Square Kilometre Array
Information about Square Kilometre Array
The Square Kilometre Array (SKA) is a proposed radio telescope which is intended to have a collecting area of approximately one square kilometre.[1] It is planned to operate at frequencies of 0.10–25 GHz, with a goal of 0.06–35 GHz, and its size will make it 50 times more sensitive than current instruments. It may incorporate multiple independent fields of view, allowing several radio astronomers to observe at once, or to look at different areas of the sky simultaneously. The SKA will create images of distant radio sources using aperture synthesis. Construction of the SKA is scheduled to begin in 2010, with initial observations in 2015. It is intended to be fully operational by 2020. It will easily be the most sensitive radio instrument ever conceived, being able to detect every active galactic nucleus (AGN) out to a redshift of 6, when the universe was less than 1 billion years old. It will have the sensitivity to detect Earth-like radio leakage at a distance of several hundred to a few thousand light years.
Design
An international consortium is working on the telescope design, to be decided in 2008. The interferometric array is expected to be composed of many elements spread over an area of several thousand kilometres. The reference design calls for a compact core of elements containing about 20% of the collecting area within a 1km-diameter region, 50% of the collecting area within an area 5 km across, 75% of the collecting area within 150 km, and the remaining elements spread up to a few thousand kilometres away.Location
The final decision on the site will be made in 2008 or 2009. The two shortlisted candidates for the core of the array are:South Africa: The core site is located at an elevation of about 1000 metres in the Karoo area of the arid Northern Cape Province, with distant stations in Ghana, Kenya, Madagascar, and Mauritius.
Australia: The core site is located at Boolardy in Western Australia, west of Meekatharra on a flat desert-like plain at an elevation of about 460 metres. The most distant stations will be located in New Zealand. [2] [3]
A preliminary list of 4 candidate host countries also included a site in the Karst Region of Guizhou in southwest China as well as a site at high elevations in a National Park in Argentina.
Funding
The SKA is expected to cost US$1.6bn,[2], with funding coming from many international sources. Preliminary plans call for 1/3 of the funding from the United States, 1/3 of the funding from Europe, and the remaining 1/3 from the rest of the world. The distribution of radio time is still a contested issue, with some countries advocating that the amount of radio time any country is given should be proportional to the amount of funding donated. Others advocate a "free skies" policy, in which the best scientific proposals are given radio time regardless of national boundaries.See also
- List of radio telescopes
- LOFAR (the Low Frequency Array, currently under construction in The Netherlands)
- Mills Cross (historical connections with the SKA development in Australia)
References
1. ^ Square Kilometre Array website.
2. ^ Amos, J. Nations vie for giant telescope, BBC News, 28 September 2006.
3. ^ Science Network WA, 16 February 2007
2. ^ Amos, J. Nations vie for giant telescope, BBC News, 28 September 2006.
3. ^ Science Network WA, 16 February 2007
External links
- "Australia may host Square Kilometre Array", Cosmos magazine, September 2006
- Australian SKA Planning Office Newsletter. CSIRO (10, April 2007). Retrieved on 2007-03-19.
- SKA South Africa web site
radio telescope is a form of directional radio antenna used in radio astronomy and in tracking and collecting data from satellites and space probes. In their astronomical role they differ from optical telescopes in that they operate in the radio frequency portion of the
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Square kilometre (U.S. spelling: square kilometer), symbol km², is a decimal multiple of the SI unit of surface area, the square metre, one of the SI derived units. 1 km² is equal to:
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- 1,000,000 m²
- 100 ha (hectare)
- 1 m² = 0.
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hertz (symbol: Hz) is the SI unit of frequency. Its base unit is cycle/s or s-1 (also called inverse seconds, reciprocal seconds). In English, hertz is used as both singular and plural.
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Radio astronomy is a subfield of astronomy that studies celestial objects in the radio frequency portion of the electromagnetic spectrum. Radio astronomy techniques are similar to optical techniques but radio telescopes have to be much larger due to the longer wavelengths being
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Aperture synthesis or synthesis imaging is a type of interferometry that mixes signals from a collection of telescopes to produce images having the same angular resolution as an instrument the size of the entire collection.
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An active galactic nucleus (AGN) is a compact region at the centre of a galaxy which has a much higher than normal luminosity over some or all of the electromagnetic spectrum (in the radio, infrared, optical,
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redshift occurs when the electromagnetic radiation, usually visible light, that is emitted from or reflected off an object is shifted toward the (less energetic) red end of the electromagnetic spectrum.
