An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy, climatology/meteorology, geophysics, oceanography and volcanology are examples of disciplines for which observatories have been constructed.[Udías, Agustín (2003). Searching the Heavens and the Earth, Kluwer Academic Publishers, p. 3.]
The term observatoire has been used in French since at least 1976 to denote any institution that compiles and presents data on a particular subject (such as public health observatory) or for a particular geographic area (European Audiovisual Observatory).
Astronomical observatories
Astronomical observatories are mainly divided into four categories: space-based, airborne, ground-based, and underground-based. Historically, ground-based observatories were as simple as containing a
mural instrument (for measuring the angle between
) or
Stonehenge (which has some alignments on astronomical phenomena).
Ground-based observatories
Ground-based observatories, located on the surface of Earth, are used to make observations in the
Radio frequency and visible light portions of the electromagnetic spectrum. Most optical telescopes are housed within a
dome or similar structure, to protect the delicate instruments from the elements. Telescope domes have a slit or other opening in the roof that can be opened during observing, and closed when the telescope is not in use. In most cases, the entire upper portion of the telescope dome can be rotated to allow the instrument to observe different sections of the night sky. Radio telescopes usually do not have domes.
For optical telescopes, most ground-based observatories are located far from major centers of population, to avoid the effects of light pollution. The ideal locations for modern observatories are sites that have dark skies, a large percentage of clear nights per year, dry air, and are at high elevations. At high elevations, the Earth's atmosphere is thinner, thereby minimizing the effects of atmospheric turbulence and resulting in better astronomical "seeing".[Leverington, David (2017) Observatories and Telescopes of Modern Times Cambridge Univ Press ][Meszaros, Stephen Paul (1986). World Atlas of Large Optical Telescopes, NASA TM 87775, p. 2.
]
Specific research study performed in 2009 shows that the best possible location for ground-based observatory on Earth is Ridge A—a place in the central part of Eastern Antarctica.
Solar observatories
Radio observatories
Beginning in 1933,
have been built for use in the field of
radio astronomy to observe the Universe in the radio portion of the electromagnetic spectrum. Such an instrument, or collection of instruments, with supporting facilities such as control centres, visitor housing, data reduction centers, and/or maintenance facilities are called
radio observatories. Radio observatories are similarly located far from major population centers to avoid electromagnetic interference (EMI) from
radio, TV,
radar, and other EMI emitting devices, but unlike optical observatories, radio observatories can be placed in
for further EMI shielding. Some of the world's major radio observatories include the Very Large Array in
New Mexico, United States,
Jodrell Bank in the
United Kingdom, Arecibo in
Puerto Rico, Parkes in New South Wales, Australia, and Chajnantor in
Chile. A related discipline is Very-long-baseline interferometry (VLBI).
Highest astronomical observatories
Since the mid-20th century, a number of astronomical observatories have been constructed at very
, above . The largest and most notable of these is the Mauna Kea Observatory, located near the summit of a volcano in Hawaiʻi. The Chacaltaya Astrophysical Observatory in Bolivia, at , was the world's highest permanent astronomical observatory
from the time of its construction during the 1940s until 2009. It has now been surpassed by the new University of Tokyo Atacama Observatory,
an optical-infrared telescope on a remote mountaintop in the
Atacama Desert of Chile.
Oldest astronomical observatories
The oldest proto-observatories, in the sense of an
observation post for astronomy,
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Wurdi Youang, Australia
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Zorats Karer, Karahunj, Armenia
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Loughcrew, Ireland
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Newgrange, Ireland
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Stonehenge, Great Britain
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Chankillo, Peru
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Chichen Itza, Mexico
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Buto, Egypt
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Abu Simbel, Egypt
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Kokino, Kumanovo, North Macedonia
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Hipparchus, Greece
[" Facts about Hipparchus: astronomical observatory, as discussed in astronomical observatory:". Encyclopædia Britannica.]
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Goseck circle, Germany
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Ujjain, India
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Arkaim, Russia
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Cheomseongdae, South Korea
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Angkor Wat, Cambodia
The oldest true observatories, in the sense of a specialized research institute,[Peter Barrett (2004), Science and Theology Since Copernicus: The Search for Understanding, p. 18, Continuum International Publishing Group, .]
