Math Art
Steiner Surface (Veronese shadow)

Steiner Surface (Veronese shadow)

Steiner Surface (Veronese shadow) is a topological surface, given by a parametrisation, immersed.

Open Steiner Surface (Veronese shadow) in the interactive viewer →

aperiodic def-parametric immersed implemented topological

About

The general name for Steiner's quartic images of the projective plane, of which the Roman surface is the symmetric member. All of them are quartics, all self-intersect, and all carry pinch points; they were among the first surfaces studied for their singularities rather than in spite of them.

Formula

x(u, v)
sin⁡(u)⁢cos⁡(v)⁢sin⁡(v)\sin\left(u\right) \cos\left(v\right) \sin\left(v\right)
y(u, v)
cos⁡(u)⁢cos⁡(v)⁢sin⁡(v)\cos\left(u\right) \cos\left(v\right) \sin\left(v\right)
z(u, v)
sin⁡(u)⁢cos⁡(u)⁢cos⁡(v)2\sin\left(u\right) \cos\left(u\right) \cos\left(v\right)^{2}

Properties

Family
topological
Given by
a parametrisation
Curvature
no condition imposed
Periodicity
not periodic
Ends
0
Embedding
immersed
Fidelity
exact
Exactness
elementary

Definition

projection angle fixed to the operator default 0 degrees, where the Veronese shadow is exactly the Roman surface; other angles sweep to the cross-cap

Sources

Chart reproduced numerically against the shipped implementation: fwd max 0.73 of tol, 0.0% of oracle beyond tol (tol floor 2.5 x 0.01739).