Top 100 host star systems ranked by the Resonance–Stability Framework

This dataset extends the Resonance–Stability Framework to the Top 100 ranked exoplanet host systems, building on the previously published Top 30. It includes a cross-match with NASA’s Sept 17, 2025 milestone confirmations (WISPIT, GJ 536 c, HD 224018, HD 28471, HIP 41378 g, K2-73, TOI-1438, TOI-2322, TOI-6303, TOI-6330), demonstrating predictive alignment between the framework’s rankings and the newest observational discoveries. Resonance–Stability Framework Equation S = 0.5 * R + 0.3 * H + 0.2 * N Where: R = Resonance proximity score(closeness of orbital period ratios to low-order p:q mean-motion resonances, e.g. 2:1, 3:2, 4:3). H = Hill stability metric(mutual Hill separation, ∆ ≥ 10 threshold, measuring long-term dynamical stability). N = No-crossing margin(checks periastron vs. apastron separation, ensuring planetary orbits do not geometrically overlap). Final System Score: For multi-planet systems, the system score is taken as the maximum S among its planet pairs (proxy for the strongest resonance–stability chain).