Dandelin spheres are touching the pale yellow plane that intersects the cone.
This construction shows how the focal points of an ellipse can be found using the Dandelin spheres. The angle bisector between the line representing the plane and a line representing the cone surface leads to the center of the respective sphere.

In geometry, the Dandelin spheres are one or two spheres that are tangent both to a plane and to a cone that intersects the plane. The intersection of the cone and the plane is a conic section, and the point at which either sphere touches the plane is a focus of the conic section, so the Dandelin spheres are also sometimes called focal spheres.[1]

The Dandelin spheres were discovered in 1822.[1][2] They are named in honor of the French mathematician Germinal Pierre Dandelin, though Adolphe Quetelet is sometimes given partial credit as well.[3][4][5]

The Dandelin spheres can be used to give elegant modern proofs of two classical theorems known to Apollonius of Perga. The first theorem is that a closed conic section (i.e. an ellipse) is the locus of points such that the sum of the distances to two fixed points (the foci) is constant. The second theorem is that for any conic section, the distance from a fixed point (the focus) is proportional to the distance from a fixed line (the directrix), the constant of proportionality being called the eccentricity.[6]

A conic section has one Dandelin sphere for each focus. An ellipse has two Dandelin spheres touching the same nappe of the cone, while hyperbola has two Dandelin spheres touching opposite nappes. A parabola has just one Dandelin sphere.

Proof that the intersection curve has constant sum of distances to foci

Consider the illustration, depicting a cone with apex S at the top. A plane e intersects the cone in a curve C (with blue interior). The following proof shall show that the curve C is an ellipse.

The two brown Dandelin spheres, G1 and G2, are placed tangent to both the plane and the cone: G1 above the plane, G2 below. Each sphere touches the cone along a circle (colored white), and .

Denote the point of tangency of the plane with G1 by F1, and similarly for G2 and F2 . Let P be a typical point on the curve C.

To Prove: The sum of distances remains constant as the point P moves along the intersection curve C. (This is one definition of C being an ellipse, with and being its foci.)

This gives a different proof of a theorem of Apollonius of Perga.[6]

If we define an ellipse to mean the locus of points P such that d(F1, P) + d(F2, P) = a constant, then the above argument proves that the intersection curve C is indeed an ellipse. That the intersection of the plane with the cone is symmetric about the perpendicular bisector of the line through F1 and F2 may be counterintuitive, but this argument makes it clear.

Cylinder case

Adaptations of this argument work for hyperbolas and parabolas as intersections of a plane with a cone. Another adaptation works for an ellipse realized as the intersection of a plane with a right circular cylinder.

Proof of the focus-directrix property

The directrix of a conic section can be found using Dandelin's construction. Each Dandelin sphere intersects the cone at a circle; let both of these circles define their own planes. The intersections of these two parallel planes with the conic section's plane will be two parallel lines; these lines are the directrices of the conic section. However, a parabola has only one Dandelin sphere, and thus has only one directrix.

Using the Dandelin spheres, it can be proved that any conic section is the locus of points for which the distance from a point (focus) is proportional to the distance from the directrix.[7] Ancient Greek mathematicians such as Pappus of Alexandria were aware of this property, but the Dandelin spheres facilitate the proof.[6]

Neither Dandelin nor Quetelet used the Dandelin spheres to prove the focus-directrix property. The first to do so may have been Pierce Morton in 1829,[8] or perhaps Hugh Hamilton who remarked (in 1758) that a sphere touches the cone at a circle which defines a plane whose intersection with the plane of the conic section is a directrix.[1][9][10][11] The focus-directrix property can be used to prove that astronomical objects move along conic sections around the Sun.[12]

Notes

  1. ^ a b c Taylor, Charles. An Introduction to the Ancient and Modern Geometry of Conics, page 196 ("focal spheres"), pages 204–205 (history of discovery) (Deighton, Bell and co., 1881).
  2. ^ Dandelin, G. (1822). "Mémoire sur quelques propriétés remarquables de la focale parabolique" [Memoir on some remarkable properties of the parabolic focale [i.e., oblique strophoid]]. Nouveaux mémoires de l'Académie royale des sciences et belles-lettres de Bruxelles (in French). 2: 171–200.
  3. ^ Kendig, Keith. Conics, p. 86 (proof for ellipse) and p. 141 (for hyperbola) (Cambridge University Press, 2005).
  4. ^ Quetelet, Adolphe (1819) "Dissertatio mathematica inauguralis de quibusdam locis geometricis nec non de curva focali" (Inaugural mathematical dissertation on some geometric loci and also focal curves), doctoral thesis (University of Ghent ("Gand"), Belgium). (in Latin)
  5. ^ Godeaux, L. (1928). "Le mathématicien Adolphe Quetelet (1796-1874)". Ciel et Terre (in French). 44: 60–64.
  6. ^ a b c Heath, Thomas. A History of Greek Mathematics, page 119 (focus-directrix property), page 542 (sum of distances to foci property) (Clarendon Press, 1921).
  7. ^ Brannan, A. et al. Geometry, page 19 (Cambridge University Press, 1999).
  8. ^ Numericana's Biographies: Morton, Pierce
  9. ^ Morton, Pierce. Geometry, Plane, Solid, and Spherical, in Six Books, page 228 (Baldwin and Cradock, 1830).
  10. ^ Morton, Pierce (1830). "On the focus of a conic section". Transactions of the Cambridge Philosophical Society. 3: 185–190.
  11. ^ Hamilton, Hugh (1758). De Sectionibus Conicis. Tractatus Geometricus. In quo, ex Natura ipsius Coni, Sectionum Affectiones facillime deducuntur. Methodo nova [On conic sections. A geometric treatise. In which, from the nature of the cone itself, relations of sections are most easily deduced. By a new method.] (in Latin). London, England: William Johnston. pp. 122–125. Liber (book) II, Propositio (proposition) XXXVII (37).
  12. ^ Hyman, Andrew. "A Simple Cartesian Treatment of Planetary Motion", European Journal of Physics, Vol. 14, page 145 (1993).

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