November 13, 2026

3 min read

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The enormous trove of galaxies and quasars will help astronomers piece together the most in-depth 3D map of the universe yet made

By Adam Kovac edited by Claire Cameron

On 12 November 2026,ESA’s Euclid space telescope released its first major batch of data: DR1-Foundation. As part of this very large data release, Euclid observed the beautiful core of the Messier 81 galaxy group, part of which is shown here.

ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin

Astronomers took a major step toward navigating the universe, thanks to the European Space Agency’s (ESA) Euclid space telescope, which just released its first major batch of observations.

Since its launch in June 2023, Euclid has been using its 600 megapixel visible-light camera to capture images of cosmos, near and far. All told, it has already managed to document nearly a billion objects, including more than 900 million galaxies and 60 million possible quasars, the ultra-bright nuclei of galaxies where ultra-hot gas is being sucked into a supermassive black hole.

Previous releases of images by Euclid had been focused on a far narrower band of sky. Now, the huge amount of data collected—more than 1.7 million gigabytes—makes the new release the “largest space-based survey of its kind, laying the foundation of future discovery in a new regime for astronomy,” said ESA director of science Carole Mundell in a statement.


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Euclid is aided in its observations by a cosmic phenomenon known as gravitational lensing. As light emitted from galaxies and other celestial objects travels through space, it interacts with the gravitational forces of other large objects. That gravity bends and magnifies the light, making it brighter and easier to detect for telescopes such as Euclid; it can even allow astronomers to determine the mass of the source. But the objects must line up just right for the lensing to occur, making them extremely rare.

According to ESA, Euclid has identified around 15,000 strong candidates for gravitational lensing, a trove that Scott Gaudi, an astronomer at Ohio State University, calls “bonkers.”

“Gravitational lenses are one of nature's toolboxes for us measuring dark matter mass, by looking for these distortions of background quasars and galaxies due to foreground structures,” Gaudi, who is not involved in the Euclid program, says. “But you can't do it from the ground. You just need the high-resolution imaging to do it.”

The Nancy Grace Roman space telescope, which relies on instruments that examine infrared light, as opposed to the optical light Euclid is designed for, will also harness gravitational lensing to see far-off cosmic objects. The two approaches are “very complementary,” says Gaudi, particularly when it comes to searching for elusive things such as dark energy and dark matter.

“Euclid is going for as much area as possible, whereas Roman is focusing in the infrared, and it's focusing on repeating observations of the same area of the sky with different roll angles and different filters," says Gaudi. "I think the joint approach of those two missions is very powerful because you can vet the big statistics you get with Euclid with a very careful controlled system with Roman.”

Euclid's latest release also includes a large amount of data on galaxy clusters. Examining how galaxies are bunched together can offer insights into how the first matter formed and organized shortly after the Big Bang. And Euclid can help astronomers begin to figure out where individual galaxies are located in relation to each other, leading to what could be the most comprehensive three dimensional map of the universe ever made.

“Euclid doesn't just look far back in time – it does so across huge areas of sky,” said Barbara Sartoris, an astrophysicist at France’s JL Lagrange laboratory in the ESA statement. “This gives us an unprecedented view of large samples of ancient galaxy clusters that were previously out of reach. We will explore these in the coming months to learn how these giants grew, and decipher what they reveal about the dark Universe.”

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Source: Scientific American · Adam Kovac

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