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Here we investigate
the relationships between the parameters of
the conic sections and the sections
themselves. When the conic is centered at
the origin its general equation is called
its central
equation.
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central equation:

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For the
ellipse we have four different
parameters a,
b,
x, and y, whose
changes we'll study for their
effects on the graph of the
ellipse.
Shown is an ellipse whose
major axis is along the X axis.
(What follows holds with the
vertical ellipse whose major axis
is along the Y
axis.)
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C
is the
distance to a focus from the
origin. a
and
b
are the
lengths of the semi major and semi
minor axis, respectively. (A
vertical ellipse would have b as
the length of the semi major axis
since it lies on the Y axis, and a
as the length of the semi minor
axis along the X axis.)
Say we keep
a
constant, that
is the length of the semi major
axis constant. Now lets vary
c.
Remember, a
is constant,
so the left hand side of the
following equation does not
change.
a2 =
c2 ↑
+
b2↓
and
a2 =
c2 ↓+
b2
↑
The triangle shows this
relationship. If c increases
and a stays
constant then the hypotenuse
a must
rotate toward the leg c.
For this to occur, the other leg
b must
decrease.
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Herea
= 6. We start
off with the cyan ellipse. Now move
the focal points toward the origin
by making c
smaller and
smaller. b
climbs the Y
axis to the limiting point
of b =
a.
At his point
our ellipse has become a circle
with radius a=b.
c2
decreases to 0
as c
decreases to
0, so we then
have
a2
=
c2
↓
0
+
b2
↑
(↓0
means
decreases toward
0)
until a2 = 0 +
b2
Now b =
a and
c is the
origin, which gives us a circle
(the magenta
ellipse).
If instead, we start with
c = 1, the
magenta ellipse and increase it to
c = 5.7,
then the ellipse flattens to the
cyan ellipse. If c continues
to increase until c = 6, that
is, c =
a, then our
ellipse has degenerated into two
line segments, one for the top and
one for the bottom of the ellipse
from x = -6 to x =
6.
a2
=
c2
↑
+
b2
↓
until
a2
=
c2
which means
a2
-
c2
=
0 = b2
so b =
0
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Now let's keep the focal
points constant, i.e.,
c
constant and
vary a
(or
b).
If a
increases, so
must b
to maintain
the equality. (Likewise if
a
decreases so
must b.)
a2↑
=
c2
+
b2↑
and
a2↓
=
c2
+
b2↓
We start with the green
ellipse. The two black dots are the
foci. Now as we increase
a,
b also
increases giving the cyan ellipse.
When we increase a to its
final value of 8, b has
increased to 5.7 and we get the
purple ellipse.
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Let's have another look
at a2 = c2 +
b2
If we allow a to
continue increasing then, with
c constant, b must
increase as well. The length of the
minor axis will approach
the length of
the major axis (but never
never become equal) but, becoming
so large that c will be
insignificant and the ellipse
approaches a very large circle
whose radius is
a.
(Since a and
b may continue to increase with no
bound, c will continue to decrease
towards 0 which is its bound. Not
until a = b will we have a circle.
But a will never exactly equal b,
so c will never exactly become
0.)
a2 ↑↑ =
c2 ↓↓ +
b2
↑↑
Now
suppose we make a equal to b. If we
allow b to increase then the major
axis moves form the X axis to the Y
axis and as b continues to increase
we start seeing a vertical ellipse
whose foci move away from the
origin along the Y axis.
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When talking about an
ellipse qualitatively (and later
with the hyperbola) we usually talk
about the ratio

This ratio is called the
eccentricity of the conic and it's
customary to use the letter
e to name this ratio.
Euler's constant is 2.71... and the
same letter e is used to
name that constant. This is fine
since you know which context it is
being used. Here, however, to
emphasize the difference, I'll use
the lower case Greek letter epsilon
ε.
ε = 
As
indicated previously, a,
b, and c form a right
triangle with a as the
hypotenuse. a, b, and c cannot
become 0 if we have an ellipse and
a must always be greater
than c (the
hypotenuse of a right triangle is
always greater then either of its
legs.) Also, for a vertical
ellipse remember that b
plays the role of a
so, in
this case, ε =
c/b.)
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the
hypotenuse is always larger
then either leg of a right
triangle
a
can never be 0 in a right
triangle
divide by a
reverse the sense of the
equation
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since neither a
nor c can be zero in a right
triangle

