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<td bgcolor="#003399"><img src="../images/spacer.gif" width="18"
height="8" border="0" /><font face="Verdana,Arial,Helvetica"
size="1" color="white"><b>Cannonballs and Honeycomb:</b> Harriot
and Kepler<b><br />
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<p><br />
 <font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> The
pyramid stacking of oranges is known to chemists as the <i>
face-centered cubic packing</i>. It is also known as the cannonball
packing, because it is commonly used for that purpose at war
memorials. The oldest example I have seen is the pyramid of
cannonballs from the 16th century that rests in front of the City
Museum of Munich. Formulas for the number of cannonballs stacked in
mounds have been known this long. In the 16th century, Sir Walter
Raleigh gave his mathematical assistant, Thomas Harriot, the task
of finding the formula. Harriot did this without
difficulty.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> As
Harriot grew in reputation as a scientist, spheres became a
favorite topic of his. To him, atoms were spheres. To understand
how they stack together is to understand nature. Numbers were
spheres. In the tradition of Pythagoras, triangular numbers are
stacked like billiard balls set in a triangle. Harriot draws
Pascal's triangle, but with a sphere packing with that many spheres
replacing each number. <img style="float: right" src="fig2a.gif" />
</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> In
1606, Kepler complained that his recent book on optics was based
entirely on theology. He turned for help to Harriot, who had been
conducting experiments in optics for years. In fact, Harriot's
knowledge of optics was so advanced that he had discovered Snell's
law - 20 years before Snell and 40 years before Descartes. Harriot
supplied Kepler with valuable data in optics, but he also tried to
persuade Kepler that the deeper mysteries of optics would be
unfolded through atomism. Unlike Kepler, Harriot was an ardent
atomist, believing that the secrets of the universe were to be
revealed through the patterns and packings of small, spherical
atoms. Kepler was skeptical. Nature abhors a vacuum, and between
the atoms lies the void.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular">
Harriot persisted. Kepler relented. In 1611, Kepler wrote a little
booklet, <i>The Six-Cornered Snowflake</i>, that influenced the
direction of crystallography for the next two centuries. This
slender essay was the ``first recorded step towards a mathematical
theory of the genesis of inorganic or organic form. (L.L. Whyte, in
<i>The Six-Cornered Snowflake</i>, Oxford Clarendon Press, Oxford,
1966.) In a discussion of sphere packings, he constructed the
face-centered cubic packing. Kepler asserted that it would be ``the
tightest possible, so that in no other arrangement could more
pellets be stuffed into the same container.'' This assertion has
come to be known as the Kepler conjecture. It went without a proof
for nearly 400 years, until August 1998, when I gave a proof with
the help of a graduate student, Samuel P. Ferguson.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> <b>
Theorem (Kepler conjecture).</b> No packing of balls of the same
radius in three dimensions has density greater than the
face-centered cubic packing. <img style="float: right"
src="fig2b.gif" /></font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> The
face-centered cubic packing is constructed by setting one layer of
balls upon another. Each layer is a regular pattern of balls in a
grid of equilateral triangles. But there are other sphere packings
that have exactly the same density (<math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>&pi;</mi>
<mo>/</mo><msqrt><mrow><mn>18</mn>
</mrow></msqrt><mo>&approx;</mo><mn>0</mn><mo>.</mo><mn>74</mn>
</math>) as
the face-centered cubic packing. The best known alternative is the
hexagonal close-packing. Its individual layers are identical to
those of the face-centered cubic. But the layers are staggered to
produce a different global packing with the same density (Figure 2a
and 2b). There is no simple list of all packings of density
<math xmlns='http://www.w3.org/1998/Math/MathML'>
<mi>&pi;</mi>
<mo>/</mo><msqrt><mrow><mn>18</mn>
</mrow></msqrt>
</math>, but there are many other possibilities. The
density of the packing in space is defined as a limit; and removing
one, two, or a hundred balls from the packing will not affect the
limiting density. Nor will removing an entire infinite layer of
balls.</font></p>

<p><font face="Arial,Helvetica,Geneva,Swiss,SunSans-Regular"> This
article gives the broad outlines of the proof of the Kepler
conjecture in the most elementary possible terms. The proof is long
(282 pages), and every aspect of it is based on even longer
computer calculations. A jury of <math xmlns='http://www.w3.org/1998/Math/MathML'>
<mn>12</mn>

</math> referees has been
deliberating on the proof since September 1998. Nobody has raised
doubts about the overall correctness of the proof. And yet, to my
knowledge, no one has made a thorough independent check of the
computer code.</font></p>
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