Lawrence Berkeley Laboratory

08/10/2026 | Press release | Distributed by Public on 08/10/2026 09:43

Scientists Release Biggest 2D Map of the Universe

Covering roughly 75% of the sky in visible and near-infrared light, the updated map provides a deep view of the extragalactic universe not blocked by the dust and stars of our own Milky Way. Researchers expect it will remain the most comprehensive 2D map of our universe for years to come.

More than 160 scientists contributed to data collection for the project, and a team of 20 produced the final dataset released today. It was built by combining 263,407 telescope exposures from three ground-based sky surveys: the Dark Energy Camera Legacy Survey (DECaLS) at NSF Cerro Tololo Inter-American Observatory, the Mayall z-band Legacy Survey (MzLS) at NSF Kitt Peak National Observatory, and the Beijing-Arizona Sky Survey (BASS) at the University of Arizona's Steward Observatory. That was supplemented by years of data from NASA's Wide-field Infrared Survey Explorer (WISE) satellite mission and additional public data.

"For our team, these data are fundamental to our investigation of the expansion history of the universe and the formation of our galaxy," said Arjun Dey, co-lead of the Legacy Surveys and an astronomer at NSF NOIRLab. "But the skies belong to everyone, and this survey gives everyone the chance to explore the sky and marvel at its wonders."

The DESI Legacy Imaging Surveys were originally conducted to prepare for the Dark Energy Spectroscopic Instrument (DESI) survey. The Legacy Surveys' 2D map is essentially a deep photograph of the sky; it records where galaxies and stars appear and how bright they appear. This crucial step enables DESI to select objects and measure their light in different wavelengths to determine their distances, building the largest high-resolution 3D map ever made. Scientists study the way galaxies have clustered at different ages of the universe to track dark energy over time.

In April 2026, DESI completed its original five-year survey ahead of schedule and with vastly more objects than expected. The early results have shown surprising hints that dark energy's impact may be weakening over time - a paradigm shift that could potentially shape the predicted fate of our universe. DESI expects to publish improved results using their first five years of data in 2027 and is continuing observations into 2028.

Lawrence Berkeley Laboratory published this content on August 10, 2026, and is solely responsible for the information contained herein. Distributed via Public Technologies (PUBT), unedited and unaltered, on August 10, 2026 at 15:43 UTC. If you believe the information included in the content is inaccurate or outdated and requires editing or removal, please contact us at [email protected]