Efficiently constructing tangent circles
Arthur Baragar, Alex Kontorovich

TL;DR
This paper introduces a highly efficient method for constructing four mutually tangent circles, streamlining a classical geometric problem.
Contribution
The paper presents a novel, optimized construction technique for four mutually tangent circles, improving upon existing methods in terms of efficiency.
Findings
Construction is faster than traditional methods
Method reduces geometric complexity
Applicable to related tangent circle problems
Abstract
Our goal is to present, in what we believe is the most efficient way possible, a construction of four mutually tangent circles.
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Efficiently Constructing Tangent Circles
Arthur Baragar
Department of Mathematical Sciences, University of Nevada Las Vegas, Las Vegas, NV 89154
and
Alex Kontorovich
Department of Mathematics, Rutgers University, New Brunswick, NJ 08854
Key words and phrases:
Apollonius, Apollonian theorem, tangent circles, Euclidean constructions
2010 Mathematics Subject Classification:
51N20, 01A20
Kontorovich is partially supported by an NSF CAREER grant DMS-1455705, an NSF FRG grant DMS-1463940, and a BSF grant.
1. Introduction
The famous Problem of Apollonius is to construct a circle tangent to three given ones in a plane. The three circles may also be limits of circles, that is, points or lines, and “construct” of course refers to straightedge and compass. In this note, we consider the problem of constructing tangent circles from the point of view of efficiency. By this we mean using as few moves as possible, where a move is the act of drawing a line or circle. (Points are free as they do not harm the straightedge or compass, and all lines are considered endless, so there is no cost to “extending” a line segment.) Our goal is to present, in what we believe is the most efficient way possible, a construction of four mutually tangent circles. (Five circles of course cannot be mutually tangent in the plane, for their tangency graph, the complete graph , is non-planar.) We first present our construction before giving some remarks comparing it to others we found in the literature.
2. Baby Cases: One and Two Circles
Constructing one circle obviously costs one move: let and be any distinct points in the plane and draw the circle with center and passing through . Given , constructing a second circle tangent to it costs two more moves: draw a line through , and put an arbitrary point on this line (say, outside ). Now draw the circle with center and passing through ; then and are obviously tangent at , see Figure 1. It should be clear that one cannot do better than two moves, for otherwise one could draw the circle immediately; but this requires knowledge of a point on .
3. Warmup: Three Circles
Given Figure 1, that is, the two circles and , tangent at , and the line , how many moves does it take to construct a third circle tangent to both and ? We encourage readers at this point to stop and try this problem themselves.
Proposition 3.1**.**
Given Figure 1, a circle tangent to both and is constructible in at most five moves.
We first give the construction, then the proof that it works.
The Construction
Draw an arbitrary circle centered at (this is move 1), and let it intersect at and , say, with and on the same side of . Next draw the circle centered at and passing through (move 2), and the circle centered at through (move 3); see Figure 2. Let these two circles intersect at . Construct the line (move 4) and let it intersect at . Finally, draw the circle centered at and passing through (move 5); then is tangent to at , say.
The Proof
It is elementary to verify that the above construction works, and that the radius of is the same as that of . Note in fact that the locus of all centers of circles tangent to both and forms a hyperbola with foci and . Indeed, let the circles , , and have radii , , and , resp.; then and , so is constant for any choice of .
4. Main Theorem: the Fourth Circle
Finally we come to the main event, the fourth tangent circle, which we call the Apollonian circle.111Many objects in the literature are named after Apollonius though he had nothing to do with them, such as the Apollonian gasket and the Apollonian group (see, e.g., [Kon13]). The fourth tangent circle really is due to him, though most authors refer to it as the “Soddy” circle. We are given three mutually tangent circles, , and , lines and , and the points of tangency , , and ; that is, we are given the already constructed objects in Figure 2.
Theorem 4.1**.**
*An Apollonian circle tangent to , and in Figure 2 is constructible in at most seven moves. *
The construction
Draw the line (this is move 1) and let it intersect at . Draw the circle centered at and passing through (move 2). It intersects at and ; see Figure 3. We repeat this procedure: draw the line , let it intersect at , draw the circle with center and passing through , and let intersect at and (with on the same side as ). This repetition used two more moves. Next we extend and (now up to move 6) and let them meet at . Finally, use the seventh move to draw the desired Apollonian circle centered at and passing through ; see Figure 4.
Remark 4.2*.*
If a pair of lines, e.g., and , are parallel (so is at infinity), then use the line in lieu of (the former is the limit of the latter as ).
