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Cosmology · Concept

Hubble Constant

Reading time: 9 minConfidence: HighLast verified: October 2026

The Hubble constant (H0) is the present-day value of the Hubble parameter: the rate at which the universe is expanding, expressed as the recession velocity per unit distance of distant galaxies. It is measured in kilometres per second per megaparsec, and current measurements fall between about 67 and 73 km/s/Mpc depending on the method, a disagreement known as the Hubble tension.

Curious

One sentence that captures itThe Hubble constant tells you how fast the universe is stretching today: a galaxy one megaparsec away recedes at about 70 kilometres per second, and one two megaparsecs away recedes twice as fast.

In 1929 Edwin Hubble showed that galaxies are moving away from us, and that farther galaxies recede faster (see Edwin Hubble). That straight-line relationship is Hubble's law, and the slope is the Hubble constant. You can explore the law interactively in the Hubble's Law simulation.

The name is slightly misleading: H0 is constant across space at any one moment, but it changes over cosmic time as the expansion speeds up or slows down. The subscript zero means “value today”. Because the number sets the overall scale of the universe's size and age, pinning it down is one of the central goals of observational cosmology.

Exploring

Worked example — the Hubble timeIf the expansion had always run at today's rate, the age of the universe would be 1/H0. With H0 = 67.4 km/s/Mpc, 1/H0 = 14.51 billion years; with H0 = 73.0 km/s/Mpc, it is 13.39 billion years. The rate has not been constant, so this is only a scale, not the true age (about 13.8 billion years; see Age of the Universe). Values computed in Python for this page.
MethodApproximate H0 (km/s/Mpc)Type
Planck 2018 CMB (assuming ΛCDM)67.4 ± 0.5Early universe
SH0ES Cepheids + Type Ia supernovae73.0 ± 1.0Late universe
Common mistake — Commonly ConfusedH0 is not a speed. It is a rate: speed per distance. Also, the recession of galaxies is mainly the stretching of space between them, not galaxies flying through space away from us, so recession speeds can exceed the speed of light for very distant galaxies without breaking relativity.

Deep Dive

Primary sourceHubble, E. (1929). “A relation between distance and radial velocity among extra-galactic nebulae.” Proceedings of the National Academy of Sciences, 15(3), 168–173.

Definition. The Hubble parameter is H(t) = ȧ/a, where a(t) is the cosmic scale factor; H0 is its value at the present time. Hubble's law v = H0d holds for distances small compared with the Hubble radius c/H0 (about 4,400 Mpc for 67.4 km/s/Mpc). The conversion 1 Mpc = 3.0857×1022 m gives H0 = 67.4 km/s/Mpc = 2.18×10−18 s−1. The critical density that sets the geometry is ρc = 3H02/(8πG) ≈ 8.5×10−27 kg/m³.

How it is measured. The “distance ladder” calibrates distances with geometry (parallax), then Cepheid variables, then Type Ia supernovae in distant galaxies (see Supernovae). The independent “early-universe” route infers H0 from the pattern of temperature fluctuations in the cosmic microwave background, assuming the standard ΛCDM model. Other routes include gravitational-wave “standard sirens” (see LIGO and Virgo), strong-lensing time delays, and the tip of the red giant branch.

The Hubble tension (unresolved). The distance-ladder value near 73 km/s/Mpc and the CMB-inferred value near 67 km/s/Mpc differ by more than the quoted uncertainties, at roughly the 5-sigma level in some analyses. Some recent analyses using tip-of-the-red-giant-branch and JWST data find intermediate values near 70, with their authors disagreeing on the implications. Whether the tension reflects undiscovered measurement systematics or new physics beyond ΛCDM, such as early dark energy, is an open question; this Codex does not take a side.

Sources

  • Hubble, E. (1929). Proceedings of the National Academy of Sciences, 15(3), 168–173.
  • Planck Collaboration (2020). Astronomy & Astrophysics, 641, A6.
  • Riess, A.G., et al. (2022). “A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.” The Astrophysical Journal Letters, 934, L7.
Last verified: October 2026 · Source: Hubble (1929); Planck 2018; Riess et al. (2022) · Confidence: high