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825: Al-Shammisiyyah Observatory, Baghdad, Iraq
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869: Sankaranarayana, Kerala, India
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1259: Maragheh Observatory, Azerbaijan, Iran
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1276: Gaocheng Astronomical Observatory, China
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1420: Ulugh Beg Observatory, Samarkand, Uzbekistan
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1442: Beijing Ancient Observatory, China
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1577: Constantinople Observatory of Taqi ad-Din, Turkey
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1580: Uraniborg, Denmark
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1581: Stjerneborg, Denmark
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1633: Leiden Observatory, Netherlands
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1642: Panzano Observatory, Italy
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1642: Round Tower, Denmark
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1667: Paris Observatory, France
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1675: Royal Greenwich Observatory, England
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1695: Sukharev Tower, Russia
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1711: Berlin Observatory, Germany
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1724: Jantar Mantar, India
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1753: Stockholm Observatory, Sweden
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1753: Vilnius University Observatory, Lithuania
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1753: Real Instituto y Observatorio de la Armada, Spain
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1759: Trieste Observatory, Italy.
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1757: Macfarlane Observatory, Scotland.
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1759: Turin Observatory, Italy.
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1764: Brera Astronomical Observatory, Italy.
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1765: Mohr Observatory, Indonesia.
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1771: Lviv Observatory, Ukraine.
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1774: Observatory of the Vatican, Italy.
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1785: Dunsink Observatory, Ireland.
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1786: Madras Observatory, India.
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1789: Armagh Observatory, Northern Ireland.
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1790: Royal Observatory of Madrid, Spain,
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1803: National Astronomical Observatory, Bogotá, Colombia.
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1811: Tartu Old Observatory, Estonia
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1812: Astronomical Observatory of Capodimonte, Naples, Italy
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1830/1842: Depot of Charts & Instruments/US Naval Observatory,
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1830: Yale University Observatory Atheneum, US
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1834: Helsinki University Observatory, Finland
[ History of astronomy at University of Helsinki 1834–1984 .]
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1838: Hopkins Observatory, Williams College, US
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1838: Loomis Observatory, Western Reserve Academy, US
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1839: Pulkovo Observatory, Russia
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1842: Cincinnati Observatory, US
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1844: Georgetown University Astronomical Observatory, US
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1847: Harvard College Observatory, US
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1854: Detroit Observatory, US
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1871: Argentine National Observatory, Argentina
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1873: Quito Astronomical Observatory, Ecuador
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1878: Lisbon Astronomical Observatory, Portugal
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1884: McCormick Observatory, US
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1888: Lick Observatory, US
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1890: Smithsonian Astrophysical Observatory, US
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1894: Lowell Observatory, US
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1895: Theodor Jacobsen Observatory, US
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1897: Yerkes Observatory, US
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1899: Kodaikanal Solar Observatory, India
Space-based observatories
Space-based observatories are telescopes or other instruments that are located in
outer space, many in
orbit around the Earth. Space telescopes can be used to observe astronomical objects at wavelengths of the electromagnetic spectrum that cannot penetrate the Earth's atmosphere and are thus impossible to observe using ground-based telescopes. The Earth's atmosphere is opaque to
ultraviolet radiation,
X-rays, and
gamma rays and is partially opaque to
infrared radiation so observations in these portions of the electromagnetic spectrum are best carried out from a location above the atmosphere of our planet.
Another advantage of space-based telescopes is that, because of their location above the Earth's atmosphere, their images are free from the effects of atmospheric turbulence that plague ground-based observations.
As a result, the angular resolution of space telescopes such as the Hubble Space Telescope is often much smaller than a ground-based telescope with a similar
aperture. However, all these advantages do come with a price. Space telescopes are much more expensive to build than ground-based telescopes. Due to their location, space telescopes are also extremely difficult to maintain. The Hubble Space Telescope was able to be serviced by the
while many other space telescopes cannot be serviced.
Airborne observatories
Airborne observatories have the advantage of height over ground installations, putting them above most of the Earth's atmosphere. They also have an advantage over space telescopes: The instruments can be deployed, repaired and updated much more quickly and inexpensively. The Kuiper Airborne Observatory and the Stratospheric Observatory for Infrared Astronomy use airplanes to observe in the
infrared, which is absorbed by
water vapor in the atmosphere. High-altitude balloons for X-ray astronomy have been used in a variety of countries.
Neutrino observatories
Example underground, underwater or under ice neutrino observatories include:
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1998–2003 GALLEX
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1999–2006 Sudbury Neutrino Observatory
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2003 Baikal Deep Underwater Neutrino Telescope
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2010 IceCube Neutrino Observatory
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2012 Helium and Lead Observatory (HALO)
Meteorological observatories
Example meteorological observatories include:
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1762 Kremsmünster Observatory, Austria
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1781 Hohenpeißenberg Meteorological Observatory, Germany
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1841 Colaba Observatory, India
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1868 Kandilli Observatory, Türkiye
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1869 Belvedere Castle in Central Park, New York
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1871 Argentine National Observatory, Argentina
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1883 Hong Kong Observatory, Hong Kong
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1885 Blue Hill Meteorological Observatory, Massachusetts
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1932 Mount Washington Observatory, New Hampshire
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1956 Mauna Loa Observatory, Hawaii
See also
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World Meteorological Organization
Marine observatories
A marine observatory is a scientific institution whose main task is to make observations in the fields of meteorology, geomagnetism and tides that are important for the navy and civil shipping. An astronomical observatory is usually also attached. Some of these observatories also deal with nautical weather forecasts and storm warnings, astronomical time services, nautical calendars and seismology.
