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Extremely Large Telescope

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with a 39.3 m (130 ft) diameter primary mirror and a 4.2 m (14 ft) diameter secondary mirror. This reduced projected costs from 1.275 billion to 1.055 billion euros and should allow the telescope to be finished sooner. The smaller secondary is a particularly important change; 4.2 m (14 ft) places it within the capabilities of multiple manufacturers, and the lighter mirror unit avoids the need for high-strength materials in the secondary mirror support spider.
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voice-coil actuators. The image distortion caused by the turbulence of the Earth's atmosphere can be corrected in real-time, as well as deformations caused by the wind upon the main telescope. The ELT's adaptive optics system will provide an improvement of about a factor of 500 in the resolution compared to the best seeing conditions achieved so far without adaptive optics.
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construction proposal for approval in December 2011. Funding was subsequently included in the 2012 budget for initial work to begin in early 2012. The project received preliminary approval in June 2012. ESO approved the start of construction in December 2014, with over 90% funding of the nominal budget secured.
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One of the goals of the ELT is the possibility of making a direct measurement of the acceleration of the Universe's expansion. Such a measurement would have a major impact on our understanding of the Universe. The ELT will also search for possible variations in the fundamental physical constants with
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The dome is to provide needed protection to the telescope in inclement weather and during the day. A number of concepts for the dome were evaluated. The baseline concept for the 40m-class ELT dome is a nearly hemispherical dome, rotating atop a concrete pier, with curved laterally-opening doors. This
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Early designs included a segmented primary mirror with a diameter of 42 metres (140 feet) and an area of about 1,300 m (14,000 sq ft), with a secondary mirror with a diameter of 5.9 m (19 ft). However, in 2011 a proposal was put forward to reduce overall size by 13% to 978 m,
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The ELT is designed to make detailed studies of the first galaxies. Observations of these early galaxies with the ELT will give clues that will help understand how these objects form and evolve. In addition, the ELT will be a unique tool for making an inventory of the changing content of the various
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The ELT will search for extrasolar planets—planets orbiting other stars. This will include not only the discovery of planets down to Earth-like masses through indirect measurements of the wobbling motion of stars perturbed by the planets that orbit them, but also the direct imaging of larger planets
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In January 2017, ESO awarded the contract for the fabrication of the 4608 edge sensors to the FAMES consortium, which is composed of French company Fogale and German company Micro-Epsilon. These sensors can measure relative positions to an accuracy of a few nanometres, the most accurate ever used in
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Science Vision and Infrastructure Roadmap and the ESFRI Roadmap. The telescope underwent a Phase B study in 2014 that included "contracts with industry to design and manufacture prototypes of key elements like the primary mirror segments, the adaptive fourth mirror or the mechanical structure (...)
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was fully funded within the ESO budget. With the 2011 changes in the baseline design (such as a reduction in the size of the primary mirror from 42 m to 39.3 m), in 2017 the construction cost was estimated to be €1.15 billion (including first generation instruments). In 2014, the start of operations
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On 11 June 2012, the ESO Council approved the ELT programme's plans to begin civil works at the telescope site, with the construction of the telescope itself pending final agreement with governments of some member states. Construction work on the ELT site started in June 2014. By December 2014, ESO
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Vernin, Jean; Muñoz-Tuñón, Casiana; Sarazin, Marc; Vazquez Ramió, Héctor; Varela, Antonia M.; Trinquet, Hervé; Miguel Delgado, José; Jiménez Fuensalida, Jesús; Reyes, Marcos; Benhida, Abdelmajid; Benkhaldoun, Zouhair; García Lambas, Diego; Hach, Youssef; Lazrek, M.; Lombardi, Gianluca; Navarrete,
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By probing the most distant objects the ELT will provide clues to understanding the formation of the first objects that formed: primordial stars, primordial galaxies and black holes and their relationships. Studies of extreme objects like black holes will benefit from the power of the ELT to gain
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The ELT dome will have a height of nearly 74 metres from the ground and a diameter of 86 metres, making it the largest dome ever built for a telescope. The dome will have a total mass of around 6100 tonnes, and the telescope mounting and tube structure will have a total moving mass of around 2800
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The 3.8-metre concave tertiary mirror, also cast from Zerodur, will be an unusual feature of the telescope. Most current large telescopes, including the VLT and the NASA/ESA Hubble Space Telescope, use two curved mirrors to form an image. In these cases, a small, flat tertiary mirror is sometimes
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With such a large opening, the ELT dome requires the presence of a windscreen to protect the telescope's mirrors (apart from the secondary), from direct exposure to the wind. The baseline design of the windscreen minimises the volume required to house it. Two spherical blades, either side of the
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who will manufacture the blanks of the 798 segments, as well as a maintenance set of 133 additional segments. This maintenance set allows segments to be removed, replaced, and recoated on a rotating basis once the ELT is in operation. The mirror is being cast from the same low-expansion ceramic
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The 2.4-metre quaternary mirror is a 2-millimeter-thick flat adaptive mirror. With up to 8000 actuators, the surface can be readjusted one thousand times per second. The deformable mirror will be the largest adaptive mirror ever made, and consists of six component petals, control systems, and
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Furthermore, the ELT's suite of instruments will allow astronomers to probe the earliest stages of the formation of planetary systems and to detect water and organic molecules in protoplanetary discs around stars in the making. Thus, the ELT will answer fundamental questions regarding planet
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Besides being designed for water-tightness, air-tightness is also one of the requirements as it is critical to minimise the air-conditioning load. The air-conditioning of the dome is necessary not only to thermally prepare the telescope for the forthcoming night but also in order to keep the
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ESO's Director General commented in a 2011 press release that "With the new E-ELT design we can still satisfy the bold science goals and also ensure that the construction can be completed in only 10–11 years." The ESO Council endorsed the revised baseline design in June 2011 and expected a
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for the first construction phase. The first stone of the telescope was ceremonially laid on 26 May 2017, initiating the construction of the dome's main structure and telescope. The telescope passed the halfway point in its development and construction in July 2023, with completion and
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Making the secondary mirror is a major challenge as it is highly convex, and aspheric. It is also very large; at 4.2 metres in diameter and weighing 3.5 tonnes, it will be the largest secondary mirror ever employed on an optical telescope and the largest convex mirror ever produced.
