HomeCosmologyHubble Tension — Two Ages of the Universe

Hubble Tension — Two Ages of the Universe

Two flat-ΛCDM universes, one calibrated to the CMB (Planck) Hubble constant and one to the local distance-ladder (SH0ES) value, expanding side by side from the closed-form Friedmann solution — watch the real ~5σ Hubble tension turn into a measurable gap in the age of the universe.

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universe-age ↗ Open standalone

Two identical flat-ΛCDM universes, side by side, differing only in which Hubble constant measurement calibrates them: one uses the cosmic-microwave-background value from Planck, the other the local Cepheid–supernova distance-ladder value from the SH0ES collaboration. Both scale factors are computed from the exact closed-form solution of the Friedmann equation for a matter-plus-dark-energy universe, so the growing separation between the two galaxy lattices as you press Play is a real, physically-derived consequence — not an animation trick — of the genuine ~9% disagreement between the two H₀ measurements that cosmologists call the Hubble tension.

⚙ Under the hood

Two flat-ΛCDM universes expand side by side from the exact Friedmann-equation solution — one calibrated to the CMB (Planck) Hubble constant, the other to the local distance-ladder (SH0ES) value — turning the real ~5σ Hubble tension into a visible, measurable gap in the universe's age.

cosmologyhubble constantfriedmann equationdark energybig bangexpansion

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