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Square Kilometre Array

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Also known as SKA, Square Kilometer Array

large multi radio telescope project aimed to be built in Australia and South Africa

Key facts

Alternative names
SKA
Location s
Meerkat National Park , South Africa and Murchison Radio-astronomy Observatory , Australia
Coordinates
30°43′16″S 21°24′40″E / 30.72111°S 21.41111°E / -30.72111; 21.41111 and 26°41′49″S 116°37′52″E / 26.69694°S 116.63111°E / -26.69694; 116.63111
Built
2018–
First light
2027 (projected)
Collecting area
1 km (11,000,000 sq ft)
Website
www .skao .int

via Wikipedia infobox

Research organization · ROR

Type
Other
Founded
2011
Location
Johannesburg, South Africa
Also known as
SKA
Status
Active

GRID grid.452213.3 · ISNI 0000 0004 0569 9009

Official website

Explore | SKAO

skao.int

Link to the official site · 4,795 chars · not written by Vinony

Wikidata facts

Area
1
Official website
www.skao.int
Image
SKA overview.jpg
Show 5 more facts
service entry
2027-00-00
Commons category
Square Kilometre Array
native label
Square Kilometre Array
inception
2011-00-00
social media followers
28251
Sources (3)

via Wikidata · CC0

~28 min read

Article

The Square Kilometre Array (SKA) is an intergovernmental international radio telescope project being built in Australia (low-frequency) and South Africa (mid-frequency). The combining infrastructure, the Square Kilometre Array Observatory (SKAO), and headquarters, are located at the Jodrell Bank Observatory in the United Kingdom. The SKA cores are being built in the Southern Hemisphere, where the view of the Milky Way galaxy is the best and radio interference is at its least.

The name refers to the notional size of the telescope's collecting area, not to the extent of the entire telescope array, which is far larger. Conceived in the 1990s, and further developed and designed by the late-2010s, the intention is that when completed it will have a total collecting area of approximately one square kilometre as originally conceived. The design of the first phase of SKA, scheduled as of 2025 for science operation in 2032, consists of 21,000 square metres (0.021 km) of collecting area of dishes. It will operate over a wide range of frequencies and its size will make it 50 times more sensitive than any other radio instrument. If built as planned, it should be able to survey the sky more than ten thousand times faster than before. With receiving stations extending out to a distance of at least 3,000 km (1,900 mi) from a concentrated central core, it will exploit radio astronomy's ability to provide the highest-resolution images in all astronomy.

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