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Much like the secondary mirror (with which it shares many design characteristics), the tertiary mirror will be slightly deformable to regularly allow deviations to be corrected. Both mirrors will be mounted on 32 points, with 18 on their backside and 14 along their edges.
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As of July 2023, all 6 petals are completed and in the process of being integrated into their support structure. The six laser sources for the adaptive optics system, which will work hand-in-hand with the quaternary mirror, have also been completed and are in testing.
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introduced to divert the light to a convenient focus. However, in the ELT the tertiary mirror also has a curved surface, as the use of three mirrors delivers a better final image quality over a larger field of view than would be possible with a two-mirror design.
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The 39-metre primary mirror will be composed of 798 hexagonal segments, each approximately 1.4 metres across and with 50 mm thickness. Two segments will be re-coated and replaced each working day, to keep the mirror always clean and highly reflective.
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The telescope will have several science instruments and will be able to switch from one instrument to another within minutes. The telescope and dome will also be able to change positions on the sky and start a new observation in a short time.
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The size of the ELT has been reduced from its original design. Even with that reduction, the ELT is significantly larger than both other planned extremely large telescopes. It has the aim of observing the universe in greater detail than the
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The pre-formed glass-ceramic blank of the secondary mirror is being polished and tested by Safran Reosc. The mirror will be shaped and polished to a precision of 15 nanometres (15 millionths of a millimetre) over the optical surface.
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Artist's impression of the Extremely Large Telescope (ELT) in its enclosure on Cerro Armazones during night-time observations. The four beams shooting skywards are lasers that create artificial stars high in the Earth's
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For the observing slit, two main designs were under study: one with two sets of nested doors, and the current baseline design, i.e. a single pair of large sliding doors. This pair of doors has a total width of 45.3 m.
999:: The Multi-AO (adaptive optics) Imaging Camera for Deep Observations (MICADO) will be the first dedicated imaging camera for the ELT and will work with the Multiconjugate adaptive Optics Relay For ELT Observations, ( 924: 1413: 665:(3 for each segment) use this information to adjust the system, keeping the overall surface shape unchanged against deformations caused by external factors such as wind, gravity, temperature changes and vibrations. 905:
Computational fluid dynamic simulations and wind tunnel work are being carried out to study the airflow in and around the dome, as well as the effectiveness of the dome and windscreen in protecting the telescope.
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The dome is designed to allow complete freedom to the telescope so that it can position itself whether it is opened or closed. It will also permit observations from the zenith down to 20 degrees from the horizon.
812:. The mirror will include a fast tip-tilt system for image stabilization that will compensate perturbations caused by wind, atmospheric turbulence, and the telescope itself before reaching the ELT instruments. 712:. Afterward, Safran Reosc will then mount, test, and complete all optical testing before delivery. This is the second-largest contract for ELT construction and the third-largest contract ESO has ever signed. 855:
One year after signing the contract, and after the laying of the first stone ceremony in May 2017, the site was handed over to ACe, signifying the beginning of the construction of the dome's main structure.
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On 19 June 2014, a major milestone towards construction of the ELT was reached. Part of Cerro Armazones was blasted. This video provides a closer look at the event. Note that only natural sound is provided.
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Four of its instruments, the first generation, will be available at or shortly after first light, while two others will begin operations later. Throughout its operation other instruments can be installed.
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A 3D view of the new road to Cerro Armazones area in the Chilean desert. The road extends from the public Route B-710 to the top of the mountain where the European Extremely Large Telescope (E-ELT) will
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avoidance locus as well as preset to a new target within 5 minutes. This requires the dome to be able to accelerate and move at angular speeds of 2 degrees/s (the linear speed is approximately 5 km/h).
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units, and multiple large science instruments. The observatory's design will gather 100 million times more light than the human eye, equivalent to about 10 times more light than the largest
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design for excellent image quality over the 10-arcminute field of view (one-third of the width of the full Moon). The fourth and fifth mirrors are (almost) flat, and respectively provide
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correction for atmospheric distortions (mirror 4) and tip-tilt correction for image stabilization (mirror 5). The fourth and fifth mirrors also send the light sideways to one of two
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by taking images 15 times sharper, although it is designed to be complementary to space telescopes, which typically have very limited observing time available. The ELT's 4.2-metre
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The air-conditioning of the telescope during the day is critical and the current specifications permit the dome to cool the telescope and internal volume by 10 °C over 12 hours.
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Complex support cells are also necessary to ensure the flexible secondary and tertiary mirrors retain their correct shape and position; these support cells will be provided by
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This video shows an artist's impression of the Extremely Large Telescope, the ELT. The protective dome is seen opening for a night observing the optical and infrared skies.
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and Cimolai and the nominated subcontractor, Italy's EIE Group. The signature ceremony took place on 25 May 2016 at ESO's Headquarters in Garching bei München, Germany.
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As of July 2023, over 70% of the mirror segment blanks and their supporting structures have been manufactured, and by early 2024 tens of segments had been polished.
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These drone visuals from Gerhard Hüdepohl show the future location of the ELT against the tranquil backdrop of the barren Chilean desert, as of September 2016.
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Construction workers using heavy machinery work in the Atacama Desert to flatten the top of the mountain for a platform large enough to host the ELT.
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ESO signed a contract for its construction, together with the main structure of the telescopes, with the Italian ACe Consortium, consisting of
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time. An unambiguous detection of such variations would have far-reaching consequences for our comprehension of the general laws of physics.
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is a re-optimisation from the previous design, aimed at reducing the costs, and it is being revalidated to be ready for construction.
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had secured over 90% of the total funding and authorized construction of the telescope to start, which will cost around one billion
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Edge sensors constantly measure the positions of the primary mirror segments relative to their immediate neighbours. 2394 position
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focal stations at either side of the telescope structure, allowing multiple large instruments to be mounted simultaneously.
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The ELT will use a novel design with a total of five mirrors. The first three mirrors are curved (non-spherical) and form a
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has an angular resolution of 1 arcminute which corresponds to separating two light sources 30 cm apart from 1 km distance.
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existing as of 2023, and will correct for atmospheric distortion. It has around 250 times the light gathering area of the
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The first generation includes four instruments: MICADO, HARMONI and METIS, along with the adaptive optics system MORFEO.
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ESO focused on the current design after a feasibility study concluded the proposed 100 m (328 ft) diameter,
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around other stars. As planned in 2011, the facility was expected to take 11 years to construct, from 2014 to 2025.
