Evidence record
Why do two good measurements of the universe disagree?
Every sentence on the exploration belongs to at least one claim below. Each says what kind of statement it is, what it rests on, what the evidence does not establish, and how far it was checked. Nothing here is a score, and none of it is a verdict on a belief or a theory.
Last checked 24 September 2026.
- Source checked: 55
- A judgement, not a fact: 14
- Presented as open: 1
If something here is wrong, misquoted, out of date or unfair, write to support@unknownoceans.com and give the claim number, which does not change.
What the question takes for granted
A measurement question with a physics question behind it: two methods for one number disagree, and the page weighs whether a measurement is wrong or the standard model of cosmology is incomplete. The measurement side is itself contested between research teams.
Both routes measure the same quantity
Contested
Both aim at the present expansion rate, but the early-universe value is inferred through the standard model, so a gap can mean a wrong measurement or a wrong model. The page says so.
Both measurements are good
Contested
The title’s "good" is the SH0ES and Planck teams’ own assessment. A rival local ladder (CCHP) gets a lower value, and the SH0ES team attributes that to sample selection.
The universe is expanding, at a rate that can be expressed as one number today
Established
The Hubble constant is the present expansion rate; every source on the page takes it as the quantity measured.
How the question is labelled
Claim: The tension
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: The tension
- Kind
- Framing. Signposting. It asserts nothing a source could check.
The question
Claim: Two ways of measuring how fast space is expanding have been getting more precise for twenty years, and further apart.
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The result was a 5% measurement of H₀, 74.2 ± 3.6 km s⁻¹ Mpc⁻¹ ... was consistent with a value of H₀ = 71.9 ± 2.6 determined from WMAP and ΛCDM alone
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The result was a 5% measurement of H 0, 74.2± 3.6 km s−1 Mpc−1 ... was consistent with a value of H 0 = 71.9± 2.6 determined from WMAP and ΛCDM alone
Supports
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 teamsection 1.2, The Hubble Tension
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The first release of CMB data from the ESA Planck mission (Planck Collaboration et al. 2014) yielded H₀ = 67.2 ± 1.2 in the context of ΛCDM, a then 2 σ reduction relative to WMAP and a difference of 3 σ from the results of R11 and F12.
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The first release of CMB data from the ESA Planck mission (Planck Collaboration et al. 2014) yielded H 0 = 67.2± 1.2 in the context of ΛCDM, a then 2 σ reduction relative to WMAP and a difference of 3 σ from the results of R11 and F12.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: Indications of any tension between the early and late Universe at that time were < 2σ in significance
What this does not establish
"Twenty years" is approximate: the SH0ES programme began in 2005, and the gap passed three standard deviations only with Planck’s first data in 2013. "Further apart" is in standard deviations; in the rival red-giant calibration the local value is lower.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 3 · checked 24 September 2026 · AI-assisted audit
Claim: One method reads the expansion rate off the infant universe, the other measures it directly in nearby galaxies.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
"Reads off" is shorthand: the early-universe value is inferred through the standard model, as the page says later.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most statistically significant tension is the 4σ to 6σ disagreement between predictions of the Hubble constant, H0, made by the early time probes in concert with the “vanilla” ΛCDM Cosmological model, and a number of late time, model-independent determinations of H0 from local measurements of distances and redshifts.
Later work looked for
Crossref, 2022 on, "Hubble tension review solutions": nothing read that reverses the review; the SH0ES and CCHP papers of 2024 and 2025 show the measurement side still contested.
Claim 4 · checked 24 September 2026 · AI-assisted audit
Claim: Both have shrunk their error bars.
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The result was a 5% measurement of H₀, 74.2 ± 3.6 km s⁻¹ Mpc⁻¹ ... was consistent with a value of H₀ = 71.9 ± 2.6 determined from WMAP and ΛCDM alone
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The result was a 5% measurement of H 0, 74.2± 3.6 km s−1 Mpc−1 ... was consistent with a value of H 0 = 71.9± 2.6 determined from WMAP and ΛCDM alone
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
What this does not establish
From ±3.6 (ladder, 2009) to ±1.04, and from WMAP’s ±2.6 to Planck’s ±0.5.
Claim 5 · checked 24 September 2026 · AI-assisted audit
Claim: The gap between them has not closed,
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
What this does not establish
The gap between the Cepheid ladder and Planck. A rival team’s red-giant ladder lands nearer the middle; see claims 52 and 53.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 6 · checked 24 September 2026 · AI-assisted audit
Claim: and that is either a mistake nobody has found or physics nobody has written down.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
The page’s summary of the two readings set out in the section on where the fault could be.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: demands a hypothesis with enough rigor to explain multiple observations
Other readings
The review also names unexpected large-scale structure as a third kind of answer, and the CCHP team reads its own lower ladder value as leaving no gap that needs new physics.
Claim 7 · checked 24 September 2026 · AI-assisted audit
Claim: A disagreement of about eight per cent does not sound like a crisis.
- Kind
- Present-day figure. A count, survey or report finding, as the named source gives it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
73.04 against 67.4 is a gap of 5.6, which is 8.4 per cent of the Planck value and 7.7 per cent of the SH0ES one.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: a difference of ∼ 9%
SH0ES described the 2016 gap (73.2 against 66.9) as about nine per cent.
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Corrected
24 September 2026. Previously: “A disagreement in the fourth significant figure does not sound like a crisis.” 67.4 and 73.04 differ in the first significant figure, not the fourth. The gap is about eight per cent.
Claim 8 · checked 24 September 2026 · AI-assisted audit
Claim: This one is.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Follows from the five-sigma difference SH0ES reports and the review’s description of a serious crisis.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
Claim 9 · checked 24 September 2026 · AI-assisted audit
Claim: Two entirely different routes to the same number keep arriving at different answers, and each route is now precise enough that the difference cannot be shrugged off as luck.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
What this does not establish
Luck here means a statistical fluctuation. Ruling that out does not rule out a systematic error, which is what the rest of the page weighs.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 10 · checked 24 September 2026 · AI-assisted audit
Two numbers, two methods
Claim: Two numbers, two methods
- Kind
- Framing. Signposting. It asserts nothing a source could check.
The early-universe route gives 67
Claim: The early-universe route gives 67
- Kind
- What a model says. What a theory or model predicts or describes, which is not the same as what has been observed.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
What this does not establish
A model-dependent inference under base ΛCDM, as the Planck paper labels it, not a direct measurement of the present.
Later work looked for
arXiv and Crossref, 2020 on, "CMB Hubble constant" and "ACT DR6": the Atacama Cosmology Telescope DR6 with Planck (arXiv:2503.14452, abstract) gives 68.22 ± 0.36, the same early-universe side of the gap; nothing that changes the claim.
