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Extremely Large Telescope

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The Extremely Large Telescope (ELT) is a massive astronomical observatory currently under construction.

The European Extremely Large Telescope
The European Extremely Large Telescope

It is designed to be the world's largest optical and mid-infrared telescope. This project is managed by the European Southern Observatory (ESO) agency. The observatory is located on top of Cerro Armazones in the Atacama Desert of northern Chile. It sits about 23 km away from the existing Paranal Observatory facilities.

Cerro Armazones night-time panorama
Cerro Armazones night-time panorama

This telescope represents a major leap in our ability to study the deep universe.

The ELT uses a sophisticated five-mirror system to collect and focus light.

The optical system of the ELT showing the location of the mirrors
The optical system of the ELT showing the location of the mirrors

The first three mirrors are curved, non-spherical surfaces. This configuration is known as a three-mirror anastigmat design. It provides excellent image quality over a field of view about one-third the width of the full Moon. The fourth mirror is a flat, thick adaptive mirror. It uses adaptive optics to correct for atmospheric distortion. This distortion happens when Earth's air bends light as it travels. The fifth mirror is a flat mirror that provides tip-tilt correction for image stabilization. These two flat mirrors also direct light sideways to two Nasmyth focal stations. This allows researchers to mount several large scientific instruments at the same time.

The primary mirror is the largest part of the telescope's optical system.

It is not one solid piece, but is made of 798 hexagonal segments. Each segment is about 1.4 meters across and 20 centimeters thick. These segments are made from a low-expansion ceramic called Zerodur. To keep the mirror highly reflective, two segments are re-coated or replaced every single working day. Edge sensors measure the position of each segment relative to its neighbors with nanometre accuracy.

First ELT Main Mirror Segments Successfully Cast
First ELT Main Mirror Segments Successfully Cast

Then, 2,394 position actuators adjust the segments to maintain the correct shape. This prevents deformations caused by wind, gravity, or temperature changes.

The secondary mirror is also a massive engineering challenge.

Blank Canvas the ELT’s M2 Mirror Blank
Blank Canvas the ELT’s M2 Mirror Blank

It is highly convex and aspheric in shape. This mirror will be 2.4 meters in diameter and weigh 3.9 tonnes. This makes it the largest secondary mirror ever used on an optical telescope. It will be mounted on a hexapod, which allows for alignment to sub-micrometer precision every few minutes. The glass-ceramic blank was cast by Schott AG. The surface is being polished by Safran Reosc to a precision of 15 nanometres. This level of precision ensures the light is focused perfectly.

History shows how the ELT design evolved to meet practical needs. Originally, the project was called the European Extremely Large Telescope (E-ELT). In 2011, a proposal was made to reduce the overall size of the telescope. The primary mirror diameter was reduced from 42 meters to 39 meters. This change reduced the projected area from 1,360 square meters to 978 square meters. This reduction helped lower estimated costs from 1.275 billion to 1.055 billion euros. It also made the construction timeline more manageable. The name was eventually shortened to the ELT in 2017.

The scale of the ELT is truly enormous when compared to other tools.

The observatory will gather 100 million times more light than the human eye. This is about 10 times more light than the largest optical telescopes available in 2025. It also has 250 times the light-gathering area of the Hubble Space Telescope. Furthermore, the ELT will provide images that are 15 times sharper than those from Hubble. These capabilities are necessary to achieve its ambitious scientific goals.

Scientists intend to use the ELT to answer fundamental questions about the cosmos. It will enable detailed studies of planets orbiting other stars. Researchers hope to detect water and organic molecules in protoplanetary disks. The telescope will also look at the very first galaxies in the Universe. It will study supermassive black holes and the nature of the dark sector. Construction work began in June 2014, and the first stone was laid in May 2017. The telescope is expected to reach "first light" in March 2029. The first scientific observations are planned for December 2030.

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🖼️ Images & Media (13)
File:The ESO Council during their meeting in Garching on 11–12 June 2012.jpg
The ESO Council during their meeting in...
File:A doorway to the Universe (DJI 0078).jpg
A doorway to the Universe (DJI 0078).jpg
File:Cerro Armazones night-time panorama.jpg
Cerro Armazones night-time panorama.jpg
File:The European Extremely Large Telescope.jpg
The European Extremely Large Telescope.jpg
File:The optical system of the ELT showing the location of the mirrors.jpg
The optical system of the ELT showing the...
File:First ELT Main Mirror Segments Successfully Cast.jpg
First ELT Main Mirror Segments...
File:E-ELT mirror segments under test.jpg
E-ELT mirror segments under test.jpg
Blank Canvas the ELT’s M2 Mirror Blank.tif
File:ELT concept.jpg
ELT concept.jpg
File:E-ELT and VLT vs Colosseum.jpg
E-ELT and VLT vs Colosseum.jpg
E-ELT Trailer.ogv
File:The First E-ELT Instruments.jpg
The First E-ELT Instruments.jpg

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