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Comparison of nominal sizes of apertures of the Extremely Large Telescope and some notable optical telescopes
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more insight into time-dependent phenomena linked with the various processes at play around compact objects.
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The dome design ensures that the dome provides sufficient ventilation for the telescope not to be limited by
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and possibly even the characterisation of their atmospheres. The telescope will attempt to image Earthlike
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distance. At 0.03 arcseconds, the contrast is expected to be 10, sufficient to search for exoplanets. The
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and, according to the ELT's specifications, will provide images 16 times sharper than those from Hubble.
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As of early 2024 the six component petals had been fabricated and are being brazed into a single unit.
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ESO Council Gives Green Light to Detailed Study of the European Extremely Large Telescope Spaceref.com
993:: The Mid-infrared ELT Imager and Spectrograph (METIS) will be a mid-infrared imager and spectrograph. 715:
The segment support system units for the primary mirror are designed and produced by CESA (Spain) and
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In terms of astronomical performance the dome is required to be able to track about the 1-degree
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The 2.7-metre by 2.2-metre quinary mirror is a tip-tilt mirror used to refine the image using
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This video shows an artist's impression of the Extremely Large Telescope, the ELT, in action.
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E-ELT The European Extremely Large Telescope – The World's Biggest Eye on the Sky (brochure)
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and a 4.2 m (14 ft) diameter secondary mirror. The telescope will be supported by
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Julio; Recabarren, Pablo; Renzi, Victor; Sabil, Mohammed; Vrech, Rubén (1 November 2011).
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elements in the Universe with time, and to understand star formation history in galaxies.
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was planned for 2024. Actual construction officially began in early 2017, and a technical
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In May 2017, ESO awarded two additional contracts. One was awarded to the German company
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An Expanded View of the Universe – Science with the European Extremely Large Telescope
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observing slit doors, slide in front of the telescope aperture to restrict the wind.
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The other contract was awarded to the French company, Safran Reosc, a subsidiary of
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The design consists of a reflecting telescope with a 39.3-metre-diameter (130-foot)
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Model of the gigantic and intricate structure inside the enclosure of the ELT.
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Astronet (2008), Bode, Michael F.; Cruz, Maria J.; Molster, Frank J. (eds.),
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This drone camera view gives an early indication of the scale of the project.
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The ASTRONET Infrastructure Roadmap: A Strategic Plan for European Astronomy
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The night sky over the construction site for the Extremely Large Telescope.
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Hippler, Stefan (2019). "Adaptive Optics for Extremely Large Telescopes".
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As of July 2023, the tertiary mirror has been cast and is in polishing.
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Notes: Future first-light dates are provisional and likely to change.
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By early 2024 this mirror was reported to be close to final accuracy.
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The second generation of instruments consists of MOSAIC and ANDES.
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A 40-metre-class mirror will allow the study of the atmospheres of
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under construction. When completed, it will be the world's largest
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ELT compared with one of the four existing VLT Unit Telescopes at
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The ELT under ideal conditions has an angular resolution of 0.005