Claim 12 · checked 24 September 2026 · AI-assisted audit
Claim: The Planck satellite mapped the light released when the universe was about 380,000 years old.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parameterssection 8, Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: astonishingly accurate description of the Universe from times prior to 380 000 years after the Big Bang, defining the last-scattering surface observed via the CMB
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background
Later work looked for
arXiv and Crossref, 2020 on, "CMB Hubble constant" and "ACT DR6": the Atacama Cosmology Telescope DR6 with Planck (arXiv:2503.14452, abstract) gives 68.22 ± 0.36, the same early-universe side of the gap; nothing that changes the claim.
Claim 13 · checked 24 September 2026 · AI-assisted audit
Claim: The pattern of hot and cold spots in that light encodes the contents and geometry of the early universe, and running the standard cosmological model forward from it predicts today’s expansion rate.
- Kind
- What a model says. What a theory or model predicts or describes, which is not the same as what has been observed.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: A combined analysis gives dark matter densityΩch2 = 0.120± 0.001 ... The joint constraint with BAO measurements on spatial curvature is consistent with a flat universe
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
What this does not establish
The parameters are extracted by fitting the six-parameter model to the maps; the expansion rate today is a consequence of that fit, not something the maps show directly.
Claim 14 · checked 24 September 2026 · AI-assisted audit
Claim: The 2018 result: a Hubble constant of 67.4 plus or minus 0.5 kilometres per second per megaparsec.
- Kind
- What a model says. What a theory or model predicts or describes, which is not the same as what has been observed.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
What this does not establish
Inferred assuming base ΛCDM. Published in Astronomy & Astrophysics in 2020 as part of the 2018 release.
Later work looked for
arXiv and Crossref, 2020 on, "CMB Hubble constant" and "ACT DR6": the Atacama Cosmology Telescope DR6 with Planck (arXiv:2503.14452, abstract) gives 68.22 ± 0.36, the same early-universe side of the gap; nothing that changes the claim.
Claim 15 · checked 24 September 2026 · AI-assisted audit
Claim: The paper adds that it finds "no compelling evidence for extensions to the base-ΛCDM model".
- Kind
- Quotes a source. The words of a named text, checked against the source.
- Review
- Source checked. The cited passage was read, and it says this.
The same abstract reports a significant, 3.6σ, tension with local measurements of the Hubble constant, and says simple extensions that partly resolve it are not favoured by the Planck data.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: We find no compelling evidence for extensions to the base-ΛCDM model.
Claim 16 · checked 24 September 2026 · AI-assisted audit
The nearby route gives 73
Claim: The nearby route gives 73
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Claim 17 · checked 24 September 2026 · AI-assisted audit
Claim: The other method does not assume a model of the early universe at all.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most statistically significant tension is the 4σ to 6σ disagreement between predictions of the Hubble constant, H0, made by the early time probes in concert with the “vanilla” ΛCDM Cosmological model, and a number of late time, model-independent determinations of H0 from local measurements of distances and redshifts.
Later work looked for
Crossref, 2022 on, "Hubble tension review solutions": nothing read that reverses the review; the SH0ES and CCHP papers of 2024 and 2025 show the measurement side still contested.
Claim 18 · checked 24 September 2026 · AI-assisted audit
Claim: It builds a ladder: measure distances to nearby Cepheid variable stars by geometry, use Cepheids to calibrate type Ia supernovae in galaxies that contain both, then use those supernovae to reach far enough that the expansion dominates.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The Cepheids are calibrated geometrically from Gaia EDR3 parallaxes, masers in NGC 4258 (here tripling that sample of Cepheids), and detached eclipsing binaries in the Large Magellanic Cloud
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Corrected
24 September 2026. Previously: “measure distances to nearby Cepheid variable stars by parallax” SH0ES anchors its Cepheids with three geometric methods, not parallax alone: Gaia parallaxes, masers in NGC 4258 and eclipsing binaries in the Large Magellanic Cloud.
Claim 19 · checked 24 September 2026 · AI-assisted audit
Claim: The 2022 measurement, using Hubble Space Telescope observations of Cepheids in the host galaxies of 42 supernovae, gives 73.04 plus or minus 1.04.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H₀).
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: We report observations from the Hubble Space Telescope (HST) of Cepheid variables in the host galaxies of 42 Type Ia supernovae (SNe Ia) used to calibrate the Hubble constant (H 0).
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Claim 20 · checked 24 September 2026 · AI-assisted audit
Claim: The uncertainty is quoted including systematics.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Claim 21 · checked 24 September 2026 · AI-assisted audit
Claim: The distance ladder, rung by rung
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: Geometry
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Corrected
24 September 2026. Previously: “Parallax” The first rung is three geometric anchors, of which parallax is one.
Claim: Nearby Cepheids get their distances from parallaxes measured by the Gaia satellite, from masers in the galaxy NGC 4258, and from eclipsing binary stars in the Large Magellanic Cloud.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The Cepheids are calibrated geometrically from Gaia EDR3 parallaxes, masers in NGC 4258 (here tripling that sample of Cepheids), and detached eclipsing binaries in the Large Magellanic Cloud
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Corrected
24 September 2026. Previously: “A nearby star shifts against the background as Earth moves around the Sun.” The rung was described as parallax alone, which no cited source described; the SH0ES paper names three geometric anchors, and the step now says what it uses.
Claim 24 · checked 24 September 2026 · AI-assisted audit
Claim: Geometry alone gives the distance.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
What this does not establish
Each anchor has its own measurement uncertainties; geometric means no stellar physics is needed to turn the measurement into a distance.
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Claim 25 · checked 24 September 2026 · AI-assisted audit
Claim: Cepheid variables
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: These stars pulse with a period that tracks their true brightness.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: obey a tight period–luminosity relation (P –L, the “Leavitt Law”)
What this does not establish
The relation depends slightly on the star’s metallicity, which is one of the systematics the page discusses.
Later work looked for
Crossref, 2023 on, "Cepheid period-luminosity relation metallicity": work refines the relation’s dependence on metallicity (the page raises it as a candidate systematic); nothing that changes the relation itself.
Claim 27 · checked 24 September 2026 · AI-assisted audit
Claim: Calibrate that relation on those stars and a Cepheid’s brightness becomes a distance anywhere it can be seen.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: obey a tight period–luminosity relation (P –L, the “Leavitt Law”) that yields extremely precise distances
What this does not establish
Cepheids can be measured to about 10 to 40 megaparsecs, the review says, which is why the ladder needs another rung.
