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<title> The Steiner in-ellipse and moments of inertia of triangles and other polygons </title>
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<h1 align="center">The Steiner in-ellipse and moments of inertia of triangles and other polygons </h1>

<h3 align="center">G. Keady and P. Scales </h3>

<h3 align="center"> </h3>

<div class="p"><!----></div>
  <h2><a name="tth_sEc1">
1</a>&nbsp;&nbsp;The triangle results</h2>  
<div class="p"><!----></div>
Given a triangle 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math> in the plane, there is an inscribed ellipse,
tangent to each side at the midpoint of the side.
This ellipse is usually called the <i>Steiner in-ellipse</i>.
There is a substantial popular literature on Steiner ellipses
including books such as [<a href="#D" name="CITED">2</a>] (where Problem 98 is particularly relevant)
and articles on the internet including in wikipedia and in mathworld.
Recent articles in publications by MAA, [<a href="#Ka1" name="CITEKa1">6</a>,<a href="#Ka2" name="CITEKa2">7</a>,<a href="#MS" name="CITEMS">9</a>] and elsewhere, e.g.<br />
<a href="http://demonstrations.wolfram.com/MardensTheorem">
http://demonstrations.wolfram.com/MardensTheorem</a><br/>
<div class="p"><!----></div>
  have called attention to it, and some of its applications.
The aim of this note is to alert readers that there are mechanics
applications, with substantial results noted in the nineteenth century literature:
see [<a href="#R" name="CITER">10</a>].

<div class="p"><!----></div>
Denote the vertices of the triangle 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math> by 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
</mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
</mrow></math>, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mn>3</mn></mrow>
</msub>
</mrow></math>, and
define its centroid 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
<mo>=</mo><mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mn>1</mn></mrow>
</msub>
<mo>+</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo>+</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mn>3</mn></mrow>
</msub>
<mo stretchy="false">)</mo><mo stretchy="false">/</mo><mn>3</mn></mrow></math>:

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> is the centre of the Steiner in-ellipse.
Considering the points in 2-dimensional real Euclidean space
we may record the coordinates in column vectors 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mi>j</mi></mrow>
</msub>
<mo>=</mo><mo stretchy="false">(</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>j</mi><mo>,</mo><mn>1</mn></mrow>
</msub>
<mo>,</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>j</mi><mo>,</mo><mn>2</mn></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mi>T</mi></mrow>
</msup>
</mrow></math>,
the superscript 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow></mrow><mrow><mi>T</mi></mrow>
</msup>
</mrow></math> denoting transpose.
The structure of the equation for the Steiner in-ellipse is,
for some positive definite matrix 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math>
<a name="eq:Adef">
</a><br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo stretchy="false">(</mo><mi>z</mi><mo>-</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mi>T</mi></mrow>
</msup>
<mi>A</mi><mo stretchy="false">(</mo><mi>z</mi><mo>-</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
<mo stretchy="false">)</mo><mo>=</mo><mn>1</mn><mo>.</mo></mrow>
    </mstyle></math></td><td width="1">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo stretchy="false">(</mo><mn>1</mn><mo stretchy="false">)</mo></mrow>
    </mstyle></math>
</td></tr></table>


The entries of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> are functions of the vertices, readily computed by
any Computer Algebra System (CAS).

<div class="p"><!----></div>
Consider mass distributed uniformly over 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math>. 
Define a second-moment tensor by
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo>=</mo><mrow><mo>[</mo>
<mtable>
<mtr><mtd columnalign="center"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mn>11</mn></mrow>
</msub>
</mrow></mtd><mtd columnalign="center"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mn>12</mn></mrow>
</msub>
</mrow></mtd></mtr>
<mtr><mtd columnalign="center"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mn>12</mn></mrow>
</msub>
</mrow></mtd><mtd columnalign="center"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mn>22</mn></mrow>
</msub>
</mrow></mtd></mtr></mtable>

