
abβ=23β.
Let a=2t and b=3t. The focus distance satisfies
c2=a2+b2.
Since one focus is (2+52β,β1), we have c=52β. Thus
52=(2t)2+(3t)2=13t2.
So t2=4, and therefore
a2=(2t)2=16,b2=(3t)2=36.
Thus the equation is
16(xβ2)2ββ36(y+1)2β=1β.
Find all intersection points in R2 of the ellipse 16x2β+9y2β=1 and the hyperbola 4x2ββ9y2β=1.
All sign combinations work, so the intersection points are
(Β±5410ββ,Β±5315ββ)β.
With focus at (0,0), directrix x=β6, and eccentricity e=32β, derive the Cartesian equation of the conic. Write it in standard form and identify the conic type.
The focus is (0,0) and the directrix is x=β6. For a point (x,y) on the conic,
PF=x2+y2β
and
d(P,β)=x+6
on the appropriate side of the directrix. Since e=32β,
x2+y2β=32β(x+6).
Square both sides:
x2+y2=94β(x+6)2.
Multiply by 9:
9x2+9y2=4x2+48x+144.
So
5x2+9y2β48xβ144=0.
Complete the square in x:
5(x2β548βx)+9y2=144.
Since
x2β548βx=(xβ524β)2β25576β,
we get
5(xβ524β)2+9y2=51296β.
Divide by 51296β:
251296β(xβ524β)2β+5144βy2β=1β.
Since 0<e<1, this conic is an ellipse.
Convert r=2βcosΞΈ10β to a Cartesian equation. Identify the conic type, eccentricity, center, vertices, and foci.
Start with
r=2βcosΞΈ10β.
Rewrite:
2rβrcosΞΈ=10.
Use r=x2+y2β and rcosΞΈ=x:
2x2+y2ββx=10.
So
2x2+y2β=x+10.
Square both sides:
4(x2+y2)=(x+10)2.
Expand:
4x2+4y2=x2+20x+100.
So
3x2+4y2β20xβ100=0.
Complete the square:
3(x2β320βx)+4y2=100.
Since
x2β320βx=(xβ310β)2β9100β,
we get
3(xβ310β)2+4y2=3400β.
Divide by 3400β:
9400β(xβ310β)2β+3100βy2β=1β.
The conic is an ellipse. From
r=2βcosΞΈ10β=1β21βcosΞΈ5β,
the eccentricity is e=21ββ. The center is (310β,0)β. Since a2=9400β, a=320β. The vertices are
(β310β,0)Β andΒ (10,0)β.
Also c=ea=310β, so the foci are
(0,0)Β andΒ (320β,0)β.
For r=3+4cosΞΈ12β, identify the conic type and eccentricity, then find the values of ΞΈ where the denominator vanishes. Explain what those angles represent geometrically.
At those angles, r is not finite. Geometrically, they give the asymptotic directions of the hyperbola.
A circle is tangent to both axes in Quadrant I and its center lies on the ellipse 25x2β+9y2β=1. Find the circleβs radius.
A circle tangent to both axes in Quadrant I has center (r,r) and radius r. Since the center lies on
25x2β+9y2β=1,
substitute (r,r):
25r2β+9r2β=1.
Then
r2(251β+91β)=1.
Compute:
251β+91β=2259+25β=22534β.
So
r2β 22534β=1βΉr2=34225β.
Since r>0,
r=34β15β=341534βββ.
Show that the conic Ax2+Cy2+Dx+Ey+F=0 has center (h,k) when Aξ =0 and Cξ =0. Derive formulas for h and k in terms of A,C,D,E, then find the center of 5x2β3y2+20x+18yβ11=0.
Start with
Ax2+Cy2+Dx+Ey+F=0,
where Aξ =0 and Cξ =0. Complete the square separately in x and y:
A(x2+ADβx)+C(y2+CEβy)+F=0.
The centers of the completed squares occur at
x=β2ADβandy=β2CEβ.
Therefore the center is
(β2ADβ,β2CEβ)β.
For
5x2β3y2+20x+18yβ11=0,
we have A=5, C=β3, D=20, and E=18. Thus
h=β2(5)20β=β2
and
k=β2(β3)18β=3.
So the center is
(β2,3)β.
For the parabola y2=4px with p>0, let a line through the focus (p,0) have slope mξ =0 and meet the parabola at two distinct points A and B. Prove that the product of the y-coordinates of A and B equals β4p2.
The parabola is
y2=4px,
and its focus is (p,0). A line through the focus with slope mξ =0 has equation
y=m(xβp).
Solve this for x:
x=p+myβ.
Substitute into the parabola:
y2=4p(p+myβ).
Expand:
y2=4p2+m4pβy.
Move everything to one side:
y2βm4pβyβ4p2=0.
This quadratic has roots equal to the y-coordinates of the two intersection points A and B. By Vietaβs formula, the product of the roots is the constant term divided by the leading coefficient:
yAβyBβ=1β4p2β.
Therefore
yAβyBβ=β4p2β.
(Bonus, 2026 USAPhO)
You are studying the motion of charged particles constrained to the xy-plane. Particle Ξ±, with charge +1Β 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=1+ecosΟr0ββ,e<1.