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Corrected
24 September 2026. Previously: “Calibrate that relation on the parallax stars and a Cepheid’s brightness becomes a distance anywhere it can be seen.” Follows the first rung, which now names all three geometric anchors.
Claim 28 · checked 24 September 2026 · AI-assisted audit
Claim: Type Ia supernovae
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: In galaxies close enough to contain measured Cepheids, the supernovae get calibrated in turn.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Claim 30 · checked 24 September 2026 · AI-assisted audit
Claim: At more than a billion times the Sun’s luminosity, they can be seen at great distances.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: SNIa exceed a billion solar luminosities
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Corrected
24 September 2026. Previously: “They are bright enough to be seen across a large fraction of the observable universe.” "A large fraction of the observable universe" is not in any cited source; the review gives their luminosity and says they are seen at great distances.
Claim 31 · checked 24 September 2026 · AI-assisted audit
Claim: The expansion
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: Far enough out, a galaxy’s recession dominates its own motion, and distance against redshift gives the rate directly.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2, Late
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most often utilized approach is to use geometry (e.g. parallax) to calibrate the luminosities of specific star types (e.g. pulsating Cepheid variables and exploding Type Ia supernovae or SNIa) which can be seen at great distances where their redshifts measure cosmic expansion.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: SNe Ia are favored to measure the Hubble expansion owing to their high precision (5% in distance per source), ubiquity, and deep reach, which reduces the impact of local flows
Later work looked for
Crossref, 2023 on, "Cepheid metallicity distance scale" and "JWST Cepheids SH0ES": JWST remeasurements (Riess and others 2024) confirm the HST Cepheid photometry; nothing that changes how the ladder is described.
Claim 33 · checked 24 September 2026 · AI-assisted audit
The gap is now larger than the errors
Claim: The gap is now larger than the errors
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 34 · checked 24 September 2026 · AI-assisted audit
Claim: Five or six units apart, with quoted uncertainties of half a unit and one.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Claim 35 · checked 24 September 2026 · AI-assisted audit
Claim: In 2009 the two routes gave 74.2 and 71.9, each uncertain by more than the gap between them,
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The first SH0ES results (Riess et al. 2009, hereafter R09) ... The result was a 5% measurement of H₀, 74.2 ± 3.6 km s⁻¹ Mpc⁻¹ ... was consistent with a value of H₀ = 71.9 ± 2.6 determined from WMAP and ΛCDM alone
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The first SH0ES results (Riess et al. 2009, hereafter R09) ... The result was a 5% measurement of H 0, 74.2± 3.6 km s−1 Mpc−1 ... was consistent with a value of H 0 = 71.9± 2.6 determined from WMAP and ΛCDM alone
The gap between 74.2 and 71.9 is 2.3; the quoted uncertainties are 3.6 and 2.6.
Corrected
24 September 2026. Previously: “Twenty years ago both numbers carried uncertainties larger than the gap,” "Twenty years ago" (2006) is not what the sources describe; the SH0ES history gives the 2009 pair, where each uncertainty exceeded the gap. The early-universe value then came from WMAP, not Planck.
Claim 36 · checked 24 September 2026 · AI-assisted audit
Claim: and it was reasonable to expect the two to converge as the measurements improved.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Follows from the two values then agreeing within their uncertainties.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: Indications of any tension between the early and late Universe at that time were < 2σ in significance
Claim 37 · checked 24 September 2026 · AI-assisted audit
Claim: They improved.
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The result was a 5% measurement of H₀, 74.2 ± 3.6 km s⁻¹ Mpc⁻¹ ... was consistent with a value of H₀ = 71.9 ± 2.6 determined from WMAP and ΛCDM alone
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The result was a 5% measurement of H 0, 74.2± 3.6 km s−1 Mpc−1 ... was consistent with a value of H 0 = 71.9± 2.6 determined from WMAP and ΛCDM alone
Claim 38 · checked 24 September 2026 · AI-assisted audit
Claim: They did not converge.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
What this does not establish
True of the Cepheid ladder against Planck. The CCHP red-giant ladder lands between them; see claim 52.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 39 · checked 24 September 2026 · AI-assisted audit
Claim: The SH0ES team puts the difference at five standard deviations,
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
What this does not establish
Five sigma measures how unlikely the gap is as a fluctuation if both uncertainties are right. It says nothing about whether a systematic error is hiding in either.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Corrected
24 September 2026. Previously: “The difference is currently around five standard deviations,” The five-sigma figure is the SH0ES team’s, comparing its value with Planck. A rival ladder (CCHP 2025) gives a smaller gap, so the figure is attributed rather than stated as the current state of the field.
Claim 40 · checked 24 September 2026 · AI-assisted audit
Claim: which is the threshold particle physicists use to call something a discovery rather than a fluctuation.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Statistics (Review of Particle Physics, chapter 40)section 40.3.2
Cited · Link answered, 19 October 2026 · The cited passage was read, 24 September 2026 · Reference work
The source reads: Often in particle physics the level of significance where an effect is said to qualify as a discovery is Z = 5, i.e., a 5σeffect
What this does not establish
A convention, and the review itself says a physicist’s belief in a new effect depends on more than the p-value.
Later work looked for
Checked the 2025 revision of the review, the current one; the convention is unchanged.
Claim 41 · checked 24 September 2026 · AI-assisted audit
Where the fault could be
Claim: Where the fault could be
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: They improved.
