Giant 50-meter observatory could pierce interstellar dust, revealing the hidden half of the cosmos

The proposed observatory will also search for the molecular building blocks of life in deep space.
The AtLAST team lowering the weather tower at site I on the Chajnantor plateau. (Cover Image Source: AtLAST Observatory)
The AtLAST team lowering the weather tower at site I on the Chajnantor plateau. (Cover Image Source: AtLAST Observatory)

Astronomers are designing a telescope that they hope will help uncover the half of the universe that remains shrouded in dust. The telescope has been named the Atacama Large Aperture Submillimeter Telescope (AtLAST)—a giant 50-meter observatory. It will sit at a location near the existing ALMA array, high in Chile's Atacama Desert, and peer into dust-covered regions that cannot be seen with ordinary telescopes. Unlike other mega-science projects, AtLAST’s creators want to operate the facility entirely without relying on fossil fuels.

Like a celestial blanket the Milky Way forms an arc high above the antennas of the Atacama Large Millimeter/submillimeter Array (Image Source: ALMA Observatory)
Like a celestial blanket the Milky Way forms an arc high above the antennas of the Atacama Large Millimeter/submillimeter Array (Image Source: ALMA Observatory)

Interstellar dust hides a vast swathe of the universe. The best way to illuminate such obscured regions is to use a gigantic submillimeter-wave telescope designed to detect electromagnetic radiation resting exactly between radio waves and infrared light. "Without submillimeter [data], we're getting a very biased picture of what's out there," said Claudia Cicone, an astrophysicist at the University of Oslo in Norway, in a statement. "We are missing the regions of space that are most obscured by dust." Telescopes like ALMA in Chile have already probed some of these dust-laden regions, but astronomers want to go further with AtLAST. The early design and prototyping phase, known as AtLAST2, will run until 2028. To make the initiative sustainable, researchers from Europe, Chile, South Africa, Canada, Taiwan, Thailand, New Zealand, Japan, and the U.S. are heavily collaborating.

Nobeyama 45 m Radio Telescope located at 1,300 m above sea level. It could facilitate unprecedented levels of optical control for AtLAST. (Cover Image Source:
Nobeyama 45 m Radio Telescope is located at 1,300 m above sea level in Japan. It could facilitate unprecedented levels of optical control for AtLAST. (Image Source: AtLAST Observatory)

They want to bring the cloudy, hidden universe to light. "With previous submillimeter facilities, we're observing the tip of the iceberg," said Cicone, one of the leads on the telescope. "With AtLAST, we will answer the question of where all the gas and dust in the universe is." ALMA captures dusty parts of the universe where stars and planets form, but it acts like a high-powered microscope. Compared to it, AtLAST will function as a wide-angle camera, focusing on broad censuses of dusty locations across the universe. "ALMA can only see an area thousands of times smaller than the Moon's surface on the sky in any given observation," said Tony Mroczkowski, an astronomer at the Institute of Space Sciences in Spain and another of AtLAST's leads.

2026
Testing the conditions at 5000m - AtLAST site characterisation continues on Chajnantor
From 28 - 31 March, five members of the AtLAST team visited the high site at Chajnantor to install instruments that will help further characterise the potential AtLAST sites, part of the ongoing efforts of Work Package 7.

Image of the AtLAST team lowering the weather tower at site I on the Chajnantor plateau 
The AtLAST team lowering the weather tower at site I on the Chajnantor plateau.
The perfect home for submillimeter telescopes
The Chajnantor Plateau is host to some of the most advanced astronomical facilities in the world. A combination of its elevation (5100m above sea level) and excellent weather conditions make it an excellent home for astronomical facilities, and as such has been chosen for the future site of AtLAST. However, the exact location is still to be decided, with two sites still in the running. Detailed characterisation of the two sites is ongoing to determine which site is most suitable for AtLAST.

