Catenoid
A catenoid is a minimal surface in three-dimensional Euclidean space, generated by rotating a catenary curve about its axis of symmetry, resulting in a surface of revolution with zero mean curvature.[1] It can be parameterized as x(u,v) = (c \cosh(v/c) \cos u, c \cosh(v/c) \sin u, v) for parameters u \in [0, 2\pi) and v \in \mathbb{R}, where c > 0 scales the surface, forming a catenoid of constant width that narrows to a "neck" and flares out asymptotically to catenary ends.[1] Discovered by Leonhard Euler in 1744 and rigorously proven to be a minimal surface by Jean-Baptiste Meusnier in 1776, the catenoid represents the first known non-planar example of a minimal surface, predating broader classifications in differential geometry.[2] As the unique axially symmetric minimal surface in \mathbb{R}^3, it spans two parallel coaxial circles when truncated, analogous to a soap film minimizing surface area between rings, and exhibits finite total curvature of -4\pi with a Morse index of 1.[2][1] The catenoid is topologically a punctured sphere (genus zero) with two ends, and its Gauss map is anti-holomorphic, covering the unit sphere except for the north and south poles, underscoring its role in the Weierstrass-Enneper representation of minimal surfaces.[2] It is the only properly embedded, non-planar minimal surface of finite topology in \mathbb{R}^3 with these properties, and by theorems such as those of Collin and Nitsche, it uniquely intersects every horizontal plane in a Jordan curve when oriented appropriately.[1] Beyond pure mathematics, the catenoid models physical phenomena like equilibrium shapes in capillarity and serves as a benchmark in computational geometry for simulating minimal surfaces via mean curvature flow.[3]Definition and Geometry
Catenary Curve Basis
The catenary curve describes the shape assumed by a perfectly flexible, inextensible chain or cable of uniform density when suspended from two points and acted upon solely by gravity.[4] Its standard equation, with the vertex at the origin, is given byy = a \cosh\left(\frac{x}{a}\right),
where a > 0 is a scaling parameter that determines the curve's width and sag, related to the horizontal tension at the lowest point and the linear density of the chain multiplied by gravity (specifically, a = T_0 / (\mu g), with T_0 the horizontal tension, \mu the mass per unit length, and g the gravitational acceleration).[4][5] The catenary's equation arises from either force balance on chain segments or variational principles minimizing potential energy subject to fixed length. In the force balance approach, consider a small segment of the chain: the horizontal tension component remains constant, while the vertical component increases with the weight supported, leading to the differential equation
\frac{d}{ds} \left( \frac{dy}{dx} \right) = \frac{1}{a},
where s is the arc length along the curve; integrating this yields the hyperbolic cosine form.[5] Alternatively, using the calculus of variations to minimize the potential energy \int y \, ds (with fixed total length) produces the Euler-Lagrange equation (y + h) y'' = 1 + (y')^2, which integrates to the same catenary solution, confirming its equilibrium shape.[5] Historically, Galileo Galilei approximated the catenary as a parabola in his 1638 Two New Sciences, based on empirical observations of hanging chains, though this was an inexact model valid only for shallow sags.[6] The true equation was rigorously derived in 1691 by Gottfried Wilhelm Leibniz, Christiaan Huygens, and Johann Bernoulli, in response to a challenge posed by Jacob Bernoulli to find the curve of a hanging chain.[6][4] Huygens had earlier coined the term "catenary" (from Latin catena, meaning chain) in a 1690 letter to Leibniz.[6] Key geometric properties include the arc length from the vertex to a point (x, y), given by s = a \sinh(x/a), which reflects the curve's hyperbolic nature.[4] The intrinsic equation relating the radius of curvature \rho and arc length is \rho a = s^2 + a^2, highlighting the catenary's non-constant curvature.[4] A common misconception, stemming from Galileo's approximation, equates the catenary to a parabola y = k x^2; while similar for small angles, the catenary grows exponentially at large distances, unlike the parabola's quadratic form.[6] When rotated about its axis of symmetry, the catenary generates the catenoid surface.[4]