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our baseline result from the Cepheid–SN Ia sample is H₀ = 73.04 ± 1.04 km s⁻¹ Mpc⁻¹, which includes systematic uncertainties
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Our baseline result from the Cepheid–SN Ia sample is H 0 = 73.04± 1.04 km s−1 Mpc−1, which includes systematic uncertainties
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The result was a 5% measurement of H₀, 74.2 ± 3.6 km s⁻¹ Mpc⁻¹ ... was consistent with a value of H₀ = 71.9 ± 2.6 determined from WMAP and ΛCDM alone
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The result was a 5% measurement of H 0, 74.2± 3.6 km s−1 Mpc−1 ... was consistent with a value of H 0 = 71.9± 2.6 determined from WMAP and ΛCDM alone
Claim 43 · checked 24 September 2026 · AI-assisted audit
Claim: They did not converge.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
What this does not establish
True of the Cepheid ladder against Planck. The CCHP red-giant ladder lands between them.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Claim 44 · checked 24 September 2026 · AI-assisted audit
Whether something is wrong with one of the measurements
Claim: Whether something is wrong with one of the measurements
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: The obvious candidate is an unknown systematic in the distance ladder:
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
The page’s judgement; the review discusses measurement errors on both sides and says no single proposed error survives the data.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2.3, Systematics
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: it is challenging to devise a single error that would suffice and we are not aware of a specific proposal that is not ruled out by the data
Claim 46 · checked 24 September 2026 · AI-assisted audit
Claim: crowding in the fields where Cepheids are measured, the metallicity dependence of the period-luminosity relation, or supernova corrections that differ between star-forming and quieter host galaxies.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: six tests of background determinations that show Cepheid measurements are accurate in the presence of crowded backgrounds
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: We present results for a comprehensive set of nearly 70 analysis variants to explore the sensitivity of H₀ to selections of anchors, SN surveys, redshift ranges, the treatment of Cepheid dust, metallicity, form of the period–luminosity relation
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: We present results for a comprehensive set of nearly 70 analysis variants to explore the sensitivity of H 0 to selections of anchors, SN surveys, redshift ranges, the treatment of Cepheid dust, metallicity, form of the period–luminosity relation
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: Rigault et al. (2015) suggested that the calibrator sample, all with spiral hosts and thus greater mean SFR, could introduce a bias in H₀
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: Rigault et al. (2015) suggested that the calibrator sample, all with spiral hosts and thus greater mean SFR, could introduce a bias in H 0
Corrected
24 September 2026. Previously: “or supernova standardisation drifting with the age of the host galaxy.” The cited paper addresses host star formation and mass (after Rigault and others), not host age. Host-age effects have been proposed elsewhere, but no cited source was read for them.
Claim 47 · checked 24 September 2026 · AI-assisted audit
Claim: Each of these has been tested hard: the 2022 SH0ES paper alone runs nearly seventy variants of its analysis.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: We present results for a comprehensive set of nearly 70 analysis variants
Corrected
24 September 2026. Previously: “Each of these has been hunted hard and independently.” "Independently" was not carried by the cited sources for these particular systematics; the SH0ES paper’s own tests are what was read.
Claim 48 · checked 24 September 2026 · AI-assisted audit
Claim: Alternative rungs, including tip-of-the-red-giant-branch distances and gravitational lensing time delays, have been used to route around the suspect steps,
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: We demonstrate consistency with measures from HST of the TRGB between SN Ia hosts and NGC 4258
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: This method is completely independent of both the supernovae and CMB analyses
Context
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The overall program aims to calibrate three independent methods: (1) Tip of the Red Giant Branch (TRGB) stars, (2) JAGB (J-Region Asymptotic Giant Branch) stars, and (3) Cepheids.
What this does not establish
The CCHP paper was read as an abstract only.
Claim 49 · checked 24 September 2026 · AI-assisted audit
Claim: and this is where the two camps part.
- Kind
- Disputed. A contested point, where the page reports a side or the disagreement.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best (highest precision) estimate is H₀ = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σ_SN), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Notation restored: Subscripts and symbols restored from the arXiv PDF (v3), whose abstract renders them as H0 = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σSN), read 2026-09-24. The text as extracted reads: Our current best (highest precision) estimate is $H_0$ = 70.39 $\pm$ 1.22 (stat) $\pm$ 1.33 (sys) $\pm$ 0.70 ($\sigma_{SN}$), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Supports
Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopessection 16, Summary and Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best estimate of H0 is 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 ... This value falls between that obtained from studies of the CMB, from BAO measurements calibrated by BBN, and the SHoES value, all without significant tension.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: we cite the mean of the two (72.53 ± 0.95 km s⁻¹ Mpc⁻¹) as representative of the combination of Cepheids and TRGB
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: we cite the mean of the two (72.53± 0.95 km s−1 Mpc−1) as representative of the combination of Cepheids and TRGB
Other readings
SH0ES holds that every alternative rung agrees with its Cepheids; CCHP holds that its red-giant and carbon-star distances give a lower value with no need for new physics.
Corrected
24 September 2026. Previously: “and the disagreement has proved stubborn rather than fragile.” One-sided. The SH0ES team finds the alternative rungs agree with its Cepheids; the CCHP team, using red giants, finds a value near 70 consistent with the standard model. Both sides are now reported.
Claim 50 · checked 24 September 2026 · AI-assisted audit
Claim: The SH0ES team finds red giants agree with its Cepheids, giving 72.53 in combination.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We demonstrate consistency with measures from HST of the TRGB between SN Ia hosts and NGC 4258, and include them simultaneously to yield 72.53 ± 0.99 km s⁻¹ Mpc⁻¹.
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: We demonstrate consistency with measures from HST of the TRGB between SN Ia hosts and NGC 4258, and include them simultaneously to yield 72.53± 0.99 km s−1 Mpc−1.
What this does not establish
Section 7.2 gives 72.53 ± 0.95 in the text and the abstract 72.53 ± 0.99; the page quotes the central value only.
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Corrected
24 September 2026. Previously: “” Added so that the red-giant check is reported with who ran it and what it gave.
Claim 51 · checked 24 September 2026 · AI-assisted audit
Claim: The Chicago-Carnegie team, measuring red giants with the Hubble and James Webb telescopes, gets 70.39 and calls it consistent with the standard model;
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best (highest precision) estimate is H₀ = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σ_SN), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Notation restored: Subscripts and symbols restored from the arXiv PDF (v3), whose abstract renders them as H0 = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σSN), read 2026-09-24. The text as extracted reads: Our current best (highest precision) estimate is $H_0$ = 70.39 $\pm$ 1.22 (stat) $\pm$ 1.33 (sys) $\pm$ 0.70 ($\sigma_{SN}$), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our results are consistent with the current standard LambdaCDM model, without the need for the inclusion of additional new physics.
Supports
Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopessection 16, Summary and Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best estimate of H0 is 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 ... This value falls between that obtained from studies of the CMB, from BAO measurements calibrated by BBN, and the SHoES value, all without significant tension.
What this does not establish
70.39 carries ±1.22 statistical, ±1.33 systematic and ±0.70 from the supernovae; JWST data alone give 68.81 (red giants) and 67.80 (carbon stars).
Later work looked for
Crossref, 2023 on, "Hubble constant JWST Cepheids SH0ES" and "Chicago-Carnegie Hubble Program": Riess and others 2024 report 73.2 ± 0.9 from the full HST set and JWST cross-checks that agree with it; Freedman and others 2025 get 70.39 from red giants. The Cepheid figure stands; the page now reports the rival value where it discusses the check.
Corrected
24 September 2026. Previously: “” Added: a published, independent red-giant ladder disagrees with the SH0ES reading of the same kind of check, and the page reported only one side.
