Largest-ever 3D map of the universe shows 47 million galaxies, from the Milky Way to 'cosmic noon' — Space photo of the week


SOURCE: LIVESCIENCE.COM
APR 19, 2026

By Jamie Carter published 2 hours ago

The largest 3D map of the universe, created with data from the Dark Energy Spectroscopic Instrument, shows 47 million galaxies in stunning detail.

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A blue and white map against a dark background. The denser areas indicate regions where galaxies and galaxy clusters have clumped together to form the strands of the cosmic web.

A small portion of DESI's year-five map of the large-scale structure of the universe. (Image credit: DESI Collaboration and DESI Member Institutions/DOE/KPNO/NOIRLab/NSF/AURA/R. ProctorImage Processing: M. Zamani (NSF NOIRLab))

Quick facts

What it is: The largest 3D map of the universe ever created

Where it is: The universe, as seen from Earth

When it was shared: April 17, 2026

This snapshot is just a small part of one of the most comprehensive and spectacular views yet of the universe — a web-like structure formed by millions of galaxies, stretching back to near the dawn of time.

Each tiny point in the image represents a galaxy mapped by the Dark Energy Spectroscopic Instrument (DESI). The galaxies aren't randomly distributed; instead, they form in filaments and clusters known as the cosmic web. Between these luminous strands of galaxies are vast empty regions known as voids, where few stars or galaxies exist.

The image is from the largest high-resolution 3D map of the universe ever created. DESI, which is mounted on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory in Arizona, uses 5,000 robotic fiber-optic sensors to capture light from distant celestial objects.

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The full DESI map of the cosmic web, showing roughly 47 million galaxies. (Image credit: DESI Collaboration and DESI Member Institutions/ DOE/ KPNO/ NOIRLab/ NSF/ AURA/ R. Proctor)

The five-year survey was supposed to gather data on 34 million galaxies and quasars (the bright cores of distant young galaxies). In practice, it detected over 47 million, along with more than 20 million nearby stars in the Milky Way. A visualization published alongside DESI's map shows how it has grown over those five years.

Some of the light captured in this image took billions of years to reach Kitt Peak, so it allows scientists to look back in time to reconstruct how the universe evolved. The result is a three-dimensional view that not only shows where galaxies are but also how they have moved and clustered over time.

Beyond its visual impact, the image plays a crucial role in probing mysterious dark energy, the name physicists have given to a force that appears to be driving the universe's accelerated expansion. It makes up roughly 70% of the universe, and its nature and distribution are among the biggest questions in physics.

By comparing the distribution of galaxies across different epochs, researchers can track how dark energy has influenced the structure of the universe over the past 11 billion years. Early DESI data has already hinted that dark energy may evolve through cosmic history ?—? a breakthrough that would fundamentally reshape scientists' understanding of the universe and its ultimate fate.

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The image is the result of a massive international collaboration. More than 900 researchers from over 70 institutions contributed to the project, which was led by Lawrence Berkeley National Laboratory and funded by the U.S. Department of Energy Office of Science.

DESI will continue observing the sky through 2028, expanding its map by about 20%. Future observations will target fainter and more distant galaxies, as well as harder-to-observe regions near the Milky Way (where stars get in the way) and in the southern sky (which requires the telescope to peer through more of Earth's atmosphere). The first results from the full dataset are anticipated in 2027.

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Jamie Carter

Jamie Carter

Live Science contributor

Jamie Carter is a Cardiff, U.K.-based freelance science journalist and a regular contributor to Live Science. He is the author of A Stargazing Program For Beginners and co-author of The Eclipse Effect, and leads international stargazing and eclipse-chasing tours. His work appears regularly in Space.com, Forbes, New Scientist, BBC Sky at Night, Sky & Telescope, and other major science and astronomy publications. He is also the editor of WhenIsTheNextEclipse.com.