Theorema Egregium

Gauss's remarkable theorem about intrinsic curvature

Theorema Egregium

Gauss's Theorema Egregium (“Remarkable Theorem”) states that Gaussian curvature K is intrinsic — it depends only on the metric (first fundamental form), not on how the surface is embedded in space.

This means a 2D being living on the surface could measure K without knowing about the surrounding 3D space. It also explains why you can't flatten an orange peel!

Interactive: Bending vs Stretching

Bend a flat sheet into a cylinder. The Gaussian curvature stays zerobecause bending doesn't change intrinsic distances. A sphere has K = 1 everywhere — you can't bend paper into a sphere without tearing or stretching!

Bent Paper (K = 0)
Sphere (K = 1)
Bent Paper K
0.0000
Always ≈ 0!
Sphere K
1.0002
Always = 1

No matter how you bend a flat sheet, its Gaussian curvature stays zero. You cannot bend paper into a sphere without stretching or tearing — that would change K!

The Theorem

“The Gaussian curvature K of a surface is an intrinsic invariant — it can be computed entirely from the first fundamental form (E, F, G) and its derivatives.”

In other words: K = K(E, F, G, Eu, Ev, Fu, ...) with no reference to the second fundamental form or the normal vector.

This was surprising because K = k1 · k2 involves principal curvatures that seem to depend on the embedding. Gauss proved they cancel out in just the right way!

Interactive: Map Projection Distortion

The Theorema Egregium explains why no flat map of Earth is perfect. The sphere has K = 1, the plane has K = 0. Since K is intrinsic, any map must distort something. The Tissot indicatrix shows what gets distorted.

Simple latitude-longitude grid. Severe distortion near poles.

Tissot ellipse (circles on sphere)
Equator

The Tissot indicatrix shows how the map distorts small circles on the sphere. No flat map can preserve both shape (K changes!) and area everywhere.

Consequences of the Theorem

Can't Flatten a Sphere

A sphere (K = 1) cannot be isometrically mapped to a plane (K = 0). Any flat map of Earth must distort either angles, areas, or distances.

Can Bend Paper

A plane (K = 0) can be bent into a cylinder or cone (also K = 0) without stretching. This is an isometry — distances are preserved.

Pizza Theorem

Why does folding a pizza slice make it stiffer? Bending in one direction forces the other curvature to zero (to keep K = 0), preventing it from drooping.

Intrinsic Geometry

A 2D being on a surface can measure K using only distances — no need to see the surface from “outside.” This led to Riemann's intrinsic geometry.

Interactive: Isometry Checker

Two surfaces are locally isometric if they have the same intrinsic geometry — same distances, same K. Compare pairs of surfaces to see which can be smoothly deformed into each other.

Cylinder (K ≈ 0.00)
Plane (K ≈ 0.00)
✓ Locally Isometric

Both have K = 0. You can unroll a cylinder into a plane without stretching!

K = 0
K > 0

Gauss's Equation for K

Gauss proved that K can be expressed purely in terms of E, F, G and their partial derivatives. For orthogonal coordinates (F = 0):

K = -1/(2√(EG)) · [∂/∂u(Gu/√(EG)) + ∂/∂v(Ev/√(EG))]

This remarkable formula shows K depends only on the metric tensorand its derivatives — exactly what a 2D being could measure!

Historical Note

Gauss published this theorem in his 1827 work “Disquisitiones generales circa superficies curvas” and reportedly called it “egregium” (remarkable) because even he was surprised by the result.

This work laid the foundation for Riemannian geometry, where Riemann generalized these ideas to spaces of any dimension — eventually leading to Einstein's general relativity.

Key Takeaways

  • Theorema Egregium: Gaussian curvature K is intrinsic — determined solely by the metric
  • Isometries preserve K: If two surfaces are locally isometric, they have the same K
  • K = 0 surfaces are developable: They can be unrolled onto a plane (cylinders, cones)
  • Maps distort: No isometric map from sphere to plane exists
  • This theorem opened the door to intrinsic geometry and eventually general relativity

Congratulations! You've completed the Differential Geometry module.