<mo>]</mo></mrow></mrow>
    </mstyle></math>
</td></tr></table>
<br />

where
<a name="eq:Iint">
</a><br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi>ij</mi></mrow>
</msub>
<mo>=</mo>
<msub><mrow><mo>&int;</mo></mrow><mrow><mi>T</mi></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>X</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
<mo>-</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>c</mi><mo>,</mo><mi>i</mi></mrow>
</msub>
<mo stretchy="false">)</mo><mo stretchy="false">(</mo>
<msub><mrow><mi>X</mi></mrow><mrow><mi>j</mi></mrow>
</msub>
<mo>-</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>c</mi><mo>,</mo><mi>j</mi></mrow>
</msub>
<mo stretchy="false">)</mo><mi>&ensp;</mi>
<msub><mrow><mi>dX</mi></mrow><mrow><mn>1</mn></mrow>
</msub>

<msub><mrow><mi>dX</mi></mrow><mrow><mn>2</mn></mrow>
</msub>
<mo>.</mo></mrow>
    </mstyle></math></td><td width="1">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></mrow>
    </mstyle></math>
</td></tr></table>


Define also a rotation 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>R</mi></mrow></math> and a reflection 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> by
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>R</mi><mo>=</mo><mrow><mo>[</mo>
<mtable>
<mtr><mtd columnalign="center"><mrow><mn>0</mn></mrow></mtd><mtd columnalign="center"><mrow><mo>-</mo><mn>1</mn></mrow></mtd></mtr>
<mtr><mtd columnalign="center"><mrow><mn>1</mn></mrow></mtd><mtd columnalign="center"><mrow><mn>0</mn></mrow></mtd></mtr></mtable>

<mo>]</mo></mrow><mi>&ensp;</mi><mo>,</mo><mi>&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;</mi><mi>&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;</mi><mi>S</mi><mo>=</mo><mrow><mo>[</mo>
<mtable>
<mtr><mtd columnalign="center"><mrow><mn>0</mn></mrow></mtd><mtd columnalign="center"><mrow><mn>1</mn></mrow></mtd></mtr>
<mtr><mtd columnalign="center"><mrow><mn>1</mn></mrow></mtd><mtd columnalign="center"><mrow><mn>0</mn></mrow></mtd></mtr></mtable>

<mo>]</mo></mrow><mi>&ensp;</mi><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

The usual area moment of inertia tensor is 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">M</mi><mo fontstyle="normal">.</mo><mi fontstyle="normal">I</mi><mo fontstyle="normal">.</mo></mrow>
</msub>
<mo>=</mo><mi>R</mi>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>

<msup><mrow><mi>R</mi></mrow><mrow><mi>T</mi></mrow>
</msup>
</mrow></math>,
though there are some authors that use 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>S</mi></mrow></math> where 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>R</mi></mrow></math> is used here.
(The results in the mechanics literature, e.g. [<a href="#R" name="CITER">10</a>],
 concern the moment of inertia tensor rather than our second-moment tensor.)

<div class="p"><!----></div>
 It is convenient to define another second moment tensor,
 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math>, this time associated with a triangle with its mass
 located at the vertices, an equal mass at each vertex.
 It happens that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math> is just a scalar multiple of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
</mrow></math>.

<div class="p"><!----></div>
Once again, these second-moment tensors are positive definite.
It can be checked (easily with a CAS
doing the routine calculations) that
matrices 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
</mrow></math> commute,
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>A</mi>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo>=</mo>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mi>A</mi><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

This leads to the following.

<div class="p"><!----></div>
<b>THEOREM.</b>
The principal axes of the second-moment tensor for the triangle coincide with
the directions of the principal axes of the Steiner in-ellipse.

<div class="p"><!----></div>
<br />A proof follows from using the fact that commuting diagonalizable matrices
are simultaneously diagonalizable, i.e. share eigenvectors.
(See [<a href="#Hor" name="CITEHor">5</a>], items 1.3.19 and 2.3.3.)

