10-95 Strengthening Core Skills 1013
College Algebra & Trignometry—
of an elliptical path (relative to some point of reference)
using skills developed in this chapter. Here we’ve seen that
the equation of a conic can be given in rectangular form,
polar form, and parametric form. Each form seems to have
its advantages. When it comes to the rotations of a conic
section, it’s hard to match the ease and versatility of the
polar form. To illustrate, recall that in polar form the
general equation of a horizontal ellipse with one focus (the
Sun) at the origin is The constant a gives
the length of the semimajor axis and e represents the
eccentricity of the orbit. With the exception of Mercury
and Pluto (a dwarf planet), the orbits of most planets are
close to circular (e is very near zero). This makes the rota-
tions difficult to see. Instead we will explore the concept
of axes rotation using “planets” with higher eccentricities.
Consider the following planets and their orbital equations.
The planet Agnesi has an eccentricity of while the
planet Erdös is the most eccentric at
We’ll investigate the
concept of conic rotations
in polar form by rotating
these ellipses. With your
calculator in polar ,
enter these three equations
on the screen and use
the settings shown in Figure
10.77 to set the window
size (use ).
The resulting graph is displayed in Figure 10.78,
showing the very hypothetical case where all planets share
the same major axis. To show a more realistic case where
the planets approach the Sun along orbits with differing
major axes, we’ll use Galois as a reference and rotate
Agnesi rad clockwise and Erdös rad counter-
12
4
max 7
Y =
MODE
Erdös:
7.875
1 0.75 cos
Galois:
5.75
1 0.7 cos
Agnesi:
2.9
1 0.5 cos
e 0.75.
e 0.5,
r
a11 e
2
2
1 e cos
.
clockwise.
This is done by
simply adjusting
the argument of
cosine in each
equation, using
for
Agnesi and
for
Erdös. The adjusted
screen is shown in Figure
10.79, and new graphs in
Figure 10.80.
Use these ideas to
explore and investigate
other rotations by com-
pleting the following
exercises.
Exercise 1: What
happens if the
angle of rotation is
? Is the orbit
identical if you
rotate by ?
Exercise 2: If the
denominator in
the equation is
changed to a sum, what effect does it have on the graph?
Exercise 3: If the sign in the numerator is changed, what
effect does it have on how the graph is generated?
Exercise 4: After resetting the orbits as originally given,
use trial and error to approximate the smallest angle of
rotation required for the orbit of Galois to intersect the
orbit of Erdös.
Exercise 5: What minimum rotation is required for the
orbit of Galois to intersect the orbit of both Agnesi and
Erdös?
Exercise 6: What is the minimum rotation required for
the orbit of Agnesi to intersect the orbit of Galois?
cosa
12
b
cosa
4
b
15
10
15
32
Figure 10.77
Figure 10.78
Figure 10.80
15
10
15
32
STRENGTHENING CORE SKILLS
Simplifying and
Streamlining
Computations for the
Rotation of Axes
While the calculations involved for eliminating the mixed xy-term require a good deal
of concentration, there are a few things we can do to simplify the overall process. Basi-
cally this involves two things. First, in Figure 10.81 we’ve organized the process in
flowchart form to help you “see” the sequence involved in finding and (for
use in the rotation formulas). Second, calculating x
2
, y
2
, and xy (from the equations
and ) as single terms and apart from
their actual substitution is somewhat less restrictive and seems to help to streamline
the algebra.
y X sin Y cos x X cos Y sin
sin cos
Figure 10.79
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