Comunicados de Prensa

13 de Noviembre 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 Octubre 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 Septiembre 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 Julio 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 Julio 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 Junio 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 Mayo 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 Mayo 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 Febrero 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 Febrero 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 Febrero 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.

29 de Octubre de 1991: This is a ground-based photo of the first minor planet ever to be visited by a spacecraft. On October 29, 1991, the NASA spacecraft Galileo will pass minor planet no. 951 Gaspra on its way to Jupiter where it will arrive in December 1995. The distance from Gaspra to the Earth will be 410 million km at the time of the fly-by.

22 de Octubre de 1991: Observations with telescopes at the La Silla observatory have revealed that the image of an extremely distant quasar, known as Q1208+1011, actually consists of two images very close to each other. It is the most distant and also the brightest quasar ever observed to have a double image.

24 de Septiembre de 1991: ESO is now awarding a major contract for its Very Large Telescope (VLT) to the "AES Consortium" of three Italian companies. It concerns the construction of the main mechanical structures of the four 8-m VLT unit telescopes, each of which will weigh more than 440 tons and yet must be machined with sub-micron precision in order to allow astronomical observations of the highest quality.

24 de Septiembre de 1991: Observations with the 3.5-m ESO New Technology Telescope by a European group of astronomers have shown that a very compact object in an extraordinary binary star, known under the astronomical designation 88433, is most probably a neutron star and not a black hole, as previously believed by most scientists. Improved observation techniques have allowed a reliable determination of the mass of this object: it is now found to weigh less than the Sun and is therefore not massive enough to be a black hole.

16 de Julio de 1991: The lonely Atacama desert is a perfect place to study distant celestial bodies in the space around us. The following story shows how this may be done, not only through powerful astronomical telescopes at isolated mountain-top observatories [1], but also down on the barren desert plain in a much more direct way.