Graphic representation of the Hubble tension (IMAGE)

Association of Universities for Research in Astronomy (AURA)

Graphic representation of the Hubble tension

Caption

This graphic represents the tension that exists between measurements of the expansion rate of the late, nearby Universe, versus what would be expected based on measurements of the early Universe, specifically the cosmic microwave background (CMB). Under the standard model of cosmology, these two approaches are expected to yield the same result, but they don’t. This discrepancy is known as the Hubble tension, and is represented in this graphic by the misalignment between the Early Route and Late Route "bridges."

Currently, the best estimate for the Hubble constant based on measurements of the CMB is about 67.2 kilometers per second per megaparsec. In 2026, the H0 Distance Network (H0DN) Collaboration delivered the most precise direct measurement of the local Hubble constant to-date, reporting a value of 73.50 ± 0.81 kilometers per second per megaparsec, corresponding to a precision of just over 1%.

Credit

NOIRLab/NSF/AURA/J. da Silva/J. Pollard

Usage Restrictions

Credit must be given to the creator.

License

CC BY

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.