Cosmos Genesis Docs

Peer-reviewed models for solar wind, radiation environments, the full electromagnetic spectrum, orbital mechanics, and satellite positioning — each with measurable accuracy claims and published references.

Distributed pipeline producing physically accurate stellar populations at any scale. Covers the initial mass function (IMF), stellar aging, many-body gravity (N-body) relaxation, and five automated physics validators with published benchmarks.

Natural language over your entire generated universe. Ask questions, traverse knowledge graphs, and integrate AI reasoning into your applications.

Three-identity autonomous engineering: developer, auditor, and knowledge guardian. Structured review gates, self-correction cycles, and full provenance tracking on every code change.

Coronal mass ejection propagation, Parker spiral field structure, and magnetospheric coupling. Physics-based forecasting of auroral activity and geomagnetic storm intensity.

Particle flux modeling across radiation belts, planetary surfaces, and deep space. Geiger-scale radiation zone mapping with dose-rate estimation for mission planning and hazard assessment.

21-band radio signal simulation spanning the full electromagnetic spectrum. Directional lobe rendering for pulsars, quasars, and active galactic nuclei with signal strength and interference modeling.

Live orbital positioning for operational satellites using two-line element set (TLE)/SGP4 propagation. Full constellation catalog coverage with SPICE kernel integration for high-precision ephemerides.

Complete trajectory simulation for interplanetary and cislunar missions. Burn sequencing, lunar orbit insertion, trans-Earth injection, and emergency return window analysis.

Author a system's evolutionary fate in real time — convert stars to white dwarfs, neutron stars, or black holes, decide each planet's outcome, and run N-body integration to stability. Lock relaxed N-body orbits back to Keplerian elements with one click.