Claim 52 · checked 24 September 2026 · AI-assisted audit
Claim: SH0ES puts the difference down to which supernovae each sample happens to include.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We show that Delta(H0)~2.5 km/s/Mpc between the CCHP JWST program and the full HST sample is entirely consistent with differences in sample selection.
Supports
JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0Figure 5 caption
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: The CCHP and SH0ES subsamples selected for JWST observations produce a large difference of 3–4 km s⁻¹ Mpc⁻¹ in H0 a priori owing to selection. The HST Cepheid and JWST distance measurements themselves are in good agreement.
Notation restored: Subscript and superscripts restored as the arXiv version (2408.11770) typesets them, read from glyph positions 2026-09-24. The text as extracted reads: The CCHP and SH0ES subsamples selected for JWST observations produce a large difference of 3–4 km s−1 Mpc−1 in H0 a priori owing to selection. The HST Cepheid and JWST distance measurements themselves are in good agreement.
What this does not establish
The SH0ES team’s own analysis of the other team’s sample. It also reports JWST red-giant, carbon-star and Cepheid values of 72.1 to 73.4 on a larger combined sample.
Other readings
CCHP does not accept that sample selection explains its lower value.
Corrected
24 September 2026. Previously: “” Added with the CCHP result, so the SH0ES response is reported too.
Claim 53 · checked 24 September 2026 · AI-assisted audit
Claim: Six lensed quasars, analysed without any distance ladder at all, gave 73.3 in 2019.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: a joint analysis of six gravitationally lensed quasars with measured time delays ... we find H₀ = 73.3 (+1.7/−1.8) km s⁻¹ Mpc⁻¹, a 2.4% precision measurement
Notation restored: Notation restored as the arXiv PDF (1907.04869) typesets it, read from glyph positions 2026-09-24: the 0 after H lowered, the −1 after s and Mpc raised, and the uncertainty set as +1.7 raised over −1.8 lowered, written here as (+1.7/−1.8). The text as extracted reads: a joint analysis of six gravitationally lensed quasars with measured time delays ... we find H0 = 73.3+1.7 −1.8 km s−1 Mpc−1, a 2.4% precision measurement
What this does not establish
Assumes flat ΛCDM for the conversion to H0, and specific forms for the lensing galaxies’ mass (see the next claim).
Later work looked for
Crossref and arXiv, 2020 on, "TDCOSMO Hubble constant": TDCOSMO IV (2020) and TDCOSMO 2025 revisit the same lenses with looser mass models; the page now reports both.
Corrected
24 September 2026. Previously: “Six lensed quasars, analysed without any distance ladder at all, gave 73.3.” Dated, because later analyses of the same lenses give different values.
Claim 54 · checked 24 September 2026 · AI-assisted audit
Claim: That precision leaned on assumptions about the lensing galaxies’ mass, and a 2025 analysis of eight lenses that loosened them gave 71.6, uncertain by three or four units either way.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: describing deflector mass density profiles by either a power-law or stars plus standard dark matter halos. The mass-sheet transform (MST) that leaves the lensing observables unchanged is considered the dominant source of residual uncertainty in H₀.
Notation restored: Subscript restored from the arXiv PDF (v3), whose abstract renders it as 𝐻0, read 2026-09-24. The text as extracted reads: describing deflector mass density profiles by either a power-law or stars plus standard dark matter halos. The mass-sheet transform (MST) that leaves the lensing observables unchanged is considered the dominant source of residual uncertainty in $H_0$.
Supports
TDCOSMO 2025: Cosmological constraints from strong lensing time delaysabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We present cosmological constraints from 8 strongly lensed quasars ... Our uncertainties are maximally conservative by accounting for the mass-sheet degeneracy in the deflectors' mass density profiles.
Supports
TDCOSMO 2025: Cosmological constraints from strong lensing time delaysabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: In the flat Λ cold dark matter (CDM), we find H₀ = 71.6 +3.9/−3.3 km s⁻¹ Mpc⁻¹.
Notation restored: Greek letter, subscript and superscripts restored from the arXiv PDF (v4), whose abstract renders it as H0 = 71.6 +3.9 −3.3 km s−1 Mpc−1, read 2026-09-24; the upper and lower errors are written after a slash. The text as extracted reads: In the flat $\Lambda$ cold dark matter (CDM), we find $H_0=71.6^{+3.9}_{-3.3}$ km s$^{-1}$ Mpc$^{-1}$.
What this does not establish
TDCOSMO IV (2020) found 74.5 +5.6/−6.1 from seven lenses with the mass models freed, and says this does not invalidate the 2019 assumptions; the 2025 value is +3.9/−3.3, and 4.6 per cent precision when non-time-delay lenses are added.
Corrected
24 September 2026. Previously: “” Added: the 2019 lensing value was presented as settled, and later work by the same collaboration shows its precision depended on mass-model assumptions.
Claim 55 · checked 24 September 2026 · AI-assisted audit
Whether the model between the two is wrong
Claim: Whether the model between the two is wrong
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: The early-universe number is not a direct measurement of today’s expansion.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most statistically significant tension is the 4σ to 6σ disagreement between predictions of the Hubble constant, H0, made by the early time probes in concert with the “vanilla” ΛCDM Cosmological model, and a number of late time, model-independent determinations of H0 from local measurements of distances and redshifts.
Supports
Planck 2018 results. VI. Cosmological parametersabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H₀ = (67.4±0.5) km s⁻¹ Mpc⁻¹
Notation restored: Subscripts and superscripts restored as the arXiv PDF (1807.06209v4) typesets them, read from glyph positions 2026-09-24; the abstract on arXiv gives H_0 and Ω_m the same way. The text as extracted reads: Assuming the base- ΛCDM cosmology, the inferred (model-dependent) late-Universe parameters are: Hubble constant H0 = (67.4±0.5) km s−1Mpc−1
Later work looked for
Crossref, 2022 on, "Hubble tension review solutions": nothing read that reverses the review; the SH0ES and CCHP papers of 2024 and 2025 show the measurement side still contested.
Claim 57 · checked 24 September 2026 · AI-assisted audit
Claim: It is a prediction, produced by evolving the standard model of cosmology forward for 13.8 billion years.
- Kind
- What a model says. What a theory or model predicts or describes, which is not the same as what has been observed.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The value of H₀ may be determined locally with measurements of distances and redshifts, and it can also be predicted from a cosmological model calibrated in the early Universe
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The value of H 0 may be determined locally with measurements of distances and redshifts, and it can also be predicted from a cosmological model calibrated in the early Universe
Supports
Planck 2018 results. VI. Cosmological parameterssection 8
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: to the present day at an age of 13.8 billion years
What this does not establish
13.8 billion years is itself a Planck ΛCDM value, from the same fit.
