Illustration accompanying Why Do Two Measurements of Cosmic Expansion Disagree?

EVIDENCE FILE 05 / COSMOLOGY

Why Do Two Measurements of Cosmic Expansion Disagree?

One method reaches back to the young universe. Another measures a ladder of nearby distances. Why don't their answers comfortably meet?

By The Last TransmissionResearch reviewed October 2026Original research explainer

THE SHORT ANSWER

The two numbers come from different chains of measurement and inference. Planck measured patterns in the cosmic microwave background and inferred today's Hubble constant by fitting the standard ΛCDM cosmological model. SH0ES calibrated the distances to Cepheid stars and supernovae, then measured expansion more directly in the nearby universe. Their published results differ beyond their stated uncertainties. That makes a problem to investigate, not proof that either team made an obvious mistake or that physics beyond established models has already been found.

THE EVIDENCE MAP / COSMOLOGY

Two routes to the same cosmic number

One route predicts the present from ancient light; the other calibrates nearby distances. The gap is the evidence to explain.

  1. 01Measurement

    Early light and nearby distances

    Planck mapped microwave-background patterns. SH0ES measured geometric anchors, Cepheids, supernovae, and galaxy redshifts.

  2. 02Interpretation

    67.4 versus 73.04

    ΛCDM turns Planck’s early-universe data into a present-day H₀ of 67.4 ± 0.5. The SH0ES distance ladder gives 73.04 ± 1.04 km/s/Mpc.

  3. 03Competing explanation

    Calibration or cosmic model?

    Unrecognized ladder systematics, assumptions in the early-universe model, or a combination could shift the comparison. A single disputed number does not identify the cause.

  4. 04Open test

    Bring in independent rulers

    Use sharper Cepheid checks and methods with different assumptions, such as lensed supernovae, to see which routes converge before naming a resolution.

TRACE THE CLAIM / THEN TEST ITResearch: Planck parameters SH0ES distance ladder NASA: independent lensed supernova

OBSERVATION / INFERENCE / LIMIT

Read the signal.

PLANCK + ΛCDM

67.4 ± 0.5

Kilometers per second per megaparsec, inferred from the early universe.

SH0ES

73.04 ± 1.04

Same units, from the Cepheid and supernova distance ladder.

CAUSE

Open

Possible systematics and extensions to the model are still tested.

INSIDE THE DATA / PUBLISHED RESULTS

Two estimates.
One unresolved gap.

Inspect the two fitted results discussed in this file. Their error bars summarize published analyses; they are a step beyond the individual observations. This deliberately selected 2018/2022 comparison explains the tension and is not a complete survey of current H₀ measurements.

Two published Hubble constant estimates with 1σ intervalsPlanck’s base ΛCDM estimate is 67.4 ± 0.5 km/s/Mpc. SH0ES is 73.04 ± 1.04 km/s/Mpc. The display uses mi/s/Mpc and 1 times the published one-sigma uncertainty. Points are fitted results from separate published analyses, not individual observations or a complete survey of current methods.PUBLISHED FITTED RESULTS / 1σ INTERVALS41.042.343.544.746.047.2Planck + base ΛCDM (2018) · 41.88 ± 0.31SH0ES distance ladder (2022) · 45.38 ± 0.65H₀ / mi/s/MpcTHE LAST TRANSMISSION · © 2026 DarkScienceDocs.com
Markers: central fitted values. Bars: ±1 times each published standard uncertainty. Miles are an exact unit conversion; the published kilometer values remain in the table. On smaller screens, scroll the chart sideways.

Per megaparsec (Mpc) means per approximately 3.26 million light-years of distance. H₀ relates recession speed to distance on large scales; it is not a spacecraft’s speed.

Published values and American-unit equivalents · uncertainties are 1σ
Analysismi/s/MpcPublished km/s/Mpc
Planck + base ΛCDM (2018) ↗41.88 ± 0.3167.40 ± 0.50
SH0ES distance ladder (2022) ↗45.38 ± 0.6573.04 ± 1.04
01 / READ THE MARKER

Same quantity, different routes.

Planck’s microwave-background observations imply a present-day H₀ when fitted with base ΛCDM. SH0ES uses geometric distance anchors, Cepheids, and Type Ia supernovae. The markers summarize those chains of inference. Moving between miles and kilometers rescales both the central values and their uncertainties equally; it cannot change their disagreement.

02 / READ THE INTERVAL

Error bars keep assumptions attached.

The quoted uncertainty is conditional on the analysis and its model. Choosing 2σ simply doubles each stated uncertainty. Under a Gaussian approximation, ±1σ encloses about 68% and ±2σ about 95% of a distribution. These intervals do not cover every unknown bias, and the toggle does not rerun either team’s fit.

03 / READ THE GAP

A discrepancy is a question.