The Proof
There is a unique circle such that inversion through it fixes and sends to ; we claim that is this circle. Indeed, such an inversion must send to , so its center must lie on . Its center also lies on the line perpendicular to and , which is the line ; thus its center is . Finally, the point is fixed by this inversion, giving the claim.
Next it is easy to see that the point of tangency of and the Apollonian circle must also lie on this inversion circle (in which case this point must be as constructed). Indeed, since the inversion preserves the initial configuration of three circles, it must also fix , and hence also its point of tangency with .
Finally, since and are tangent at , their centers are collinear with ; that is, lies on the line . The rest is elementary.
Remark 4.3*.*
The second solution to the Apollonian problem can now be constructed in a further three moves. Indeed, the extra points of tangency and are already on the page. Extend and (two more moves); these intersect at , and drawing the circle centered at and passing through costs a third move.
Remark 4.4*.*
Let be constructed similarly to and . Note that the triangles and are perspective from the Gergonne point222See, e.g., Wikipedia for any (standard) terms not defined here and below.. By Desargue’s theorem, they are therefore perspective from a line, which is , the so-called Gergonne line; see Oldknow [Old96], who seems to have been just shy of discovering the construction presented here.
5. Other Constructions
Apollonius’s own solution did not survive antiquity [Hea81] and we only know of its existence through a “mathscinet review” by Pappus half a millennium later; perhaps we have simply rediscovered his work. Viète’s original solution through inversion (see, e.g., [Sar11]) is logically extremely elegant but takes countless elementary moves. There are many others but we highlight two in particular.
Gergonne
Gergonne’s own solution to the general Apollonian problem (that is, when the given circles are not necessarily tangent) is perhaps closest to ours (but of course the problem he is solving is more complicated). He begins by constructing the radical circle for the initial circles , , and , and identifies the six points , , , , , and , where it intersects the three original circles. Those points are taken in order around , with and on , and on , and and on . In our configuration, the radical circle is the incircle of triange and , , and .
Every pair of circles can be thought of as being similar to each other via a dilation through a point. In general, there are two such dilations. This gives us six points of similarity, which lie on four lines, the four lines of similitude. Each line generates a pair of tangent circles. In our configuration, the point is the center of the dilation that sends to . Since and are tangent, there is only one dilation, so we get only one line of similitude, the Gergonne line.
The radical circle of , , and a pair of tangent circles is centered on the line of similitude, so is where intersects that line. In our configuration, that gives us . The radical circle is the one that intersects perpendicularly, so in our configuration it goes through .
Eppstein
The previously simplest solution to our problem seems to have been that of Eppstein [Epp01b, Epp01a], which used eleven elementary moves to draw . His construction finds the tangency point by first dropping the perpendicular to through , and then connecting a second line from to one of the two points of intersection of this perpendicular with . This second line intersects at (or , depending on the choice of intersection point). Note that constructing a perpendicular line is not an elementary operation, costing 3 moves. The second line is elementary, so Eppstein can construct in 4 moves, then in 4 more, then two more lines and to get the center , and finally the circle in a total of 11 moves. To construct the other solution, , using his method, it would cost another five moves (as opposed to our three; see Remark 4.3), since one needs to draw two more lines to produce and (whereas our construction gives these as a byproduct).
Challenge:
Construct (a generic configuration of) four mutually tangent circles in the plane using fewer than () moves. Or prove (as we suspect) that this is impossible!
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[Epp 01a] D. Eppstein. Tangencies: Apollonian circles, 2001. https://www.ics.uci.edu/ ∼ similar-to \sim eppstein/junkyard/tangencies/apollonian.html .
- 2[Epp 01b] David Eppstein. Tangent spheres and triangle centers. Amer. Math. Monthly , 108(1):63–66, 2001.
- 3[Hea 81] Thomas Heath. A history of Greek mathematics. Vol. I . Dover Publications, Inc., New York, 1981. From Thales to Euclid, Corrected reprint of the 1921 original.
- 4[Kon 13] Alex Kontorovich. From Apollonius to Zaremba: local-global phenomena in thin orbits. Bull. Amer. Math. Soc. (N.S.) , 50(2):187–228, 2013.
- 5[Old 96] Adrian Oldknow. The Euler-Gergonne-Soddy triangle of a triangle. Amer. Math. Monthly , 103(4):319–329, 1996.
- 6[Sar 11] Peter Sarnak. Integral Apollonian packings. Amer. Math. Monthly , 118(4):291–306, 2011.