Corrected
24 September 2026. Previously: “It is a prediction, produced by evolving the standard model of cosmology forward for thirteen billion years.” Planck gives the present age as 13.8 billion years; "thirteen billion" understated it.
Claim 58 · checked 24 September 2026 · AI-assisted audit
Claim: If that model is missing something, the prediction can be precise and wrong.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Follows from the early value being a model-dependent inference.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most statistically significant tension is the 4σ to 6σ disagreement between predictions of the Hubble constant, H0, made by the early time probes in concert with the “vanilla” ΛCDM Cosmological model, and a number of late time, model-independent determinations of H0 from local measurements of distances and redshifts.
Claim 59 · checked 24 September 2026 · AI-assisted audit
Claim: The review that classifies the proposals sorts them into early dark energy, late dark energy, extra relativistic degrees of freedom, extra interactions, modified gravity and six other families, and cites more than a thousand papers doing it.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: We include more than 1000 references
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: these categories: Early Dark Energy, Late Dark Energy, Dark energy models with 6 degrees of freedom and their extensions, Models with extra relativistic degrees of freedom, Models with Extra Interactions, Unified cosmologies, Modified gravity, Inflationary models, Modified recombination history, Physics of the critical Phenomena, and Alternative proposals.
Later work looked for
Crossref, 2022 on, "Hubble tension review solutions": nothing read that reverses the review; the SH0ES and CCHP papers of 2024 and 2025 show the measurement side still contested.
Corrected
24 September 2026. Previously: “modified gravity and a dozen other families” The review has eleven categories; five are named on the page, so six others, not a dozen.
Claim 60 · checked 24 September 2026 · AI-assisted audit
Claim: None has made a strong case.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: While no specific proposal makes a strong case for being highly likely or far better than all others
What this does not establish
A 2021 review. Later proposals are not covered by it.
Corrected
24 September 2026. Previously: “None of them is comfortable: some improve the fit only by paying for the degrees of freedom they add, and most fixes for the expansion rate break something else that the same data constrains.” The review says some proposals are "formally successful, improving the fit ... in light of their additional degrees of freedom", which the page read as the opposite. "Most fixes break something else" was stronger than the review, which says successful models are "often" at odds with other probes.
Claim 61 · checked 24 September 2026 · AI-assisted audit
Claim: Models that ease the tension on Planck’s data alone often disagree with other probes, and many ease it by widening the error bar rather than by moving the number.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 15, Summary and Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: these a priori successful cosmological models are often not in agreement with additional cosmological probes ... Moreover, the Hubble constant tension is alleviated due to an increase in the error bars of H0, rather than by an increase in the Hubble constant itself
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: In many cases, reduced tension comes not simply from a change in the value of H0 but also due to an increase in its uncertainty due to degeneracy with additional physics
Claim 62 · checked 24 September 2026 · AI-assisted audit
Claim: Two ways the tension resolves
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: A measurement problem
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: Some step in the distance ladder, or in the Planck analysis, carries an error nobody has found.
- Kind
- Hypothesis. A proposed explanation, not an established one.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: demands a hypothesis with enough rigor to explain multiple observations
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2.3, Systematics
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: it is challenging to devise a single error that would suffice and we are not aware of a specific proposal that is not ruled out by the data
What this does not establish
The review knows of no single proposed error that survives the data; an answer of this kind may need several unrelated errors.
Other readings
CCHP’s reading is that the local value is lower than SH0ES finds, which narrows the gap without new physics.
Claim 65 · checked 24 September 2026 · AI-assisted audit
Claim: Would be unglamorous,
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
A judgement about how the answer would be received, not about which answer is right.
Claim 66 · checked 24 September 2026 · AI-assisted audit
Claim: and is how the 1980s dispute over this number, 50 against 100, ended: in the middle.
- Kind
- Historical claim. A statement about the past that historical evidence can test.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2.3
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: might argue for a true value of H₀ “in the middle”, e.g. ∼ 70 km s⁻¹ Mpc⁻¹, as the easiest to accommodate, as was the resolution of the 1980’s debate between 50 and 100
Notation restored: Subscript and superscripts restored as the arXiv PDF (2103.01183) typesets them, read from glyph positions 2026-09-24. The text as extracted reads: might argue for a true value of H0 “in the middle”, e.g.∼ 70 km s−1 Mpc−1, as the easiest to accommodate, as was the resolution of the 1980’s debate between 50 and 100
What this does not establish
The review adds that the analogy breaks down: the old dispute was between measurements of the same kind at the same distances, and pointed straight at systematics.
Corrected
24 September 2026. Previously: “Would be unglamorous and is historically the way most such disagreements have ended.” "Most such disagreements" had no source. The review supports one precedent, the 1980s dispute, and the page now names it.
Claim 67 · checked 24 September 2026 · AI-assisted audit
Claim: Has survived a decade of deliberate searching by the team that made the measurement, though a rival team’s red-giant distances land nearer the middle.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We find a 5σ difference with the prediction of H0 from Planck CMB observations under ΛCDM, with no indication that the discrepancy arises from measurement uncertainties or analysis variations considered to date.
Supports
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 teamabstract, last sentence
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H₀ remains unknown
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H 0 remains unknown
Supports
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 teamsection 1.1, The SH0ES Program
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The first SH0ES results (Riess et al. 2009, hereafter R09)
Supports
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best (highest precision) estimate is H₀ = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σ_SN), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Notation restored: Subscripts and symbols restored from the arXiv PDF (v3), whose abstract renders them as H0 = 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 (σSN), read 2026-09-24. The text as extracted reads: Our current best (highest precision) estimate is $H_0$ = 70.39 $\pm$ 1.22 (stat) $\pm$ 1.33 (sys) $\pm$ 0.70 ($\sigma_{SN}$), based on the TRGB method alone, with a total of 24 SN Ia calibrators from both HST and JWST data.
Supports
Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopessection 16, Summary and Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: Our current best estimate of H0 is 70.39 ± 1.22 (stat) ± 1.33 (sys) ± 0.70 ... This value falls between that obtained from studies of the CMB, from BAO measurements calibrated by BBN, and the SHoES value, all without significant tension.
What this does not establish
"A decade" counts from Planck’s first release in 2013, when the gap reached three standard deviations.
Later work looked for
Crossref, 2022 on, "Hubble tension" and "Chicago-Carnegie Hubble Program JWST": SH0ES (Riess and others 2024) still finds the gap; the CCHP team (Freedman and others 2025, and its erratum, which does not touch H0) finds 70.39 and no need for new physics. The page now attributes the five-sigma figure to SH0ES and reports the disagreement.
