Auxiliary Telescopes
The four Auxiliary Telescopes (ATs) are 1.8m diameter telescopes that feed light into the Very Large Telescope Interferometer at ESO's Paranal Observatory. Uniquely for telescopes of this size, they can be moved from place to place around the VLT platform and are self-contained. They were built by AMOS (Belgium). Further information can be found here: eso0402.
The top part of each AT is a round enclosure, made from two sets of three segments, which open and close. The role of the enclosure is to protect the delicate 1.8-metre telescope from the desert conditions. The enclosure is supported by the boxy transporter section, which also contains electronics cabinets, liquid cooling systems, air-conditioning units, power supplies, and more. During astronomical observations the enclosure and transporter are mechanically isolated from the telescope, to ensure that no vibrations compromise the data collected.
VLT Auxiliary Telescope enclosure:
- Height: 630 cm
- Diameter: 390 cm
The transporter section runs on tracks, so the ATs can be moved to 30 different observing locations. As the VLT Interferometer (VLTI) acts rather like a single telescope as large as the group of telescopes combined, changing the positions of the ATs means that the VLTI can be adjusted according to the needs of the observing project.
Latest Images
Follow the Auxiliary Telescopes on these live images updated every hour during daytime. The telescopes can be relocated to many different stations to change their geometric configuration. The live images show some of the most used stations, but there might be no telescope there. Click on the thumbnails to enlarge.
A1 station LIVE (). Here you may be able to see the AT1
K0 station LIVE (). Here you may be able to see the AT3. On extremely clear days the magnificent 6739-metre volcano Llullaillaco is visible in the background of this photograph. It is an amazing 190 kilometres away on the border with Argentina.
G1 station LIVE (). Here you may be able to see the AT4
Auxiliary Telescopes
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