<div class="p"><!----></div>
<br />Rather more is true. It can be shown that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>R</mi>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>

<msup><mrow><mi>R</mi></mrow><mrow><mi>T</mi></mrow>
</msup>
</mrow></math>
is just a scalar multiple of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math>.

<div class="p"><!----></div>
<br />The result, with a different proof, is at page 26 of [<a href="#R" name="CITER">10</a>].
There is a substantial literature on moments of inertia of triangles
including [<a href="#G" name="CITEG">3</a>,<a href="#Hop" name="CITEHop">4</a>,<a href="#T" name="CITET">11</a>].

<div class="p"><!----></div>
<br /> <h2><a name="tth_sEc2">
2</a>&nbsp;&nbsp;Polygons and polynomials</h2>

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.1">
2.1</a>&nbsp;&nbsp;Moments of inertia for systems of equal point masses</h3>

<div class="p"><!----></div>
Consider next a polynomial of degree 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math>, and, for the sake of definiteness,
suppose that all the roots are distinct. Suppose also that the sum of the roots is
zero, which is only supposed to save some writing in some future formulae:
<a name="eq:pDef">
</a><br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>p</mi><mo stretchy="false">(</mo><mi>z</mi><mo stretchy="false">)</mo><mo>=</mo>
<munderover><mo>&Pi;</mo><mrow><mi>i</mi><mo>=</mo><mn>1</mn> </mrow>
<mrow><mi>n</mi></mrow></munderover><mo stretchy="false">(</mo><mi>z</mi><mo>-</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
<mo stretchy="false">)</mo><mo>,</mo><mi>&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;</mi>
<munderover><mo>&sum;</mo><mrow><mi>i</mi><mo>=</mo><mn>1</mn> </mrow>
<mrow><mi>n</mi></mrow></munderover>
<msub><mrow><mi>z</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
<mo>=</mo><mn>0</mn><mo>.</mo></mrow>
    </mstyle></math></td><td width="1">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo stretchy="false">(</mo><mn>3</mn><mo stretchy="false">)</mo></mrow>
    </mstyle></math>
</td></tr></table>


With polynomial 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo stretchy="false">(</mo><mi>z</mi><mo stretchy="false">)</mo></mrow></math> we associate a polygon with 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math> vertices.
With its derivative 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo>'</mo><mo stretchy="false">(</mo><mi>z</mi><mo stretchy="false">)</mo></mrow></math> we can associate, similarly, a 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>1</mn><mo stretchy="false">)</mo></mrow></math>-gon.

<div class="p"><!----></div>
The set of vertices is the important item, defining both the polynomial and,
possibly less importantly, the polygon.
Below we define the second-moment matrix 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math> for any 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math>-gon
with equal masses located at the vertices and taking the moments about the
vertex-centroid.
The connection with the Steiner in-ellipse is that if one repeatedly differentiates the
polynomial until one reaches a cubic, then finds the Steiner in-ellipse associated
with the triangle defined from the roots of the cubic, the principal axes of

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math> are the axes of the Steiner in-ellipse.
Intermediate results on the way through to this are also memorable.

