Hubble constant — published H0 estimates and their errors, 1929–2019
The Hubble constant H0 is the expansion rate of the universe. Published estimates have come down from above 500 in 1929 to about 70, and their error bars shortened a few hundredfold on the way. This chapter counts how often the errors quoted in two compilations covered the distance to a later reference value: the question of the physical-constants chapter, asked of individual measurements instead of editions.
- In Huchra's list (1929–2010, 548 rows) the yearly median relative error halved every 58.7 years; in Table A2 (1976–2019, 163 rows) every 13.9 years.
- Against Planck 2018, 25.9% of Huchra's list lies beyond twice the quoted error (normal: 4.6%); against Riess et al. 2022, 31.9%. Table A2: 25.9% and 23.9%. Under either reference the quoted errors miss more often than a normal distribution predicts.
- A Student-t fitted to the z has ν ≈ 2.30–1.97 (Huchra's list): a heavy tail. The edition-pair ν of the physical-constants chapter is 1.00.
- The chapter does not decide which side of the tension is right; it counts whether quoted errors covered the distance to a later reference.
At a glance
What is measured
The Hubble constant H0 is the recession velocity of galaxies divided by their distance, in km s⁻¹ Mpc⁻¹. Unlike a CODATA edition, an H0 estimate has no "next edition": several teams publish values by different methods in the same year, and today early-universe (cosmic microwave background) and late-universe (distance ladder) measurements give different values. The chapter therefore sets every estimate against two reference values and counts, for both, whether the quoted error covered the distance to the reference. No analogue of the edition-to-edition move (M2) is published.
The two sources and their terms
Metrics
Chronology and method
Sources: J. Huchra, Estimates of the Hubble Constant (hubble.plot.dat, last updated 2010-10-07), Harvard-Smithsonian Center for Astrophysics; assembled as part of the NASA/HST Key Project on the Extragalactic Distance Scale. Aggregates only. · Faerber, T.; López-Corredoira, M. A Chi-Squared Analysis of the Measurements of Two Cosmological Parameters over Time. Universe 2020, 6, 114, doi:10.3390/universe6080114, Appendix Table A2 (read from arXiv:2008.04035v1). CC BY 4.0.