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The optical system of the ELT showing the location of the mirrors
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The official trailer for the ELT showing the preliminary design.
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In January 2017, ESO awarded a contract for the mirror blank to
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An artist's impression of a close-up of ELT primary mirror.
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Record mirror for Euro telescope BBC Online August 7 2006
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contains an unencyclopedic or excessive gallery of images
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Size comparison between the ELT and other telescope domes
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Publications of the Astronomical Society of the Pacific
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Buildings and structures under construction in Chile
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which corresponds to separating two light sources 1
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ESO The Extremely Large Telescope ("E-ELT") Project
2420:Gilmozzi, Roberto; Spyromilio, Jason (March 2007). 2012:"European Extremely Large Telescope given go-ahead" 1854:"Europe Downscales Monster Telescope to Save Money" 893: 639: 3705:EPICS: direct imagine of exoplanets with the E-ELT 2753:"First ELT Main Mirror Segments Successfully Cast" 2419: 1096:, the second largest optical telescope in Europe. 3895: 3215:"Construction of the ELT Dome Foundations Begins" 359: 5926: 2672: 2670: 2668: 2422:"The European Extremely Large Telescope (E-ELT)" 2373: 1310:(650 ly) distance, or two light sources 30 3477: 3059: 3057: 2490: 2053: 2051: 1921: 3926:Space Telescope European Coordinating Facility 3561: 3540: 3519: 3407: 3405: 2678:"Contracts Signed for ELT Mirrors and Sensors" 2597:"Contracts Signed for ELT Mirrors and Sensors" 2309: 2307: 2276: 2184: 1092:is the same size as the primary mirror on the 5092: 4446: 4432: 4185: 3881: 3582: 3498: 2852: 2665: 2452: 2450: 2145:"ESO To Build World's Biggest Eye on the Sky" 2035: 1948: 1946: 1707:List of largest optical reflecting telescopes 1357:beside adjacent text, in accordance with the 3763:"Artist's rendering of the ELT in operation" 3684:"Giant Magellan Telescope – 6th mirror cast" 3603: 3054: 2803:"Compañía Española de Sistemas Aeronáuticos" 2469: 2125: 2123: 2048: 3402: 3388: 3386: 2848: 2846: 2844: 2304: 1881: 1879: 1877: 1875: 1873: 1871: 1800: 1621:Artist's rendering of the ELT in operation. 1351:removing excessive or indiscriminate images 859: 5099: 5085: 4439: 4425: 4192: 4178: 3888: 3874: 2447: 2210: 2005: 2003: 1943: 1743:List of highest astronomical observatories 676:Cast of the first ELT main mirror segments 338: 316: 299: 284: 270: 254: 241: 228: 214: 189: 169: 155: 138: 76: 59: 43: 3629: 3611:"GMT Overview – Giant Magellan Telescope" 3413:"ESO – The First Objects in the Universe" 2556: 2413: 2120: 1851: 1373:Learn how and when to remove this message 818: 508:ESO Council meets at ESO headquarters in 30:For the general type of observatory, see 3383: 2855:"ESO's ELT halfway through construction" 2841: 2496: 2029: 1868: 1847: 1845: 1843: 1841: 1839: 1560:A video describing what the ELT will be. 1044: 1036: 963: 920: 871: 827: 792:The AdOptica consortium, partnered with 729: 695: 671: 648: 615: 608:concept studies for eight instruments". 567: 538: 503: 2955: 2953: 2544:Journal of Astronomical Instrumentation 2540: 2477:"ESO – Europe's Window on the Universe" 2329: 2162: 2137: 2000: 1806: 1786:Cerro Tololo Inter-American Observatory 746:, who cast it later the same year from 298:743.4 m (2,439 ft 0 in) 14: 5927: 3663:"Extremely Large Telescope – Timeline" 3439:"First Instruments for E-ELT Approved" 700:Several segments of the primary mirror 471:The project was originally called the 430:(ESO) agency, it is located on top of 227:39.3 m (128 ft 11 in) 5080: 4420: 4173: 3869: 1836: 1633:Diagram of the 40m-class ELT primary 368:Location of Extremely Large Telescope 5838: 5059: 4504: 4153: 3637:"About TMT – Thirty Meter Telescope" 2950: 2009: 1897: 1329: 823: 783: 543:ELT construction status in June 2024 283:978 m (10,530 sq ft) 27:Major astronomical facility in Chile 5935:Astronomical observatories in Chile 4201:Astronomical observatories in Chile 3337:"E-ELT Phase B Final Design Review" 2355:"ESO's collaboration with industry" 2337:"The E-ELT Moves Closer to Reality" 1595:Rendering of the MICADO instrument. 1349:Please help improve the section by 725: 253:3.75 m (12 ft 4 in) 240:4.09 m (13 ft 5 in) 24: 3742:"The Milky Way above the ELT site" 1852:Schilling, Govert (14 June 2011). 1738:List of astronomical observatories 959: 767: 530:Roque de los Muchachos Observatory 473:European Extremely Large Telescope 25: 5966: 4898:Nancy Grace Roman Space Telescope 4378:National Astronomical Observatory 3804: 2906:from the original on 14 June 2024 2284:"The E-ELT Construction Proposal" 2065:. 