Astronomy

Euclid Just Mapped 900 Million Galaxies

ESA’s Euclid space telescope released its first big batch of survey data: about 1,900 square degrees of sky, more than 900 million galaxies, and 15,000 cosmic lenses. It is only 14% of the job.

Two bright oval galaxies on a dark field of stars and tiny distant galaxies, a large spiral at upper right and a smaller one at lower left, with faint blue wisps of dust

The core of the Messier 81 galaxy group, about 12 million light-years away, from Euclid’s DR1-Foundation release. Messier 81 is on the right and NGC 3077 on the left; the blue wisps are galactic cirrus, dust clouds in our own galaxy. The frame covers about five full Moons of sky and took Euclid just over an hour to capture. Resized only. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin (CC BY-SA 3.0 IGO).

Euclid looked at one patch of sky, about five times the size of the full Moon, for just over an hour. The picture at the top of this page is what came back: the core of the Messier 81 galaxy group, around 12 million light-years away.

It is one image out of something much bigger. On Nov. 12, 2026, the European Space Agency released DR1-Foundation, the first major batch of data from its Euclid space telescope since launch in July 2023. According to the University of Oxford, part of the Euclid Consortium, Euclid has catalogued more than 900 million galaxies across the area released so far.

A map of 1,900 square degrees

The new data cover around 1,900 square degrees of sky, an area ESA compares to 9,500 full Moons. Oxford puts it at about 5% of the whole sky. The observations were gathered over about 13 months, from spring 2024 to spring 2025, by a telescope Oxford describes as a million miles from Earth.

ESA says the release includes raw data, calibrated images, catalogues and spectra, about 1.7 million gigabytes in all. Earlier Euclid releases held a few days of observations over around 60 square degrees, said Valeria Pettorino, ESA’s Euclid project scientist. “We’re now releasing more than a year of data covering a significantly larger area. This unlocks ground-breaking science.”

A wide, irregularly shaped patchwork of star-filled sky on black, crossed on the left by web-like blue clouds, with a bright small oval galaxy among them and a few small black rectangular gaps
Part of the new release: a mosaic of 740 Euclid observations covering 367 square degrees of the northern sky, nearly 500 gigapixels in size. The small bright oval at lower left is Messier 81, inside blue clouds of galactic cirrus. The black gaps are areas the survey avoided because of very bright stars, or regions masked out after heavy X-ray hits. Resized only. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin (CC BY-SA 3.0 IGO).

Single stars, 12 million light-years away

In the image at the top, the large spiral on the right is Messier 81, the biggest galaxy in the group. ESA calls it a “grand design” spiral: a bright center and well-defined arms rich in gas and dust. The smaller galaxy on the left is NGC 3077, one of its neighbors. Messier 81’s gravity influences nearby galaxies like it, triggering bursts of star formation and changing their shape over time.

The faint blue threads drifting across the frame are not out there with the galaxies. ESA calls them galactic cirrus: dusty clouds inside our own galaxy, hanging in the foreground between us and Messier 81.

See where Messier 81 is in your skyIt sits near the Big Dipper. The live map shows where to point and when it is up.

Zoom in further and the haze of Messier 81’s disc breaks apart. ESA says the galaxy is close enough for Euclid’s sharp optics to capture its individual stars.

A dense field of stars and small galaxies fading into a broad pale glow on the right, with a loose patch of bluish stars just left of center and a bright star with long spikes at lower left
Euclid at full resolution. The haze on the right is the star-filled disc of Messier 81. The loose patch of blue stars left of center is Holmberg IX, a dwarf irregular galaxy; red-hued specks are galaxies much farther away. Resized only. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin (CC BY-SA 3.0 IGO).

15,000 cosmic magnifying glasses

A strong gravitational lens forms when a foreground galaxy lines up with a more distant one, and its gravity bends the background galaxy’s light into arcs or rings. They are rare. ESA says only about one galaxy in several thousand acts as a lens.

To find them, according to Oxford, the team showed galaxies to trained machine-learning lens finders. The results were then checked by eye, by volunteers in the citizen science project Space Warps and by the Euclid strong lensing team. Some 68 million images have been classified so far, revealing about 15,000 high-quality strong lenses. ESA says it is the largest strong lens catalogue ever, bigger than all previous catalogues combined.

A three-by-three grid of galaxies with glowing golden centers, several circled by thin blue rings, arcs and curved streaks of light
Nine strong lenses from the new catalogue. Top row: a classic galaxy–galaxy lens, an Einstein ring in a face-on spiral, an inclined dusty disc. Middle: an edge-on dusty lens, a lensed galaxy with star-forming regions, a compound lens. Bottom: a galaxy group lens, a lensed quasar, another galaxy group lens. Resized only. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by N. Lines and T. Li (CC BY-SA 3.0 IGO).

“Citizen scientists have played a central role in delivering what is the largest set of strong lenses known to date,” said Aprajita Verma of Oxford, one of the leads of Space Warps. “Tantalisingly, we also know we haven’t found everything and there’s yet much more Euclid data to come.”

A dark sky crowded with hundreds of galaxies, spirals and fuzzy ellipticals in white, blue and orange, with two large pale elliptical galaxies near the top
Euclid’s close-up of the rich galaxy cluster Abell 3128, about 800 million light-years away. At the very center is a strong lens: blue arcs made from the light of a more distant galaxy, warped by mass in the foreground. Resized only. Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin (CC BY-SA 3.0 IGO).

Only the first piece

The release also holds Euclid’s first big batch of spectra: more than 160 million, Oxford says. Each one splits an object’s light into a rainbow, which can reveal how far away it is and what it is made of. With distances, scientists can start placing galaxies into the 3D structure of the Universe and the cosmic web, a mesh of filaments made mostly of invisible dark matter.

That map is the real goal. Euclid was built to explore two of astronomy’s biggest mysteries, dark matter and dark energy. And for all its size, this release covers only about 14% of the area Euclid is meant to survey over six years.

The next part, the full DR1, is scheduled for June 16, 2027, ESA says. It will add weak lensing, the much subtler stretching of galaxy shapes by gravity, and how galaxies and galaxy clusters fit into the cosmic web. “So much discovery is yet to come,” Pettorino said.

Bottom line: Euclid’s first big data release holds more than 900 million galaxies by Oxford’s count, plus about 15,000 strong lenses, and it covers only about 14% of the sky the mission plans to map. The 3D map that is meant to probe dark matter and dark energy is still being built.

No Ground. Stay curious.

Tags: Euclid, ESA, DR1, galaxies, Messier 81, gravitational lensing, dark matter, dark energy, sky survey