Example marine observatories include:
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1676 Royal Greenwich Observatory at London
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1753 Real Instituto y Observatorio de la Armada in San Fernando, Spain
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1830 United States Naval Observatory
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1868 German Maritime Observatory in Hamburg
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1871–1918 Austro-Hungarian Pola Naval Observatory, in what is now Pula, Croatia
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1882 Observatoire Oceanologique de Villefranche, France
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1908 St. Andrews Biological Station, Canada
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2006 European Multidisciplinary Seafloor and water column Observatory (EMSO)
See also
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Fixed-point ocean observatory
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Integrated Ocean Observing System
Magnetic observatories
A magnetic observatory is a facility which precisely measures the total intensity of Earth's
magnetic field for field strength and direction at standard intervals. Geomagnetic observatories are most useful when located away from human activities to avoid disturbances of anthropogenic origin, and the observation data is collected at a fixed location continuously for decades. Magnetic observations are aggregated, processed, quality checked and made public through data centers such as INTERMAGNET.
[Gupta, Harsh (ed) (2021). Encyclopedia of Solid Earth Geophysics, Springer , p. 774.][ Principal Facts of the Earth's Magnetism U.S. Coast and Geodetic Survey, 1919 pp57-59]
The types of measuring equipment at an observatory may include (torsion, declination-inclination fluxgate, proton precession, Overhauser-effect), variometer (3-component vector, total-field scalar), dip circle, inclinometer, earth inductor, theodolite, self-recording magnetograph, magnetic declinometer, azimuth compass. Once a week at the absolute reference point calibration measurements are performed.[Jankowski, J. and Sucksdorff, C. (1996) IAGA Guide for Magnetic Measurements and Observatory Practice ]
Example magnetic observatories include:
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1833 Göttingen Observatory, Germany
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1840 Toronto Magnetic and Meteorological Observatory, Canada
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1842 Kew Observatory, UK
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1904 Eskdalemuir Observatory, UK
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1961 Boulder Geomagnetic Observatory, Colorado
Seismic observatories
Example seismic observation projects and observatories include:
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International Seismological Summary
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Lamont–Doherty Earth Observatory
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EarthScope
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GEOSCOPE Observatory
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World-Wide Standardized Seismograph Network
Geodetic observatories
Cosmic-ray observatories
Gravitational wave observatories
Example gravitational wave observatories include:
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LIGO
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European Gravitational Observatory
Wildlife observatories
Volcano observatories
A volcano observatory is an institution that conducts the monitoring of a
volcano as well as research in order to understand the potential impacts of active volcanism. Among the best known are the Hawaiian Volcano Observatory and the Vesuvius Observatory. Mobile volcano observatories exist with the
USGS VDAP (Volcano Disaster Assistance Program), to be deployed on demand. Each volcano observatory has a geographic area of responsibility it is assigned to whereby the observatory is tasked with spreading activity forecasts, analyzing potential volcanic activity threats and cooperating with communities in preparation for volcanic eruption.
See also
Further reading
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Aubin, David; Charlotte Bigg, and H. Otto Sibum, eds. The Heavens on Earth: Observatories and Astronomy in Nineteenth-Century Science and Culture (Duke University Press; 2010) 384 pages; Topics include astronomy as military science in Sweden, the Pulkovo Observatory in the Russia of Czar Nicholas I, and physics and the astronomical community in late 19th-century America.
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Brunier, Serge, et al. Great Observatories of the World (2005).
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Dick, Steven. Sky and Ocean Joined: The U.S. Naval Observatory 1830–2000 (2003).
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Gressot Julien and Jeanneret Romain, « Determining the right time, or the establishment of a culture of astronomical precision at Neuchâtel Observatory in the mid-19th century », Journal for the History of Astronomy, 53
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Leverington, David. Observatories and Telescopes of Modern Times – Ground-Based Optical and Radio Astronomy Facilities since 1945. Cambridge University Press, Cambridge 2017, .
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McCray, W. Patrick. Giant Telescopes: Astronomical Ambition and the Promise of Technology (2004); focuses on the Gemini Observatory.
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Sage, Leslie, and Gail Aschenbrenner. A Visitor's Guide to the Kitt Peak Observatories (2004).
External links
