Astronomers directly detect hydrogen signal from billions of light-years away
New CapabilitiesMeerKAT telescope validates technique that could map the universe's structure far faster than galaxy surveys
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Overview
Updated 1 hour agoAstronomers have directly detected an extremely faint radio signal from hydrogen gas that existed billions of years ago. The detection, made with South Africa's MeerKAT telescope, validates hydrogen intensity mapping, a technique that could map the universe's large-scale structure far faster than traditional galaxy surveys.
Instead of hunting individual galaxies, the method measures the combined hydrogen glow across enormous volumes of space. The signal traveled roughly 4 to 5 billion years to Earth, from when the universe was about 10 to 9 billion years old. The results appeared in the Astrophysical Journal Letters.
Why it matters
This could let astronomers map the universe's structure in a fraction of the time, deepening our understanding of dark matter and cosmic evolution.
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People Involved
Organizations Involved
UK university whose Jodrell Bank Centre for Astrophysics led the research.
South Africa's radio astronomy body, built and operates the MeerKAT array.
International radio astronomy project that will incorporate MeerKAT and other arrays.
Timeline
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First direct hydrogen intensity mapping detection announced
Today Scientific announcementTeam led by University of Manchester uses 96 hours of MeerKAT data to detect hydrogen signal at redshifts 0.32 and 0.44, published in Astrophysical Journal Letters.
Historical Context
2 moments from history that rhyme with this story — and how they unfolded.
Discovery of the 21-cm hydrogen line (1951)
Harvard researchers Harold Ewen and Edward Purcell detected the radio emission from neutral hydrogen in the Milky Way, using a small horn antenna on a roof. The 21-centimeter line became the backbone of radio astronomy.
Astronomers used the line to map the Milky Way's spiral arms and gas distribution.
Today, the 21-cm line is a standard probe of the interstellar medium and, at cosmological distances, the cosmic hydrogen distribution.
The new detection extends that fundamental tool to the distant universe, measuring hydrogen at cosmic scales rather than within our galaxy.
CfA Redshift Survey (1986)
Astronomers at the Harvard-Smithsonian Center for Astrophysics charted the velocities of thousands of galaxies, producing the first 3D map of the cosmic neighborhood. The map revealed the 'Great Wall', a vast sheet of galaxies millions of light-years across.
It demonstrated the extent of large-scale structure in the universe.
Redshift surveys became a cornerstone of cosmology, used to measure dark matter distribution and the universe's expansion.
Hydrogen intensity mapping aims to achieve what galaxy surveys do, but far faster by measuring all galaxies' combined hydrogen glow instead of detecting each one individually.
