Since Galileo (1564-1642) and his 37 mm telescope in 1609, ground-based telescopes have continued to grow in size to collect more light. The performance of an optical telescope depends mainly on the diameter of its primary mirror, which determines its ability to capture light and resolve fine details of distant objects. The largest current instruments, such as the Gran Telescopio Canarias (GTC) or the Very Large Telescopes (VLT), use segmented or coupled mirrors to achieve impressive diameters.
Mechanical and thermal constraints limit the manufacture of monolithic mirrors beyond 8 meters. Modern telescopes therefore adopt segmented mirrors controlled by actuators to maintain a perfect optical surface. The future Extremely Large Telescope (ELT) of the ESO in Chile will embody the pinnacle of this technology with a 39.3-meter mirror composed of 798 hexagonal segments. The table below lists the 20 largest ground-based optical telescopes in operation or under construction, ranked by equivalent diameter of the primary mirror.
Rank | Name | Location | Country | Diameter (m) | Year | Type |
---|---|---|---|---|---|---|
1 | ELT | Cerro Armazones | Chile | 39.3 | 2028 | Segmented |
2 | TMT | Mauna Kea | United States | 30.0 | ~2030 | Segmented |
3 | GMT | Cerro Las Campanas | Chile | 25.4 | ~2029 | Segmented |
4 | GTC | La Palma | Spain | 10.4 | 2009 | Segmented |
5 | Keck I | Mauna Kea | United States | 10.0 | 1993 | Segmented |
6 | Keck II | Mauna Kea | United States | 10.0 | 1996 | Segmented |
7 | SALT | South Africa | RSA | 9.2 | 2005 | Segmented |
8 | VLT UT1 to UT4 | Cerro Paranal | Chile | 8.2 | 1998–2001 | Monolithic |
9 | Subaru | Mauna Kea | Japan | 8.2 | 1999 | Monolithic |
10 | Gemini North | Mauna Kea | United States | 8.1 | 1999 | Monolithic |
11 | Gemini South | Cerro Pachón | Chile | 8.1 | 2000 | Monolithic |
12 | LBT | Mount Graham | United States | 8.4×2 | 2004 | Double mirror |
13 | Magellan I & II | Cerro Las Campanas | Chile | 6.5 | 2000 | Monolithic |
14 | MMT | Arizona | United States | 6.5 | 2000 | Monolithic |
15 | Palomar Hale | California | United States | 5.1 | 1948 | Monolithic |
16 | Baade | Cerro Las Campanas | Chile | 6.5 | 2002 | Monolithic |
17 | Hooker | Mount Wilson | United States | 2.5 | 1917 | Monolithic |
18 | ESO 3.6 | La Silla | Chile | 3.6 | 1976 | Monolithic |
19 | Canada-France-Hawaii | Mauna Kea | Canada/France | 3.6 | 1979 | Monolithic |
20 | Anglo-Australian | Siding Spring | Australia | 3.9 | 1974 | Monolithic |
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