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A clearer look at the birth of the universe

First light for the new cosmic microwave background telescope
24 March 2025
The Large Aperture Telescope at the Simons Observatory | Photo Flucerod, CC BY-SA 4.0, Wikimedia

In the Atacama Desert in Chile, a new telescope offers a closer look at the birth of the universe than ever before. The Simons Observatory Large Aperture Telescope (LAT) uses 100,000 detectors to observe the cosmic microwave background (CMB)— the afterglow of the big bang. The telescope’s assembly was finished this February, and it has now completed a successful test observation: the ‘first light’.

FSE Science Newsroom | Text René Fransen

Scientists from the Van Swinderen Institute (VSI) for Particle Physics and Gravity and the Kapteyn Institute for Astronomy of the University of Groningen will be involved in analysing the data provided by this new observatory over the next ten years.

Until now, the most advanced measurements of the CMB were made by the European Planck Space Telescope, between 2009 and 2013. The Simons Observatory is expected to be almost ten times more sensitive.

Installation of the last mirror
Installatie van de laatste spiegel van de Large Aperture Telescope, februari 2025 | Foto M. Devlin

New physics

Observations made by the LAT provide information about the formation of the universe, because the CMB contains clues about the underlying physics of the Big Bang. At the time when this relic radiation was generated — not long after the Big Bang — processes were occurring at much higher energy levels than could ever be achieved in any man-built particle accelerator. The type of physics responsible for the production of this relic radiation has thus never been seen before. Cosmologists expect this background radiation to reveal specific patterns of new physics.

Daan Meerburg (VSI) is a senior advisory member of the team that will analyse the data and has been involved in this project from the beginning. The VSI will make significant contributions to the search for these patterns in data collected by the observatory.

The new observatory will also be able to measure—albeit indirectly—the temperature of gas surrounding galaxies and galaxy clusters. Astrophysicist Luca Di Mascolo of the Kapteyn Institute will use these data to refine models of galaxy formation. Consequently, the observatory will help us to gain a more complete understanding of the history of the universe, how its structure grew and evolved, and how it came to be as we see it today.

More information on the Simons Observatory website.

Last modified:24 March 2025 09.59 a.m.
View this page in: Nederlands

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