List of highest astronomical observatories
This is a list of the highest astronomical observatories in the world, considering only ground-based observatories and ordered by elevation above mean sea level. The main list includes only permanent observatories with facilities constructed at a fixed location, followed by a supplementary list for temporary observatories such as transportable telescopes or instrument packages. For large observatories with numerous telescopes at a single location, only a single entry is included listing the main elevation of the observatory or of the highest operational instrument if that information is available.
History of high altitude astronomical observatories
Prior to the late 19th century, almost all astronomical observatories throughout history were located at modest elevations, often close to cities and educational institutions for the simple reason of convenience. As air pollution from industrialization and light pollution from artificial lighting increased during the Industrial Revolution, astronomers sought observatory sites in remote locations with clear and dark skies, naturally drawing them towards the mountains. The first permanent mountaintop astronomical observatory was the Lick Observatory constructed from 1876 to 1887, at the modest elevation of atop Mount Hamilton in California. The first high altitude observatory was constructed atop the Pic du Midi de Bigorre in the French Pyrenees starting in 1878, with its first telescope and dome installed in 1904. Astronomical observations were also made from Mont Blanc in the late 1800s.A few other high altitude observatories were constructed through the first half of the 20th century. However, the two most important and prominent of the early 20th century observatories, Mount Wilson Observatory and Palomar Observatory, were both located on mid-elevation mountaintops of about in southern California. The stunning successes and discoveries made there using the world's largest telescopes, the 100-inch Hooker Telescope and 200-inch Hale Telescope, spurred the move to ever higher sites for the new generation of observatories and telescopes after World War II, along with a worldwide search for locations which had the best astronomical seeing.
Since the mid-20th century, an increasing number of high altitude observatory sites have been developed at locations around the world, including numerous sites in Arizona, Hawaii, Chile, and the Canary Islands. The initial wave of high-altitude sites were mostly in the range, but astronomers soon sought even higher sites above. Among the largest, best developed, and most renowned of these high altitude sites is the Mauna Kea Observatory located near the summit of a volcano in Hawaii, which has grown to include over a dozen major telescopes during the four decades since it was founded. In the first decade of the 21st century, there has been a new wave of observatory construction at very high altitudes above, with such observatories constructed in India, Mexico, and most notably the Atacama Desert in northern Chile, now the site of several of the world's highest observatories. The scientific benefits of these sites outweigh the numerous logistical and physiological challenges which must be overcome during the construction and operation of observatories in remote mountain locations, even in desert, polar, and tropical island sites which magnify the challenges but confer additional observational advantages.
Sites at high altitude are ideal for optical astronomy and provide optimal seeing, being above a significant portion of the Earth's atmosphere with its associated weather, turbulence, and diminished clarity. In particular, sites on mountaintops within about of the ocean often have excellent observing conditions above a stable inversion layer throughout much of the year. High altitude sites are also above most of atmosphere's water vapor, making them ideal for infrared astronomy and submillimeter astronomy as those wavelengths are strongly absorbed by water vapor. On the other hand, high altitude does not offer as significant an advantage for radio astronomy at longer wavelengths, so relatively few radio telescopes are located at such sites. At the far end of the spectrum, for the extremely short wavelengths of x-ray and gamma ray astronomy, along with high-energy cosmic rays, high altitude observations once again offers significant advantages, enough that many experiments at these wavelengths have been conducted by balloon-borne or even by space telescopes, although a number of high-altitude ground-based sites have also been used. These include the Chacaltaya Astrophysical Observatory in Bolivia, which at was the world's highest permanent astronomical observatory from the time of its construction during the 1940s until surpassed in 2009 by the new University of Tokyo Atacama Observatory, an optical-infrared telescope on a remote mountaintop in Chile.