For a repulsive interaction (hyperbola),
r=ecosΟβ1r0ββ,e>1.
You have a camera that takes three snapshots of a moving particle at equal time intervals.
(A) A particle Ξ², with charge β1Β C, moves under the electrostatic force of particle Ξ±. In three consecutive snapshots, its positions are
(0,β5Β m),(3Β m,0),(0,5Β m).
Assuming the motion is governed only by the Coulomb interaction with Ξ±, determine the maximum distance that particle Ξ² reaches from the origin.
(B) Now particle Ξ² is replaced by particle Ξ³, which has charge +2Β C and is free to move in the plane. In three consecutive snapshots, its positions are
(3Β m,β4Β m),(2Β m,0),(3Β m,4Β m).
Assuming the motion is governed only by the Coulomb interaction with Ξ±, determine the angle ΞΈ, measured from the positive x-axis, of the velocity of particle Ξ³ at a large time.
(C) A family of particles, each identical to particle Ξ³ (that is, each has charge +2Β C), approaches from infinity in the xy-plane. All particles have the same speed vββ far from the origin and move along lines parallel to the initial asymptotic direction of particle Ξ³ from part (B). The particles are injected one at a time, so they do not interact with one another.
For each trajectory, define the impact parameterB 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± denote the total deflection angle of the trajectory, i.e. the angle between the incoming and outgoing asymptotic directions.
(i) Using the conic form of the trajectory, derive a formula for B(Ξ±).
(ii) Using the result of part (B), express B(Ξ±) in terms of r0β.
For part (A), use the attractive model
r=1+ecosΟr0ββ.
Since the first and third snapshots are at (0,β5) and (0,5), while the middle snapshot is at (3,0), and the time intervals are equal, the path is symmetric about the x-axis. Therefore, (3,0) is the closest point to the origin, called the pericenter.
At pericenter, Ο=0, so
rminβ=1+er0ββ=3.
The other two photographed points are on the y-axis. There,
Ο=Β±2Οβ,r=5.
Since cos(Β±2Οβ)=0,
5=1+e(0)r0ββ=r0β.
So
r0β=5.
Now use the pericenter equation:
3=1+e5β.
Thus,
1+e=35β,
so
e=32β.
The farthest point on the ellipse is the apocenter, where Ο=Ο and cosΟ=β1. Therefore,
rmaxβ=1βer0ββ=1β32β5β=15.
So
rmaxβ=15Β mβ.
For part (B), use the repulsive model
r=ecosΟβ1r0ββ.
Again, the first and third snapshots are symmetric about the x-axis, and the middle snapshot is at (2,0). Since the snapshots are equally spaced in time, (2,0) is the point of closest approach.
At closest approach,
rminβ=eβ1r0ββ=2.
Thus,
r0β=2(eβ1).
Now use the point (3,4). Its distance from the origin is
r=32+42β=5,
and
cosΟ=rxβ=53β.
Substitute into the polar equation:
5=eβ 53ββ1r0ββ.
Using r0β=2(eβ1),
5=53βeβ12(eβ1)β.
Multiply through:
5(53βeβ1)=2(eβ1).
So
3eβ5=2eβ2,
which gives
e=3.
Then
r0β=2(eβ1)=4.
At large times, the particle approaches an asymptote of the hyperbola. The asymptote occurs when the denominator goes to zero:
ecosΟβ1=0.
Therefore,
cosΟ=e1β=31β.
Thus the outgoing velocity direction at large positive time is
ΞΈ=arccos(31β)β
measured from the positive x-axis. Numerically,
ΞΈβ70.5β.
For part (C), for a repulsive inverse-square force, the trajectory is
r=ecosΟβ1r0ββ,e>1.
The asymptotes occur when the denominator vanishes:
ecosΟβ1=0.
Thus,
cosΟ=e1β.
The two asymptotes are symmetric about the x-axis, so the total deflection angle is
Ξ±=2Ο=2arccos(e1β).
Hence,
cos(2Ξ±β)=e1β,
so
e=cos(Ξ±/2)1β.
Now relate the impact parameter B to the conic parameters. Starting from
The impact parameter B is the perpendicular distance from the origin to the incoming asymptote. For a line
y=m(xβh),
the distance from the origin is
m2+1ββ£mhβ£β.
Here
m=e2β1β
and
h=e2β1er0ββ.
Therefore,
B=(e2β1)+1βe2β1ββ e2β1er0βββ.
Since (e2β1)+1β=e,
B=e2β1βr0ββ.
Now substitute
e=cos(Ξ±/2)1β.
Then
e2β1=cos2(Ξ±/2)1ββ1=tan2(2Ξ±β).
So
e2β1β=tan(2Ξ±β).
Therefore,
B(Ξ±)=r0βcot(2Ξ±β)β.
For the particular trajectory in part (B), the asymptote angle satisfies
cos(2Ξ±β)=31β,
so
tan(2Ξ±β)=22β.
Therefore, for any trajectory whose asymptote angle matches the one from part (B),
B=r0βcot(2Ξ±β)=22βr0ββ.
For the specific particle in part (B), r0β=4, so
B=22β4β=2βΒ m.
Note that the answer may be different depending on how you define the asymptote angle, so always match your work instead of necessarily matching solutions.