<div class="p"><!----></div>
The derivative, of course is
<a name="eq:pPrimeDef">
</a><br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>p</mi><mo>'</mo><mo stretchy="false">(</mo><mi>z</mi><mo stretchy="false">)</mo><mo>=</mo><mi>n</mi>
<munderover><mo>&Pi;</mo><mrow><mi>j</mi><mo>=</mo><mn>1</mn> </mrow>
<mrow><mi>n</mi><mo>-</mo><mn>1</mn></mrow></munderover><mo stretchy="false">(</mo><mi>z</mi><mo>-</mo>
<msubsup><mrow><mi>z</mi></mrow><mrow><mi>j</mi> </mrow>
<mrow><mo>'</mo></mrow></msubsup>
<mo stretchy="false">)</mo><mo>,</mo><mi>&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;</mi>
<munderover><mo>&sum;</mo><mrow><mi>j</mi><mo>=</mo><mn>1</mn> </mrow>
<mrow><mi>n</mi><mo>-</mo><mn>1</mn></mrow></munderover>
<msubsup><mrow><mi>z</mi></mrow><mrow><mi>j</mi> </mrow>
<mrow><mo>'</mo></mrow></msubsup>
<mo>=</mo><mn>0</mn><mo>.</mo></mrow>
    </mstyle></math></td><td width="1">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo stretchy="false">(</mo><mn>4</mn><mo stretchy="false">)</mo></mrow>
    </mstyle></math>
</td></tr></table>


The centroid of the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>1</mn><mo stretchy="false">)</mo></mrow></math>-gon associated with 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo>'</mo></mrow></math> and the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math>-gon associated with

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi></mrow></math> coincide. 
There is a nice picture, associated with illustrating the Gauss-Lucas Theorem, at the
Mathematica demonstrations site,<br />
<a href="http://demonstrations.wolfram.com/LucasTheorem/">
http://demonstrations.wolfram.com/LucasGaussTheorem</a>
 <br />
We will return to this later.

<div class="p"><!----></div>
The previous sentence refers to a fact about the first moments.
Consider next the second-moment matrices:
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
<mo>=</mo><mrow><mo>[</mo>
<mtable>
<mtr><mtd columnalign="center"><mrow><mo>&sum;</mo>
<msubsup><mrow><mi>x</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
</mrow></mtd><mtd columnalign="center"><mrow><mo>&sum;</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>i</mi></mrow>
</msub>

<msub><mrow><mi>y</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
</mrow></mtd></mtr>
<mtr><mtd columnalign="center"><mrow><mo>&sum;</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>i</mi></mrow>
</msub>

<msub><mrow><mi>y</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
</mrow></mtd><mtd columnalign="center"><mrow><mo>&sum;</mo>
<msubsup><mrow><mi>y</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
</mrow></mtd></mtr></mtable>

<mo>]</mo></mrow><mo>,</mo><mi>&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;</mi><mi>I</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
<mo>=</mo><mrow><mo>[</mo>
<mtable>
<mtr><mtd columnalign="center"><mrow><mo>&sum;</mo><mo stretchy="false">(</mo><mi>x</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></mtd><mtd columnalign="center"><mrow><mo>&sum;</mo><mi>x</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
<mi>y</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
</mrow></mtd></mtr>
<mtr><mtd columnalign="center"><mrow><mo>&sum;</mo><mi>x</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
<mi>y</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
</mrow></mtd><mtd columnalign="center"><mrow><mo>&sum;</mo><mo stretchy="false">(</mo><mi>y</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow></mtd></mtr></mtable>

<mo>]</mo></mrow><mi>&ensp;</mi><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

We will show that these matrices have the same eigenvectors, and will do this 
by showing that the matrices commute.

<div class="p"><!----></div>
The commutator 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo><mi>I</mi><mi>I</mi><mo>'</mo><mo>-</mo><mi>I</mi><mo>'</mo><mi>I</mi><mo stretchy="false">)</mo></mrow></math> of two symmetric matrices 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>I</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>I</mi><mo>'</mo></mrow></math> is
necessarily skew symmetric and it is the zero matrix iff
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>I</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mn>12</mn></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>I</mi></mrow><mrow><mn>11</mn></mrow>
</msub>
<mo>-</mo>
<msub><mrow><mi>I</mi></mrow><mrow><mn>22</mn></mrow>
</msub>
<mo stretchy="false">)</mo><mo>-</mo>
<msub><mrow><mi>I</mi></mrow><mrow><mn>12</mn></mrow>
</msub>
<mo stretchy="false">(</mo><mi>I</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mn>11</mn></mrow>
</msub>
<mo>-</mo><mi>I</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mn>22</mn></mrow>
</msub>
<mo stretchy="false">)</mo><mo>=</mo><mn>0</mn><mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

