Separate Directional Pressure Channels and Earth Axial Orientation A revised testable extension of the Thermodynamic Model
This paper reassesses the hypothesis that Earth axial orientation may reflect distinct pressure channels within the Thermodynamic Model. The revised formulation incorporates developments from the later circulation, redshift, interaction-layer, ozone, lunar-distance and comet studies. The Sun is treated as the dominant local pressure and orbital reference. Five external directions are retained as separate candidate channels: Gaia BH1, Gaia BH2, Gaia BH3, A0620-00 and OGLE-2011-BLG-0462. The Solar System boundary supplies a weaker and more distributed background in the model. No black-hole directions are averaged into a fictitious source. Each channel retains its own direction, amplitude, coupling, delay and torque. Gaia BH1 is presently 89.42 degrees from Earth axis and is therefore almost transverse to it. Gaia BH3 is 75.07 degrees from the axis and supplies a different axial and transverse geometry. The angular relationship is a hypothesis-generating observation rather than evidence of causation. A uniform pressure through Earth centre cannot tilt the planet, so a viable mechanism requires asymmetric coupling, a lever arm, dissipation and angular-momentum conservation. The revised paper also recognizes that several physically separate sources may be statistically unidentifiable in a single axial record. It excludes modern magnetic-pole drift and geomagnetic reversals from the axial claim, retains conventional lunar, solar and geophysical torques as the comparison baseline, and sets out cross-planet and out-of-sample tests.
Authors
- Björn Vernharðsson
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-09-14
- DOI
- https://doi.org/10.5281/zenodo.22753144
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- preprint