A catenary is the static shape of an ideal flexible, inextensible chain hanging under its own gravitational weight in a uniform gravitational field, with uniform linear mass density along its arc length. With the lowest point above , one convenient vertical origin givesHere has units of length. The supports and the chain's arc length determine the scale and position; horizontal and vertical shifts give the general catenary. [ref]
https://www.damtp.cam.ac.uk/user/reh10/lectures/nst-mmii-handout3.pdf. Robert Hunt, Cambridge Mathematical Methods II: worked example, The Catenary
For , the three points at have heights , , and . If heights should instead be measured from the lowest point, subtract :The same three heights are then approximately , , and . The shift changes the vertical origin and preserves the catenary shape.
A hanging chain follows a scaled hyperbolic cosine, with an optional shift of its lowest point to zero
. The left panel marks on . The right panel puts the lowest point at zero, compares three positive scales , and shows the local parabola for . Details.The scale also measures tension: if is its constant horizontal component, is the linear mass density, and is the magnitude of gravitational acceleration, then . A short force balance explains this. For the portion from the lowest point to , with arc length , vertical tension balances its gravitational weight and horizontal tension givesApplying differentiation yields . The proposed hyperbolic cosine solves this differential equation, because and . This is the mechanism behind the shape, under the stated ideal chain assumptions.
The same identity simplifies the arc length between symmetric supports at :For , , exceeding the horizontal span of two. A larger at fixed gives a shallower sag: the Taylor series gives . Thus a parabola is a local approximation, while the exact ideal chain shape is a catenary. The useful connection is that the same hyperbolic Pythagorean identity controls its coordinates, force balance, and arc length.
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