Using the specific entries for our matrices
<a name="eq:commutator">
</a><br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<mtable align="right" width="80%">
<mtr><mtd columnalign="right" columnspan="1"><mrow><mo stretchy="false">(</mo><mi>I</mi><mi>I</mi><mo>'</mo><mo>-</mo><mi>I</mi><mo>'</mo><mi>I</mi><mo stretchy="false">)</mo><mo>=</mo><mn>0</mn></mrow>
</mtd><mtd columnalign="left">
<mrow><mo>&Leftrightarrow;</mo></mrow>
</mtd><mtd columnalign="left">
<mrow><mi>c</mi><mo>:</mo><mo>=</mo><mo>&sum;</mo><mi>x</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
<mi>y</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
<mo>&sum;</mo><mo stretchy="false">(</mo>
<msubsup><mrow><mi>x</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
<mo>-</mo>
<msubsup><mrow><mi>y</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
<mo stretchy="false">)</mo><mo>-</mo><mo>&sum;</mo>
<msub><mrow><mi>x</mi></mrow><mrow><mi>i</mi></mrow>
</msub>

<msub><mrow><mi>y</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
<mo>&sum;</mo><mo stretchy="false">(</mo><mo stretchy="false">(</mo><mi>x</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>-</mo><mo stretchy="false">(</mo><mi>y</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">)</mo></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo stretchy="false">)</mo><mo>=</mo><mn>0</mn></mrow>
</mtd></mtr>
<mtr><mtd columnalign="right" columnspan="1"><mrow></mrow>
</mtd><mtd columnalign="left">
<mrow><mo>&Leftrightarrow;</mo></mrow>
</mtd><mtd columnalign="left">
<mrow><mi>c</mi><mo>:</mo><mo>=</mo><mi fontstyle="normal">Im</mi><mrow><mo>(</mo>
<mover><mrow><mo>&sum;</mo><mo stretchy="false">(</mo><mi>z</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">) </mo></mrow><mrow><mn>2</mn></mrow>
</msup>
</mrow>
<mo stretchy="true">&OverBar;</mo></mover>
<mo>&sum;</mo>
<msubsup><mrow><mi>z</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
<mo>)</mo></mrow><mo>=</mo><mn>0</mn><mo>.</mo></mrow>
</mtd><mtd columnalign="right">&emsp;&emsp;&emsp;&emsp;&emsp;&emsp;<mo stretchy="false">(</mo><mn>5</mn><mo stretchy="false">)</mo></mtd></mtr>
</mtable>
</mrow>
    </mstyle></math>
</td></tr></table>
<br />


<div class="p"><!----></div>
We now return to considering the polynomials 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo>'</mo></mrow></math>.
Considering the coefficient of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>z</mi></mrow><mrow><mi>n</mi><mo>-</mo><mn>2</mn></mrow>
</msup>
</mrow></math> is 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi></mrow></math> and of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msup><mrow><mi>z</mi></mrow><mrow><mi>n</mi><mo>-</mo><mn>3</mn></mrow>
</msup>
</mrow></math> of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo>'</mo></mrow></math>, we have
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mi>n</mi>
<munder><mo>&sum;</mo><mrow><mi>j</mi><mo>,</mo><mi>k</mi><mi>&ensp;</mi><mi>j</mi><mo>&ne;</mo><mi>k</mi></mrow>
</munder>
<mi>z</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>
<mi>z</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>k</mi></mrow>
</msub>
<mo>=</mo><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>2</mn><mo stretchy="false">)</mo>
<munder><mo>&sum;</mo><mrow><mi>i</mi><mo>,</mo><mi>k</mi><mi>&ensp;</mi><mi>i</mi><mo>&ne;</mo><mi>k</mi></mrow>
</munder>

