This view of the rising Earth greeted the Apollo 8 astronauts as they came from behind the Moon after the fourth nearside orbit. Earth is about five degrees above the horizon in the photo. The unnamed surface features in the foreground are near the eastern limb of the Moon as viewed from Earth. The lunar horizon is approximately 780 kilometers from the spacecraft. Width of the photographed area at the horizon is about 175 kilometers. On the Earth 240,000 miles away, the sunset terminator bisects Africa.
This view of the rising Earth greeted the Apollo 8 astronauts as they came from behind the Moon after the fourth nearside orbit. Earth is about five degrees above the horizon in the photo. The unnamed surface features in the foreground are near the eastern limb of the Moon as viewed from Earth. The lunar horizon is approximately 780 kilometers from the spacecraft. Width of the photographed area at the horizon is about 175 kilometers. On the Earth 240,000 miles away, the sunset terminator bisects Africa.

Extremely Large Telescope

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4 min read

The name is not poetry. It is not metaphor. The Extremely Large Telescope is exactly what it says: a telescope so large that its 39.3-meter primary mirror would stretch across a football pitch, its dome rises 80 meters above the desert floor, and its resolution will exceed the Hubble Space Telescope's by a factor of fifteen. The European Southern Observatory is building it on Cerro Armazones, a 3,046-meter peak in Chile's Atacama Desert that was dynamited flat to make room. First light is planned for 2029, and when the dome doors open, astronomers will have an instrument capable of directly imaging planets orbiting other stars.

A Mirror Made of 798 Pieces

No single mirror 39 meters wide could be cast, transported, or supported. Instead, the ELT's primary mirror is a mosaic of 798 hexagonal segments, each 1.45 meters across and polished to a surface accuracy of 7.5 nanometers -- roughly one ten-thousandth the width of a human hair. German company Schott AG casts the blanks from Zerodur, a ceramic that barely expands or contracts with temperature changes. French firm Safran Reosc then polishes one segment per day to meet the seven-year production schedule. An additional 133 maintenance segments allow individual pieces to be swapped out and recoated on a rotating basis without ever leaving a gap. Three actuators per segment, 2,394 in total, constantly adjust the mosaic against wind, gravity, and thermal distortion, keeping the surface stable to within nanometers.

Five Mirrors and a Trick of Atmosphere

What makes the ELT truly revolutionary is not just its size but its optical design. Five mirrors work in concert: three curved mirrors form a three-mirror anastigmat that delivers sharp images across a field of view one-third the width of the full Moon, while a fourth mirror -- a deformable surface of six petals rippling with voice-coil actuators -- corrects for atmospheric turbulence in real time. The fifth mirror handles tip-tilt stabilization. Together, they deliver adaptive optics that improve resolution by a factor of 500 compared to the best natural seeing conditions. Six laser guide star units shoot beams into the upper atmosphere, creating artificial reference points that let the system measure and cancel the blurring caused by turbulent air above the desert.

The Dome on the Flattened Peak

At 93 meters in diameter, the ELT dome dwarfs the Roman Colosseum. Its total mass exceeds 6,100 tonnes, yet it must rotate smoothly enough to track celestial targets, accelerating to 2 degrees per second -- about the speed of a fast walk along its circumference. A pair of curved sliding doors open a 41-meter slit to the sky. Behind them, a windscreen of four spherical blades shields the mirrors from the Atacama's persistent winds. By day, an air-conditioning system cools the interior so that the telescope reaches thermal equilibrium with the night air before sunset, preventing heat shimmer from degrading observations. The Italian ACe Consortium, led by Astaldi and Cimolai, won the construction contract in 2016. As of early 2026, the dome structure is nearing completion, with full dome closure expected in 2027.

What It Will See

The ELT's science goals read like a wish list for the next century of astronomy. Its ANDES spectrograph will search for biosignatures in the atmospheres of Earth-like exoplanets. MICADO, its first imaging camera, will resolve individual stars in galaxies tens of millions of light-years away. HARMONI will function as the workhorse spectroscope, dissecting light from the most distant objects in the universe. The telescope will probe the nature of dark energy by measuring the acceleration of cosmic expansion, test whether the fundamental constants of physics have changed over time, and image the environments around supermassive black holes. Compared to the largest optical telescope operating today, the 10.4-meter Gran Telescopio Canarias, the ELT will collect nearly fifteen times more light.

Cerro Armazones, Where the Air Thins

The Atacama Desert was chosen for the same reasons it has attracted observatories for decades: extreme aridity, high altitude, and some of the clearest skies on Earth. Cerro Armazones sits 23 kilometers from ESO's existing Paranal Observatory, home of the Very Large Telescope. The site receives fewer than ten millimeters of rainfall per year. The atmosphere is so thin and dry at 3,046 meters that infrared and submillimeter radiation passes through with minimal absorption -- precisely the wavelengths needed to study forming stars and distant galaxies. Costing approximately 1.4 billion euros, the ELT is the most expensive ground-based telescope ever constructed. Two rival projects, the Giant Magellan Telescope and the Thirty Meter Telescope, are also targeting the 2030s, but the ELT's 39-meter aperture will give it the largest light-collecting area of any optical telescope in history.

From the Air

Located at 24.59°S, 70.19°W atop Cerro Armazones at 3,046 m elevation in Chile's Atacama Desert. The dome structure is visible from altitude as a large circular feature on the flattened mountaintop. Nearest airport is Andrés Sabella Gálvez International Airport (SCFA/ANF) in Antofagasta, approximately 130 km to the northwest. The Paranal Observatory with its four VLT domes is visible 23 km to the west. Clear skies prevail year-round. Terrain is extremely arid with barren brown mountain ridges.