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SETI (Search for Extra-Terrestrial Intelligence) is the name for a number of organized efforts to detect Extraterrestrial life. A number of efforts with "SETI" have been organized, including projects funded by the United States Government.
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1 light-year =
SI units
01015 m 01012 km
Astronomical units
0103 AU 0 pc
US customary / Imperial units
01015 ft 01012 mi
A light-year or lightyear (symbol: SI units
01015 m 01012 km
Astronomical units
0103 AU 0 pc
US customary / Imperial units
01015 ft 01012 mi
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This article or section contains information about scheduled or expected future events.
It may contain tentative information; the content may change as the event approaches and more information becomes available.
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It may contain tentative information; the content may change as the event approaches and more information becomes available.
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astronomical interferometer is an array of telescopes or mirror segments acting together to probe structures with higher resolution. Astronomical interferometers are widely used for optical astronomy, infrared astronomy, submillimetre astronomy and radio astronomy.
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array is a data structure consisting of a group of elements that are accessed by indexing. In most programming languages each element has the same data type and the array occupies a contiguous area of storage. Most programming languages have a built-in array data type.
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1 kilometre =
SI units
0 m 0106 mm
US customary / Imperial units
0 ft 0 mi
A kilometre (American spelling: kilometer, symbol kmSI units
0 m 0106 mm
US customary / Imperial units
0 ft 0 mi
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Karoo (a Khoisan word of uncertain etymology [1]) is a semi-desert region of South Africa. It has two main sub-regions - the Great Karoo in the north and the Little Karoo in the south.
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Northern Cape is a large, sparsely populated province of South Africa, created in 1994 when the Cape Province was split up. Its capital is Kimberley. It includes the Kalahari Gemsbok National Park, which is part of a trans-frontier park with Botswana.
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Boolardy Station () is a remote sheep station in the north-west of Western Australia, about 194 km north-north-east of Pindar and 200 km west-south-west of Meekatharra. It is within the Shire of Murchison and situated on pastoral lease no.
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Western Australia
Flag Coat of Arms
Slogan or Nickname: Wildflower State or the "Golden State"
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Capital Perth
Government Constitutional monarchy
Governor Ken Michael
Premier Alan Carpenter (ALP)
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Flag Coat of Arms
Slogan or Nickname: Wildflower State or the "Golden State"
Other Australian states and territories
Capital Perth
Government Constitutional monarchy
Governor Ken Michael
Premier Alan Carpenter (ALP)
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Meekatharra
Western Australia
Location of Meekatharra in Western Australia (red)
Population: 945
Postcode: 6642
Elevation: 517 m
Location:
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Western Australia
Location of Meekatharra in Western Australia (red)
Population: 945
Postcode: 6642
Elevation: 517 m
Location:
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Karst topography is a landscape shaped by the dissolution of a soluble layer or layers of bedrock, usually carbonate rock such as limestone or dolomite. These landscapes display distinctive surface features and underground drainages, and in some examples there may be little or no
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贵州省
Guìzhōu Shěng
Abbreviations: 黔 or ? (Pinyin: Qián or Guì)
Origin of name 贵 guì - Gui Mountains
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Guìzhōu Shěng
Abbreviations: 黔 or ? (Pinyin: Qián or Guì)
Origin of name 贵 guì - Gui Mountains
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dólar estadounidense (Spanish)
dólar amerikanu (Tetum)
dólar americano
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This is a list of radio telescopes that are or have been used for radio astronomy. It includes both single dishes and interferometer arrays. They are listed by region, then by name; unnamed telescopes are in reverse size order at the end of the lists.
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LOFAR is the LOw Frequency ARray for radio astronomy. It is an ambitious project to build an interferometric array of radio telescopes distributed across the Netherlands and Germany, and possibly other European countries such as Great Britain, France and Sweden, with a total
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"Ik zal handhaven" (Dutch)
"I shall stand fast"1
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Bernard Mills built the two-dimensional Mills Cross Telescope in 1954 at the Fleurs field station of the Australian Commonwealth Scientific and Industrial Research Organisation in the area known now as Badgerys Creek, about 40km west of Sydney, New South Wales, Australia.
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BBC News is the department within the BBC responsible for the corporation's news-gathering and production of news programmes on BBC television, radio and online. Producing 120 hours of output daily,[1]
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