Gravitational waves refine cosmic expansion rate express

Original: "First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis"
arXiv:2601.04774v1 · 2026-01-08 · CC BY 4.0 · 1 min
Combining gravitational wave signals with galaxy surveys yields a more precise measurement of how fast the universe is growing.

Measuring the universe’s expansion is like timing a race when the track stretches. Neutron star mergers act as standard sirens: their gravitational waves ring out with a known “volume,” so fainter signals mean greater distance.

A new study paired the siren from merger GW170817 with a galaxy map tracing matter, including dark matter (invisible mass first detected by Vera Rubin). The result: the Hubble constant (named after Edwin Hubble) is 67.9 km/s per megaparsec, so a galaxy 3.26 million light-years away recedes at that speed — with just 6.4% uncertainty.

This value eases a cosmic dispute: the early universe’s afterglow suggests slower expansion, while nearby exploding stars point to faster. The new number falls between them, highlighting the strength of cross-checking methods. Remarkably, the spacetime ripples from GW170817 jiggled our detectors by less than a proton’s width, yet clocked the universe’s growth.

The term 'standard siren' echoes 'standard candle,' but while candles use light, sirens use gravitational waves, a clever twist on an old cosmic yardstick.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
hubble constant measurement standard siren hubble constant lisa gravitational wave detection root hertz gw170817 sigma signal averaging Hubble's law cosmic explorer cosmological parameters LIGO gravitational wave detector noise reduction cosmic distance measurement james webb space telescope five sigma standard candle einstein telescope event