Appendix P — Derivation 16: Orbital Motion from Mutual Anchoring

Appendix P — Derivation 16: Orbital Motion from Mutual Anchoring

(Foundations v1.0 • 2025-06-10)

Planetary orbits arise in Phase-Biased Geometry (PBG) because two
coherence fields bias one another’s motion. No Newton force, no curved
metric: each body simply follows the steepest-descent path in the
anchoring-cost landscape
.


1 Two anchored modes

For bodies 1 and 2 with masses M1,2 the locked kernel
(Foundations §2) gives

Φi(r)=Nirekr,Ni=c2Mi4πα,k=β/α.

Define Bi=c2Φi (units J).


2 Interaction cost

Total anchoring interaction

Cint=[ρ1B22+ρ2B12]d3x,

with ρi(x) each envelope’s density (ρiδ
for point mass).


3 Equation of motion (imports universal rule)

From Foundations §3:

mr¨=mc2Φ1(ρ2B12).

For kr1 this reduces to Newton’s
r¨=GM1r/r3, but the exact PBG force uses
ekr(1+kr).


4 Orbital precession

Because B(r)2r2e2kr, the potential deviates
slightly from 1/r. Expanding to first order in kr yields the
well-known advance

Δϖ=6πGM1a(1e2)c2(Mercury: 43/century),

identical to GR but here caused by the Yukawa correction rather than
metric curvature.


5 Stability & multi-body generalisation


Take-home

Orbits in PBG are paths that keep the combined anchoring cost of all
bodies minimal
. Apparent “gravity” is the gradient
c2Φ, already fixed by {α,β,γ} — no force
law or spacetime metric required.

Appendix O - Photon Structure | [Index](./Appendix Master) | Appendix Q - Galaxy-Scale Lensing