Comunicados de Prensa

19 de Mayo de 1998: With the VLT UT1 First Light just one week away, the ultimate activities that lead up to this important event have started at the Paranal Observatory. Following successful optical alignment tests, cf. ESO Press Release 05/98, the 8.2-m primary mirror has been removed from the first Unit Telescope (UT1). It is now in the Mirror Maintenance Building (MMB) and is being prepared for coating with a thin, highly reflective aluminium layer.

13 de Mayo de 1998: Two weeks before the moment of "First Light" of Unit Telescope no. 1 of the Very Large Telescope (VLT) , the ESO Team at the Paranal Observatory reports good progress of the preparatory work.

13 de Mayo de 1998: In December 1987, the ESO Council decided to embark upon the Very Large Telescope (VLT), Europe's astronomical flagship facility for the early 21st century.

30 de Abril de 1998: This is another video clip with recent footage from the Paranal Observatory, illustrating the continuing progress of the VLT project. It was obtained in mid-April 1998 by the ESO EPR Video Team and forms part of the video tape ( UT1-FLE-VNR1 ) with selected video material for broadcast use, issued in connection with the VLT First Light Event.

27 de Abril de 1998: Following the successful installation of the 8.2-m Zerodur main mirror at the first of the four Unit Telescopes (UT1) of the ESO Very Large Telescope (VLT) on April 16, work now continues on the optical alignment of the complex system.

17 de Abril de 1998: The world's largest optical mirror - with 8.2-m diameter and a surface of more than 50 m 2 , polished to the highest perfection - was today put in place at the First VLT Unit Telescope (UT1) at the Paranal Observatory.

24 de Marzo de 1998: The assembly work on the first VLT 8.2-m Unit Telescope (UT1) at Paranal is now entering the final phases. The excellent progress continues and the project is on schedule for the First Light Event in late May.

11 de Marzo de 1998: The European Southern Observatory is building the world's largest optical telescope, the Very Large Telescope (VLT) , at the ESO Paranal Observatory in Chile. The VLT consists of four 8.2-m unit telescopes and several smaller, moveable Auxiliary Telescopes. When coupled as the giant VLT Interferometer (VLTI) , they will together provide the sharpest images ever obtained by any optical telescope. It will in principle be able to see an astronaut on the surface of the Moon, 400,000 km away.

10 de Marzo de 1998: The VLT assembly work at the ESO Paranal Observatory continues in great strides. During the past week, the mirror cell for the 8.2-m main mirror (the M1 cell ) was successfully attached to the bottom of the telescope tube of Unit Telescope 1 (UT1). The present `picture story' illustrates the various phases of this delicate operation.

5 de Marzo de 1998: We continue the publication of video clips which illustrate the rapid progress of the VLT project. The present footage of the ISAAC (Infrared Spectrometer and Array Camera) instrument for the ESO Very Large Telescope was obtained last week by the ESO EPR Video Team at the ESO Headquarters in Garching.

3 de Marzo de 1998: We continue the publication of video clips which illustrate the rapid progress of the VLT project. The present footage of the FORS (FOcal Reducer/low dispersion Spectrograph) instrument for the ESO Very Large Telescope was obtained by the ESO EPR Video Team during a recent mission to DLR (Deutsche Forschungsanstalt für Luft- und Raumfahrt e.V.) in Oberpfaffenhofen near Munich (Germany).

17 de Febrero de 1998: Now that the big mechanical pieces of the first 8.2-metre unit telescope (UT1) of ESO's Very Large Telescope (VLT) have been assembled, the work areas have shifted towards the many other components that are needed to make the first giant optical telescope in the southern hemisphere operational. Although most of these items may be of less impressive dimensions, they are equally indispensable to make a telescope of this size and weight point towards a given direction and follow the motion of the celestial objects to be observed with superior accuracy.

30 de Enero de 1998: While famous Comet Hale-Bopp continues its long voyage towards the outer reaches of the solar system, observations proceed with telescopes in the southern hemisphere. These research programmes aim at a better understanding of the further development of this very active comet as it moves away from the Sun and slowly cools. Among the key questions are for instance: "When will it cease to display a dust tail?" and "Will the nucleus undergo outbursts during which much fresh material will be dispensed into space, as this has occasionally happened by other comets (e.g. Halley)?"

29 de Enero de 1998: SOFI, ESO's new infrared imager/spectrometer, saw first light at the NTT telescope on December 6, 1997, as planned and less than two years after the start of its detailed design. The acronym stands for 'Son OF ISAAC', the larger Infrared Spectrometer And Array Camera being built by ESO for the VLT.

23 de Enero de 1998: We show here five high-resolution photographic images (4-6 Mbytes) from the ESO Paranal Observatory, the site of ESO's Very Large Telescope Array (VLT).

22 de Enero de 1998: This spring, teachers across Europe will enjoy support for exciting, novel educational projects on astronomy, navigation and environmental observations. The largely web-based and highly interactive SEA & SPACE programme makes it possible for pupils to perform field experiments and astronomical observations and to obtain and process satellite images. A contest will take the best pupils for one week to Lisbon (Portugal), to Europe's space port in Kourou (French Guyana) where the European launcher lifts off or to ESO's Very Large Telescope at the Cerro Paranal Observatory in Chile, the largest optical telescope in the world.

16 de Enero de 1998: We continue the publication of video clips from the Paranal Observatory by showing aerial scenes of the VLT site and an overall view of Unit Telescope 1 in its enclosure. The footage was obtained by the ESO EPR Video Team during a recent mission.

13 de Enero de 1998: Within a few months, the first 8.2-meter Unit Telescope of the ESO Very Large Telescope (VLT) array will open its eye towards the sky above the Atacama desert. As documented by recent Press Photos from ESO, the construction work at the Paranal VLT Observatory is proceeding rapidly. Virtually all of the telescope components, including the giant Zerodur mirror, are now on the mountain.

22 de Diciembre de 1997: We publish here as first examples three clips from the transport of the first VLT 8.2-m Zerodur mirror (M1) from the port of Antofagasta to the Paranal Observatory, as obtained by the ESO EPR Video Team.

19 de Diciembre de 1997: The present collection of twelve high-resolution photographic images illustrates the transport of the first VLT 8.2-m Zerodur mirror (M1) to Paranal. They are suitable for high-quality reproduction and complement the digital, less detailed ESO Press Photos 33a-f/97 which were published one week ago with information about this important event.