The Giant Magellan Telescope (GMT) is a ground-based, extremely large telescope currently under construction at Las Campanas Observatory in Chile's Atacama Desert. With a primary mirror diameter of 25.4 meters, it is expected to be the largest Gregorian telescope ever built, observing in optical and mid-infrared wavelengths (320–25,000 nm). Commissioning of the telescope is anticipated in the early 2030s. The GMT will feature seven of the world's largest mirrors, collectively providing a light-collecting area of 368 square meters. It is expected to have a resolving power approximately 10 times greater than the Hubble Space Telescope and four times greater than the James Webb Space Telescope. However, it will not be able to observe in the same infrared frequencies as space-based telescopes. The GMT will be used to explore a wide range of astrophysical phenomena, including the search for signs of life on exoplanets and the study of the cosmic origins of chemical elements. The casting of the GMT's primary mirrors began in 2005, and construction at the site started in 2015. By 2023, all seven primary mirrors had been cast, the first of seven adaptive secondary mirrors was under construction, and the telescope mount was in the manufacturing stage. Other subsystems of the telescope were in the final stages of design. The project, with an estimated cost of US$2 billion, is being developed by the GMTO Corporation, a consortium of research institutions from seven countries: Australia, Brazil, Chile, Israel, South Korea, Taiwan, and the United States.
Site
The telescope is located at Las Campanas Observatory, which is also home to the Magellan Telescopes. The observatory is situated approximately 115 km (71 mi) north-northeast of La Serena, and 180 km (112 mi) south of Copiapó, at an altitude of 2,516 m (8,255 ft). The site has been owned by the Carnegie Institution for Science since 1960. Las Campanas was selected as the location for the GMT due to its exceptional astronomical seeing conditions and clear weather throughout much of the year. The sparse population in the surrounding Atacama Desert, combined with favorable geographical conditions, ensures minimal atmospheric and light pollution. This makes the area one of the best locations on Earth for long-term astronomical observation. The observatory's southern hemisphere location also provides access to significant astronomical targets, including the galactic center of the Milky Way, the nearest supermassive black hole (Sagittarius A*), the nearest star to the Sun (Proxima Centauri), the Magellanic Clouds, and numerous nearby galaxies and exoplanets.
Design and status
The Giant Magellan Telescope's Gregorian design will produce the highest possible image resolution of the universe over the widest field of view with only two light collecting surfaces, making it the most optically proficient of all extremely large telescopes in the 30-meter class.
Performance specifications
Site preparation began with the first blast to level the mountain peak on March 23, 2012. In November 2015, construction was started at the site, with a ground-breaking ceremony. In January 2018, WSP was awarded the contract to manage construction of the Giant Magellan Telescope. The casting of the first mirror, in a rotating furnace, was completed on November 3, 2005. A third segment was cast in August 2013, the fourth in September 2015, the fifth in 2017, the sixth in 2021, and the last in 2023. Polishing of the first mirror was completed in November 2012. Ingersoll Machine Tools finished constructing a manufacturing facility to manufacture the Giant Magellan Telescope mount in Rockford, Illinois, in December 2021. As of 2022, construction of the telescope mount was underway. The structure is expected to be delivered to Chile at the end of 2025.
Enclosure The Giant Magellan Telescope enclosure is a 65-metre-tall (213 ft) structure that shelters the telescope's mirrors and components from the extreme weather and earthquakes in the Atacama Desert, Chile. The 4,800-ton enclosure can complete a full rotation in a little more than three minutes and is designed with a closed-cycle forced-air convection system to maintain a thermal equilibrium within the telescope enclosure and reduce ambient thermal gradients across the primary mirror surface. The enclosure design provides the telescope pier with a seismic isolation system that can survive the strongest earthquakes expected over the 50-year lifetime of the observatory and will allow the telescope to quickly return to operations after the more frequent, but less intense seismic events that are experienced several times per month. In March 2022, engineering and architecture firm IDOM was awarded the contract to finalize the telescope's enclosure design by 2024.
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