The UPC’s Centre for Sensors, Instruments and Systems Development (CD6) participates with IDOM in the construction of the Extremely Large Telescope (ELT), promoted by the European Southern Observatory (ESO). The ELT will be the world's largest ground-based optical and near-infrared telescope and is being built at an altitude above 3,000 m, on the Armazones Hill (Atacama Desert, Chile). It is expected to come into operation in 2027.
The Centre for Sensors, Instruments and Systems Development (CD6) of the Universitat Politècnica de Catalunya · BarcelonaTech (UPC), based on the Terrassa Campus, is working on the design of the optical system that will be used to calibrate the 39-metre main mirror—the world’s largest one—of the Extremely Large Telescope (ELT). This revolutionary visible and infrared telescope will be the largest eye ever built to observe the sky and will pave the way for a new generation of ground-based optical telescopes.
With its unique five-mirror design, along with state-of-the-art technology to correct atmospheric distortions, the ELT will provide images 15 times sharper than those from the Hubble Space Telescope. It will allow deep exploration of the universe in great detail, which will lead to further advances in astrophysical knowledge.
One of the goals of the telescope is to detect and study Earth-like planets around other stars and it could become the first telescope to find evidence of life outside our Solar System. It will also probe the farthest reaches of the cosmos, revealing the properties of the earliest galaxies and the nature of the dark universe.
The telescope's five mirrors will have different shapes, sizes and roles, designed to work in perfect coordination, a pioneering optical design that will allow it to reveal the Universe in unprecedented detail. The primary mirror M1 will contain thousands of highly sophisticated components that will allow it to collect light from the night sky and reflect it onto the secondary mirror. Convex M2, the largest secondary mirror ever used in a telescope, about 4 meters in diameter, will hang above M1 and reflect light to M3, which in turn transmits it to a flat adaptive mirror, the M4, above. This fourth mirror will change the shape of its surface a thousand times per second to correct distortions caused by atmospheric turbulence, before sending the light to the M5, a tiltable flat mirror that will stabilize the image and send it to the ELT instruments.
The most spectacular mirror from a technological point of view is the primary mirror M1, which the CD6 researchers at UPC are involved. It is a concave mirror, 39.3 meters in diameter and a radius of curvature of 68.7 meters. Being too large to be made from a single piece of glass, the main mirror is made up of individual hexagonal segments, each about five centimeters thick, about 1.5 meters in diameter and 250 kg in weight, spaced apart for a distance of 4 mm. As a whole, the structure consists of six sectors made up of 133 segments of different shapes and functions. In total, there are 798 hexagonal segments that will act as a single mirror.
The giant dome will house the telescope and its interior structure, providing protection from the extreme environment of the Atacama desert. The dome will be 80 metres high and have a diameter of about 88 metres, giving it a footprint roughly equivalent to that of a football pitch. The upper part of the dome will rotate to allow the telescope to point in any direction through its large observing slit.
Once it is fully equipped with optics and scientific instruments, the telescope is estimated to weigh about 3,700 tons.
From the construction of the immense structure of the telescope dome to the casting of the mirrors, the development of the ELT is the result of the work and collaboration of several leading European companies and research centers, such as IDOM and CD6 of UPC.
As work on manufacturing and designing elements of the ELT in Europe progresses steadily, the ELT is expected to deliver the first scientific observations in September 2027, about half a year after an initial “telescope technical first light”.