This framework enables comparative analysis and anomaly detection in exoplanetary systems, suggesting new insights into planetary structures.
This paper introduces a coverage-aware, data-driven framework for diagnosing the architecture of exoplanetary systems using catalog observables. The method integrates orbital spacing, excitation, mass hierarchy, and resonance structure into a unified diagnostic applied across multi-planet systems. The framework enables comparative analysis and anomaly detection without imposing dynamical stability or formation assumptions.
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Peter Brunzelle (2026) studied this question.
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