Eureka V  - Araya2 V1.5 Frozen Operator Audit

NASA PSCompPars Confirmation of the Roche–Tauro Topology for Extreme Hot Jupiters

Eureka V — Araya2 V1.5 presents the first frozen-operator population audit of the Araya2 Roche–Tauro State-Space Topology using a NASA PSCompPars-derived sample of extreme Hot Jupiters and giant short-period exoplanets.

This record moves Araya2 beyond isolated benchmark cases. The Roche–Tauro topology published in Eureka IV is now tested against an expanded external population using a frozen, non-recalibrated Araya2 classification operator. The result is direct and structurally significant: systems traditionally treated as disconnected orbital-decay anomalies are reorganized into ordered state-space positions.

The central conclusion of this publication is:

The anomaly is no longer an anomaly; it becomes a position within the state-space topology.

Under the Araya2 framework, WASP-12b is no longer merely an extreme tidal-decay outlier. It is classified as a Roche–Tauro amplification state. WASP-19b is no longer a contradictory near-Roche system with suppressed or unresolved decay behavior. It is classified as a Roche–Tauro suppression state. WASP-103b, HIP 65 A b and WASP-121b emerge as critical-boundary systems, while the wider population remains organized inside the stable mesh field.

This transforms the problem. What conventional tidal interpretation often treats through case-by-case dissipation coefficients, separate explanatory patches, or system-specific anomaly handling is reframed by Araya2 as a unified geometric population structure. The outlier is not discarded, forced or patched. It is located.

This release is deliberately public and non-enabling. It does not disclose the proprietary Araya2 calculation engine, internal constants, private calibration terms or generative derivation. It discloses only the classification consequence: the extreme Hot-Jupiter population can be separated into stable mesh, critical-boundary, Roche-suppression and Roche-amplification regimes within a single Roche–Tauro state-space topology.

Eureka V therefore establishes a timestamped technical priority record for the Araya2 Anomaly Repositioning Principle:

An apparent anomaly is not necessarily an exception to the system; it may be a state-position not yet mapped by the prevailing framework.

With this audit, Araya2 advances from a proposed exoplanetary topology to a frozen-operator population classification framework. The infrastructure is now prepared for the next consistency frontier: applying the same state-space logic to low-acceleration gravitational systems, beginning with Gaia DR3 wide binaries.