4 December 2014. Archived from 1980:"The E-ELT construction proposal" 1824:from the original on 8 March 2024 803: 644: 551:The design phase of the 5-mirror 5912: 5900: 5888: 5876: 5864: 5837: 5826: 5825: 5596:Southern African Large Telescope 5058: 5047: 5046: 4719: 4713: 4707: 4401: 4400: 4152: 4136: 4125: 4124: 3934: 3821:Final stage for telescope design 1682: 1670: 1665:Rendering of ELT during the day. 1658: 1642: 1626: 1614: 1600: 1588: 1565: 1529: 1509: 1488: 1470: 1448: 1428: 1408: 1387: 1359:Manual of Style on use of images 1334: 1199:Southern African Large Telescope 916: 894:Ventilation and air-conditioning 706:Safran Electronics & Defense 640:ELT mirror and sensors contracts 590:Southern African Large Telescope 379: 358: 351: 5022:Habitable zone for complex life 4937:Nautilus Deep Space Observatory 3916:Llano de Chajnantor Observatory 3780: 3755: 3734: 3709: 3698: 3676: 3655: 3452: 3431: 3357: 3329: 3304: 3279: 3254: 3229: 3207: 3182: 3157: 3132: 3107: 3082: 3028: 3003: 2978: 2918: 2886: 2861: 2816: 2795: 2770: 2745: 2720: 2695: 2640: 2614: 2589: 2534: 2399: 2347: 2081: 2010:Amos, Jonathan (11 June 2012). 1751:Llano de Chajnantor Observatory 1124:Extremely Large Telescope (ELT) 572:Cerro Armazones at night (2010) 496:planned at that time for 2028. 3831:Ground Telescope to Super Size 2853:Roberto Tamai (19 June 2024). 2381:"ESO – Preparing a Revolution" 2110:"Groundbreaking for the E-ELT" 2036:James Vincent (19 June 2014). 1915: 1756:Atacama Large Millimeter Array 1747:Other observatories in Chile: 1733:Overwhelmingly Large Telescope 578:Overwhelmingly Large Telescope 49:Artist's impression of the ELT 13: 1: 5950:Telescopes under construction 5940:European Southern Observatory 5106: 3897:European Southern Observatory 3811:ESO Extremely Large Telescope 3194:European Southern Observatory 2149:European Southern Observatory 1987:European Southern Observatory 1909:European Southern Observatory 1891:European Southern Observatory 1794: 1032: 884: 518:European Southern Observatory 428:European Southern Observatory 168:3,046 m (9,993 ft) 151:European Southern Observatory 72:European Southern Observatory 4987:Space Interferometry Mission 4370:Santiago Metropolitan Region 4100:Astronomy & Astrophysics 2934:(in Spanish). Archived from 1724:(planned completion in 2025) 7: 1776:Cerro Armazones Observatory 1694: 563: 512:bei München, Germany, 2012. 10: 5971: 4861:James Webb Space Telescope 1712:List of optical telescopes 1325: 1314:apart from roughly 12,000 1272: 1254: 1235: 1216: 1197: 1178: 1159: 1140: 1122: 1094:William Herschel Telescope 1070:extremely large telescopes 1062:largest optical telescopes 499: 29: 5820: 5612: 5589:Large Binocular Telescope 5554:Extremely Large Telescope 5547:Extremely large telescope 5520: 5403: 5343: 5264: 5226: 5187: 5180: 5114: 5042: 5017:Discoveries of exoplanets 5004: 4992:Terrestrial Planet Finder 4960: 4909: 4872: 4817: 4735: 4728: 4705: 4472: 4454: 4448:Exoplanet search projects 4396: 4368: 4325: 4295: 4207: 4119: 4091: 4028: 3943: 3932: 3903: 3460:"Instruments | ELT | ESO" 2575:10.1142/S2251171719500016 1717:Large Binocular Telescope 1291: 1180:Large Binocular Telescope 968:The first ELT instruments 944:formation and evolution. 620:Schematic view of the ELT 611: 405:Extremely Large Telescope 390: 377: 346: 325: 307: 292: 279: 262: 249: 236: 223: 202:extremely large telescope 197: 177: 164: 146: 104: 85: 67: 54: 42: 38:Extremely Large Telescope 32:extremely large telescope 5561:Gran Telescopio Canarias 4315:Giant Magellan Telescope 1728:Gran Telescopio Canarias 1722:European Solar Telescope 1237:Gran Telescopio Canarias 1161:Giant Magellan Telescope 1074:Giant Magellan Telescope 1066:Gran Telescopio Canarias 910:telescope optics clean. 860:Astronomical performance 586:Gran Telescopio Canarias 413:astronomical observatory 385:Related media on Commons 5656:Astrology and astronomy 5366:Gravitational radiation 3365:"ESO – E-ELT Enclosure" 2361:. ESO. 22 December 2017 2192:"E-ELT: Finding a home" 1072:include the 25 m/368 m 1064:operating today is the 626:three-mirror anastigmat 520:(ESO) Council selected 237:Secondary diameter 5575:Hubble Space Telescope 1355:moving relevant images 1218:Hobby–Eberly Telescope 1142:Thirty Meter Telescope 1086:Hubble Space Telescope 1078:Thirty Meter Telescope 1057: 1042: 969: 932: 877: 833: 819:ELT dome and structure 735: 701: 677: 654: 621: 573: 544: 516:On 26 April 2010, the 513: 466:Hubble Space Telescope 250:Tertiary diameter 55:Alternative names 5679:Astroparticle physics 5414:Australian Aboriginal 3485:"ESO HARMONI Webpage" 3262:"Cimolai – Home Page" 2732:www.micro-epsilon.com 2465:. ESO Science Office. 1954:"ESO – Are We Alone?" 1048: 1040: 967: 930: 875: 831: 734:ELT's M2 mirror blank 733: 699: 675: 652: 619: 571: 560:is planned for 2028. 