Phaethon: Relativistic Tidal Ring Observatory

Phaethon is an interactive, real-time astrophysical visualization engine that models the evolution of a collisionless ring of orbiting test particles under the combined gravitational influence of a central black hole and a massive, eccentric stellar intruder.

The simulation uses Newtonian gravitational dynamics, symplectic Velocity Verlet integration, and weak-field General Relativistic corrections to model orbital motion, energy exchange, angular momentum evolution, and tidal disruption. As the intruder approaches the ring, differential gravitational forces stretch and perturb individual particles, producing density waves, orbital distortions, gaps, tidal streams, and high-energy debris structures.

Its physics engine incorporates Keplerian circular orbits, Kepler’s Third Law, Schwarzschild-inspired 1PN perihelion precession, tidal acceleration scaling, and Hamiltonian energy-conservation diagnostics to provide a scientifically grounded model of gravitational interactions.

On the visualization side, Phaethon combines GPU-accelerated particle rendering, procedural stellar and black-hole environments, gravitational-lensing-inspired visual effects, temperature-based color mapping, dynamic debris fields, and a NASA/JPL-inspired scientific telemetry interface.

Users can interact with the simulation in real time, adjust the simulation speed, pause and reset the system, toggle relativistic corrections, inspect tidal-field behavior, and observe how a seemingly ordered orbital structure evolves into a complex, dynamically disturbed environment.

The core objective of Phaethon is to bridge computational astrophysics and cinematic scientific visualization—turning abstract gravitational equations into an observable, interactive demonstration of orbital mechanics, tidal disruption, and emergent cosmic structure.

Note: The simulation uses documented approximations rather than full General Relativity, magnetohydrodynamics, or particle-collision physics.