Characterising the wind on Chajnantor
Since February 2023, instruments known as sonic anemometers have been installed to record the wind properties at the two potential sites for AtLAST. These measurements provide crucial information to the AtLAST team and will help to determine which site is preferable, as well as informing the telescope design and operations teams with real data to work with, rather than just simulations. The current results were highlighted in the recent AtLAST Forum talk by Pamela Pizarro:



 

During this visit, the team set out to identify the origin of spurious signals seen in the data of one anemometer and found out the issue was due to a faulty power supply. This was fixed after an extensive debugging procedure, which included lowering the tower and performing major tower maintenance. At such extreme elevations and conditions, we are really pushing the limits to what is possible and even simple devices (such as a power supply) need to be checked both in the lab and on the high site.

In parallel to the activities on the wind towers, Andrey Baryshev worked on the installation of a new geostationary satellite tracking interferometer that will characterise distortions to astronomical signals across the main dish of AtLAST. A first interferometer is now operational on site II, and an identical type of this system will soon be installed on site I to provide a real-time comparison between both potential sites. These data will then be joined with the wind data from the towers to provide a full characterisation of daily and seasonal variations at both sites.

Is the soil suitable for AtLAST?
In addition to wind studies, it is also important to understand the soil properties and its suitability for supporting a structure as large and as heavy as AtLAST. Soil studies have previously been performed close to site I (specifically for the APEX site). However, site II will need a soil study of its own and therefore preparations for this were made during this visit. This was done by Carlos De Breuck and Juan-Pablo Pérez-Beaupuits, who determined the exact coordinates of the edges of Site II that can be provided to the chosen company to perform the soil study.

Overall, plans are well underway to characterise the two potential sites for AtLAST and the information provided on these site visits (and by the instruments installed) will help guide the site selection and help us choose the future home for AtLAST.

Images from the visit
See more images here: Site Visit March 2026

AtLAST team working on the weather tower at site I. (Image Source:
 AtLAST team working on the weather tower at site I. (Image Source: AtLAST Observatory)

"ALMA is powerful, but you can't map the sky with a microscope. In comparison, AtLAST will image an area up to 16 Moons in size with every observation, so we can map the hell out of the universe," he said. To map the sky at that scale, the telescope will "need to move fast to map back and forth," said Mroczkowski. "With a huge field of view, we would create a pretty large map of the sky quickly." AtLAST has a primary 50-meter dish designed with aluminum panels in the mirror and a massive structure backed by steel. Weighing about 4,400 tonnes, it will use a 12-meter secondary mirror to gather and focus faint submillimeter radiation coming from distant locations. Perched in the exceptionally thin and dry atmosphere at an altitude of over 5 kilometers, it will give us a pristine, moisture-free window into the universe.

View of site II in Atacama desert where soil studies will take place. (Image Source: AtLAST Observatory)
View of site II in Atacama desert where soil studies will take place. (Image Source: AtLAST Observatory)

It is always difficult to run a power-hungry 50-meter observatory in such a remote location. To avoid fossil fuels, researchers are testing combinations of solar power, advanced battery arrays, solid-state metal hydride energy storage, as well as kinetic regeneration to recover the telescope's braking energy as it decelerates from sweeping scans. The team has set a benchmark by planning to use near-zero-carbon power to produce the steel and aluminum. It means that ambitious mega-science can be done without harming the climate. What could AtLAST achieve? It could shed light on cold gas and dust that aid star formation, while also looking closer to home. "We can study the solar atmosphere and the variability of solar flares as has never been done before," said Cicone.

Galaxies and stars across the universe. (Image Source:mik38/istock/Getty images plus)
Galaxies and stars across the universe. (Image Source:mik38/istock/Getty images plus)

When peering into deep space, astronomers often hit a wall known as the "confusion limit," where the sheer density of background objects causes their light to blur together. "You don't know if the light is coming from one galaxy, 10 galaxies, or 1,000 galaxies," said Cicone. "AtLAST will recover these missing galaxies," she said. It has the potential to find up to 50 million previously unseen galaxies in just 1,000 hours of observations. Besides stars and galaxies, AtLAST is capable of spotting complex molecules that might be the building blocks of life embedded within star-forming debris disks. As Mroczkowski noted, mapping these regions could ultimately help astronomers answer how life emerges in the universe, and how it develops and evolves.

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