<msub><mrow><mi>z</mi></mrow><mrow><mi>i</mi></mrow>
</msub>
<mi>z</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>k</mi></mrow>
</msub>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

From this, on using the centroid conditions, first moment conditions, of
equations&nbsp;(<a href="#eq:pDef">3</a>,<a href="#eq:pPrimeDef">4</a>) we have
<br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow><mo>&sum;</mo><mo stretchy="false">(</mo><mi>z</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi>j</mi></mrow>
</msub>

<msup><mrow><mo stretchy="false">) </mo></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>=</mo>
<mfrac><mrow><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>2</mn><mo stretchy="false">)</mo></mrow>
<mrow><mi>n</mi></mrow>
</mfrac>
<mo>&sum;</mo>
<msubsup><mrow><mi>z</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>
<mo>.</mo></mrow>
    </mstyle></math>
</td></tr></table>
<br />

 Using this in the expression 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>c</mi></mrow></math> of equation&nbsp;(<a href="#eq:commutator">5</a>), we have
 that
 <br />
<table width="100%"><tr><td align="center">
    <math xmlns="http://www.w3.org/1998/Math/MathML">
    <mstyle displaystyle="true"><mrow>
<mtable align="right" width="80%">
<mtr><mtd columnalign="right" columnspan="1"><mrow><mi>c</mi></mrow>
</mtd><mtd columnalign="left">
<mrow><mo>=</mo></mrow>
</mtd><mtd columnalign="left">
<mrow>
<mfrac><mrow><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>2</mn><mo stretchy="false">)</mo></mrow>
<mrow><mi>n</mi></mrow>
</mfrac>
<mi fontstyle="normal">Im</mi><mrow><mo>(</mo><mo stretchy="false">&verbar;</mo><mo>&sum;</mo>
<msubsup><mrow><mi>z</mi></mrow><mrow><mi>i</mi> </mrow>
<mrow><mn>2</mn></mrow></msubsup>

<msup><mrow><mo stretchy="false">&verbar;</mo></mrow><mrow><mn>2</mn></mrow>
</msup>
<mo>)</mo></mrow></mrow>
</mtd></mtr>
<mtr><mtd columnalign="right" columnspan="1"><mrow></mrow>
</mtd><mtd columnalign="left">
<mrow><mo>=</mo></mrow>
</mtd><mtd columnalign="left">
<mrow><mn>0</mn><mo>.</mo></mrow>
</mtd></mtr>
</mtable>
</mrow>
    </mstyle></math>
</td></tr></table>
<br />

 This establishes that the matrices 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>I</mi>
<msub><mrow><mo>'</mo></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math> commute and 
 hence share eigenvectors.

<div class="p"><!----></div>
Now consider the picture, showing not just the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math>-gon and the 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo><mi>n</mi><mo>-</mo><mn>1</mn><mo stretchy="false">)</mo></mrow></math>-gon
associated with 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi></mrow></math> and 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>p</mi><mo>'</mo></mrow></math> respectively, but also the roots for the higher order derivatives.
See the picture associated with the Gauss-Lucas Theorem, at the
Mathematica demonstrations site.
Eventually we get to a cubic polynomial, a triangle, and its Steiner in-ellipsoid.
The axes of this ellipsoid are the principal axes for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math>,
and for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msubsup><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi> </mrow>
<mrow><mo stretchy="false">(</mo><mi>k</mi><mo stretchy="false">)</mo></mrow></msubsup>
</mrow></math> for any, e.g. 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>k</mi></mrow></math>-th, derivative's set of points.

