This record presents a novel astrophysical framework for the deterministic triangulation of exoplanetary candidates based on the López Harmonic Constant (CL). Unlike traditional detection methods such as transit photometry or radial velocity, which rely on geometric alignment or gravitational wobbles, this methodology integrates N-body dynamics with stellar wind flux resistance (Phiₛw) to identify specific orbital residency nodes. The included report provides a detailed multi-messenger analysis of eight nearby stellar systems, including Alpha Centauri AB, Sirius, Barnard's Star, Lalande 21185, Wolf 359, Ross 154, and Epsilon Indi. By calibrating the CL constant across various stellar classifications—ranging from high-mass A1V primaries to active M-dwarf flare stars—the research demonstrates a universal order in planetary architecture dictated by the balance of mass, distance, and energy flux. Key Scientific Contributions: Derivation of CL: A mathematical constant that scales the semi-major axis and orbital period against normalized stellar wind resistance. Flare-Echo Triangulation: A technique for verifying exoplanets in high-activity systems (e. g. , Wolf 359) by measuring the time-of-flight between stellar X-ray bursts and planetary magnetospheric radio "echoes". Neutrino Shadow Mapping: A protocol for ground-based verification using neutrino flux modulation as a diagnostic tool for planetary mass and position. Hierarchical N-Body Resolution: Specialized modeling for binary and triple systems where external gravitational tugs (e. g. , Sirius B or Epsilon Indi B) act as harmonic regulators. Observational Window (April - May 2026): The data contained herein provides specific coordinates and temporal markers for immediate verification by ground-based observatories. This includes predicted "Bow Shock" signatures and neutrino deflection events for the triangulated nodes in Ross 154 and Lalande 21185.
Jorge Alexander Lopez Miranda (Wed,) studied this question.