Lumenis IO: Proxima Centauri System — Full Causal Reconstruction and Habitability Analysis (2025)

This paper presents the first full causal reconstruction of the Proxima Centauri planetary system (b + c) using the Lumenis IO Engine Full Causal-Validation Edition. The simulation spans 4.5 billion years of planetary evolution under physical field dynamics — including orbital, magnetic, and atmospheric progression — without observational seeding. Results replicate the system’s current coordinates (RA 217.43°, Dec −62.68°) and mean orbital velocity (24.07 km/s), confirming a stable evolutionary pathway driven by Slow Drift / Field Realignment. The findings suggest that Proxima b retains partial atmospheric integrity and terminator-zone habitability potential, while Proxima c remains dynamically stable as a cold super-Earth. This research contributes to understanding exoplanetary formation and survivability around magnetically active red-dwarf stars.