542: 507: 268:0.005 arcsecond  5671:Astronomers Monument 5603:Very Large Telescope 5150:Astronomical symbols 3965:(under construction) 3911:La Silla Observatory 3569:"ESO MOSAIC Webpage" 3548:"ESO MORFEO Webpage" 3527:"ESO MICADO Webpage" 3036:"ESO – E-ELT Optics" 2622:"ESO – E-ELT Optics" 2523:on 23 September 2015 2172:. ESO. 26 April 2010 1781:La Silla Observatory 1769:Very Large Telescope 1651:Cerro Paranal, Chile 1306:apart from 200  1274:Very Large Telescope 1049:ELT compared to the 691:Very Large Telescope 481:protoplanetary disks 280:Collecting area 198:Telescope style 94:Antofagasta Province 5744:List of astronomers 5157:Astronomical object 5027:Lists of exoplanets 4798:detected exoplanets 4310:Magellan Telescopes 4237:Llano de Chajnantor 3921:Paranal Observatory 3826:Green light for ELT 3590:"ESO HIRES Webpage" 3506:"ESO METIS Webpage" 3217:. 27 September 2019 2961:"M2 and M3 Mirrors" 2938:on 27 February 2017 2567:2019JAI.....850001H 2441:2007Msngr.127...11G 2317:. ESO. 15 June 2011 2239:2011PASP..123.1334V 2170:"E-ELT Site Chosen" 1764:Paranal Observatory 1702:Lists of telescopes 126:24.5893°S 70.1916°W 122: /  39: 5955:Astronomy projects 5730:Physical cosmology 4942:New Worlds Mission 4209:Antofagasta Region 2551:(2): 1950001–322. 2343:. 9 December 2011. 2233:(909): 1334–1346. 1960:on 17 January 2013 1817:The New York Times 1058: 1043: 970: 933: 878: 834: 736: 702: 693:mirrors in Chile. 678: 655: 622: 601:extrasolar planets 574: 545: 514: 462:optical telescopes 264:Angular resolution 206:infrared telescope 131:-24.5893; -70.1916 98:Antofagasta Region 37: 5852: 5851: 5737:Quantum cosmology 5723:Planetary geology 5516: 5515: 5227:Celestial subject 5074: 5073: 5012:Detection methods 5000: 4999: 4414: 4413: 4167: 4166: 3967: 3090:"www.adoptica.it" 2703:"FOGALE nanotech" 2513:978-3-923524-63-1 2293:, 2 December 2011 2069:on 23 August 2020 1856:. Science Insider 1576: 1555: 1519: 1499: 1478: 1459: 1438: 1418: 1397: 1383: 1382: 1375: 1320:unaided human eye 1296: 1295: 928: 824:Dome construction 784:Quaternary mirror 401: 400: 210:Nasmyth telescope 16:(Redirected from 5962: 5917: 5916: 5915: 5905: 5904: 5903: 5893: 5892: 5891: 5881: 5880: 5869: 5868: 5867: 5860: 5845: 5841: 5840: 5833: 5829: 5828: 5813: 5804: 5797: 5790: 5783: 5774: 5767: 5760: 5758:Medieval Islamic 5753: 5746: 5739: 5732: 5725: 5718: 5711: 5702: 5695: 5688: 5681: 5674: 5665: 5658: 5651: 5644: 5642:Astroinformatics 5637: 5630: 5623: 5621:Archaeoastronomy 5605: 5598: 5591: 5584: 5582:Keck Observatory 5577: 5570: 5563: 5556: 5549: 5542: 5535: 5509: 5500: 5493: 5486: 5479: 5477:Medieval Islamic 5472: 5465: 5458: 5451: 5444: 5437: 5430: 5423: 5416: 5396: 5389: 5382: 5375: 5368: 5361: 5354: 5336: 5327: 5320: 5313: 5306: 5304: 5296: 5294: 5282: 5275: 5255: 5248: 5241: 5219: 5212: 5205: 5198: 5185: 5184: 5173: 5166: 5159: 5152: 5145: 5136: 5129: 5122: 5101: 5094: 5087: 5078: 5077: 5062: 5061: 5050: 5049: 4902: 4894: 4886: 4865: 4857: 4847: 4839: 4831: 4810: 4800: 4793: 4785: 4782: 4769: 4761: 4758: 4747: 4733: 4732: 4723: 4717: 4711: 4515:FINDS Exo-Earths 4441: 4434: 4427: 4418: 4417: 4404: 4403: 4194: 4187: 4180: 4171: 4170: 4156: 4155: 4142:Portal:Astronomy 4140: 4128: 4127: 4006: 3988: 3980: 3963: 3938: 3890: 3883: 3876: 3867: 3866: 3799: 3798: 3796: 3794: 3784: 3778: 3777: 3775: 3773: 3759: 3753: 3752: 3750: 3748: 3738: 3732: 3731: 3729: 3727: 3713: 3707: 3702: 3696: 3695: 3693: 3691: 3680: 3674: 3673: 3671: 3669: 3659: 3653: 3652: 3650: 3648: 3643:on 8 August 2011 3639:. 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5139: 5138: 5137: 5123: 5115: 5112: 5111: 5104: 5103: 5096: 5089: 5081: 5072: 5071: 5069: 5068: 5056: 5043: 5040: 5039: 5037: 5036: 5035: 5034: 5024: 5019: 5014: 5008: 5006: 5002: 5001: 4998: 4997: 4995: 4994: 4989: 4984: 4977: 4972: 4964: 4962: 4958: 4957: 4955: 4954: 4949: 4944: 4939: 4934: 4929: 4924: 4919: 4913: 4911: 4907: 4906: 4904: 4903: 4895: 4887: 4876: 4874: 4870: 4869: 4867: 4866: 4864:(2021–present) 4858: 4856:(2021–present) 4848: 4846:(2019–present) 4840: 4838:(2018–present) 4832: 4830:(2013–present) 4821: 4819: 4815: 4814: 4812: 4811: 4803: 4802: 4801: 4786: 4770: 4762: 4748: 4739: 4737: 4730: 4729:Space missions 4726: 4725: 4706: 4704: 4702: 4701: 4696: 4691: 4686: 4681: 4676: 4671: 4666: 4661: 4656: 4651: 4646: 4641: 4636: 4631: 4626: 4621: 4616: 4611: 4606: 4605: 4604: 4594: 4589: 4584: 4579: 4574: 4569: 4564: 4559: 4554: 4549: 4544: 4539: 4534: 4533: 4532: 4527: 4517: 4512: 4507: 4502: 4497: 4492: 4487: 4482: 4476: 4474: 4470: 4469: 4467: 4466: 4461: 4459:Exoplanetology 4455: 4452: 4451: 4444: 4443: 4436: 4429: 4421: 4412: 4411: 4409: 4408: 4397: 4394: 4393: 4391: 4390: 4385: 4383:Cerro El Roble 4380: 4374: 4372: 4366: 4365: 4363: 4362: 4357: 4352: 4346: 4341: 4331: 4329: 4323: 4322: 4320: 4319: 4318: 4317: 4312: 4301: 4299: 4297:Atacama Region 4293: 4292: 4290: 4289: 4284: 4279: 4269: 4263: 4258: 4253: 4248: 4243: 4234: 4229: 4219: 4213: 4211: 4205: 4204: 4197: 4196: 4189: 4182: 4174: 4165: 4164: 4162: 4161: 4149: 4133: 4120: 4117: 4116: 4114: 4113: 4111:Xavier Barcons 4108: 4103: 4095: 4093: 4089: 4088: 4086: 4085: 4080: 4075: 4070: 4065: 4060: 4055: 4050: 4045: 4040: 4034: 4032: 4026: 4025: 4023: 4022: 4017: 4012: 4007: 3999: 3994: 3989: 3981: 3973: 3968: 3958: 3953: 3947: 3945: 3941: 3940: 3933: 3931: 3929: 3928: 3923: 3918: 3913: 3907: 3905: 3901: 3900: 3893: 3892: 3885: 3878: 3870: 3864: 3863: 3853: 3848: 3843: 3838: 3833: 3828: 3823: 3818: 3813: 3806: 3805:External links 3803: 3801: 3800: 3779: 3754: 3733: 3708: 3697: 3675: 3654: 3628: 3617:on 9 June 2011 3602: 3581: 3560: 3539: 3518: 3497: 3476: 3451: 3430: 3401: 3382: 3356: 3328: 3303: 3278: 3253: 3228: 3206: 3181: 3156: 3131: 3106: 3081: 3053: 3027: 3002: 2977: 2949: 2917: 2885: 2860: 2840: 2815: 2794: 2778:"Safran Reosc" 2769: 2744: 2719: 2694: 2664: 2639: 2613: 2588: 2533: 2512: 2506:, p. 43, 2489: 2468: 2446: 2435:(127): 11–19. 