Planetary Axial Hydrodynamics in a 4D Continuum: Vacuum Friction as the Primary Source of Anomalous Heat and Asymmetric Magnetism
Abstract
This theoretical paper challenges the stochastic "giant impact" models traditionally used to explain the extreme axial tilts, thermal anomalies, and asymmetric magnetic fields of planets like Venus and Uranus. Using the framework of the Superfluid Vacuum Theory (SVT) and the Topologically Resonant Fractal Continuum (TRFK), we model the ecliptic not as empty space, but as a macroscopic rotating current of a 4D incompressible superfluid driven by the Sun. We formulate the Hypothesis of Topological Friction, demonstrating that angular misalignment between a planet's rotation and the ecliptic flow results in deterministic fluid-dynamic consequences. We mathematically define how retrograde rotation (Venus, ~180°) maximizes viscous dissipation, degrading macroscopic kinetic shear into anomalous thermal energy. Conversely, orthogonal rotation (Uranus, ~98°) maximizes cross-flow shear, elegantly explaining its radically off-center and tilted magnetic dipole as a direct geometric distortion of vacuum vorticity.
Fields of Study & Subjects
Astro and Planetary Science
Relativity and Gravitational Theory
Stellar
planetary
and galactic studies
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 6 March 2026
- Language
- EN
- Document type
- Preprint