A yellow-highlighted map of the sky showing the Euclid first data release Wide Survey coverage across the celestial sphere

Euclid’s First Data Release Catalogues 900 Million Galaxies and 15,000 Lenses

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Written by Seth Sebastian

2026-11-15

The European Space Agency (ESA) has released the first large batch of data from its Euclid space telescope, and the Euclid first data release catalogues more than 900 million galaxies. The release, named DR1-Foundation, contains about 13 months of observations. It is the first major data release since Euclid launched in July 2023.

Euclid is on a six-year mission to map about one-third of the sky in three dimensions. ESA says the new data gives researchers the building blocks for the largest 3D map of the cosmos ever made.

A mosaic built from 740 observations

The headline image is a northern-sky mosaic stitched from 740 separate exposures. Together they cover 367 square degrees, and at full resolution the image runs to about 500 gigapixels.

Infographic showing Euclid's sky survey at several zoom levels, from wide views to fine detail.
This infographic shows Euclid’s survey at several scales. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

Zoomed in, the mosaic moves from thousands of galaxies to individual systems. Some sit relatively close to Earth, while others emitted their light billions of years ago. Faint background galaxies, which a smaller field of view would miss, add to the detail.

For a closer look at a single spiral galaxy, Subaru Telescope’s detailed view of M77’s galactic loop shows how much structure ground-based observatories can reveal.

Collage of several gravitational lenses, where a distant galaxy's light is bent into arcs.
This collage shows different types of gravitational lenses captured by Euclid. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by N. Lines and T. Li

The mosaic is part of a wider survey. The two image regions sit inside a footprint of about 1,900 square degrees. ESA compares that area with 9,500 full Moons. The release also includes a separate collection covering 148 square degrees of the southern sky.

Gravitational lenses in unprecedented numbers

The Euclid first data release contains roughly 15,000 strong gravitational lens candidates. Earlier searches had identified only a few hundred such systems over several decades. The source describes it as the largest catalogue of its kind.

Close-up view of Messier 81, a bright spiral galaxy with sweeping arms against black space.
A close-up view of Messier 81. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

A gravitational lens forms when a massive object bends light from a more distant source. A foreground galaxy can stretch the light of a background galaxy into curved arcs, multiple images, or a nearly complete ring. The exact shape depends on how the two galaxies line up and how mass sits in the foreground object.

Wide-field view of NGC 1291, a glowing galaxy surrounded by distant stars and background galaxies.
A wide-field view of NGC 1291. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

Lenses also help measure how much mass a galaxy holds. The bending comes from everything in the foreground system, including its stars and dark matter. Researchers study the distortions to estimate that mass.

Quasars and galaxy clusters

The Euclid first data release also lists more than 60 million quasar candidates. Quasars are the bright cores of distant galaxies, where supermassive black holes pull in surrounding gas and dust. That material forms a hot accretion disc and releases large amounts of radiation as it spirals inward.

Close-up view of NGC 1291 showing its bright central core and detailed inner structure.
A close-up view of NGC 1291. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

Some quasars are bright enough to detect across billions of light years. Their light lets astronomers study galaxies from early cosmic history, when the Universe was only about 5 percent of its current age. Euclid has identified candidates from that era.

Stretched rainbow streaks of light showing the spectra of distant objects against a dark background.
The stretched rainbows of light are the spectra of distant objects. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by B. Granett

The survey also captures galaxy clusters. Euclid imaged the Horologium Supercluster, the Messier 81 galaxy group, and the cluster Abell 3128. Abell 3128 is a cluster that holds hundreds of galaxies. The ring galaxy NGC 1291 also appears among the prominent targets.

Visible-light view of the same field, showing stars and galaxies against dark space.
The spectral image above is also captured by Euclid in visible light. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by B. Granett

Euclid also detects intracluster light, a faint glow that fills the space between galaxies in a cluster. This light comes from stars that gravitational interactions have pulled away from their host galaxies. Euclid has detected it in hundreds of clusters, giving researchers material to study how galaxies interact and evolve.

Euclid first data release: measuring distances with spectra

Images show what distant galaxies look like. Spectra help astronomers estimate how far away they are and what they are made of. A spectrum splits light into its component wavelengths, and certain gases leave recognizable markers in that pattern. The Euclid first data release, DR1-Foundation, includes spectra from more than 160 million sources.

Messier 81 galaxy group, several galaxies scattered across a dark field of view.
The Messier 81 galaxy group. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

The spacecraft carries a 1.2-metre telescope and two scientific instruments. The Visible Instrument (VIS) uses 36 CCD detectors to produce images with about 600 megapixels. The Near-Infrared Spectrometer and Photometer (NISP) records near-infrared light and gathers additional data on each source.

Euclid's wide view of the Horologium Supercluster, a dense region filled with galaxies.
Euclid’s view of the Horologium Supercluster. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

Robotic cameras on other worlds document unfamiliar landscapes in similar detail. Curiosity rover’s panorama of Mars’ yardang layer offers a useful comparison for how spacecraft imaging captures terrain.

Aiming at dark matter and dark energy

ESA says the mission aims to shed light on two of the biggest questions in cosmology: dark energy and dark matter. Dark matter emits no detectable light, yet its gravity shapes how galaxies form and cluster.

Euclid will map the cosmic web, the long filaments of galaxies and clusters separated by sparse regions. Tracing that structure across different distances should show how the Universe developed over billions of years.

Dark energy describes the unknown influence behind the accelerating expansion of the Universe. Euclid will measure galaxy distances and track the growth of cosmic structures. Those measurements will provide evidence for testing competing explanations.

Release timing differs between sources. The main article says ESA expects the complete Data Release 1 in mid-2027. That release will add weak gravitational lensing measurements and more information about galaxy clusters.

What the mission team says

“These are far more than beautiful pictures; today marks a scientific milestone in our study of the cosmos,” she said. She added that the release demonstrates the excellence of European technology, science and international collaboration.

“We’re now releasing more than a year of data covering a significantly larger area. This unlocks ground-breaking science.”

The Euclid first data release gives astronomers more sky, more galaxies and more lenses than any single team can review by hand. The next releases will show which of these objects change what researchers understand about the dark Universe.

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A yellow-highlighted map of the sky showing the Euclid first data release Wide Survey coverage across the celestial sphere
Over roughly one year, Euclid Wide Survey covered around 1900 deg2 of sky, shown here in yellow. Credit: ESA/Euclid/Euclid Consortium/NASA; ESA/Gaia/DPAC; ESA/Planck Collaboration

H/T diyphotography.net

Frequently asked questions

How many galaxies does Euclid’s first data release catalogue include?

The Euclid first data release, named DR1-Foundation, catalogues more than 900 million galaxies. It contains about 13 months of observations and is the first major data release since Euclid launched in July 2023.

How many gravitational lens candidates are in the Euclid data release?

The release contains roughly 15,000 strong gravitational lens candidates. Earlier searches had identified only a few hundred such systems over several decades.

What is Euclid’s mission and how long will it last?

Euclid is on a six-year mission to map about one-third of the sky in three dimensions. The data gives researchers the building blocks for what ESA says will be the largest 3D map of the cosmos ever made.

How many quasar candidates does the Euclid data release list?

The Euclid first data release lists more than 60 million quasar candidates. Quasars are the bright cores of distant galaxies, where supermassive black holes pull in surrounding gas and dust.

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