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Loading contentHow the universe is measured, rung by rung — from the geometry of parallax to the exploding stars that reach across the cosmos — and how following the ladder to its top revealed the Hubble tension. Built on real methods and measurements; values are not invented and proposed resolutions are labelled unconfirmed.
Gravitational-wave sources whose distance can be read directly from the shape of the waveform, with no calibration ladder at all — the gravitational analogue of a standard candle. A merging neutron-star pair with an electromagnetic counterpart yielded the first standard-siren measurement of the Hubble constant.
The sharp, near-constant peak brightness that red giant stars reach just before the helium flash — a robust standard candle that can be measured in a galaxy's halo, away from crowding and dust. It provides an independent route to calibrating Type Ia supernovae, and its Hubble-constant value sits between the Cepheid and CMB results.
The programme that measures the Hubble constant from the local distance ladder — anchoring Cepheids with parallax, using them to calibrate Type Ia supernovae, and reading the expansion rate from supernovae in the smooth Hubble flow. Its value comes out consistently higher than the one inferred from the early universe, and that gap is the Hubble tension.
The fraction of the universe's total energy density that is in matter — dark matter plus ordinary baryonic matter — today. Together with the dark-energy density it sets the geometry and the fate of the universe; it is measured most precisely from the cosmic microwave background.