Information from the European Southern Observatory ESO Press Photos 21a-b/00 28 August 2000 For immediate release | |
"First Light" Approaches for Fourth VLT Unit Telescope YEPUN's Secondary Mirror Now in Place |
ESO Press Photo 21a/00 [Preview; JPEG: 400 x 300; 49k] [Full size; JPEG: 1280 x 960; 533k] The reflectivity of the fourth VLT M2 Beryllium mirror is being measured after the successful coating process. (This digital photo was obtained on August 27, 2000). |
ESO Press Photo 21b/00 [Preview; JPEG: 400 x 300; 74k] [Full size; JPEG: 1280 x 960; 664k] Installation of the M2 Mirror in its cell, at the top of the mechanical structure of YEPUN . During this operation, the telescope is moved to the horizontal position. This scene is reflected in the primary 8.2-m Zerodur mirror - it can be seen that the M2 mirror cover is still on. (This digital photo was obtained on August 27, 2000). | | |
These days, the ESO staff at Paranal is having a strong feeling of "déja-vu". Only seven months after the third 8.2-m VLT Unit Telescope, MELIPAL , achieved "First Light", this crucial moment is now rapidly approaching for YEPUN , the fourth and last of the giants at the ESO observatory. Following successful coating with a thin layer of aluminium in early June 2000, the 8.2-m primary Zerodur mirror (M1) was placed in its supporting cell and safely attached to the mechanical structure of YEPUN on July 31. On August 26, the 1.1-m M2 Beryllium Mirror for YEPUN was coated. Again, this delicate operation went very well and the measured reflectivity was excellent, about 91%. The M2 mirror and its support were then assembled and successfully installed at the telescope on Sunday, August 27. Before the optical mirrors were installed, and with dummies in their place, careful tests were made of most telescope functions. In particular, this included accurate balancing of the 450-tonnes telescope frame on its hydrostatic oil bearings, as well as precise adjustment of all motions. It now remains for the ESO engineers to do the final performance optimization of the entire telescope. The work on the fourth telescope has been particularly noticeable because a large proportion of the assembly, integration, tuning and testing was organised and executed by ESOs young group of capable engineers and technicians. As the engineering staff at Paranal has grown and during the earlier work on the first three telescopes, they have been acquiring the necessary expertise to autonomously integrate and maintain the 8.2-m telescopes. During the coming "First Light" observations, light from the selected celestial objects will be registered by the VLT Test Camera at the Cassegrain Focus. This comparatively simple instrument was also used for the consecutive "First Light" events for ANTU ( May 1998 ), KUEYEN ( March 1999 ) and MELIPAL ( January 2000 ). It is mounted on the telescope's optical axis within the M1 Mirror Cell, just behind the main mirror. It is planned to make one or more of these first images available on the web soon thereafter. This is the caption to ESO PR Photos 21a-b/00 . They may be reproduced, if credit is given to the European Southern Observatory. Note, however, that since these photos were electronically recorded and were primarily obtained to document the ongoing activities at Paranal, they are not of full professional quality for photographic reproduction. © ESO Education & Public Relations Department Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany |