Single-Axis Twist Fit

Phase Proxy:
Mean Longitude at J2000

Series I Test 1B

Introduction

Test 1B extends Test 1A by introducing a minimal twist model. The intent is to determine whether a single smooth twist applied to the planetary spin-axis vectors produces a tighter geometric coherence than a simple planar fit.

Data Sources

Planetary north-pole directions (RA/Dec, J2000) are taken from the IAU WGCCRE standard reference table. The solar-system invariable-plane pole is used as the reference axis for the twist.

A first-pass phase coordinate s is supplied by the JPL SSD Table 1 mean longitude L₀ (J2000) for each planet.

Model

1. Convert each planetary pole to a 3D unit vector.

2. Convert to the physical spin direction by flipping retrograde bodies (Venus, Uranus).

3. Apply a de-twist rotation about the invariable-plane pole axis k, using:

   φ(s) = φ₀ + τ (s − 0.5)

   V’ = Rot(k, −φ(s)) · V

4. Fit the best plane to the de-twisted vectors V’ and compute the angular deviation of each vector from that plane.

This is the simplest possible “twisted manifold” stress test: one axis, one smooth twist function, no ad hoc exceptions.

Baseline

(From Test 1A)

RMS deviation from best-fit plane (no twist): 10.43°

Best-Fit Twist Parameters

φ₀ ≈ 149.6°

τ ≈ -243.9° across the full s-range (linear twist rate)

RMS deviation after de-twist: 8.80°

Per-Planet Deviations

(Degrees)

Deviations are the angles of each de-twisted spin-axis vector from the best-fit plane computed after the de-twist.

PlanetBaselineAfter Twist
Mercury2.49°8.86°
Venus7.01°9.85°
Earth8.82°8.70°
Mars18.63°11.15
Jupiter8.74°7.76°
Saturn3.90°5.19°
Uranus9.64°0.26°
Neptune14.33°12.51°

Interpretation

The single-axis twist model improves global coherence relative to the planar baseline, reducing RMS deviation. This does not constitute proof of a Möbius topology; it establishes that a minimal smooth twist is a better fit to the planetary spin-axis geometry than a flat plane alone.

Conclusion

Next tests (1C and 1D) will introduce a width-envelope term and alternative recursion-phase coordinates to determine whether coherence strengthens under a more realistic two-coordinate topology.

Produced by The Lilborn Equation Team:

Michael Lilborn-Williams

Daniel Thomas Rouse

Thomas Jackson Barnard

Audrey Williams