The central values differ by 5.64 km/s/Mpc, or 3.50 mi/s/Mpc. Treating the quoted errors as independent and Gaussian gives 5.64 ÷ √(0.5² + 1.04²) ≈ 4.9σ. This transparent calculation uses rounded published summaries. It cannot identify an overlooked systematic, assign a probability to physics beyond established models, or replace the teams’ likelihood analyses.

Sources, assumptions, and a downloadable record

Planck Collaboration, Planck 2018 results VI: Cosmological parameters: base-ΛCDM estimate 67.4 ± 0.5 km/s/Mpc (68% uncertainty). Riess et al. (2022), A Comprehensive Measurement of the Local Value of the Hubble Constant: baseline Cepheid–supernova result 73.04 ± 1.04 km/s/Mpc, including systematics. These points are transcribed published fit summaries, rather than raw CMB maps, Cepheid photometry, or independent reanalyses.

Conversion: 1 mile = 1.609344 kilometers exactly. Values and errors are divided by that factor, with rounding only for display. Error-bar lengths are plotted in the same units as their centers. The separation calculation assumes no cross-covariance between the two summaries and uses the quadrature sum of their 1σ errors.

INSIDE THE EVIDENCE

The chain of reasoning.

Each step has a different level of certainty. Follow the measured result into the explanation, then see where the trail ends.

01 / COSMOLOGY

The ancient-light route

The cosmic microwave background preserves a pattern from the early universe. Planck measured that pattern precisely. To turn it into a value for the expansion rate today, researchers adopt a model of what the universe contains and how it evolved. In the standard ΛCDM model, their analysis gives 67.4 kilometers per second per megaparsec, with a stated uncertainty of 0.5. It is a model-dependent inference about the present from old light, not a direct speedometer reading taken in today's local universe.

02 / COSMOLOGY

The nearby-distance route

The SH0ES team built a distance ladder. Geometric anchors calibrate Cepheid variable stars. Cepheids then calibrate the brightness of Type Ia supernovae in galaxies farther away. Comparing those distances with how quickly those galaxies recede yields an expansion rate around 73.04 in the team's comprehensive published analysis, with an uncertainty of 1.04 in the same units. Each rung carries its own tests and possible systematic effects. The disagreement has persisted through substantial work on those rungs.

03 / COSMOLOGY

What a megaparsec has to do with it

A value of 73 kilometers per second per megaparsec means that, in the nearby expansion relation, an additional megaparsec of distance corresponds to roughly 73 more kilometers per second of recession speed. A megaparsec is about 3.26 million light-years. These numbers do not say that a galaxy at one megaparsec physically speeds up by 73 kilometers per second each second. They describe a relationship between distance and observed recession, after careful treatment of local motions and measurement assumptions.

04 / COSMOLOGY

A tension is not yet an answer

Possible resolutions range from an unrecognized calibration or modeling effect to an additional ingredient in cosmology. There are also independent methods, such as other distance indicators and gravitational lensing, that help test the picture; they do not all share the same assumptions. additional measurements can narrow the possibilities without immediately settling them. Webb observations, for example, can scrutinize crowded Cepheid fields, but confirming one part of a ladder would not by itself identify the source of the entire discrepancy.

05 / COSMOLOGY

The question that remains

Can one consistent account explain both the early-universe pattern and the nearby distance scale? If a hidden measurement bias closes the gap, that would be a major result. If multiple independent routes keep it open, a change to the model may be required. This is why the Hubble tension matters: the comparison presses two successful ways of studying the cosmos against one another and forces us to examine the bridge between them.

THE EASY MISREADING

The Planck value is conditional on a cosmological model. The difference between 67 and 73 does not by itself prove a force, a broken universe, or that one telescope is defective.

PRIMARY RESEARCH & MISSION RECORDS

Check the source.

These are the studies and mission records behind this explainer. The illustrated article and Field Note continue the investigation.

  1. Planck 2018 cosmological parameters
  2. Riess et al., SH0ES distance-ladder measurement
  3. NASA: Hubble constant and the tension

FOLLOW THE THREAD

Stay with the question.

Two careful ways of measuring cosmic expansion continue to return answers that do not comfortably meet.

Watch the related documentary
The Universe Is Beginning to Disagree

MORE EVIDENCE FILES

Keep looking.

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FOLLOW THE NEXT MEASUREMENT

The question continues.

Science countdowns

FROM THE ILLUSTRATED ARCHIVE

Follow this thread further.

LIGHT LAB

What did the light
have to cross?

Move foreground galaxies to explore gravitational lensing, build a spectrum, measure parallax, or shift a source’s light to explore radial motion.

Enter Light Lab

SCIENTIFIC INQUIRY / APPLIED HERE

Explore all twelve principles
08 Independent lines of evidence

Two routes carry different assumptions.

The early-universe inference and nearby distance measurements arrive through different chains of evidence. Their disagreement prompts checks of calibration, analysis, and cosmological assumptions. Identify where the routes are independent and where a shared uncertainty might still enter.

Ask yourself Do these sources contain separate measurements, or are they retelling the same result?

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