| Aperture (meters) | Name | Location | Latitude; Longitude Altitude |
Comments |
|---|---|---|---|---|
| 10.0 | Keck | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4123 m |
mirror composed of 36 segments |
| Keck II | future optical interferometry! | |||
| ~10 | SALT | South African Astronomical Observatory | 32 23 S; 20 49 E; 1759 m | based on the HET design |
| 9.2 | Hobby-Eberly | Mt. Fowlkes, Texas | 30 40 N; 104 1 W 2072 m |
very inexpensive: spherical segmented mirror; fixed elevation; spectroscopy only |
| 8.4 | Large Binocular Telescope | Mt. Graham, Arizona | 32 42 N; 109 53 W 3170 m |
eventually will have a pair of 8.4-m mirrors giving the light gathering of an 11.8m and the resolution of a 23-m |
| 8.3 | Subaru | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4100 m |
NAOJ |
| 8.2 | Antu | Cerro Paranal, Chile | 24 38 S; 70 24 W 2635m |
now operate independently in the future will be units of Very Large Telescope |
| Kueyen | ||||
| Melipal | ||||
| Yepun | ||||
| 8.1 | Gillett | Mauna Kea, Hawaii | 1950 N; 155 28 W 4100 m |
aka Gemini North |
| Gemini South | Cerro Pachon, Chile | 30 20 S;70 59 W (approx) 2737 m |
twin of Gemini North | |
| 6.5 | MMT | Mt. Hopkins, Arizona | 31 41 N; 110 53 W 2600 m |
|
| Walter Baade | La Serena, Chile | 29 00.2 S; 4 42 48 W 2282 m |
aka Magellan I; Las Campanas Obs. | |
| Landon Clay | aka Magellan II | |||
| 6.0 | Bolshoi Teleskop Azimutalnyi | Nizhny Arkhyz, Russia | 43 39 N; 41 26 E 2070m |
Large Altazimuth Telescope |
| LZT | British Columbia, Canada | 49.28 N; 122.57 W 395m |
Liquid mirror, points only at the zenith; UBC | |
| 5.0 | Hale | Palomar Mountain, California | 33 21 N; 116 52 W 1900 m |
|
| 4.2 | William Herschel | La Palma, Canary Islands, Spain | 28 46 N; 17 53 W 2400 m |
Observatorio del Roque de los Muchachos |
| SOAR | Cerro Pachon, Chile | 70 44 W; 30 14 S 2738 m |
Brazil/USA; CTIO | |
| 4.0 | Victor Blanco | Cerro Tololo, Chile | 30 10 S;70 49 W 2200 m |
CTIO |
| 3.9 | Anglo-Australian | Coonabarabran, NSW, Australia | 31 17 S;149 04 E | Siding Spring Obs. |
| 3.8 | Mayall | Kitt Peak, Arizona | 31 57 N; 111 37 W 2100 m |
NOAO |
| UKIRT | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4200 m |
dedicated to infrared | |
| 3.7 | AEOS | Maui, Hawaii | 20 42 30 N; 156 15 29 W 3058 m |
mostly military |
| 3.6 | "360" | Cerro La Silla, Chile | 29 15 S; 70 44 W 2400 m |
European Southern Obs. |
| Canada-France-Hawaii | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4200 m |
||
| Telescopio Nazionale Galileo | La Palma, Canary Islands, Spain | 28 45 N; 17 53 W 2387 m |
Italian | |
| 3.5 | MPI-CAHA | Calar Alto, Spain | 37 13 N; 2 33 W 2200 m |
|
| New Technology | Cerro La Silla, Chile | 29 15 S; 70 44 W 2400 m |
European Southern Obs. | |
| ARC | Apache Point, New Mexico | 32 47 N; 105 49 W 2788 m |
mostly remote controlled | |
| WIYN | Kitt Peak, Arizona | 31 57 N; 111 37 W 2100 m |
Wisconsin, Indiana, Yale, NOAO | |
| Starfire | Kirtland AFB, New Mexico | 1900 m |
military | |
| 3.0 | Shane | Mount Hamilton, California | 37 21 N; 121 38 W 1300 m |
Lick Observatory |
| NASA IRTF | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4160 m |
infrared | |
| 2.7 | Harlan Smith | Mt. Locke, Texas | 30 40 N; 104 1 W 2100 m |
McDonald Obs.; see also |
| 2.6 | BAO | Byurakan, Armenia | 40 20N; 44 17 E 1405 m |
Byurakan Astrophysical Observatory |
| Shajn | Crimea, Ukraine | 44 44 N; 34 E 600 m |
Crimean Astrophysical Observatory | |
| 2.5 | Hooker | Mt. Wilson, California | 34 13N; 118 4 W 1700 m |
built in 1917 |
| Isaac Newton | La Palma, Canary Islands, Spain | 28 45 N; 17 53 W 2382 m |
Observatorio del Roque de los Muchachos | |
| Nordic Optical | ||||
| du Pont | La Serena, Chile | 29 00.2 S; 4 42 48 W 2282 m |
Las Campanas Obs. | |
