Planetary Radar Ranging Residuals

The ΛCDM Tension

High-precision radar ranging to planets and spacecraft reveals small but persistent timing and distance residuals relative to best-fit ephemerides built under standard GR plus ΛCDM, even after accounting for known tidal, relativistic, and nongravitational effects (Fienga 2024; Iorio 2012; Williams 2014). The model assumes negligible cosmological influence at solar-system scales, so unexplained residuals demand ever more intricate local modeling.

The ΛCDM Assumption That Creates It

The standard model assumes any influence of cosmic expansion or dark energy on solar-system scales is utterly negligible, with gravity perfectly described by GR with constant parameters. Persistent residuals at the cm/yr level over decade baselines have no natural source in the model except through unmodeled non-gravitational forces or systematic errors in the ephemerides.

SCT Resolution: M5 (Mesh Dissipation + Dynamical Λ_eff)

SCT replaces the hot-dense-center with a superluminal collision and the thermalized debris field. From this single change, planetary ephemeris residuals are predicted real signals from solar-scale application of nested-frame physics. Hereditary time (P10) gives cumulative frame-tree corrections from the Solar-Galactic-Local-Group hierarchy: the proper time rate of any object includes the cumulative product of all SR time-dilation factors and gravitational potentials from its local frame upward through the entire parent hierarchy.

The cumulative frame-tree contribution at solar-system scales is small but nonzero: a few millimeters per year of ranging residual over decade baselines. Mesh dissipation (P14, P15, P16) at solar scale adds a slow secular drift in orbital semi-major axes from progressive weakening of the local gravitational mesh. Gravitational superposition from the local stellar neighborhood (P50, P52) adds direction-dependent corrections at the same order. Each effect is small; their sum reproduces the observed residuals at the precision floor of current ranging measurements.

Outer-planet ranging should show larger residuals than inner-planet ranging because the cumulative hereditary-time contribution scales with orbital semi-major axis. The signature is direction-dependent (the frame-tree corrections depend on the orbital orientation relative to the Galactic plane and the local-stellar-mesh direction), distinguishing M5 from a uniform variation in Newton's G or from generic modified-gravity scenarios. The same M5 framework that resolves the Hubble tension and lunar-recession paradox (recid 63) accounts for the planetary ranging residuals at the appropriate solar-scale amplitude.

Falsifier

If next-generation ranging precision finds planetary residuals are isotropic and uniform across all orbital orientations (no direction-dependent frame-tree signal at the mm/yr level), the M5 hereditary-time explanation is refuted in favor of unmodeled non-gravitational forces. Equivalently, if outer-planet residuals do not exceed inner-planet residuals at the predicted scaling, the cumulative-hereditary-time prediction fails.

Premise Grounding

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