<div class="p"><!----></div>
     <h3><a name="tth_sEc2.2">
2.2</a>&nbsp;&nbsp;Area moments of inertia for polygons</h3>

<div class="p"><!----></div>
We define a polygon as an ordered list of vertices, and may suppose that the
coordinates of the vertices are represented as pairs of reals or,
as 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi>j</mi></mrow>
</msub>

<msubsup><mrow><mo stretchy="false">)</mo></mrow><mrow><mi>j</mi><mo>=</mo><mn>1</mn> </mrow>
<mrow><mi>n</mi></mrow></msubsup>
</mrow></math> complex numbers.
The generalization of the preceding formula,
equation&nbsp;(<a href="#eq:Iint">2</a>) for 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math> from triangles 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math> to
general polygons merely requires us to replace the region of integration

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math> by the polygon 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>P</mi></mrow></math>, and it is useful to note that 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mi>c</mi></mrow>
</msub>
</mrow></math> could be,
in this more general context, any point, and we prefer to indicate the
centre about which the moments are taken by 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mo>*</mo></mrow>
</msub>
</mrow></math>.
(In engineering applications it is likely that crossed polygons and so on
would not occur, but they are not a problem in the following.)
It is well known that there are multivariate polynomial expressions for
the entries of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
</mrow></math> in terms of the coordinates of the vertices:
see&nbsp;[<a href="#Bo" name="CITEBo">1</a>], for example.
The formulae have been coded in many languages and are,
for example, in <i>Mathematica</i>'s Structural Mechanics Pack.

<div class="p"><!----></div>
The Parallel Axes Theorem is a well-known result indicating how the
moment matrices 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mo>*</mo></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math> change as 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mo>*</mo></mrow>
</msub>
</mrow></math> changes.
The open question we have is whether there might be some simple
formula for the point we take moments about so that the eigenvectors of

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mo>*</mo></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math> align with the axes of the Steiner in-ellipse of the preceding
subsection. For triangles, the result is mentioned in &#167;1, namely that
the area centroid, which coincides with the vertex average, is such a point.
For quadrilaterals, the area centroid need no longer coincide with the
vertex average, and it happens that if we take moments about the vertex average
the principal axes coincide with the axes of the Steiner in-ellipse 
(and, in fact, denoting the vertex average by 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>z</mi></mrow><mrow><mi fontstyle="normal">VA</mi></mrow>
</msub>
</mrow></math>, we have
that the  matrix 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">area</mi></mrow>
</msub>
<mo stretchy="false">(</mo>
<msub><mrow><mi>z</mi></mrow><mrow><mi fontstyle="normal">VA</mi></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math> is a scalar multiple of

<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
<mo stretchy="false">)</mo></mrow></math>.)
We have no results for polygons with larger numbers of sides.

<div class="p"><!----></div>
 <h2><a name="tth_sEc3">
3</a>&nbsp;&nbsp;Tetrahedra and higher dimensions</h2>

<div class="p"><!----></div>
There are generalizations to higher dimensions, presumably to 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi></mrow></math>-dimensions,
though the mechanics literature stops at 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>n</mi><mo>=</mo><mn>3</mn></mrow></math>.
Let 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>T</mi></mrow></math> be a tetrahedron in Euclidean 3-space.
Define the <i>Steiner in-ellipsoid</i> to be the inscribed ellipsoid
tangent to each face at the face's centroid.
The centre of the Steiner ellipsoid is located at the centroid of the
tetrahedron.
(Steiner ellipsoids have already been defined in earlier literature,
from the 1940s and possibly earlier.
As in the plane case, these usually refer to circum-ellipsoids.)
Once again, the equation of the ellipsoid can be written
in the form of equation&nbsp;(<a href="#eq:Adef">1</a>), with, now, 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math> a 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mn>3</mn><mo>&times;</mo><mn>3</mn></mrow></math> matrix.
An analogue, for this three dimensional situation,
 of the theorem above is available in [<a href="#R" name="CITER">10</a>], pp28-30, i.e.
 that the principal axes of inertia correspond to the eigenvectors of 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mi>A</mi></mrow></math>.
 (See also [<a href="#Ki" name="CITEKi">8</a>].)
 The CAS-based proof techniques we used also generalize:
 it is easy to verify, with the obvious definitions of the
 
