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Co-authored-by: me <me@tane.dev>
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Introduce a new 'Hybrid' simulation mode that combines N-Body physics with Keplerian corrections to improve orbital stability at high simulation speeds.
The existing N-Body mode quickly becomes unstable at high time scales (e.g., above 96x), leading to moons flying off and satellites crashing. This 'Hybrid' mode addresses these issues by periodically applying Keplerian corrections to stabilize orbits, ensuring more robust and accurate long-term simulations while maintaining N-Body realism.