Extremely large telescope

Comparison of nominal sizes of primary mirrors of the above extremely large telescopes and some notable optical telescopes (click for detail)
Extremely Large Telescopes compared to some existing telescopes (hover with mouse over image)

 · European Extremely Large Telescope (top left)
 · Thirty Meter Telescope (top right)
 · Giant Magellan Telescope (bottom left)
 · Comparison: Large Binocular Telescope, Keck Observatory,    Very Large Telescope, Gran Telescopio Canarias

An extremely large telescope (ELT) is an astronomical observatory featuring a telescope with an aperture for its primary mirror from 20 metres up to 100 metres across,[1] when discussing reflecting telescopes of optical wavelengths including ultraviolet (UV), visible, and near infrared wavelengths. Among many planned capabilities, ELTs are planned to increase the chance of finding Earth-like planets around other stars.[2] Telescopes for radio wavelengths can be much bigger physically, such as the 300 metres (330 yards) aperture fixed focus radio telescope of the Arecibo Observatory. Freely steerable radio telescopes with diameters up to 100 metres (110 yards) have been in operation since the 1970s.

These telescopes have a number of features in common, in particular the use of a segmented primary mirror (similar to the existing Keck telescopes), and the use of high-order adaptive optics systems.[3][4] See also the List of largest optical reflecting telescopes for other large finished telescopes.

Although ELT designs are large, they can have smaller apertures than the aperture synthesis on many large optical interferometers. However, they may collect much more light, along with other advantages.

ELTs

The top three ELTs that are being funded, with two smaller but completed large telescopes for comparison (background yellow). In the early 2000s, all three targeted completion in 2018, although this slipped to 2022 for the TMT[5] and 2024 for the E-ELT.[6]

Image Name Aperture (m) Area (m²) Primary mirror Altitude (m) First
light
Notes Refs
European Extremely Large Telescope
(E-ELT)
39.3 978 798 × 1.45 m
hexagonal (f/1)
3060 2024 Under construction: Cerro Armazones Obs., Chile [6][7][8]
Thirty Meter Telescope
(TMT)
30 655 492 × 1.45 m
hexagonal (f/1)
4050 2024 On hold: Mauna Kea Obs., Hawaii [3][5]
Giant Magellan Telescope
(GMT)
24.5 368 7 × 8.4 m
circular (f/0.71)
2516 2021 Under construction: Las Campanas Obs., Chile;
4 mirrors cast (4/7 M1)
[4][9]
Large Binocular Telescope
(LBT)
11.8 equiv area
22.8 equiv detail limit
111 2 × 8.4 m
circular
3221 2008 largest non-segmented mirrors;
Located on Mount Graham in Arizona
[10]
Gran Telescopio Canarias
(GTC)
10.4 74 36 × 1.9 m
hexagonal
2275 2008 Largest single mirror.
Located on Roque de los Muchachos Obs. in the Canary Islands
[11]
Note: Aperture of LBT: the baseline is obtained via aperture synthesis

The Keck Observatory (2 x 10 m) and the Very Large Telescope, of the European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile, is also of note, with 4 × 8.2 m and 4 × 1.8 m, all on separate mounts but in one building for interferometry.

Budget

Possible budget figures, which are estimates and can vary over time.

Name Cost
(est USD)
Alternate
European Extremely Large Telescope (E-ELT) $1400 million €1055 million (Euros)
Thirty Meter Telescope (TMT) $1200 million
Giant Magellan Telescope (GMT) $700 million
Large Binocular Telescope (LBT) $120 million
Gran Telescopio Canarias (GTC) $172 million €130 million (Euros)

Projects

There were several telescopes in various stages in the 1990s and early 2000s, and some developed into construction projects.

Funded construction
Projects

Some of these projects have been cancelled, or merged into ongoing ELTs.

See also

References

External links

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