Within its first year of operation, the James Webb Space Telescope detected massive, well-formed well-formed galaxies at redshifts as high as 13 – meaning they already existed only 325 million years after the Big Bang. According to ΛCDM, such galaxies should not have had time to accumulate sufficient mass, should not appear so evolved (with defined structure and mature stellar populations), and should be rarer and smaller at such high redshifts. The abundance, size, and apparent maturity of these early galaxies challenges both the timeline and mechanisms assumed in ΛCDM. While some argue that adjustments to star formation efficiency or feedback processes might resolve this, others view it as a more serious anomaly, possibly requiring rethinking cosmic expansion history, matter content, or the nature of early gravitational collapse.
The unusually early, massive galaxies revealed by JWST present a serious problem for ΛCDM because, within that framework, there simply isn’t enough time for such systems to form. The problem only arises if the ΛCDM timeline is treated as a literal record of events, stretching cleanly from a hot dense beginning to the present day. If that whole history is taken for granted, the new data look impossible.
2PC removes that expectation. If the early universe is not an earlier physical era but an observational surface reconstructed from the present cosmic state, then this question, like so many others, changes shape. Instead of asking how real galaxies managed to assemble so quickly in a young universe, we must ask why the structures that appear on the reconstructed early surface have the mass and maturity that they do.
One potential explanation is that the pattern we see is a by-product of the same selection constraints that shape the rest of the embodied branch. If complex life requires a particular set of large-scale conditions, and those conditions depend on the way structure develops over cosmic time, then only those retrodicted early surfaces that support a viable long-term path to embodiment will appear within Phase 2. This does not mean that LUCAS needed distant galaxies to form early in a literal past. It means that in the version of the cosmos where everything was just right for LUCAS to evolve in the Milky Way, conditions across the entire cosmos favoured the early development of this kind of galaxies. Indeed, here might be the answer to the question we were left in the section about psychegenesis concerning which "cosmic egg" is selected for realisation. There are infinite possible cosmoses in the Pythagorean ensemble, but the existence of these galaxies suggests that the selected cosmos (the next in the queue to hatch) is the one where conscious life evolves in the shortest period of time. The selected cosmos is not the one that “wants” consciousness fastest, but the one whose global structure reaches representational stability earliest under the same physical laws. This would mean that not only do we live in a cosmos where everything is just right for the evolution of conscious organisms, but the one where everything is so exceptionally just right that the evolution of LUCAS also happens as quickly as is physically possible. If future observations revealed that galaxy formation was delayed until significantly later cosmic times (say, z < 5 for massive galaxies) this would present a challenge to the 'fast track' interpretation, suggesting that selection favors other constraints over temporal efficiency. This is a second novel empirical prediction.
A similar pattern appears in the case of extreme quasars such as Ton 618, whose central black hole is so massive that, under standard assumptions, it appears to violate the Eddington limit (the maximum rate that objects can acquire mass). Within ΛCDM this again presents itself as a timing and growth problem: there is not enough time for a black hole to reach such a mass through ordinary, radiation-limited accretion without invoking exotic seeds or prolonged super-Eddington phases. As with the JWST galaxies, the difficulty only arises if the inferred early universe is treated as a literal record of gradual physical construction.
Readers will be familiar with the logic now. Ton 618 does not require a historical episode in which physical limits were repeatedly broken; it requires only that the retrodicted early surface of the embodied branch contains black holes whose integrated mass and luminosity histories are globally consistent with the present state of the cosmos. The Eddington limit constrains local accretion dynamics, not the structure of a globally selected spacetime history reconstructed from an already-realised world. Seen this way, extreme early quasars are not anomalies but further expressions of the same selection constraint suggested by the JWST data.