Hubble's Law Distance Calculator

Enter a galaxy's redshift and the Hubble constant to estimate its recession velocity and distance using Hubble's Law.

Redshift inputs

Enter the measured redshift and the Hubble constant to use.

Estimated distanceEnter values above.
Recession velocity
Distance in light-years
Hubble constant used
Quick insight

Hubble's Law Distance Calculator

Enter a redshift and Hubble constant to estimate recession velocity and distance.

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What Is a Hubble's Law Distance Calculator?

Hubble's Law states that a galaxy's recession velocity is proportional to its distance: v = H0 × d. This calculator rearranges that relationship to estimate a galaxy's distance from its redshift and a chosen value for the Hubble constant, H0 — the same basic method used to derive rough distances to galaxies too far away for direct measurement.

Redshift happens because the universe's expansion stretches the wavelength of light in transit; the more a galaxy's spectral lines have shifted toward red, the faster it is receding and, by Hubble's Law, the farther away it is.

How to Read Your Results

Estimated Distance

The primary result, in megaparsecs (Mpc) — the standard astronomical distance unit for cosmological scales (1 Mpc ≈ 3.26 million light-years).

Recession Velocity

The speed at which the galaxy is moving away from us, estimated from redshift using v = cz.

Distance in Light-Years

The same distance converted to millions of light-years, often a more intuitive unit for a general audience.

Hubble Constant Used

Confirms which value of H0 was applied, since published estimates of H0 range from about 67 to 73 km/s/Mpc depending on the measurement technique — a real, unresolved discrepancy in cosmology known as the "Hubble tension."


Real-World Example

A galaxy is measured with a redshift of z = 0.02. Using H0 = 70 km/s/Mpc:

QuantityValue
Redshift (z)0.02
Recession velocity≈ 5,996 km/s
Estimated distance≈ 85.7 Mpc (≈ 280 million ly)

Tips for Using This Calculator

  • This v = cz approximation is only reliable for small redshifts (roughly z < 0.1) — at higher redshifts, relativistic effects require a full cosmological model.
  • Try a range of H0 values (67–73) to see how sensitive the distance estimate is to the ongoing Hubble tension debate.
  • Local galaxies also have their own "peculiar velocity" from gravitational interactions, which adds noise to redshift-based distance estimates at close range.

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Note: This calculator uses the simple non-relativistic v = cz approximation and a single flat value for H0. It is not accurate for high-redshift objects and does not model dark energy or the full cosmological distance ladder.

Last updated: August 2026 · Reviewed by: Simple Calculator Tools Editorial Team