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Mathematics LibreTexts

3.3: The Extended Plane

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Consider again inversion about the circle C given by |zz0|=r, and observe that points close to z0 get mapped to points in the plane far away from z0. In fact, a sequence of points in C whose limit is z0 will be inverted to a sequence of points whose magnitudes go to . Conversely, any sequence of points in C having magnitudes marching off to will be inverted to a sequence of points whose limit is z0.

With this in mind, we define a new point called the point at infinity, denoted . Adjoin this new point to the plane to get the extended plane, denoted as C+. Then, one may extend inversion in the circle C to include the points z0 and . In particular, inversion of C+ in the circle C centered at z0 with radius r, iC:C+C+, is given by

iC(z)={r2(¯zz0)+z0 if zz0, if z=z0z0 if z= .

Viewing inversion as a transformation of the extended plane, we define z0 and to be symmetric points with respect to the circle of inversion.

The space C+ will be the canvas on which we do all of our geometry, and it is important to begin to think of as “one of the gang,” just another point to consider. All of our translations, dilations, and rotations can be redefined to include the point .

So where is in C+? You approach as you proceed in either direction along any line in the complex plane. More generally, if {zn} is a sequence of complex numbers such that |zn| as n, then we say limnzn=. By convention, we assume is on every line in the extended plane, and reflection across any line fixes .

Theorem 3.3.1

Any general linear transformation extended to the domain C+ fixes .

Proof

If T(z)=az+b where a and b are complex constants with a0, then by limit methods from calculus, as |zn|, |azn+b| as well. Thus, T()=.

So, with new domain C+, we modify our fixed point count for the basic transformations:

  • The translation Tb of C+ fixes one point ().
  • The rotation about the origin Rθ of C+ fixes 2 points (0 and ).
  • The dilation T(z)=kz of C+ fixes 2 points, (0 and ).
  • The reflection rL(z) of C+ about line L fixes all points on L (which now includes ).
Example 3.3.1: Some Transformations Not Fixing .

The following function is a transformation of C+

T(z)=i+1z+2i,

a fact we prove in the next section. For now, we ask where T sends , and which point gets sent to .

We tackle the second question first. The input that gets sent to is the complex number that makes the denominator 0. Thus, T(2i)=.

To answer the first question, take your favorite sequence that marches off to , for example, 1,2,3,. The image of this sequence, T(1),T(2), T(3), consists of complex fractions in which the numerator is constant, but the denominator grows unbounded in magnitude along the horizontal line Im(z)=2. Thus, the quotient tends to 0, and T()=0.

As a second example, you can check that if

T(z)=iz+(3i+1)2iz+1,

then T(i2)= and T()=12.

We emphasize that the following key results of the previous section extend to C+ as well:

  • There exists a unique cline through any three distinct points in C+. (If one of the given points in Theorem 3.2.1 is , the unique cline is the line through the other two points.)
  • Theorem 3.2.3 applies to all points z not on C, including z=z0 or .
  • Inversion about a cline preserves angle magnitudes at all points in C+ (we discuss this below).
  • Inversion preserves symmetry points for all points in C+ (Theorem 3.2.5 holds if p or q is ).
  • Theorem 3.2.7 now holds for all clines that do not intersect, including concentric circles. If the circles are concentric, the points symmetric to both of them are and the common center.
Stereographic Projection

We close this section with a look at stereographic projection. By identifying the extended plane with a sphere, this map offers a very useful way for us to think about the point .

Definition: Unit 2-Sphere

The unit 2-sphere, denoted S2, consists of all the points in 3-space that are one unit from the origin. That is,

S2={(a,b,c)R3 | a2+b2+c2=1}.

We will usually refer to the unit 2-sphere as simply “the sphere.” Stereographic projection of the sphere onto the extended plane is defined as follows. Let N=(0,0,1) denote the north pole on the sphere. For any point PN on the sphere, ϕ(P) is the point on the ray NP that lives in the xy-plane. See Figure 3.3.1 for the image of a typical point P of the sphere.

im-stpro.svg
Figure 3.3.1: Stereographic projection. (Copyright; author via source)

The stereographic projection map ϕ can be described algebraically. The line through N=(0,0,1) and P=(a,b,c) has directional vector NP=a,b,c1, so the line equation can be expressed as

r(t)=0,0,1+ta,b,c1.

This line intersects the xy-plane when its z coordinate is zero. This occurs when t=11c, which corresponds to the point (a1c,b1c,0).

Thus, for a point (a,b,c) on the sphere with c1, stereographic projection ϕ:S2C+ is given by

ϕ((a,b,c))=a1c+b1ci.

Where does ϕ send the north pole? To , of course. A sequence of points on S2 that approaches N will have image points in C with magnitudes that approach .

Angles at .

If we think of as just another point in C+, it makes sense to ask about angles at this point. For instance, any two lines intersect at , and it makes sense to ask about the angle of intersection at . We can be guided in answering this question by stereographic projection, thanks to the following theorem.

Theorem 3.3.2

Stereographic projection preserves angles. That is, if two curves on the surface of the sphere intersect at angle θ, then their image curves in C+ also intersect at angle θ.

Thus, if two curves in C+ intersect at we may define the angle at which they intersect to equal the angle at which their pre-image curves under stereographic projection intersect. The angle at which two parallel lines intersect at is 0. Furthermore, if two lines intersect at a finite point p as well as at , the angle at which they intersect at equals the negative of the angle at which they intersect at p. As a consequence, we may say that inversion about a circle preserves angle magnitudes at all points in C+.

Exercises

Exercise 3.3.1

In each case find T() and the input z0 such that T(z0)=.

  1. T(z)=(3z)(2z+i).
  2. T(z)=(z+1)eiπ/4.
  3. T(z)=(az+b)(cz+d).
Exercise 3.3.2

Suppose D is a circle of Apollonius of p and q. Prove that p and q are symmetric with respect to D.

Hint

Recall the circle C in the proof of Theorem 3.2.6. Show that p and q get sent to points that are symmetric with respect to iC(D).

Exercise 3.3.3

Determine the inverse stereographic projection function ϕ1:C+S2. In particular, show that for z=x+yi,

ϕ1(x,y)=(2xx2+y2+1,2yx2+y2+1,x2+y21x2+y2+1).


This page titled 3.3: The Extended Plane is shared under a CC BY-SA 4.0 license and was authored, remixed, and/or curated by Michael P. Hitchman via source content that was edited to the style and standards of the LibreTexts platform.

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