Highest permanent observatories
Permanent observatories above 3,000 m:Observatory Name | Elevation | Observatory Site | Location | Coordinates | Established | Type of Observatory | Major Instruments |
University of Tokyo Atacama Observatory | Cerro Chajnantor | Atacama Desert, Chile | 2009 | Optical, infrared | |||
Chacaltaya Astrophysical Observatory | Chacaltaya | Andes, Bolivia | 1946 | Cosmic ray, gamma ray | |||
James Ax Observatory | Cerro Toco | Atacama Desert, Chile | 2011 | Microwave | POLARBEAR | ||
Atacama Cosmology Telescope | Cerro Toco | Atacama Desert, Chile | 2007 | Microwave | |||
Llano de Chajnantor Observatory | Llano de Chajnantor | Atacama Desert, Chile | 1999 | Millimeter wave, submillimeter | ALMA, APEX, QUIET | ||
Shiquanhe Observatory | Shiquanhe, Ngari Plateau | Tibet Autonomous Region, China | 2011 | Optical | - | ||
Large Latin American Millimeter Array | Alto de Chorillos | Salta, Argentina | Under Construction | Submillimeter | LLAMA, | ||
Llano de Chajnantor Observatory | Pampa La Bola | Atacama Desert, Chile | 2002 | Submillimeter | ASTE, NANTEN2 | ||
Large Millimeter Telescope Alfonso Serrano | Sierra Negra | Puebla, Mexico | 2006 | Microwave | |||
Indian Astronomical Observatory | Mount Saraswati | Hanle, Ladakh, India | 2001 | Infrared, gamma ray, Optical | Himalayan Chandra Telescope, HAGAR | ||
Meyer-Womble Observatory | Mount Evans | Colorado, United States | 1996 | Optical, Infrared | |||
Yangbajing International Cosmic Ray Observatory | Yangbajain | Tibet Autonomous Region, China | 1990 | Cosmic ray | |||
Mauna Kea Observatory | Mauna Kea | Hawaii, United States | 1967 | Optical, infrared, submillimeter | Keck, UKIRT, Gemini North, Subaru, JCMT, CSO, SMA, CFHT | ||
High Altitude Water Cherenkov Gamma-Ray Observatory | Sierra Negra | Puebla, Mexico | 2013 | Gamma ray | |||
Barcroft Observatory | White Mountain Peak | California, United States | 1976 | Infrared, millimeter wave | |||
Very Long Baseline Array, Mauna Kea Site | Mauna Kea | Hawaii, United States | 1986 | Radio telescope | |||
Llano del Hato National Astronomical Observatory | Llano del Hato | Andes, Venezuela | 1970s | Optical telescope | 1-m Askania Schmidt camera, a 65-cm Zeiss refractor, a 1-m Zeiss reflector and a 50-cm Askania double astrograph | ||
Iranian National Observatory | Mount Gargash | Isfahan, Iran | 2010s | Optical telescope | Under Construction | ||
Sphinx Observatory | Jungfraujoch | Bernese Alps, Switzerland | 1937 | Optical telescope | |||
Mauna Loa Observatory | Mauna Loa | Hawaii, United States | 1957 | Optical, millimeter wave | Mauna Loa Solar Observatory, AMiBA | ||
Magdalena Ridge Observatory | South Baldy | New Mexico, United States | 1999 | Optical, infrared | |||
Mount Graham International Observatory | Mount Graham | Arizona, United States | 1993 | Optical, submillimeter | LBT, HHST, VATT | ||
Gornergrat Observatory | Gornergrat | Pennine Alps, Switzerland | 1967 | Infrared, submillimeter | Gornergrat Infrared Telescope, KOSMA | ||
Peak Terskol Observatory | Peak Terskol | North Caucasus, Russia | 1980 | Optical | |||
European Extremely Large Telescope | Cerro Armazones | Atacama Desert, Chile | Not completed | Optical, near infrared | |||
Haleakala Observatory | Haleakala | Hawaii, United States | 1964 | Optical, millimeter wave | Pan-STARRS, LCOGT Faulkes Telescope North, AEOS | ||
Notre Dame University-Louaiz Observatory | Mount Lebanon | Peak Al-Znanir, Lebanon | Not completed | Optical telescope | Under Construction |
Highest temporary observatories
Temporary observatories above 3,000 m:Observatory Name | Elevation | Observatory Site | Location | Coordinates | Established | Type of Observatory | Major Instruments |