Corrected
24 September 2026. Previously: “Has survived a decade of deliberate attempts to find it, using independent methods.” Independent methods do not all agree: the CCHP red-giant ladder gives about 70. Attributed, with the other side stated.
Claim 68 · checked 24 September 2026 · AI-assisted audit
Claim: A physics problem
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: The standard model of cosmology is incomplete, and the early-universe prediction inherits the gap.
- Kind
- Hypothesis. A proposed explanation, not an established one.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The most statistically significant tension is the 4σ to 6σ disagreement between predictions of the Hubble constant, H0, made by the early time probes in concert with the “vanilla” ΛCDM Cosmological model, and a number of late time, model-independent determinations of H0 from local measurements of distances and redshifts.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: While no specific proposal makes a strong case for being highly likely or far better than all others
What this does not establish
Proposed, not shown: no specific model makes a strong case, the review says.
Other readings
The measurement reading in the other column.
Claim 70 · checked 24 September 2026 · AI-assisted audit
Claim: Would mean that a model which fits almost every other probe is incomplete.
- Kind
- What the field holds. The settled view of a field, as a review, a consensus statement or a reference work gives it. Not one study.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 15
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: The ΛCDM cosmological model, a simple and elegant framework, has been found to provide a very good fit to almost all of the observational probes available until present
Later work looked for
Crossref, 2021 on, "ΛCDM tensions": the Planck paper itself notes smaller tensions (lensing amplitude, galaxy clustering), and DESI baryon-acoustic results since 2024 have been read by their authors as hints of evolving dark energy; neither was read in full here, and "almost every" allows for them.
Corrected
24 September 2026. Previously: “Would be the first crack in a model that has otherwise fitted everything for twenty-five years.” Overstated: the model does not fit everything (Planck itself reports smaller tensions), and "first crack" was a claim no source made.
Claim 71 · checked 24 September 2026 · AI-assisted audit
Claim: No proposed fix has yet made a strong case over the others.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: While no specific proposal makes a strong case for being highly likely or far better than all others
What this does not establish
As of the 2021 review.
Corrected
24 September 2026. Previously: “Every proposed fix so far costs more in fit elsewhere than it buys here.” Contradicted by the cited review, which says some proposals are formally successful and improve the fit; what it does say is that none makes a strong case.
Claim 72 · checked 24 September 2026 · AI-assisted audit
What is actually unresolved
Claim: What is actually unresolved
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Which it is
Claim: Which it is
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: Nobody knows.
- Kind
- Open question. Something the page says is not known.
- Review
- Presented as open. The page says this is unresolved, and the review found that it is.
Supports
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 teamabstract, last sentence
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H₀ remains unknown
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H 0 remains unknown
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: While no specific proposal makes a strong case for being highly likely or far better than all others
Claim 75 · checked 24 September 2026 · AI-assisted audit
Claim: That sentence is the reason this question is on this site rather than in a textbook: it is not a gap in public understanding, it is a gap in the field’s.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
SH0ES calls the source of the discrepancy unknown; the review says no proposal makes a strong case.
Supports
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 teamabstract, last sentence
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026
The source reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H₀ remains unknown
Notation restored: Subscript and superscripts restored as the arXiv version of the paper (2112.04510) typesets them: the 0 after H is lowered and set small, the −1 after s and after Mpc raised, read from glyph positions 2026-09-24. The text as extracted reads: The source of this now long-standing discrepancy between direct and cosmological routes to determining H 0 remains unknown
Claim 76 · checked 24 September 2026 · AI-assisted audit
Claim: What would settle it is more independent routes to the same number.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
The review calls for additional probes and for broadening the measurements.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: pointing to the need for additional probes
Claim 77 · checked 24 September 2026 · AI-assisted audit
Claim: Gravitational-wave sirens, which measure distance directly from the physics of a merger without any ladder at all, are one such route:
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
A gravitational-wave standard siren measurement of the Hubble constantabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: This approach does not require any form of cosmic “distance ladder” (Freedman et al. 2001)
Supports
A gravitational-wave standard siren measurement of the Hubble constantabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: the distance to the source inferred purely from the gravitational-wave signal
Corrected
24 September 2026. Previously: “Gravitational-wave sirens, which measure distance directly from the physics of a merger without any ladder at all, are the most promising:” "The most promising" was a ranking no cited source made. A 2018 forecast of two per cent from sirens within five years has not been met.
Claim 78 · checked 24 September 2026 · AI-assisted audit
Claim: the first, in 2017, gave a value consistent with both camps and an uncertainty far too wide to choose between them.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
A gravitational-wave standard siren measurement of the Hubble constantabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: We determine the Hubble constant to be 70.0 (+12.0/−8.0) km s⁻¹ Mpc⁻¹ ... This is consistent with existing measurements (Planck Collaboration et al. 2016; Riess et al. 2016), while being completely independent of them
Notation restored: Notation restored as the paper’s LaTeX abstract on arXiv (1710.05835) sets it, 70.0^{+12.0}_{-8.0} km s^{-1} Mpc^{-1}, read 2026-09-24; the uncertainty is written here as (+12.0/−8.0). The text as extracted reads: We determine the Hubble constant to be 70.0+12.0 −8.0 km s−1 Mpc−1 ... This is consistent with existing measurements (Planck Collaboration et al. 2016; Riess et al. 2016), while being completely independent of them
Later work looked for
arXiv and Crossref, 2018 on, "standard siren Hubble constant GWTC-3": the 2023 GWTC-3 analysis of 47 events gives 68 +12/−7 with GW170817, still far too wide to decide; page now cites it.
Claim 79 · checked 24 September 2026 · AI-assisted audit
Claim: There are not yet enough of them.
- Kind
- Observation. Something measured or seen, as the named source reports it.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
Constraints on the Cosmic Expansion History from GWTC-3section 6, Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Astronomical observation · Measurement
The source reads: using these 47 GW events, our results are still dominated by the systematic effects induced by the assumptions made about the GW source population. ... In the future, with significantly more both bright and dark sirens it will be possible to make robust measurements of H0
What this does not establish
Its combined value with GW170817 is 68, with an uncertainty of +12 and −7 or −8 (the arXiv abstract and PDF differ), far too wide to decide between 67 and 73.
Later work looked for
arXiv and Crossref, 2018 on, "standard siren Hubble constant GWTC-3": the 2023 GWTC-3 analysis of 47 events gives 68 +12/−7 with GW170817, still far too wide to decide; page now cites it.
Claim 80 · checked 24 September 2026 · AI-assisted audit
How it ends
Claim: How it ends
- Kind
- Framing. Signposting. It asserts nothing a source could check.
