Difference between revisions of "Observatory" - New World Encyclopedia

From New World Encyclopedia
(→‎External links: Checked links, added Retrieved dates.)
Line 13: Line 13:
 
====Optical observatories====
 
====Optical observatories====
  
For optical telescopes, most ground-based observatories are located far from major centers of population in order 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 "[[astronomical seeing|seeing]]".<ref>{{cite book
+
For optical telescopes, most ground-based observatories are located far from major centers of population in order 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 "[[astronomical seeing|seeing]]".<ref name=Chaisson>Chaisson, Eric and Steve McMillan. 2002. ''Astronomy Today''. Upper Saddle River, NJ: Prentice Hall. ISBN 0130935603 V1, 0130935719 V2.</ref> Sites that meet the above criteria for modern observatories include the [[southwestern United States]], [[Hawaii]], the [[Andes Mountains]], and [[Australia]].<ref name=Chaisson/> Major optical observatories include [[Mauna Kea Observatory|Mauna Kea]], HI, USA, [[Roque de los Muchachos Observatory]] in the [[Canary Islands]], [[Paranal Observatory]] in [[Chile]] and [[Kitt Peak]] observatory in the USA. The largest observatory in the equatorial belt is [[Observatorio Nacional de Llano del Hato]] in [[Venezuela]].
  | last = Chaisson| first = Eric| coauthors = McMillan, Steve| title = Astronomy Today, Fourth Edition| pages = 116-119|publisher = [[Prentice Hall]]| date = 2002}}</ref> Sites that meet the above criteria for modern observatories include the [[southwestern United States]], [[Hawaii]], the [[Andes Mountains]], and [[Australia]].<ref>{{cite book
 
  | last = Chaisson| first = Eric| coauthors = McMillan, Steve| title = Astronomy Today, Fourth Edition| pages = 119|publisher = [[Prentice Hall]]| date = 2002}}</ref> Major optical observatories include [[Mauna Kea Observatory|Mauna Kea]], HI, USA, [[Roque de los Muchachos Observatory]] in the [[Canary Islands]], [[Paranal Observatory]] in [[Chile]] and [[Kitt Peak]] observatory in the USA. The largest observatory in the equatorial belt is [[Observatorio Nacional de Llano del Hato]] in [[Venezuela]].
 
  
 
====Radio observatories====
 
====Radio observatories====
Line 25: Line 23:
 
[[Image:Hubble 01.jpg|thumb|200px|right|The [[Hubble Space Telescope]], a space-based observatory.]]
 
[[Image:Hubble 01.jpg|thumb|200px|right|The [[Hubble Space Telescope]], a space-based observatory.]]
  
Space-based observatories are telescopes or other instruments that are located in [[outer space]], many in [[orbit]] around the Earth. Space-based observatories 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 [[Opacity (optics)|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.<ref>{{cite book
+
Space-based observatories are telescopes or other instruments that are located in [[outer space]], many in [[orbit]] around the Earth. Space-based observatories 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 [[Opacity (optics)|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.<ref name=Chaisson/> 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.<ref>[http://history.nasa.gov/hubble/index.html A Brief History of the Hubble Space Telescope: Why a Space Telescope?] NASA. Retrieved December 7, 2007.</ref> 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 can be serviced by the [[Space Shuttle]] while many other space telescopes can not be serviced at all.<ref>[http://amazing-space.stsci.edu/resources/explorations/groundup/lesson/eras/space/page3.php A  Era of Space Telescopes]. Space Telescope Science Institute. Retrieved December 7, 2007.</ref>
  | last = Chaisson| first = Eric| coauthors = McMillan, Steve| title = Astronomy Today, Fourth Edition| publisher = [[Prentice Hall]]| date = 2002}}</ref> 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.<ref>{{cite web|publisher=NASA|url=http://history.nasa.gov/hubble/index.html|title=A Brief History of the Hubble Space Telescope: Why a Space Telescope?|accessdate=2006-08-14}}</ref> 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 can be serviced by the [[Space Shuttle]] while many other space telescopes can not be serviced at all.<ref>{{cite web|publisher=Space Telescope Science Institute|url=http://amazing-space.stsci.edu/resources/explorations/groundup/lesson/eras/space/page3.php|title=A  Era of Space Telescopes|accessdate=2006-09-14}}</ref>
 
  
 
===Oldest astronomical observatories===
 
===Oldest astronomical observatories===
Line 65: Line 62:
  
 
== References ==
 
== References ==
 +
* Brunier, Serge, Anne-Marie Lagrange, and Catherine Cesarsky. 2005. ''Great Observatories of the World''. Buffalo, NY: Firefly Books. ISBN 1554070554.
 +
* Rieke, George H. 2006. ''The last of the great observatories : Spitzer and the era of faster, better, cheaper at NASA''. Tucson, AZ: University of Arizona Press. ISBN 0816525226.
 +
* Zirker, J.B. 2005. ''An Acre of Glass: A History and Forecast of the Telescope''. Baltimore, MD: Johns Hopkins University Press. ISBN 0801882346.
  