Receiver Lab Telescope | Cerro Sairecabur | Atacama Desert, Chile | 2002 | Submillimeter, 1–2 THz | |||
PLATO | Dome A | East Antarctic Ice Sheet, Antarctica | 2008 | Optical, submillimeter | |||
Concordia Station | Dome C | East Antarctic Ice Sheet, Antarctica | 2005 | Optical, infrared, submillimeter |
Other important high altitude observatories
This is a selected list of the most important and notable high altitude observatories between 1700 and 3000 m; it is not intended to list all of the numerous observatories worldwide in this elevation range:Observatory Name | Elevation | Observatory Site | Location | Coordinates | Established | Type of Observatory | Major Instruments |
Sierra Nevada Observatory | Sierra Nevada | Granada, Spain | 1981 | Optical | |||
Pic du Midi Observatory | Pic du Midi de Bigorre | Pyrenees, France | 1878 | Optical, solar | |||
Amundsen-Scott South Pole Station / Martin A. Pomerantz Observatory | South Pole | East Antarctic Ice Sheet, Antarctica | 1994 | Microwave, millimeter, neutrino, submillimeter | SPT, AMANDA, IceCube, QUaD | ||
Cerro Armazones Observatory | Cerro Armazones | Atacama Desert, Chile | 1995 | Optical telescope | Hexapod-Telescope | ||
National Astronomical Observatory | Sierra de San Pedro Mártir | Baja California, Mexico | 1967 | Optical telescope | |||
Apache Point Observatory | Sacramento Peak | New Mexico, United States | 1984 | Optical, solar | SDSS, Dunn Solar Telescope | ||
Cerro Pachón | Cerro Pachón | Atacama Desert, Chile | 2000 | Optical, infrared | Gemini South, SOAR | ||
National Astronomical Observatory | Metropolitan Area of Bogotá | Bogotá, Colombia | 1803 | Optical telescope | |||
Paranal Observatory | Cerro Paranal | Atacama Desert, Chile | 1999 | Optical, infrared | VLT, VISTA | ||
Fred Lawrence Whipple Observatory | Mount Hopkins | Arizona, United States | 1966 | Optical, gamma ray | MMT, VERITAS | ||
Roque de los Muchachos Observatory | Roque de los Muchachos | La Palma, Canary Islands | 1979 | Optical, infrared, solar, gamma ray | MAGIC, GTC, WHT, TNG, NOT, INT | ||
Teide Observatory | Pico del Teide | Tenerife, Canary Islands | 1964 | Optical, solar, microwave | VTT, BRT, OGS, VSA | ||
La Silla Observatory | La Silla | Atacama Desert, Chile | 1969 | Optical telescope | NTT, ESO | ||
Las Campanas Observatory | Cerro Las Campanas | Atacama Desert, Chile | 1971 | Optical telescope | Magellan Telescopes, GMT | ||
Lowell Observatory | Flagstaff | Arizona, United States | 1894 | Optical telescope | |||
Cerro Tololo Inter-American Observatory | Cerro Tololo | Atacama Desert, Chile | 1967 | Optical telescope | Victor M. Blanco Telescope | ||
Calar Alto Observatory | Calar Alto | Almería, Spain | 1975 | Optical telescope | |||
Very Large Array | Plains of San Agustin | New Mexico, United States | 1975 | Radio telescope | |||
Kitt Peak National Observatory | Kitt Peak | Arizona, United States | 1960 | Optical, solar, radio telescope | Mayall, WIYN, McMath-Pierce, VLBA | ||
Special Astrophysical Observatory of the Russian Academy of Science | Mount Pastukhov | Caucasus Mountains, Russia | 1966 | Optical telescope | BTA-6 | ||
Yunnan Astronomical Observatory | rural Kunming, Yunnan, China | rural Kunming, Yunnan, China | 1972 | Optical telescope, Radio, Solar, Infrared | Lijiang 2.4m telescope, Fuxian Lake 1m solar tower, ynao 1m telescope, 10m radio telescope. | ||
Mount Wilson Observatory | Mount Wilson | California, United States | 1908 | Optical, solar | Hale Telescope, Hooker Telescope | ||
Palomar Observatory | Palomar Mountain | California, United States | 1936 | Optical telescope | Hale Telescope, Samuel Oschin telescope |