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9.1
Definition (
)
We define a function

as follows.
If
, then
is the point on the unit circle such that the length
of
the arc joining
to
(measured in the counterclockwise direction)
is
equal to
. (There is an optical illusion
in the figure. The length of segment
is equal to the length of
arc
.)
Thus to find

, you should start at

and move along
the
circle in a counterclockwise direction until you've traveled a distance

.
Since the circumference of the circle is

, we see that

.
(Here we assume Archimedes'
result that the area
of a circle is half the circumference times the radius.)
If

, we define
 |
(9.2) |
where

is the reflection about the horizontal axis. Thus if

, then

is
the
point obtained by starting at

and moving

along the unit circle in
the
clockwise direction.
Remark: The definition of
depends on several ideas that we have not
defined
or stated assumptions about, e.g., length of an arc and
counterclockwise
direction. I believe that the amount of work it takes to formalize these
ideas at this
point is not worth the effort, so I hope your geometrical intuition will carry
you
through this chapter. (In this chapter we will assume quite a bit
of Euclidean geometry, and a few properties of area that
do not follow from our assumptions stated in chapter 5.)
A more self contained treatment of the trigonometric functions
can be found in [44, chapter 15], but the treatment given
there uses ideas that we will consider later, (e.g. derivatives,
inverse functions,
the intermediate value theorem, and the fundamental theorem of calculus)
in order to define the trigonometric functions.
We have the following values for
:
 |
 |
 |
(9.3) |
 |
 |
 |
(9.4) |
 |
 |
 |
(9.5) |
 |
 |
 |
(9.6) |
 |
 |
 |
(9.7) |
In general
 |
(9.8) |
9.9
Definition (Sine and cosine.)
In terms of coordinates, we write
(We read ``

" as `` cosine of

", and we read ``

" as
`` sine of

".)
Since
is on the unit circle, we have
and
The equations (9.3) - (9.8) show that
and
In equation (9.2) we defined
Thus for
,
and it follows that
In terms of components
and consequently
Let
be arbitrary real numbers. Then there exist integers
and
such that
and
. Let
Then
, so
Suppose
(see figure). Then the length of the arc joining
to
is
which is the same as the
length of
the arc joining
to
. Since equal arcs in a
circle subtend
equal chords, we have
and hence
 |
(9.10) |
You can verify that this same relation holds when
.
Proof: From (9.10) we know
i.e.,
Hence
By expanding the squares and using the fact that
for
all
,
we conclude that
 |
(9.16) |
This is equation (9.13). To get equation (9.12) replace
by
in
(9.16). If we take
in equation (9.16) we
get
or
If we replace
by
in this equation we get
Now in equation (9.16) replace
by
and get
or
which is equation (9.14). Finally replace
by
in this last
equation to
get (9.15).
In the process of proving the last theorem we proved the following:
9.17
Theorem (Reflection law for sin and cos.) For all
,
 |
(9.18) |
9.19
Theorem (Double angle and half angle formulas.)
For all
we have
9.20
Exercise.
A
Prove the four formulas stated in theorem
9.19.
Proof: We have
and
By adding these equations, we get (9.22).
By subtracting the first from the
second,
we get (9.24).
In equation (9.24) replace
by
and replace
by
to get
or
This yields equation (9.25).
9.27
Exercise.
Prove equations (
9.23) and (
9.26).
From the geometrical description of sine and cosine, it follows that as
increases
for
to
,
increases from
to
and
decreases from
to
. The identities
indicate that a reflection about the vertical line through
carries
the graph of sin onto the graph of cos, and vice versa.
The condition
indicates that the reflection
about the
vertical axis carries the graph of
to itself.
The relation
shows that
i.e., the graph of
is carried onto itself by a rotation through
about the origin.
We have
and
, so
and
(approximately).
With this information we can make a reasonable sketch of the graph of
and
(see the figure above)
9.29
Exercise.
A
Complete the following table of sines and cosines:
Include an explanation for how you found
and
(or
and
). For the
remaining values
you do not need to include an explanation.
Most of the material from this section
was discussed by Claudius Ptolemy (fl.
127-151
AD). The functions considered by Ptolemy were not the sine and cosine, but the
chord, where the chord of an arc
is the length of the segment joining
its
endpoints.
 |
(9.30) |
Ptolemy's chords are functions of arcs (measured in degrees), not of numbers.
Ptolemy's
addition law for
was (roughly)
where
is the diameter of the circle, and
Ptolemy produced tables equivalent to tables of
for
in intervals of
.
All
calculations were made to 3 sexagesimal (base
) places.
The etymology of the word sine is
rather curious[42, pp 615-616].
The function we call sine was first
given a name by Aryabhata near the start of the sixth century AD.
The name meant ``half chord''
and was later shortened to jya meaning ``chord''. The Hindu
word was translated into Arabic as jîba, which was a meaningless
word phonetically derived from jya, but (because the vowels
in Arabic were not written) was written the same as
jaib, which means bosom. When the Arabic was
translated into Latin it became sinus. (Jaib means bosom, bay,
or breast: sinus means bosom, bay or the fold of a toga around the
breast.) The English word sine is derived from sinus phonetically.
9.31
Entertainment (Calculation of sines.)
Design a computer program that will take as
input a
number

between

and

, and will calculate

. (I choose

instead of

so that you do
not need to know the value of

to do
this.)
Next: 9.2 Calculation of
Up: 9. Trigonometric Functions
Previous: 9. Trigonometric Functions
  Index
Ray Mayer
2007-09-07