Chapter I
A Formula That Ignored Measurement
Euclid's geometry is about lengths, angles and areas. In 1750 Euler noticed something about solids that involved none of them. Count the vertices , edges and faces of any convex polyhedron (a cube, a tetrahedron, the panels of a football), and
A cube gives . An icosahedron gives . Squash the solid, bend its faces, stretch it into any shape, and the count never changes. It was a fact about how the pieces are connected, not how large they are. Leibniz had once wished for an analysis situs, a geometry of position rather than magnitude. Euler, who had already solved the bridges of Königsberg by ignoring distances, supplied its first real theorem.
That is why the field's parent is Euclidean geometry. The formula was born as a theorem about Euclid's solids, and it had to be pried loose from them.
Chapter II
The Counterexamples
The formula did not stay simple. In 1813 Simon Lhuilier produced solids where it fails: a polyhedral picture frame gives , and each extra tunnel lowers the count by two. Lakatos later made this episode famous as a case study in how mathematics grows. Every counterexample was met either by narrowing the definition of "polyhedron" or by realising that the formula measured something new.
The second response won. measures the number of holes, the genus, and it is a property of the surface, not of any particular way of cutting it into faces. By the mid-nineteenth century Riemann was using the same kind of count to classify surfaces, and Möbius and Jordan were classifying closed surfaces completely by it.
Chapter III
Poincaré Attaches Algebra to Shape
Higher dimensions needed more than one number. Henri Poincaré's Analysis Situs (1895) and its five supplements supplied two new tools. One was the fundamental group, which records how loops in a space can and cannot be deformed into one another. The other was an early form of homology, which counts holes of every dimension through Betti numbers. Topology became the study of the algebraic shadows that shapes cast.
His work was brilliant and famously loose. Proofs depended on intuitions that later generations had to rebuild. L. E. J. Brouwer put it on a rigorous footing around 1911–12 with the idea of the degree of a map. With it he proved two landmark results: every continuous map of a ball to itself has a fixed point, and spaces of different dimensions cannot be topologically the same.
Chapter IV
From Numbers to Groups
The decisive shift came from algebra. Around 1925 Emmy Noether, in her Göttingen lectures and in conversation with visiting topologists, pointed out that Betti numbers are only the sizes of richer objects: homology groups. A group can be mapped to another group, and a continuous map between spaces induces exactly such a map between their homology groups. Topology became functorial. Spaces and maps on one side are matched faithfully by algebra on the other, so a question about shape can be answered by computing with algebra.
The rest of the century built on that insight: cohomology, homotopy groups, fibrations and spectral sequences. By 1950 the field had its own axioms, from Samuel Eilenberg and Norman Steenrod, and had spread across mathematics. And it fed directly into geometric topology. Poincaré's conjecture was stated in terms of his own fundamental group.
Chapter V
A Closer Look: Counting the Holes in a Doughnut
Algebraic topology turns "how many holes?" into a computation. Start with the Euler characteristic. Cut a surface into vertices, edges and faces in any way you like and compute . The answer never depends on the cutting.
For a torus, take a single square and glue its opposite edges together: left to right makes a tube, then top to bottom closes the tube into a doughnut. After gluing, all four corners of the square are the same point, the two horizontal edges are one edge, and the two vertical edges are one edge. So
A sphere, cut like a cube, gives . In general a surface with holes has , so the Euler characteristic detects the holes.
Homology records more. The first homology group of the torus is : two independent loops, one around the tube and one through the hole, that cannot be deformed into each other or shrunk away. For the sphere, : every loop shrinks. Because deformation never changes these groups, they prove at once that no stretching turns a doughnut into a ball, the kind of impossibility statement the field exists to make. And Euler's number reappears: is the alternating sum of the ranks of the homology groups, here .
Chapter VI
Wrapping Spheres Around Spheres
The simplest-looking questions in the field are still unanswered. How many ways can one sphere be wrapped around another? Heinz Hopf's discovery in 1931 that a 3-sphere wraps nontrivially around a 2-sphere, in infinitely many distinct ways, showed that these homotopy groups of spheres are wild. Computing them has driven the field's most powerful machinery for more than ninety years. Some of the answers now come from computer-assisted calculation, and the table still has no visible end.