Disks (like pennies) can be arranged in the plane in a closepacked rhombic lattice, with lattice angle . The fraction of the plane occupied by the disks, known as the packing fraction, is given by . For a square lattice with , . When , the array becomes a hexagonal lattice, with the maximum possible value of the packing fraction: . Choosing "disks" shows the lattice and packing fraction for selected values of . The packing of spheres in 3D space is a far more complex problem, as discussed in the Details. The lattice is defined by two angles and , with the second angle determining the relative displacement of successive planar layers. The spheres in each layer are placed directly over the cavities in the preceding layer. Since there are two possible sets of cavities, a regular arrangement of layers can be either a sequence like a b c a b c … or an alternative sequence like a b a b a b …. In either case, the packing fraction is given by . Choosing gives a simple cubic lattice with packing fraction . Choosing gives either the cubic closest packing (for a b c …) or hexagonal closest packing (for a b a b …). In either case, . Kepler's conjecture claims that this is the maximum possible packing fraction for spheres in 3D. Most practicing physicists would be quite satisfied that this result is correct, but mathematicians are another story, as described in Details. In the graphics for "spheres", you can move the layers apart for a closer view of their structure.
According to legend, Sir Walter Scott posed a question to his mathematical assistant, Thomas Harriot, about the most efficient stacking of cannonballs on the decks of his ships [1]. Around 1606, Harriot wrote about the problem to his colleague Johannes Kepler, best known for his work on planetary orbits. Kepler concluded that an arrangement known as facecentered cubic packing, a pattern well known to fruit sellers, is the optimal arrangement. (See the graphic for "cannonballs".) This has become known as Kepler's conjecture or simply the sphere packing problem. This states that no packing arrangement of equally sized spheres in threedimensional Euclidean space has a greater average density than that of either the facecentered cubic packing or the hexagonal close packing. In either of these packing arrangements, the spheres occupy approximately 74% of the space. The explicit value for the packing fraction is given by . The Kepler conjecture is included as part of the eighteenth problem in the celebrated list compiled in 1900 by David Hilbert. In 1998, Thomas Hales at Princeton University, following an approach suggested by László Fejes Tóth (1953), announced a proof of the Kepler conjecture. This was a proof by exhaustion involving the checking of many individual cases using lengthy computer calculations. Annals of Mathematics accepted the proof in 2005 but stated that they were only 99% certain of its validity [2]. Not until 2017 was Hales's work finally pronounced to be a proven result by the Forum of Mathematics, Pi [3]. [3] T. Hales, M. Adams, G. Bauer, T. D. Dang, J. Harrison, L. T. Hoang, C. Kaliszyk, et al., "A Formal Proof of the Kepler Conjecture," Forum of Mathematics, Pi, 5, 2017 e2. doi:10.1017/fmp.2017.1.
