The observable universe has always remained below its own gravitational radius—yet it is not the interior of a black hole. This apparent paradox, derivable from the Friedmann equations, suggests that three-dimensional space is not the fundamental level of physical description. In this work: (1) we derive the global gravitational constraint Rp ≲ Rg valid in every cosmic epoch; (2) we prove with a causal no-go theorem that this constraint does not imply a black hole-type geometry; (3) we show that, within standard physics, the resolution that survives the exclusion of alternatives is holographic: fundamental information resides on a two-dimensional boundary, while the interior volume is an emergent reconstruction. The ingredients of this argument—Friedmann cosmology, covariant entropy bounds, holographic counting—are individually well established. What has been missing is their systematic combination into a closed logical chain. If this chain were trivial, holographic cosmology would already be the dominant paradigm and inflation would be recognized as optional. It is not, which suggests the synthesis itself is the contribution. The framework dissolves what we call the “spacetime island” problem: in standard physics, coordinates are treated as primitives disconnected from the informational language of quantum theory and statistical mechanics. Holographic emergence reconnects them. Giving up one or two “fundamental” dimensions is a gain in parsimony and unification, not a loss. Observable consequences follow. The Gaussianity of the CMB emerges from the central limit theorem applied to boundary degrees of freedom. Primordial gravitational waves are expected to be strongly suppressed (r < 10−3); a robust detection at r > 10−2 would falsify the minimal framework. Recent observations—the absence of predicted dark matter subhalos in high-resolution lensing, the anomalous pressure in cluster mergers—provide independent hints that the standard picture has cracks where this framework offers natural explanations.