Notas de Imprensa

15 de Abril de 1994: Very difficult and time-consuming observations performed with the ESO 3.5-metre New Technology Telescope (NTT) in November 1993 by an international team of astronomers [1], indicate that up to 90 percent of the matter in a distant giant galaxy maybe of a kind that cannot be seen by normal telescopes.

18 de Fevereiro de 1994: Eight years after the passage of Comet Halley in early 1986, astronomers at the European Southern Observatory have succeeded in obtaining an image [1] of this famous object at a distance of no less than 2,820 million km from the Sun. The comet is now about as far away as giant planet Uranus. It recently passed the halfway mark towards the most distant point of its very elongated 76-year orbit. The image shows the 6 x 15 km avocado-shaped nucleus as an extremely faint point of light without any surrounding dust cloud. It appears that the surface is now completely frozen and the comet has ceased to emit dust and gas. This observation was made with the ESO 3.58 metre New Technology Telescope (NTT). It is by far the faintest and most distant image ever recorded of this comet.

3 de Fevereiro de 1994: On Wednesday, February 16, 1994, seven NASA and ESA astronauts and their spouses will spend a day at the Headquarters of the European Southern Observatory. They are the members of the STS-61 crew that successfully repaired the Hubble Space Telescope during a Space Shuttle mission in December 1993. This will be the only stop in Germany during their current tour of various European countries.

27 de Janeiro de 1994: Astronomers all over the world are preparing themselves for observations of a most unique event: during a period of six days in July 1994, at least 21 fragments of comet Shoemaker-Levy 9 will collide with giant planet Jupiter. At the European Southern Observatory, an intensive observational campaign with most of the major telescopes at La Silla is being organized with the participation of a dozen international teams of astronomers. This is the first time ever that it has been possible to predict such a collision. Although it is difficult to make accurate estimates, it is likely that there will be important, observable effects in the Jovian atmosphere.

27 de Janeiro de 1994: On 23 February 1994, it will be exactly seven years since the explosion of Supernova 1987A in the Large Magellanic Cloud [1] was first observed, at a distance of approx. 160,000 light-years. It was the first naked-eye supernova to be seen in almost four hundred years. Few events in modern astronomy have met with such an enthusiastic response by the scientists and this famous object has been under constant surveillance ever since. After several years of relative quiescence, things are now beginning to happen in the immediate neighbourhood of SN 1987A. Recent observations with the ESO 3.5 m New Technology Telescope (NTT) indicate that interaction between the stellar material which was ejected during the explosion and the surrounding ring-shaped nebulae has started. This signals the beginning of a more active phase during which the supernova is likely to display a number of new and interesting phenomena, never before observed.

20 de Dezembro de 1993: The ESO Council [1] took a number of important decisions in its December 1993 meeting. In particular, it unanimously agreed to proceed with the modified plan for the construction of the ESO Very Large Telescope at the Paranal mountain in Chile.

5 de Novembro de 1993: A group of young people, aged between 16 and 18 years and with a special interest in astronomy, are about to experience two most exciting and formative weeks at the European Southern Observatory, first at the ESO Headquarters in Garching and then at the ESO La Silla Observatory in Chile.

20 de Agosto de 1993: This press release is only available in German.

20 de Agosto de 1993: This press release is only available in German.

29 de Junho de 1993: On June 25, 1993, Schott Glaswerke (Mainz, Germany) officially handed over to ESO the largest mirror blank ever made. Weighing 22,000 kilograms and with a diameter of 8.2 metres, the blank has a thickness of only 177 millimetres.

24 de Junho de 1993: The delegations of the Government of Chile and of the International Organisation ESO [1] report on the outcome of their discussions regarding the installation of the largest telescope in the world "The Very Large Telescope" and "Very Large Telescope Interferometer" (VLT /VLTI) at Cerro Paranal (in the Chilean region II — Antofagasta) and the clarification of the future relations between ESO and Chile. The object of these discussions was a closer cooperation between ESO and Chile to the mutual benefit of this country and the eight European member countries of ESO.

22 de Junho de 1993: ESO's Contribution to the European Week for Scientific Culture The European Southern Observatory is pleased to announce the launch of its new programme "Future Astronomers of Europe". It is organised in conjunction with the European Week for Scientific Culture (November 22 -27, 1993), with support from the Commission of the European Communities.

3 de Junho de 1993: The recent identification of the optical image of a pulsar in the Large Magellanic Cloud is a fine illustration of astronomy as a high-tech international science. It is the first extragalactic pulsar to be so identified and only the third radio pulsar, after those in the Crab and Vela nebulae in the Milky Way, for which this has been possible.

3 de Junho de 1993: Although astronomy is an exact natural science, chance sometimes plays an important role. The recent discovery during an otherwise routine observation of the hitherto brightest known double quasar [1] would not have been possible without some luck.

1 de Junho de 1993: On March 28, 1993, American astronomers David Jewitt and Jane Luu on Hawaii discovered a slow-moving minor planet of magnitude 23. More observations were made the following night, confirming the unusual motion and indicating that it is located at a very large distance from the Sun, possibly far beyond Pluto, the outermost known, major planet. It was given the preliminary designation 1993 FW (IAU Circular 5730)

14 de Maio de 1993: ESO, the European Southern Observatory, in reply to questions raised by the media would like to clarify its position with regard to recent events which concern the relations between ESO and the Republic of Chile, the host state for the ESO observatories in the southern hemisphere.

27 de Março de 1993: The past decades have witnessed a dramatic increase in our knowledge of the Universe we live in. New instruments for astronomical observations and analysis are unveiling the secrets of deep space at an ever-increasing pace. Detailed studies of planets, stars, nebulae, galaxies and strange, exotic celestial objects have provided us with new insights into the formation, structure and evolution of our Universe.

29 de Janeiro de 1993: This photo is a composite of five exposures of Minor Planet no.~4179, also known as Toutatis, obtained with the 3.5-m ESO New Technology Telescope on December 21, 1992, by ESO-astronomer Jesper Storm. At this time, Toutatis was about 13 million km from the Earth, i.e. 33 times more distant than the Moon. On December 8, this Minor Planet passed within 3.6 million km from the Earth, but at that time it was not possible to observe it with ground-based optical telescopes, because it was situated between the Earth and the Sun. However, very good radar images were obtained which showed thecratered surface of the object.

3 de Dezembro de 1992: The Council of the European Southern Observatory [1], meeting at the ESO Headquarters in Garching on December 1-2, 1992, has decided to initiate a Programme by this organisation, aimed at supporting some of the scientifically most active and internationally highly esteemed astronomical institutes and research groups in Central and Eastern Europe (C&EE).

13 de Novembro de 1992: Based on observations just obtained with the ESO New Technology Telescope at La Silla, a group of Italian astronomers [1] have securely identified the optical emission from the mysterious GEMINGA object. Although GEMINGA is the second strongest source of energetic gamma-rays in the sky, its optical image is extremely faint and the real nature of this strange object has long been a subject of debate. The present break-through became possible when the astronomers discovered and accurately measured the object's motion in the sky. As a consequence, GEMINGA is now believed to be the closest neutron star known to us, at a distance of no more than 300 light-years, possibly even smaller.