The Deep-Time Stability of the Solar System: A Full-Scale 100-Million-Year Reverse Evolution of Circumsolar Fields

This paper introduces a groundbreaking reconstruction of early Solar System field dynamics, evolving the system 100 million years backward with unprecedented detail. The simulation exposes long-range structural coherence, total topological stability, and deeply ordered field behavior across all nodes. These findings challenge conventional assumptions about early Solar System chaos and instead reveal a deeply structured, self-stabilizing environment extending across millions of years. This work sets a new standard for planetary system modelling and opens the door to a fundamentally different understanding of Solar System formation.