Comunicados de Prensa

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.

12 de Diciembre de 1997: Just as the first 8.2-metre Zerodur VLT primary mirror (M1) is arriving at the Paranal Observatory, there are also good news about the first of the 1.2-m Beryllium VLT secondary mirrors (M2) and its Supporting Unit . This assembly is placed at the top of the VLT 'telescope tube'.

12 de Diciembre de 1997: Another historic event in ESO's Very Large Telescope Project has just occurred. The first giant mirror is on the mountain! The blanks for the four 8.2-metre VLT mirrors of Zerodur were produced by the Schott Glaswerke (Mainz, Germany) and have been polished at the REOSC factory (St. Pierre du Perray, France). For more information, see ESO Press Release 15/95. The first of the four mirrors left France in early November 1997 en route to Paranal. The transport was organized by the Gondrand company.

2 de Diciembre de 1997: The main structure of the ESO Very Large Telescope (VLT) has been designed, produced and assembled by an Italian consortium composed of Ansaldo Energia (Genova), European Industrial Engineering (Venice) and SOIMI (Milan). A total of four identical structures have been built, one for each of the four VLT 8.2-m Unit Telescopes.

24 de Noviembre de 1997: When is a minor object in the solar system a comet? And when is it an asteroid? Until recently, there was little doubt. Any object that was found to display a tail or appeared diffuse was a comet of ice and dust grains, and any that didn't, was an asteroid of solid rock. Moreover, comets normally move in rather elongated orbits, while most asteroids follow near-circular orbits close to the main plane of the solar system in which the major planets move.

17 de Noviembre de 1997: After a long journey from Europe, the first Very Large Telescope mirror cell (VLT M1 cell) and a concrete 8.2-m dummy mirror were unloaded in the Port of Antofagasta on October 31, 1997. From here, they were transported by special trucks to the Paranal Observatory.

22 de Octubre de 1997: During the past month, there has been much action in many different areas at the ESO Paranal Observatory. Work has continued on the assembly of various components of the telescope structures and on the surface of the summit platform, as well as in connection with the maintenance and storage facilities near the base camp at the foot of the mountain.

8 de Octubre de 1997: After having passed behind the Sun (as seen from the Earth), Comet Hale-Bopp is now again well visible to observers in the southern sky. Although this famous object is now three times farther away than when it passed its closest point to the Sun (the perihelion) on April 1, 1997, it is still quite bright, especially when compared to other comets that have been observed at the same distance. Its magnitude is now around 5, i.e. when seen in a dark sky it is just visible with the unaided eye. However, it is seen better through moderate-size binoculars and is of course still more interesting when observed with a large, professional telescope.

22 de Septiembre de 1997: With the completed assembly of the heavy parts that form the mechanical structure of the first (UT1) of the four large VLT Unit Telescopes, the integration of the motor that will move the telescope around the (horizontal) altitude axis is now about to start.