The Fornax dwarf spheroidal hosts five old globular clusters, including the relatively massive Fornax 3, currently observed at radii of order 1 kpc. In a cuspy ΛCDM dark halo these clusters should have experienced strong dynamical friction and spiraled into Fornax's center within a few Gyr, creating a nuclear star cluster that is not observed (Tremaine 1976; Cole 2012; Read 2006; Boldrini 2020). The classic Fornax timing problem.
The standard model has Fornax embedded in a cuspy CDM halo whose strong dynamical friction should have driven the globular clusters inward by now. Resolving the Fornax 3 problem within ΛCDM demands either a large constant-density CDM core (difficult to produce in cuspy CDM simulations), modified gravity, or non-standard dark matter. None of these is parsimonious within minimal ΛCDM.
SCT replaces the hot-dense-center with a superluminal collision and the thermalized debris field. From this single change, the Fornax 3 timing problem dissolves entirely. Fornax has no CDM particle halo (P50, P51, P52, P54): its apparent dynamical mass comes from gravitational superposition through the Φ_mesh contribution from the broader Local Group cosmic-web. The mesh-based effective halo gives a smooth cored profile by construction, not a cuspy NFW.
With no cuspy CDM particle population to couple to, dynamical friction on the globular clusters is dramatically reduced. The clusters can persist at their current radii indefinitely without spiraling into Fornax's center. The absence of a nuclear star cluster is the predicted SCT outcome rather than an unsolved ΛCDM puzzle. Angular-momentum inheritance (P31, P32) gives the cluster orbital structure inherited from cascade-stream parent geometry, naturally producing the observed near-circular orbits at 1-kpc radii.
Sibling pockets (P58, P59, P60) provide the broader Local Group context. Pre-existing matter (P25) gives Fornax + clusters their stellar populations from in-cycle nucleosynthesis on cascade-thermalized gas. The same M6 framework that produces the no-DM-particle resolutions for galaxy rotation curves (recid 112), peak statistics deficit (recid 71), Bullet Cluster (recid 220), and the broader dwarf-galaxy mass-to-light ratios accounts for the Fornax timing problem. There is no need for cored CDM halos, modified gravity, or non-standard dark matter.
If precision Gaia + JWST Fornax mapping demands a CDM-particle halo at the ΛCDM cuspy abundance to explain the dynamics (no Φ_mesh-based smooth-profile signature, no reduced-friction signature on globular cluster orbits), the M6 no-DM-particle explanation is refuted. The signature SCT prediction is the globular clusters persisting at current radii indefinitely with no detectable inward orbital decay.