 
==External links==
 
==External links==
  
*[http://www.library.northwestern.edu/archives/findingaids/dearborn.pdf Dearborn Observatory Records, Northwestern University Archives, Evanston, Illinois]
+
*[http://www.library.northwestern.edu/archives/findingaids/dearborn.pdf Dearborn Observatory Records, Northwestern University Archives, Evanston, Illinois]. Retrieved December 7, 2007.
*[http://www.eso.org/~ndelmott/obs_sites.html Coordinates and satellite images of astronomical observatories on Earth]
+
*[http://www.eso.org/~ndelmott/obs_sites.html Coordinates and satellite images of astronomical observatories on Earth]. Retrieved December 7, 2007.
*[http://solarsystem.nasa.gov/missions/profile.cfm?MCode=EbO Earth-based Observatories Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]
+
*[http://solarsystem.nasa.gov/missions/profile.cfm?MCode=EbO Earth-based Observatories Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]. Retrieved December 7, 2007.
*[http://www.whoi.edu/sbl/liteSite.do?litesiteid=7732&articleId=11729 Ocean Observatory Information],  [[Woods Hole Oceanographic Institution]]
+
*[http://www.whoi.edu/sbl/liteSite.do?litesiteid=7732&articleId=11729 Ocean Observatory Information]. Woods Hole Oceanographic Institution. Retrieved December 7, 2007.
*[http://www.whoi.edu/institutes/occi/viewTopic.do?o=read&id=541 Climate Change Observing Systems Information from the Ocean & Climate Change Institute], [[Woods Hole Oceanographic Institution]]
+
*[http://www.whoi.edu/institutes/occi/viewTopic.do?o=read&id=541 Climate Change Observing Systems Information from the Ocean & Climate Change Institute]. Woods Hole Oceanographic Institution. Retrieved December 7, 2007.
*[http://www.observatory-guide.org/ Milkyweb Astronomical Observatory Guide] worlds largest database of astronomical observatories since 2001 - about 2000 entries
+
*[http://www.observatory-guide.org/ Milkyweb Astronomical Observatory Guide]. Worlds largest database of astronomical observatories since 2001 - about 2000 entries. Retrieved December 7, 2007.
*[http://www.whoi.edu/institutes/coi/viewTopic.do?o=read&id=365 Coastal Observatory Information from the Coastal Ocean Institute], [[Woods Hole Oceanographic Institution]]
+
*[http://www.whoi.edu/institutes/coi/viewTopic.do?o=read&id=365 Coastal Observatory Information from the Coastal Ocean Institute]. Woods Hole Oceanographic Institution. Retrieved December 7, 2007.
*[http://www.platial.com/hundredflowers/map/3555#Planetaria_and_Observatories Map: Planetaria and Observatories]
+
*[http://www.platial.com/hundredflowers/map/3555#Planetaria_and_Observatories Map: Planetaria and Observatories]. Retrieved December 7, 2007.
 
+
*[http://cleardarksky.com/cgi-bin/find_clock.py?keys=%22%5C%28observatoire%5C%7Cobservatory%5C%7Cobservatories%5C%29%22&type=text&doit=Find List of amateur and professional observatories in North America with custom weather forecasts]. Retrieved December 7, 2007.
*[http://cleardarksky.com/cgi-bin/find_clock.py?keys=%22%5C%28observatoire%5C%7Cobservatory%5C%7Cobservatories%5C%29%22&type=text&doit=Find List of amateur and professional observatories in North America with custom weather forecasts]
+
* [http://vulcan.wr.usgs.gov/Vhp/framework.html USGS volcano observatories]. Retrieved December 7, 2007.
 
+
* [http://www.wovo.org World Organization of Volcano Observatories]. Retrieved December 7, 2007.
* [http://vulcan.wr.usgs.gov/Vhp/framework.html USGS volcano observatories]
+
* [http://www.wovo.org/dir-contents.htm directory of volcano observatories]. Retrieved December 7, 2007.
* [http://www.wovo.org World Organization of Volcano Observatories]
+
* [http://www.ov.ingv.it/index_eng.htm Osservatorio Vesuviano]. Retrieved December 7, 2007.
* [http://www.wovo.org/dir-contents.htm directory of volcano observatories]
 
* [http://www.ov.ingv.it/index_eng.htm Osservatorio Vesuviano]
 
  
 
[[Category:Physical sciences]]
 
[[Category:Physical sciences]]

Revision as of 21:24, 7 December 2007

This article is about scientific observatories.
File:DSCF2941.JPG
Molėtai Astronomical Observatory in Lithuania.

An observatory is a location used for observing terrestrial and/or celestial events. Astronomy, climatology/meteorology, geology, oceanography and volcanology are examples of disciplines for which observatories have been constructed. Historically, observatories were as simple as containing an astronomical sextant (for measuring the distance between stars) or Stonehenge (which has some alignments on astronomical phenomena).

Astronomical observatories

Ground-based observatories

Paranal Observatory, home of the Very Large Telescope, a cluster of four large (8.2 meter diameter) telescopes.

