Abstract
This technical disclosure establishes a standalone, deterministic framework modeling planetary-scale volatile outgassing as a direct fluid-mechanical consequence of subsurface substrate shear stress. By executing an un-truncated cross-reduction of recent Martian gas seepage datasets against the Eckes Earth Geodynamic Invariant equations under Material Volumetric Monism, we demonstrate that the red planet behaves as a sub-threshold phase-relaxation engine. Lacking an active tectonic node network to continuously vent internal structural entropy, Mars' large, low-density, sulfur-rich liquid core generates immense localized back-pressure at the core-mantle boundary (CMB). This paper provides the exact metrological transformations, explicit ASCII topological core diagrams, and cross-silo syntactic proofs required to show how this internal shear stress physically fractures the rigid, single-plate Martian lithosphere along strict Eulerian lines, venting volatile wave states to the surface to maintain absolute baseline equilibrium (\(z=0\)) against the background cosmic medium.
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Recommended Citation
Eckes, Christopher L., "Technical Disclosure Specification: SPEC-397: Interplanetary Geodynamic Invariants: Modeling Martian Volatile Outgassing and Core-Mantle Boundary Shear Stress as a Sub-Threshold Phase-Relaxation Engine", Technical Disclosure Commons, ()
https://www.tdcommons.org/dpubs_series/12914