2412: 2398: 2372: 2346: 2328: 2303: 2275: 2247:10.1086/662995 2209: 2183: 2161: 2136: 2131:"ELT Timeline" 2119: 2098: 2095:. 26 May 2017. 2080: 2047: 2028: 1999: 1971: 1942: 1914: 1896: 1867: 1835: 1798: 1796: 1793: 1791: 1790: 1789: 1788: 1783: 1778: 1773: 1772: 1771: 1761: 1760: 1759: 1745: 1740: 1735: 1730: 1725: 1719: 1714: 1709: 1704: 1698: 1696: 1693: 1692: 1691: 1688: 1681: 1679: 1676: 1669: 1667: 1664: 1657: 1655: 1648: 1641: 1639: 1632: 1625: 1623: 1620: 1613: 1610: 1609: 1606: 1599: 1597: 1594: 1587: 1584: 1583: 1580: 1564: 1562: 1559: 1528: 1526: 1523: 1508: 1506: 1503: 1487: 1485: 1482: 1469: 1467: 1463: 1447: 1445: 1442: 1427: 1425: 1422: 1407: 1405: 1401: 1386: 1381: 1380: 1342: 1340: 1333: 1327: 1324: 1294: 1293: 1289: 1288: 1286: 1283: 1280: 1277: 1270: 1269: 1267: 1264: 1261: 1258: 1252: 1251: 1249: 1246: 1243: 1240: 1233: 1232: 1230: 1227: 1224: 1221: 1214: 1213: 1211: 1208: 1205: 1202: 1195: 1194: 1192: 1189: 1186: 1183: 1176: 1175: 1173: 1170: 1167: 1164: 1157: 1156: 1154: 1151: 1148: 1145: 1138: 1137: 1135: 1132: 1129: 1126: 1120: 1119: 1116: 1113: 1108: 1103: 1034: 1031: 1030: 1029: 1019: 1009: 1008: 994: 988: 961: 958: 918: 915: 895: 892: 886: 883: 861: 858: 825: 822: 820: 817: 805: 804:Quinary mirror 802: 785: 782: 769: 766: 727: 724: 646: 645:Primary mirror 643: 641: 638: 613: 610: 565: 562: 501: 498: 450:primary mirror 436:Atacama Desert 426:. Part of the 399: 398: 391: 388: 387: 375: 374: 367: 366: 357: 356: 350: 349: 348: 347: 344: 343: 327: 323: 322: 309: 305: 304: 296: 290: 289: 281: 277: 276: 266: 260: 259: 251: 247: 246: 238: 234: 233: 225: 221: 220: 199: 195: 194: 179: 175: 174: 166: 162: 161: 148: 144: 143: 106: 102: 101: 87: 83: 82: 69: 65: 64: 56: 52: 51: 48: 26: 9: 6: 4: 3: 2: 5967: 5956: 5953: 5951: 5948: 5946: 5943: 5941: 5938: 5936: 5933: 5932: 5930: 5920: 5910: 5908: 5898: 5896: 5886: 5884: 5879: 5874: 5872: 5862: 5861: 5858: 5844: 5835: 5832: 5823: 5822: 5819: 5812: 5808: 5803: 5799: 5796: 5792: 5789: 5785: 5784: 5782: 5778: 5773: 5769: 5766: 5762: 5759: 5755: 5752: 5748: 5747: 5745: 5741: 5738: 5734: 5731: 5727: 5724: 5720: 5717: 5713: 5710: 5706: 5701: 5697: 5696: 5694: 5693:Constellation 5690: 5687: 5683: 5680: 5676: 5673: 5672: 5667: 5664: 5660: 5657: 5653: 5650: 5646: 5643: 5639: 5636: 5632: 5629: 5625: 5622: 5618: 5617: 5615: 5611: 5604: 5600: 5597: 5593: 5590: 5586: 5583: 5579: 5576: 5572: 5569: 5565: 5562: 5558: 5555: 5551: 5548: 5544: 5541: 5537: 5534: 5530: 5529: 5527: 5525: 5519: 5508: 5504: 5499: 5495: 5494: 5492: 5488: 5485: 5481: 5478: 5474: 5471: 5467: 5464: 5460: 5457: 5453: 5450: 5446: 5443: 5439: 5436: 5432: 5429: 5425: 5422: 5418: 5415: 5411: 5410: 5408: 5406: 5402: 5395: 5391: 5388: 5384: 5381: 5377: 5374: 5370: 5367: 5363: 5360: 5356: 5353: 5349: 5348: 5346: 5344:Other methods 5342: 5335: 5331: 5326: 5322: 5321: 5319: 5315: 5312: 5308: 5305: 5298: 5293: 5288: 5284: 5281: 5280:Submillimetre 5277: 5274: 5270: 5269: 5267: 5263: 5254: 5250: 5249: 5247: 5243: 5240: 5239:Extragalactic 5236: 5232: 5231: 5229: 5225: 5218: 5214: 5211: 5207: 5204: 5203:Observational 5200: 5197: 5193: 5192: 5190: 5186: 5183: 5179: 5172: 5168: 5165: 5161: 5158: 5154: 5151: 5147: 5144: 5140: 5135: 5131: 5130: 5128: 5124: 5121: 5117: 5116: 5113: 5109: 5102: 5097: 5095: 5090: 5088: 5083: 5082: 5079: 5067: 5066: 5057: 5055: 5054: 5045: 5044: 5041: 5033: 5030: 5029: 5028: 5025: 5023: 5020: 5018: 5015: 5013: 5010: 5009: 5007: 5003: 4993: 4990: 4988: 4985: 4983: 4982: 4978: 4976: 4973: 4971: 4970: 4966: 4965: 4963: 4959: 4953: 4950: 4948: 4945: 4943: 4940: 4938: 4935: 4933: 4930: 4928: 4925: 4923: 4920: 4918: 4915: 4914: 4912: 4908: 4899: 4896: 4891: 4888: 4883: 4882: 4878: 4877: 4875: 4871: 4862: 4859: 4854: 4853: 4849: 4844: 4841: 4836: 4833: 4828: 4827: 4823: 4822: 4820: 4816: 4807: 4804: 4799: 4795: 4794: 4790: 4787: 4781: 4780: 4774: 4771: 4766: 4763: 4757: 4752: 4749: 4744: 4741: 4740: 4738: 4734: 4731: 4727: 4722: 4716: 4710: 4700: 4699:ZIMPOL/CHEOPS 4697: 4695: 4692: 4690: 4687: 4685: 4682: 4680: 4677: 4675: 4672: 4670: 4667: 4665: 4662: 4660: 4657: 4655: 4652: 4650: 4647: 4645: 4642: 4640: 4637: 4635: 4632: 4630: 4627: 4625: 4622: 4620: 4617: 4615: 4612: 4610: 4607: 4603: 4600: 4599: 4598: 4595: 4593: 4590: 4588: 4585: 4583: 4580: 4578: 4575: 4573: 4570: 4568: 4565: 4563: 4560: 4558: 4555: 4553: 4550: 4548: 4545: 4543: 4540: 4538: 4535: 4531: 4528: 4526: 4523: 4522: 4521: 4518: 4516: 4513: 4511: 4508: 4506: 4503: 4501: 4498: 4496: 4493: 4491: 4488: 4486: 4483: 4481: 4478: 4477: 4475: 4471: 4465: 4462: 4460: 4457: 4456: 4453: 4449: 4442: 4437: 4435: 4430: 4428: 4423: 4422: 4419: 4407: 4399: 4398: 4395: 4389: 4388:Manuel Foster 4386: 4384: 4381: 4379: 4376: 4375: 4373: 4371: 4367: 4361: 4358: 