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Extremely large telescope

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An extremely large telescope (ELT) is an astronomical observatory featuring an optical telescope with an aperture for its primary mirror from 20 metres up to 100 metres across, 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. 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.

Contents

Extremely large telescope Extremely large telescope Wikipedia

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.

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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

Extremely large telescope European Extremely Large Telescope Wikipedia

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, measure 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.

Projects

Extremely large telescope Postcard The EELT European Extremely Large Telescope ESO

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

Funded construction
  • GMT: Giant Magellan Telescope
  • E-ELT: European Extremely Large Telescope
  • TMT: Thirty Meter Telescope
  • Projects

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

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  • GSMT: Giant Segmented Mirror Telescope, merged into TMT
  • OWL: Overwhelmingly Large Telescope, passed over in favor of E-ELT
  • VLOT: Very Large Optical Telescope, merged into TMT
  • LAT: Large Atacama Telescope
  • EURO50: European 50-metre Telescope, merged into the E-ELT.
  • LPT: Large Petal Telescope
  • JELT: Japanese ELT Project. Japan joined the TMT project in 2008.
  • CELT: California Extremely Large Telescope; CELT became/merged into TMT project.
  • Swedish Extremely Large Telescope Project.
  • MAXAT
  • References

    Extremely large telescope Wikipedia


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