| Sloan Digital Sky Survey | Apache Point, New Mexico | 32 47 N; 105 49 W 2788 m |
huge wide-field detector | |
| 2.45 | CHARA | Mt. Wilson, California | 34 13N; 118 4 W 1700 m |
interferometer using 6 1-m scopes |
| 2.4 | Hiltner | Kitt Peak, Arizona | 31 57 N; 111 37 W 2100 m |
MDM Observatory |
| Hubble Space Telescope | Low Earth orbit! | varies 600 km |
||
| 2.3 | WIRO | Jelm Mtn., Wyoming | 41 03 N; 106 00 W 2900 m |
infrared |
| ANU | Coonabarabran, NSW, Australia | 31 17 S;149 04 E | Siding Spring Obs. | |
| Bok | Kitt Peak, Arizona | 31 57 N; 111 37 W 2100 m |
Steward Obs. | |
| Vainu Bappu | Kavalur, India | 12 34 N; 78 50 E 700 m |
Indian Institude of Astrophysics | |
| 2.2 | ESO-MPI | Cerro La Silla, Chile | 29 15 S; 70 44 W 2335 m |
|
| MPI-CAHA | Calar Alto, Spain | 37 13 N; 2 33 W 2200 m |
||
| UH | Mauna Kea, Hawaii | 19 50 N; 155 28 W 4200 m |
2.1 Kitt Peak 2.1 McDonald (Struve) 2.1 INAOE, Puebla, Mexico 2.1 UNAM, San Pedro Martir, Mexico 2.1 El Leoncito, Argentina 2.0 Ondrejov, Czech Republic 2.0 Tusi Astronomical Obs., Shemakha, Azerbaijan 2.0 Hanle, India (a few hundred meters higher than Mauna Kea) 2.0 (Schmidt) Tautenburg Germany 2.0 Ukrainian Academy of Sciences, Terskel, Caucasus 2.0 MAGNUM (Haleakala, may still be in progress) 2.0 Lyot, Pic-du-Midi, France 2.0 Faulkes Telescope North 2.0 Faulkes Telescope South
| Aperture | Name | Location | Comments |
|---|---|---|---|
| 21.4 (7x8.4) | Giant Magellan Telescope | Chile? | six off-axis segments plus one central segment form one optical surface |
| 16.4 (4x8.2) | Very Large Telescope | Cerro Paranal, Chile | all four units now operational; will be combined as an interferometer |
| 14.6 (2x10) | Keck Interferometer | Mauna Kea, Hawaii | Keck I and II plus several small outrigger scopes |
| 10.4 | Gran Telescopio Canarias | La Palma, Canary Islands, Spain | segmented mirror based on Keck |
| 8 | LSST | Cerro Pachon, Chile | aka Dark Matter Telescope; a fast wide field survey scope |
| 4.2 | LAMOST | Xinglong Station, China | Beijing Astronomical Observatory |
| DCT | Happy Jack, Arizona | Lowell Observatory wide field telescope | |
| 4 | Vista | Cerro Paranal, Chile | wide field survey scope |
| 2.5 | SOFIA | stratosphere | airborne infrared |
| VST | Cerro Paranal, Chile | wide field survey scope | |
| 2.3 | Aristarchos | Mt. Helmos, Greece | National Observatory of Athens |
| 4x1.8 | Pan-STARRS | Hawaii | Four separate telescopes; optimized for surveys; cheaper than LSST |
| 2.4+10x1.4 | Magdalena Ridge Observatory | Socorro, New Mexico | one single scope plus 10 mirror interferometer |
| Aperture | Name | Comments |
|---|---|---|
| 100 | OWL | OverWhelmingly Large Telescope |
| 50 | Euro50 | |
| 42 | E-ELT | European Extremely Large Telescope |
| 30-50 | MaxAT | |
| ~40 | LAMA | array of liquid mirrors |
| 30 | TMT | Thirty Meter Telescope (was CELT, VLOT, GSMT) |
| Others | ||
| Aperture | Name | Location | Comments |
|---|---|---|---|
| 42 | LAMA | Chile | liquid mirror array |
| 25 | Cornell Atacama Telescope | Atacama, Chile | optimized for far IR, next to ALMA |
| 6.5 | JWST | L2 Halo orbit | aka NGST; cost reduced from initial 8m plans |
| 4 | ATST | Haleakala, Hawaii | Advanced Technology Solar Telescope |
| 2.5 | The MLO 100 inch | Mt. Laguna, CA | |
| 2.0 | Indian Astronomical Observatory | Hanle, India | 4500m altitude |
| 1.86 | Dominion Astrophysical Observatory | Victoria, Canada | was once (briefly) the largest telescope in the world |
| 1.8 | The Leviathan of Parsonstown | Birr, Ireland | Lord Rosse's famous scope restored |
| 1.5 | Hexapod Telescope | La Silla | unique mount utilizing 6 hydraulic "legs" |
| 1.2 | Samuel Oschin Telescope | Palomar Mountain, California | found the "tenth planet" |
| 1 | Yerkes Observatory | Williams Bay, Wisconsin | world's largest refractor |