VERY LARGE TELESCOPE NaCo Calibration Plan - ESO 2025

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List of telescopes #NameAperture (m) 1 Extremely Large Telescope (ELT) 39.3 2 Thirty Meter Telescope (TMT) 30.0 3 Giant Magellan Telescope (GMT) 24.5 4 Large Binocular Telescope (LBT) 11.8 (equiv. area) 22.8 (equiv. detail limit)1 more row
THE VERY LARGE ARRAY One of the worlds premier astronomical radio observatories, consists of 27 radio antennas in a Y-shaped configuration on the Plains of San Agustin fifty miles west of Socorro, New Mexico. Each antenna is 25 meters (82 feet) in diameter.
The 39-metre-diameter primary mirror, which will be made up of 798 individual hexagonal segments each measuring 1.4 metres across, will be by far the largest ever made for an optical telescope. Together, the segments will collect tens of millions of times as much light as the human eye.
But ESOs operational Very Large Telescope (VLT) and under-construction Extremely Large Telescope (ELT), as well as the southern site of the proposed Cherenkov Telescope Array Observatory (CTAO-South) in which ESO is a partner, stand just a few kilometers from the proposed INNA project, a 3000-hectare array of wind
When completed, it will be the worlds largest optical and near-infrared extremely large telescope. Part of the European Southern Observatory (ESO) agency, it is located on top of Cerro Armazones in the Atacama Desert of northern Chile.
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