A surface of revolution is invariant under rotations around a fixed axis and is locally generated by rotating a profile curve.
A solid of revolution is the three-dimensional region swept out by rotating a planar region about an axis in its plane. Perpendicular slices are disks or annuli, making volume, center-of-mass, and moment-of-inertia integrals one-dimensional.
Put for the profile parametrizationWith unit normal , the principal curvatures areConsequently and .
A parallel of a surface of revolution is the circle obtained by fixing the profile parameter and varying the rotation angle. Its radius is the distance from the rotation axis.
For the arc-length meridian metric , a unit-speed parallel has and . Its radial geodesic equation is satisfied exactly when . Thus extrema of the radius, and any other stationary radii, give geodesic circles. If every parallel is geodesic, the surface is a circular cylinder.
A meridian is the intersection of a surface of revolution with a plane containing the rotation axis. It is formed from a profile curve and its half-turn about the axis.
Suppose a smooth profile has , just to the right of , and . Use as a local parameter and write . The rotated surface is smooth at the pole if and only ifnear zero for a smooth function . It is then locally the smooth graph . Equivalently, the even reflection is smooth; in particular all odd derivatives of at zero vanish and the profile meets the rotation axis orthogonally. The analogous condition holds at the other endpoint.
A catenoid is the surface of revolution obtained by rotating a catenary about its directrix. One conformal parametrization is
For the standard catenoid, the two principal curvatures are opposite, so its mean curvature vanishes. Its Gaussian curvature is , which also shows that no neighbourhood is locally isometric to a plane, cylinder, or regular part of a cone, all of which have zero Gaussian curvature.
For the catenoid profile spanning fixed-endpoint rings, the second variation of isThis refers to axisymmetric graph variations, not all possible changes in surface topology. Strict positivity for every nonzero admissible variation gives a strict local minimum in the topology: the positive lowest Dirichlet eigenvalue of the regular Sturm-Liouville problem gives coercivity, and sufficiently small coefficient perturbations preserve it. The zero variation must be excluded from a strict-positivity hypothesis.
Forthe area density after integrating over is . If every height interval has area times its length, continuity forcesWhere , the sign of is constant and has derivative . Hence the profile lies on a circle of radius .
For the surfaces generated by and ,The diffeomorphism matches these curvatures, although comparison of the first fundamental forms shows that no local isometry exists.
For an arc-length profile with radius , the equation isThus gives locally, while gives wherever . At their mean curvatures are respectivelyso different choices of give locally noncongruent surfaces with the same constant Gaussian curvature.
For , rotate the unit-speed profilenear . Since , the resulting regular surface of revolution has . At its principal curvatures are and , so the point is not umbilical when and no neighbourhood of it lies on a sphere.
A circular cylinder of radius has induced metric locally equal to with . Its Riemann curvature tensor therefore vanishes, despite its nonzero extrinsic curvature. With outward unit normal and convention , its trace is and its principal curvatures are and zero. Its averaged mean curvature is . The angular identification changes global topology, not local flatness.
For a geodesic in the metric , the cyclic coordinate givesEquivalently, the geodesic meets parallels according to Clairaut's relation.
Let a compact smooth surface of revolution have exactly two poles, and let be the Clairaut first integral for a surface of revolution of a complete unit-speed geodesic. If , then , so the geodesic avoids open neighbourhoods of both poles. If , then is constant away from the poles and the geodesic lies in a meridian of a surface of revolution, whose complement contains a nonempty open set. Thus no complete geodesic has dense image.
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