What a resolution would look like
Claim: What a resolution would look like
- Kind
- Framing. Signposting. It asserts nothing a source could check.
Claim: If it is a systematic, the fix will be dull and specific: a recalibration, a better treatment of one population of stars, and the two numbers will slide together over a few years.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
A possibility, in the section of the page that says so.
What this does not establish
A projection, not a finding. The review doubts a single error could do it; see the next sentence.
Claim 83 · checked 24 September 2026 · AI-assisted audit
Claim: It may take more than one:
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2.3, Systematics
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: it is challenging to devise a single error that would suffice and we are not aware of a specific proposal that is not ruled out by the data
Corrected
24 September 2026. Previously: “” Added: the sentence before implied one fix would do, and the cited review says no single proposed error survives the data.
Claim 84 · checked 24 September 2026 · AI-assisted audit
Claim: the 2021 review of the tension knew of no single proposed error that the data had not already ruled out.
- Kind
- What scholars argue. A report of what specialists argue, or where they disagree.
- Review
- Source checked. The cited passage was read, and it says this.
Supports
In the realm of the Hubble tension: a review of solutionssection 2.2.3, Systematics
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: it is challenging to devise a single error that would suffice and we are not aware of a specific proposal that is not ruled out by the data
What this does not establish
As of 2021.
Claim 85 · checked 24 September 2026 · AI-assisted audit
Claim: If it is physics, it will show up in other places at once, because a change to the model moves more than one number.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Follows from the review’s point that a solution must explain multiple observations, and that models which fix the Hubble constant often disagree with other probes.
Supports
In the realm of the Hubble tension: a review of solutionsabstract
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: demands a hypothesis with enough rigor to explain multiple observations
Supports
In the realm of the Hubble tension: a review of solutionssection 15, Summary and Conclusions
Cited · Link answered, 19 October 2026 · Read in full, 24 September 2026 · Review of the field
The source reads: these a priori successful cosmological models are often not in agreement with additional cosmological probes ... Moreover, the Hubble constant tension is alleviated due to an increase in the error bars of H0, rather than by an increase in the Hubble constant itself
Corrected
24 September 2026. Previously: “If it is physics, the change is to the early universe rather than to the nearby one, and it will show up in other places at once.” The cited review classifies late-time proposals (late dark energy, modified gravity) alongside early-time ones and names both among its best options; saying the change must be early was a side the review does not take.
Claim 86 · checked 24 September 2026 · AI-assisted audit
Claim: That is the useful property of this kind of tension.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
Claim 87 · checked 24 September 2026 · AI-assisted audit
Claim: A real crack is never local.
- Kind
- This page’s reading. A judgement the page makes from the evidence. Others read it differently.
- Review
- A judgement, not a fact. Reviewed for whether it is fairly put and follows from the checked claims. No source can confirm it.
A figure of speech for the sentence before, not a law.
Claim 88 · checked 24 September 2026 · AI-assisted audit
What was read
- Planck 2018 results. VI. Cosmological parametersPlanck Collaboration, Astronomy & Astrophysics · arXiv:1807.06209v4 (9 August 2021), the version of record’s text; read abstract, section 8 and searched the restRead in full, 24 September 2026 · Copyright; quoted briefly
- 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 teamRiess and others, The Astrophysical Journal Letters · arXiv:2112.04510v3 (18 July 2022); read abstract, sections 1, 7.2 to 7.4Read in full, 24 September 2026 · Copyright; quoted briefly
- H0LiCOW XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 sigma tension between early and late Universe probesWong, Suyu, Chen and others, Monthly Notices of the Royal Astronomical Society 498 · arXiv:1907.04869v2 (6 November 2019); read abstract and introductionRead in full, 24 September 2026 · Copyright; quoted briefly
- A gravitational-wave standard siren measurement of the Hubble constantLIGO, Virgo and partner collaborations, Nature · arXiv:1710.05835v1 (16 October 2017); read abstract and openingRead in full, 24 September 2026 · Copyright; quoted briefly
- In the realm of the Hubble tension: a review of solutionsDi Valentino and others, Classical and Quantum Gravity 38 · arXiv:2103.01183v3 (5 June 2021); read abstract, sections 2.2, 2.3 and 15Read in full, 24 September 2026 · Copyright; quoted briefly
- Statistics (Review of Particle Physics, chapter 40)G. Cowan and L. Lista, Particle Data Group · Particle Data Group, Review of Particle Physics, chapter 40, revised June 2025, PDF dated 1 December 2025; read section 40.3.2The cited passage was read, 24 September 2026 · Copyright; quoted brieflyPDF text extraction joins "5σ" and "effect"; the excerpt keeps that spacing so it can be matched.
- Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space TelescopesFreedman, Madore, Hoyt and others, The Astrophysical Journal 985 · arXiv:2408.06153v3 (17 March 2025), the PDF read as extracted text, with the abstract as served on arXiv; the ApJ erratum (10.3847/1538-4357/ae146d) was read in full and does not touch H0Read in full, 24 September 2026 · CC BY 4.0Abstract excerpts keep the arXiv abstract’s LaTeX markup as served, with the notation restored for display from the PDF.
- JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0Riess and others, The Astrophysical Journal 977 · arXiv:2408.11770v2 (28 October 2024), the PDF read as extracted text, with the abstract as served on arXivRead in full, 24 September 2026 · arXiv non-exclusive distribution licence; quoted briefly
- TDCOSMO IV: Hierarchical time-delay cosmography, joint inference of the Hubble constant and galaxy density profilesBirrer and others, Astronomy & Astrophysics 643 · arXiv:2007.02941v3 (19 December 2020), the PDF read as extracted text, with the abstract as served on arXivRead in full, 24 September 2026 · arXiv non-exclusive distribution licence; quoted brieflyThe arXiv title joins its two parts with a double hyphen; the page’s title uses a comma.
- TDCOSMO 2025: Cosmological constraints from strong lensing time delaysTDCOSMO Collaboration, Astronomy & Astrophysics 704 · arXiv:2506.03023v4 (21 December 2025), the PDF read as extracted text, with the abstract as served on arXivRead in full, 24 September 2026 · CC BY 4.0
- Constraints on the Cosmic Expansion History from GWTC-3LIGO, Virgo and KAGRA collaborations, The Astrophysical Journal 949 · arXiv:2111.03604v2 (19 November 2021), the PDF read as extracted text, with the abstract as served on arXivRead in full, 24 September 2026 · CC BY 4.0The abstract as served gives the 47-event value as 68 +12/−7; the v2 PDF gives 68 +12/−8.