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow><mn>3</mn><mo>&times;</mo><mn>3</mn></mrow></math> matrices,  
<math xmlns="http://www.w3.org/1998/Math/MathML">
<mrow>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
<mi>A</mi><mo>=</mo><mi>A</mi>
<msub><mrow><mi>I</mi></mrow><mrow><mi fontstyle="normal">point</mi></mrow>
</msub>
</mrow></math>.

<div class="p"><!----></div>

<h2>References</h2>

<dl compact="compact">
 <dt><a href="#CITEBo" name="Bo">[1]</a></dt><dd>
S.F. Bockman, Generalizing the formula for areas of polygons to moments,
<i>Amer. Math. Monthly</i>  <b>96</b> (Feb 1989), 131-132.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITED" name="D">[2]</a></dt><dd>
H. Dorrie, <i>100 Great Problems of Elementary Mathematics, Their History and Solution</i>,
 translated (from German to English) by D. Antin, Dover, New York, 1965.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEG" name="G">[3]</a></dt><dd>
N.M. Gibbins,
The moment of inertia of a triangle about any line in its plane,
<i>Math. Gazette</i> <b>12</b> (1925), 392.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEHop" name="Hop">[4]</a></dt><dd>
W. Hope-Jones,
Moment of inertia of a triangular lamina,
<i>Math. Gazette</i> <b>39</b> (1955), 145.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEHor" name="Hor">[5]</a></dt><dd>
R.A. Horn and C.A. Johnson,
<i>Matrix Analysis</i>,
Cambridge U.P., New York, 1985.

<div class="p"><!----></div>
 </dd>
 <dt><a href="#CITEKa1" name="Ka1">[6]</a></dt><dd>
 D. Kalman, The most marvelous theorem in mathematics, 
 <i>Journal of Online Mathematics and its Applications</i>, 
available at <br />
<tt>http://www.JOMA.org</tt> (for journal), <br />
<tt>http://mathdl.maa.org/mathDL/4/?pa=content&amp;sa=viewDocument&amp;nodeID=1663</tt>
 (direct to article).

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEKa2" name="Ka2">[7]</a></dt><dd>
D. Kalman, An elementary proof of Marden's Theorem,
<i>Amer. Math. Monthly</i>  <b>115</b> (Apr 2008), 330-338.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEKi" name="Ki">[8]</a></dt><dd>
C. W. Kilmister,
Some further remarks on moments of inertia,
<i>Math. Gazette</i>, <b>44</b> (1960), 224-225.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITEMS" name="MS">[9]</a></dt><dd>
D. Minda and S. Phelps,
Triangles, Ellipses and Cubic Polynomials
<i>Amer. Math. Monthly</i> (Oct 2008)

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITER" name="R">[10]</a></dt><dd>
E.J.  Routh, 
<i>The Elementary Part of a Treatise on the Dynamics of a System of Rigid Particles</i>,
MacMillan and Co.: London, 1891.

<div class="p"><!----></div>
</dd>
 <dt><a href="#CITET" name="T">[11]</a></dt><dd>
A. Talbot,
Equimomental systems,
<i>Math. Gazette</i> <b>36</b> (1952), 95-110.

<div class="p"><!----></div>

<div class="p"><!----></div>
 
<div class="p"><!----></div>
</dd>
</dl>Grant Keady,<br />
School of Mathematics and Statistics,
University of Western Australia<br />
email: <tt>keady@maths.uwa.edu.au</tt>

<div class="p"><!----></div>
<br />P. Scales,<br />
Balanced Engineering Advice, Woodlands 6018, Australia<br />
email: <tt>peterscales@perthpcug.org.au</tt><br />

<div class="p"><!----></div>

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