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 other similar structure to protect the delicate instruments from the elements. Telescope domes contain a slat or other opening in the roof that can be opened during observing and then closed when the telescope is not in use. In most cases, the entire upper portion of the telescope dome can be rotated in order to allow the instrument to observe different sections of the night sky. Radio telescopes usually do not have domes.

Optical observatories

For optical telescopes, most ground-based observatories are located far from major centers of population in order 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".[1] Sites that meet the above criteria for modern observatories include the southwestern United States, Hawaii, the Andes Mountains, and Australia.[1] Major optical observatories include Mauna Kea, HI, USA, Roque de los Muchachos Observatory in the Canary Islands, Paranal Observatory in Chile and Kitt Peak observatory in the USA. The largest observatory in the equatorial belt is Observatorio Nacional de Llano del Hato in Venezuela.

Radio observatories

Beginning in the 1930s, radio telescopes have been built for use in the field of radio astronomy. Such an instrument, or a collection of them, with outbuildings for such things as control centers, data reduction centers, and maintenance are called radio observatories. Radio observatories are similarly located far from major centers of population in order to avoid electromagnetic interference (EMI) from radio, TV, radar, and other EMI emitting devices. But unlike optical observatories, radio observatories will be placed in valleys to further shield them from EMI. Some of the major radio observatories are at Socorro, in New Mexico, USA, Jodrell Bank in the UK, Arecibo, Puerto Rico and Parkes in New South Wales, Australia.

Space-based observatories

Main article: Space observatory
The Hubble Space Telescope, a space-based observatory.

Space-based observatories are telescopes or other instruments that are located in outer space, many in orbit around the Earth. Space-based observatories 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.[1] 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.[2] 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 can be serviced by the Space Shuttle while many other space telescopes can not be serviced at all.[3]

Oldest astronomical observatories

Far East's oldest astrological observatory constructed between 632 - 646 in Cheomseongdae

Some of the oldest observatories include:

Volcano observatories

A volcano observatory is an institution that conducts research and monitoring of a volcano. Each observatory provides continuous and periodic monitoring of the seismicity, other geophysical changes, ground movements, volcanic gas chemistry, and hydrologic conditions and activity between and during eruptions. They also provide a detailed record of eruptions in progress. These observations serve to characterize eruptive behavior, identify the nature of precursory activity leading to eruption, define the processes by which different types of deposits are emplaced, and specify the hazards that could be unleashed by each kind of eruption. From direct observation of precursory signs, it is possible to anticipate eruptions.

In times of volcanic unrest, observatories issue warnings and recommendations - they take on an advisory role for decision-making governmental civil defense agencies (FEMA in the U.S.) and ideally continue producing observational data.

Mobile volcano observatories exist with the USGS VDAP (Volcano Disaster Assistance Program), to be deployed on demand.

Underlying all observatory operations is an ongoing program of fundamental research in volcanic processes, supplemented by collaborative studies with universities, government agencies (in the U.S. for instance with other USGS centers, and NOAA), industry and NGOs. Such research typically includes direct interpretation of the monitoring and eruption data, and it leads to formulation of conceptual models that can be tested by theoretical or laboratory simulations of volcanic systems. Almost all observatories are members of the World Organization of Volcano Observatories (WOVO). The oldest volcano observatory is the Osservatorio Vesuviano (founded 1841) in Naples, now a member of the Italian government agency INGV.

See also

Notes

  1. 1.0 1.1 1.2 Chaisson, Eric and Steve McMillan. 2002. Astronomy Today. Upper Saddle River, NJ: Prentice Hall. ISBN 0130935603 V1, 0130935719 V2.
  2. A Brief History of the Hubble Space Telescope: Why a Space Telescope? NASA. Retrieved December 7, 2007.
  3. A Era of Space Telescopes. Space Telescope Science Institute. Retrieved December 7, 2007.

References
ISBN links support NWE through referral fees

  • Brunier, Serge, Anne-Marie Lagrange, and Catherine Cesarsky. 2005. Great Observatories of the World. Buffalo, NY: Firefly Books. ISBN 1554070554.
  • Rieke, George H. 2006. The last of the great observatories : Spitzer and the era of faster, better, cheaper at NASA. Tucson, AZ: University of Arizona Press. ISBN 0816525226.
  • Zirker, J.B. 2005. An Acre of Glass: A History and Forecast of the Telescope. Baltimore, MD: Johns Hopkins University Press. ISBN 0801882346.

External links

Credits

New World Encyclopedia writers and editors rewrote and completed the Wikipedia article in accordance with New World Encyclopedia standards. This article abides by terms of the Creative Commons CC-by-sa 3.0 License (CC-by-sa), which may be used and disseminated with proper attribution. Credit is due under the terms of this license that can reference both the New World Encyclopedia contributors and the selfless volunteer contributors of the Wikimedia Foundation. To cite this article click here for a list of acceptable citing formats.The history of earlier contributions by wikipedians is accessible to researchers here:

The history of this article since it was imported to New World Encyclopedia:

Note: Some restrictions may apply to use of individual images which are separately licensed.