now
combining the
inequalities

So,
for an ellipse we have:
0 < ε
< 1
We've just
shown that as
ε →
1 the ellipse
flattens
and
as
ε →
0, the
ellipse approaches a
circle.
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From
the smallest to the largest
eccentricity we have the red
ellipse #1, then the blue ellipse
#3, and finally the gray ellipse
#2.
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Here
we see three ellipses that have the
same eccentricity. The triangles
show the relationships between a,
b, and c for each ellipse. These
right triangles are similar
triangles; the ratios of their
sides are the same. In particular
c/a is the same.
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ADVANCED:
(ALGEBRA 2)
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There's a deeper meaning in the
eccentricity. And this meaning
comes from its derivation which
follows. The algebra is a bit
involved but is explained
fully.
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An ellipse has a
directrix, but it hasn't been
necessary to discuss until now.
What we want to show is that for
any point on the ellipse, the ratio
of the distance from that point to
a focus (d1)
and the distance from that point to
the directrix ( d2)
is constant and equals
ε.
These distances are shown
above.
We want to
show that d1/d2
=
ε.
The strategy
we'll use is to find expressions in
terms of the constants a and c and
relate them to the common point
(x,y). We'll see that by doing this
we eliminate the x and
y.
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Pythagorean
theorem on smaller gray
triangle.
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Pythagorean
theorem on larger triangle
that includes y as a leg.
(2c: from focus to focus = c
+ c = 2c)
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Isolate
y2
in each equation.
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Set equations
equal. Remember, the goal is
to relate d1 to
d2 and eliminate
the x and y.
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Expand, watch
the minus signs.
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last
equation simplified
definition
of an ellipse, will be used now and
again shortly (4 steps later)
divide the
previous two equations noting that
r2 -
d12 = (r +
d1)(r - d1)
so
(r +
d1)(r - d1) /
(r + d1) = (r -
d1)
now solve
for d1
We need to
eliminate r so that we can use
d1 alone in terms of a,
c and x. Use the previous red
equation above to replace r.
Now, solve
for d1, then for
x*.
From the
graph: the distance from the
directrix to P(x,y) is the distance
from origin to the directrix
(a2/c) minus the
distance from the origin to x,
which is x. ( referring to the x in
the point P(x,y)) Substitute this
expression for x into the next
equation.
Doing this
we eliminate x.
Simplify,
watching the minus sign in front of
the a.
Multiply both
sides by c, then divide both sides
by ad2
like
this:
cd2
=
ad1
cd2
/
ad2
=
ad1/ad2
c/a =
d1/d2
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*
Here are the
missing
steps:
d1
=
a - cx/a
d1
-
a = -cx/a
a(d1
-
a) = -cx
a(d1
-
a)/(-c) =
-cx/(-c)
a(a -
d1)/c
= x
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subtract a
from both sides
divide both
sides by -c
(dividing by
a negative number interchanges the
terms in a difference)
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Example:
The
earth's orbit is an ellipse with an
eccentricity of 0.017. The length of half
its major axis is
92.956x106 meters. What
are the closest and furthest distances from
the earth to the sun?
Solution:
First of
all, the eccentricity is much smaller than
1, so we expect the orbit to be close to
that of a circle.
The sun
is one focus at a distance c from
the center of the ellipse. The vertex
closest to the sun is therefore a -
c. We have a, we can get
c from the eccentricity. 0.017 =
c/a, so c = 0.017a =
0.017( 92.956x106)
=1.580252x106.
a -
c = 92.956x106
- 1.580252x106
= 91.375748 x 106
miles
The
vertex furthest from the sun is the
distance from the sun to the center of the
ellipse, c, plus the distance to the
opposite vertex, a, that is, c +
a.
1.580252x106
+ 92.956x106 =
94.536252 x 106
miles
Even
though ε
is very small, the orbit is still
elliptical but in many ways a circle is
easier to deal with than an ellipse, so a
circle is not a bad
approximation.
In this
case (ignoring the power
106) a = 92.956,
b = 92.942 and c =
1.58
When
b equals a we have a circle;
in this case b is within 0.02% of
a.
b = (
a2 - c2
)½
= (92.956
2 - 1.58 2)
½ =
92.942
(92.956 - 92.942)/92.956 =
0.014/92 = 0.000151 0.000151 x 100% =
0.0151%)
Example:
Repeat
the previous calculations for the planet
pluto. Pluto's ε =0.249
and its
major axis has the
length 3.67x109
miles.
a
is ½
the length of the major axis.
a =
1.835x109.
c/a = 0.249 so
c =
0.249(1.835x109
)
=
0.4569x109
The closet
point to the sun is a - c
=
1.835x109
-
0.4569x109
=
1.378x109
miles.
The furthest
point from the sun is c
+ a = 0.4569x109
+
1.835x109
=
2.291x109
miles.
The following graph
is a plot of both orbits, earth's and
pluto's, using the values we calculated.
The sun is at the origin, the intersection
of the two yellow lines. (The major axis of
our solar system's planets are not
necessarily collinear nor are the orbits
necessarily coplanar, we'll ignore these
facts for now. We only want to show a
simple comparative graph.)
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