New Technology Telescope
The 3.58-metre New Technology Telescope (NTT) was inaugurated in 1989. It broke new ground for telescope engineering and design and was the first in the world to have a computer-controlled main mirror.
The main mirror is flexible and its shape is actively adjusted during observations by actuators to preserve the optimal image quality. The secondary mirror position is also actively controlled in three directions.
This technology, developed by ESO, known as active optics, is now applied to all major modern telescopes, such as the Very Large Telescope at Cerro Paranal and the future European Extremely Large Telescope.
The design of the octagonal enclosure housing the NTT is another technological breakthrough. The telescope dome is relatively small, and is ventilated by a system of flaps that makes air flow smoothly across the mirror, reducing turbulence and leading to sharper images.
Star formation, protoplanetary systems, Galactic center, spectroscopy.
- Images taken with NTT
- Images of NTT
- For scientists: More details can be found on the telescope page.
- ESO press releases with results from the New Technology Telescope
|Name:||New Technology Telescope|
|Enclosure:||Compact optimised enclosure|
|Type:||Optical & near-infrared telescope|
|Optical design:||Ritchey-Chrétien reflector|
|Diameter. Primary M1:||3.58 m|
|Material. Primary M1:||ZeroDur Schott|
|Diameter. Secondary M2:||0.875 m|
|Material. Secondary M2:||ZeroDur Schott|
|Diameter. Tertiary M3:||0.84 m X 0.60 m (elliptical)|
|First Light date:||23 March 1989|