Notas de Imprensa

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.

2 de Outubro de 1992: A new planet has just been found in the outer solar system. Although the observations do not yet allow an accurate determination of its orbit, it appears that it is situated about 6,000 million km away, outside the orbit of the outermost, known planet, Pluto. No other object has ever been found this far out in the solar system.

14 de Setembro de 1992: An exhibition about Astronomy and the European organization for astronomy (ESO) will soon open at the Science and Technical Museum "Leonardo da Vinci" in Milan, Italy.

18 de Agosto de 1992: Minor Planet (4015) was discovered in 1979. It is of the Earth–crossing "Apollo" type and moves in an elongated orbit around the Sun; the period of revolution is 4.3 years.

13 de Agosto de 1992: Italian astronomers, working from the Astronomical Observatory in Trieste, have performed remote observations with the ESO 3.5 metre New Technology Telescope (NTT) at La Silla, Chile. This is the first time ever that such observations have been made directly from an astronomical institute in one of the ESO member countries. Quite unexpectedly, a "cosmic mirage", that is a gravitational lens in a distant cluster of galaxies, was found during these observations.

10 de Julho de 1992: This photo shows Comet Grigg-Skjellerup, as imaged by the ESO 3.6 m telescope at the La Silla Observatory in the early morning of July 10, 1992, just 15 hours before the Giotto encounter with this comet. The observation was made by Dr. Klaus Jockers from the Max-Planck-Institut für Aeronomie (Katlenburg-Lindau, Germany), and in the course of a special monitoring programme in support of the Giotto Extended Mission. The digital image was transmitted to the ESO Headquarters in Garching via the permanent satellite link, immediately following the observations. The photo is a composite of four one-minute red-sensitive exposures. The other objects in the field are galactic stars.

1 de Julho de 1992: This photo shows Comet Grigg-Skjellerup, which will be visited by the Giotto spacecraft of the European Space Agency (ESA) on July 10, 1992

10 de Junho de 1992: In its 67th meeting in Garching on June 4 and 5, 1992 the Council of ESO appointed Prof. Riccardo Giacconi as Director General for the period 1993-1997. He succeeds Prof. Harry van der Laan whose five year term ends this year.

13 de Maio de 1992: This negative photo shows a small sky area in the direction of Comet Halley, obtained by ESO astronomers Alain Smette and Olivier Hainaut with the ESO 3.5-metre New Technology Telescope (NTT) in the morning of April 6, 1992

7 de Maio de 1992: NASA's Hubble Space Telescope (HST) has revealed an unusual and fascinating new optical jet in the nucleus of the elliptical galaxy NGC 3862.

22 de Abril de 1992: The photo shows a model of the ESO 16-metre equivalent Very Large Telescope (VLT), as it will appear on the Paranal mountain in the Chilean Atacama desert towards the end of the present decade. The VLT will become the world's largest optical telescope when it is ready.

21 de Abril de 1992: On April 24, 1992, the French Minister for Research and Space, Professor Hubert Curien, will inaugurate a unique, new optical facility of R.E.O.S.C [2] , at Saint Pierre du Perray, near Paris. The delicate polishing of the giant mirrors for ESO's 16-metre equivalent Very Large Telescope (VLT) will take place here.

25 de Fevereiro de 1992: Messier 87 (M87) is a giant galaxy, situated right at the centre of one of the largest and nearest clusters of galaxies, the Virgo Cluster; its distance is about 50 million light-years) and several thousand galaxies belong to this cluster, but none is brighter and heavier than Messier 87. Already in 1918, photos showed the presence of a jet in M87, i.e. a long and thin feature, extending in a westerly direction from the centre of this galaxy. This jet bears witness to the violent processes at the centre of M87 and has led many astronomers to think that there is a giant black hole in there. Recent observations with the Hubble Space Telescope have strengthened this suspicion.

24 de Fevereiro de 1992: This photo shows the newly discovered minor planet 1992 AD which is the most distant in the solar system. It was obtained at the ESO La Silla Observatory on 5 February 1992. The telescope followed the planet whose 16.7 magnitude image is round; the stars in the field are seen as short trails. The diffuse trail at the upper right corner is that of a galaxy

5 de Fevereiro de 1992: The ESO 16-metre equivalent Very Large Telescope (VLT) [1] will be equipped with technologically advanced instruments that record the light collected by the large mirrors.