4356: 4353: 4350: 4347: 4345: 4344:Vera C. Rubin 4342: 4340: 4336: 4333: 4332: 4330: 4328: 4324: 4316: 4313: 4311: 4308: 4307: 4306: 4303: 4302: 4300: 4298: 4294: 4288: 4285: 4283: 4280: 4277: 4273: 4270: 4267: 4264: 4262: 4259: 4257: 4254: 4252: 4249: 4247: 4244: 4242: 4238: 4235: 4233: 4230: 4227: 4223: 4220: 4218: 4215: 4214: 4212: 4210: 4206: 4202: 4195: 4190: 4188: 4183: 4181: 4176: 4175: 4172: 4160: 4159: 4150: 4148: 4147: 4143: 4139: 4134: 4132: 4131: 4122: 4121: 4118: 4112: 4109: 4107: 4104: 4102: 4101: 4097: 4096: 4094: 4090: 4084: 4081: 4079: 4076: 4074: 4071: 4069: 4066: 4064: 4061: 4059: 4056: 4054: 4051: 4049: 4046: 4044: 4041: 4039: 4036: 4035: 4033: 4027: 4021: 4018: 4016: 4013: 4011: 4008: 4003: 4000: 3998: 3995: 3993: 3990: 3985: 3982: 3977: 3974: 3972: 3969: 3966: 3962: 3959: 3957: 3954: 3952: 3949: 3948: 3946: 3942: 3937: 3927: 3924: 3922: 3919: 3917: 3914: 3912: 3909: 3908: 3906: 3902: 3898: 3891: 3886: 3884: 3879: 3877: 3872: 3871: 3868: 3861: 3860:archive.today 3857: 3854: 3852: 3849: 3847: 3844: 3842: 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2592: 2584: 2580: 2576: 2572: 2568: 2564: 2559: 2554: 2550: 2546: 2545: 2537: 2519: 2515: 2509: 2502: 2501: 2493: 2478: 2472: 2461: 2460: 2453: 2451: 2442: 2438: 2434: 2430: 2429:The Messenger 2423: 2416: 2408: 2402: 2386: 2382: 2376: 2360: 2359:Xavier Bacons 2356: 2350: 2342: 2338: 2332: 2316: 2310: 2308: 2292: 2285: 2279: 2260: 2256: 2252: 2248: 2244: 2240: 2236: 2232: 2228: 2221: 2213: 2197: 2193: 2187: 2171: 2165: 2150: 2146: 2140: 2132: 2126: 2124: 2115: 2111: 2105: 2103: 2094: 2090: 2084: 2068: 2064: 2060: 2054: 2052: 2043: 2039: 2032: 2017: 2013: 2006: 2004: 1988: 1981: 1975: 1959: 1955: 1949: 1947: 1931: 1927: 1923: 1918: 1910: 1906: 1900: 1892: 1888: 1882: 1880: 1878: 1876: 1874: 1872: 1855: 1848: 1846: 1844: 1842: 1840: 1823: 1819: 1818: 1813: 1809: 1803: 1799: 1787: 1784: 1782: 1779: 1777: 1774: 1770: 1767: 1766: 1765: 1762: 1757: 1754: 1753: 1752: 1749: 1748: 1746: 1744: 1741: 1739: 1736: 1734: 1731: 1729: 1726: 1723: 1720: 1718: 1715: 1713: 1710: 1708: 1705: 1703: 1700: 1699: 1685: 1680: 1673: 1668: 1661: 1656: 1652: 1645: 1640: 1636: 1629: 1624: 1617: 1612: 1611: 1603: 1598: 1591: 1586: 1585: 1563: 1527: 1507: 1486: 1468: 1446: 1426: 1406: 1385: 1384: 1377: 1374: 1365: 1360: 1356: 1352: 1346: 1343:This section 1341: 1332: 1331: 1323: 1321: 1317: 1313: 1309: 1305: 1301: 1290: 1287: 1284: 1281: 1278: 1275: 1271: 1268: 1265: 1262: 1259: 1257: 1253: 1250: 1247: 1244: 1241: 1238: 1234: 1231: 1228: 1225: 1222: 1219: 1215: 1212: 1209: 1206: 1203: 1200: 1196: 1193: 1190: 1187: 1184: 1181: 1177: 1174: 1171: 1168: 1165: 1162: 1158: 1155: 1152: 1149: 1146: 1143: 1139: 1136: 1133: 1130: 1127: 1125: 1121: 1117: 1114: 1109: 1104: 1101: 1100: 1097: 1095: 1091: 1087: 1081: 1079: 1075: 1071: 1067: 1063: 1056: 1052: 1047: 1039: 1027: 1023: 1020: 1017: 1014: 1013: 1012: 1006: 1002: 998: 995: 992: 989: 986: 983: 982: 981: 978: 974: 966: 957: 953: 949: 945: 941: 939: 917:Science goals 914: 911: 907: 903: 901: 891: 882: 874: 870: 867: 857: 853: 849: 847: 842: 838: 830: 816: 813: 811: 801: 797: 795: 790: 781: 778: 774: 765: 762: 758: 756: 751: 749: 745: 740: 732: 723: 720: 718: 713: 711: 707: 698: 694: 692: 688: 683: 674: 670: 669:a telescope. 666: 664: 659: 651: 637: 635: 631: 627: 618: 609: 606: 602: 597: 595: 591: 587: 583: 579: 570: 561: 559: 554: 549: 541: 537: 533: 531: 527: 523: 519: 511: 506: 497: 495: 490: 484: 482: 478: 474: 469: 467: 463: 459: 455: 451: 448: 443: 441: 437: 433: 429: 425: 422: 421:near-infrared 418: 414: 410: 406: 395: 389: 386: 382: 376: 354: 345: 341: 336: 328: 324: 319: 313: 310: 306: 302: 297: 295: 291: 287: 282: 278: 273: 267: 265: 261: 257: 252: 248: 244: 239: 235: 231: 226: 222: 217: 211: 207: 203: 200: 196: 192: 180: 176: 172: 167: 163: 158: 152: 149: 145: 141: 135: 107: 103: 99: 95: 91: 88: 84: 79: 73: 70: 66: 62: 57: 53: 46: 41: 33: 19: 5919:Solar System 5669: 5649:Astrophysics 5628:Astrobiology 5553: 5292:Far-infrared 5246:Local system 5181:Astronomy by 5171:... in space 5064: 5051: 4979: 4967: 4879: 4850: 4824: 4777: 4694:XO Telescope 4644:Project 1640 4473:Ground-based 4355:Cerro Tololo 4335:Cerro Pachón 4305:Las Campanas 4225: 4151: 4135: 4123: 4098: 3964: 3960: 3791:. 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Index

E-ELT
extremely large telescope

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European Southern Observatory
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Cerro Armazones
Antofagasta Province
Antofagasta Region
24°35′21″S 70°11′30″W / 24.5893°S 70.1916°W / -24.5893; -70.1916
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European Southern Observatory
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extremely large telescope
infrared telescope
Nasmyth telescope
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Angular resolution
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Focal length
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dome
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elt.eso.org

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