Rotating Liquid Mirror

2D twin of the ZENITH LM-9 observatory: a meridian cross-section with traced rays, the surface profile, the focal spot and the spin-up of the liquid.

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Mirror

A liquid in rigid rotation settles into a perfect paraboloid whose focal length depends only on the spin rate.

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Model checks

The science

What is modelled

In the frame rotating at ω, each liquid element feels gravity and the centrifugal force, so the free surface is an equipotential z = ω² r² / (2 g): an exact paraboloid with focal length f = g / (2 ω²). At 1.25 rad/s this is 3.14 m, the 3D page's reference value. Rays are traced with the law of reflection on the true surface normal.

Equations

  • Surface slope: dz/dr = ω² r / g.
  • Spin-up: the liquid approaches the drive speed on the Ekman time ∼ H / √(ν ω) (3x for the plot).
  • Coma of a paraboloid: ∼ 3 θ / (16 N²) radians, N = f / D.

Checks run in the page

  • Integrated surface slope against the closed form.
  • Exact ray tracing finds the focus at g/(2ω²).
  • The traced coma length matches 3θ/(16N²) for a slow mirror.

Meridian-plane tracing only; ripple, vibration and the mercury vapour hazard are not modelled.

What to try
  • Press Compare with rigid sphere: the sphere of the same curvature blurs on-axis rays (spherical aberration), the liquid paraboloid does not.
  • Raise the off-axis angle until the green spot grows a one-sided tail (coma).
  • Reduce the depth of the liquid and watch the spin-up get faster.
Surface profile
Focal-plane spot (rays per bin)
Focal length against spin rate
Spin-up of the liquid
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