Skip to main content

Section 5.4 Application: Polar Coordinates

Cartesian coordinates such as discussed in Section 1.1 are not the only way to represent points in the plane. We can also represent them by indicating the distance, r, from the origin and the angle, φ, from the x-axis as shown in Figure 5.22.
Figure 5.22. Polar coordinates of a point in the plane
If we assume that r>0 and φ[0,2π) then every point except the origin has the unique representation
x=rcosφy=rsinφ.
Hence R2 is the image of the strip [0,)×[0,2π) under the transformation
g(r,φ):=(rcosφ,rsinφ).
We want to apply the transformation formula from the previous section to find out how to integrate a function given in polar coordinates. To do so we need to compute the Jacobian determinant of g. The Jacobian matrix is given by
Jg(r,φ)=[rrcosφφrcosφrrsinφφrsinφ]=[cosφrsinφsinφrcosφ].
Hence the Jacobian determinant is
detJg(r,φ)=det[cosφrsinφsinφrcosφ]=rdet[cosφsinφsinφcosφ]=r(cos2φ+sin2φ)=r0.
Applying the transformation formula we see that
(5.8)g(D)f(x,y)dxdy=Df(rcosφ,rsinφ)rdrdφ.

Example 5.23. Are of a disc.

Compute the area of a disc of radius R.
Solution.
A disc, D, with radius R is given in polar coordinates by
{(r,φ):0rR,0φ<2π}.
Hence by (5.2), (5.8) and Fubini’s theorem
area(D)=D1dxdy=0R02πrdrdφ=02πr22|0Rdφ=02πR22dφ=πR2.

Example 5.24. Area of an ellipse.

Compute the area of the ellipse
x2a2+y2b21.
Solution.
We aim to find a function mapping a circle onto the given ellipse. If we set x=au and y=bv then
x2a2+y2b2=a2u2a2+b2v2b2=u2+v2=1,
showing that the ellipse, E, is the image of the disc, D, given by u2+v21, under the (linear) transformation
g(u,v):=(au,bv)=[a00b][uv].
According to the transformation formula (5.7) we get
area(E)=E1dxdy=det[a00b]D1dudv=abD1dudv
Using the result from the previous example to compute the last integral we see that the area of the ellipse is abπ.