B
Geometry and trigonometry
13
Cartesian and polar co-ordinates
13.1 Introduction
There are two ways in which the position of a point
in a plane can be represented. These are
(a) byCartesian co-ordinates, i.e. (x,y), and
(b) bypolar co-ordinates, i.e. (r,θ), whereris a
‘radius’ from a fixed point andθis an angle from
a fixed point.
13.2 Changing from Cartesian into
polar co-ordinates
In Fig. 13.1, if lengthsxandyare known, then the
length ofrcan be obtained from Pythagoras’ theo-
rem (see Chapter 12) sinceOPQis a right-angled
triangle. Hencer^2 =(x^2 +y^2 )
from which, r=
√
x^2 +y^2
Figure 13.1
From trigonometric ratios (see Chapter 12),
tanθ=
y
x
from which θ=tan−^1
y
x
r=
√
x^2 +y^2 andθ=tan−^1
y
x
are the two for-
mulae we need to change from Cartesian to polar
co-ordinates. The angleθ, which may be expressed
in degrees or radians, mustalwaysbe measured from
the positivex-axis, i.e. measured from the lineOQ
in Fig. 13.1. It is suggested that when changing from
Cartesian to polar co-ordinates a diagram should
always be sketched.
Problem 1. Change the Cartesian co-ordinates
(3, 4) into polar co-ordinates.
A diagram representing the point (3, 4) is shown in
Fig. 13.2.
Figure 13.2
From Pythagoras’ theorem,r=
√
32 + 42 =5 (note
that−5 has no meaning in this context). By trigono-
metric ratios,θ=tan−^143 = 53. 13 ◦or 0.927 rad.
[note that 53. 13 ◦= 53. 13 ×(π/180) rad= 0 .927 rad]
Hence (3, 4) in Cartesian co-ordinates corres-
ponds to (5, 53.13◦) or (5, 0.927 rad) in polar
co-ordinates.
Problem 2. Express in polar co-ordinates the
position (−4, 3).
A diagram representing the point using the Cartesian
co-ordinates (−4, 3) is shown in Fig. 13.3.