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Euclid Telescope Finds Quasars Within 700 Million Years of the Big Bang
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Euclid Telescope Finds Quasars Within 700 Million Years of the Big Bang

The sharp-eyed and far-seeing Euclid space telescope has picked up 31 early quasars that have evaded detection until now.

Original source cited and editorially framed by Cosmos Week. Sky & Telescope
Editorial signatureCosmos Week Editorial Desk
Published13 Jul 2026 12: 00 UTC
Updated2026-07-13
Coverage typeScience journalism
Evidence levelJournalistic coverage
Read time4 min read

Key points

  • Focus: The sharp-eyed and far-seeing Euclid space telescope has picked up 31 early quasars that have evaded detection until now
  • Detail: Science reporting: verify primary technical documentation
  • Editorial reading: science reporting; whenever possible, verify the cited primary source.
Full story

The sharp-eyed and far-seeing Euclid space telescope has picked up 31 early quasars that have evaded detection until now. The post Euclid Telescope Finds Quasars Within 700 Million Years of the Big Bang appeared first on Sky & Telescope. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

That matters because astrophysics becomes persuasive only when an observed signal can be tied to a physically defensible explanation. Compact objects such as neutron stars and black holes are natural laboratories for extreme physics, but the distance and complexity of these systems make interpretation difficult without multi-wavelength coverage and careful modeling. A detection without a mechanism is only half a result. the other half comes from showing that the signal fits quantitatively inside a coherent physical picture rather than merely being consistent with a broad family of models. The post Euclid Telescope Finds Quasars Within 700 Million Years of the Big Bang appeared first on Sky & Telescope. (You can unsubscribe anytime) The sharp-eyed and far-seeing Euclid space telescope has picked up 31 early quasars that have evaded detection until now.

Weeks after probing the heart of the Milky Way, the astronomers behind the European Space Agency’s Euclid telescope have announced another discovery from this wide- and sharp-eyed. One of these is the new record-holder, it formed within just 670 million years of the Big Bang.

Over its first 1½ years, the Euclid space telescope has already surveyed 3, 000 square degrees, almost a tenth of the whole sky, thanks to its wide field of view. The resolution and sensitivity of each Euclid image is equivalent to that of the Hubble Space Telescope, but every few-hours-long pointing captures a field of sky 270 times larger.

For those residing within the universe’s first 770 million years (equivalent to redshifts greater than 7), there’s only expected to be one every 100 square degrees or so. Using Euclid Yang and colleagues more than doubled that number, with 12 new early quasars, as well as 19 additional ones that were born within the first 830 million years (that.

The broader interest lies in turning an observational clue into something that can be weighed against competing models of the underlying physics. Astrophysics does not have the luxury of controlled experiments; everything is inferred from radiation that traveled across cosmic distances under conditions that cannot be reproduced in a terrestrial laboratory. This makes the interpretation chain longer and more uncertain than in bench science, but it also means that a well-constrained measurement of an extreme object carries theoretical information that no earthbound experiment can provide.

We now have a real window onto how the bulk of the first black holes grew, and how they shaped the galaxies around them. Silvia Belladitta (also at Max Planck) led a team that investigated this galaxy using the Northern Extended Millimeter Array (NOEMA) in France, discovering a vast reservoir of gas.

Because this item comes through Sky & Telescope as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to see whether independent datasets and physical modeling converge on the same interpretation. Multi-wavelength follow-up, combining X-ray, radio and optical data where possible, is typically what separates a compelling detection from a robust physical characterization. In high-energy astrophysics, results that initially looked definitive have been revised when data from a second messenger arrived; the current result should be read with that history in mind.

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