Picture of the Week

30 November 2009: After almost two months of life-changing experiences, bringing the excitement of astronomy to young children in Chile, Bolivia and Peru, the journey of the GalileoMobile Project has come to an end. As illustrated in this image, the astronomers and educators in the Galilomobile team visited numerous schools and villages during their expedition, engaging young students in educational activities about astronomy and science, and offering amazing stargazing opportunities to the local communities, in a region with one of the clearest skies on Earth. Last week the team visited ESO’s Very Large Telescope (VLT), then continued to Taltal, the closest town to the VLT’s home, Cerro Paranal. Around sunset on 26 November, the GalileoMobile team showed the community of Taltal the highlights of the whole voyage, a voyage that covered around 5,000 kilometres through the Andes. The GalileoMobile was received with great enthusiasm by the people of Taltal. Hundreds of students took ...

23 November 2009: This dramatic triptych shows the Moon rise from left to right through the night sky over ESO’s Very Large Telescope (VLT) observatory at Paranal in northern Chile. Already aloft in the heavens and glowing in the centre of the image is Venus, Earth’s closest planetary neighbour. Shining to Venus’s right, the giant, though more distant planet, Jupiter appears as a small orb that seems to rotate around Venus as time passes. Such apparent celestial near misses — although the heavenly bodies are actually tens to hundreds of millions of kilometres apart — are called conjunctions. Still other sights delight in the sky over Paranal. The radiant, reddish plane of the Milky Way smoulders on the horizon, with massive bands of dust giving this bright region a mottled complexion. On the ground, an 8.2-metre VLT Unit Telescope on the right and a 1.8-metre Auxiliary Telescope to the left silently witness the ...

16 November 2009: A probe was launched last Friday (13 November 2009) from ESO’s Paranal observatory in northern Chile — home of the Very Large Telescope (VLT) — aboard a weather balloon. Such probes, called radiosondes, measure various atmospheric parameters and transmit them to a receiver on the ground. Researchers from ESO, the University of Lethbridge (Canada) and Universidad de Valparaiso (Chile) are currently in the middle of a 12-day programme, during which they plan to launch 29 radiosondes. Each night, parallel observations with the VLT instruments UVES, CRIRES and VISIR are carefully orchestrated to coincide with two additional radiosonde launches, while an infrared radiometer provides continuous coverage. This powerful combination of instruments and methods will provide a better understanding of the distribution and amount of water vapour in the atmosphere above Paranal, which is highly relevant for astronomical observations. The knowledge gained from these data can be used to optimise science operations ...

9 November 2009: The Milky Way arches across this rare 360-degree panorama of the night sky above the Paranal platform, home of ESO’s Very Large Telescope. The image was made from 37 individual frames with a total exposure time of about 30 minutes, taken in the early morning hours. The Moon is just rising and the zodiacal light shines above it, while the Milky Way stretches across the sky opposite the observatory. The open telescope domes of the world’s most advanced ground-based astronomical observatory are all visible in the image: the four smaller 1.8-metre Auxiliary Telescopes that can be used together in the interferometric mode, and the four giant 8.2-metre Unit Telescopes. To the right in the image and below the arc of the Milky Way, two of our galactic neighbours, the Small and Large Magellanic Clouds, can be seen. Links Extended to 360 x 180 degrees (with black) version of this image

2 November 2009: A laser beam shoots out of Yepun, the fourth Unit Telescope of Europe’s flagship observatory, ESO’s Very Large Telescope (VLT). This beam is used to create an artificial star above Paranal to assist the adaptive optics instruments on the VLT. Adaptive optics is a technique that allows astronomers to overcome the blurring effect of the atmosphere and obtain images almost as sharp as would be possible if the whole telescope were placed in space, above Earth's atmosphere. Adaptive optics, however, requires a nearby reference star that has to be relatively bright, thereby limiting the area of the sky that can be surveyed. To overcome this difficulty, astronomers at Paranal use a powerful laser that creates an artificial star where and when they need it (see eso0607 and eso0727). Launching such a powerful laser from a telescope is a state-of-the-art technology, whose set-up and operation is a continuous challenge. As seen ...

26 October 2009: Sitting in the stunning environment surrounding ESO’s Very Large Telescope (VLT) on Cerro Paranal, Chile, are Joe Liske from ESO and Eva Noyola from the Max Planck Institute for Extraterrestrial Physics. The photo is a still image from the recently released 3D film, The EYE 3D — Life and Research on Cerro Paranal, directed by Nikolai Vialkowitsch. The movie, starring the two young scientists, as well as other people involved in the exciting activities at the VLT, offers a brand new, three-dimensional take on the life and research of astronomers. It has been produced by parallax raumprojektion and fact&film, in close collaboration with ESO and other partners and will be coming soon in cinemas across Germany. Don’t forget to wear red-cyan glasses to enjoy the spectacular 3D effect! Links The movie's ESO web page The movie’s external web page: http://www.theeye3d.eu The EYE 3D, press kit (German, PDF format)

19 October 2009: Portrayed in this beautiful image is the spiral galaxy NGC 1448, with a prominent disc of young and very bright stars surrounding its small, shining core. Located about 60 million light-years away from the Sun, this galaxy has recently been a prolific factory of supernovae, the dramatic explosions that mark the death of stars : after a first one observed in this galaxy in 1983, two more have been discovered during the past decade. Visible as a red dot inside the disc, in the upper right part of the image, is the supernova observed in 2003 (SN 2003hn), whereas another one, detected in 2001 (SN 2001el), can be noticed as a tiny blue dot in the central part of the image, just below the galaxy’s core. If captured at the peak of the explosion, a supernova might be as bright as the whole galaxy that hosts it. This image was ...

12 October 2009: This amazing panorama shows the observing platform of ESO’s Very Large Telescope (VLT) on Cerro Paranal, in Chile. Taken in the early morning, with the Moon still high in the sky, the air of peace and tranquility is in stark contrast to the frantic activity at the observatory. The four giant 8.2-metre Unit Telescopes of the VLT are all targeting specific celestial objects, helping astronomers in their daily quest to understand the mysteries of the Universe. A laser is fired from Unit Telescope 4, Yepun, to help the adaptive optics system of the telescope, and counteract the blurring effect of the atmosphere, allowing very sharp images to be obtained. Meanwhile, three of the four smaller 1.8-metre Auxiliary Telescopes are working together in interferometric mode to obtain an even more detailed view of a different cosmic object. A QuickTime VR is also available on this link. #L

5 October 2009: Sparkling at the edge of a giant cloud of gas and dust, the Flame Nebula, also referred to as NGC 2024, is in fact the hideout of a cluster of young, blue, massive stars, whose light sets the gas ablaze. Located 1,300 light-years away towards the constellation of Orion, the nebula owes its typical colour to the glow of hydrogen atoms, heated by the stars. The latter are obscured by a dark, forked dusty structure in the centre of the image and are only revealed by infrared observations. This image is based on data acquired with the 1.5-metre Danish telescope at ESO’s La Silla Observatory in Chile, combining three exposures in the filters B (40 seconds), V (80 seconds) and R (40 seconds).

28 September 2009: Through three giant images, the GigaGalaxy Zoom project reveals the full sky as it appears with the unaided eye from one of the darkest deserts on Earth, then zooms in on a rich region of the Milky Way using an amateur telescope, and finally uses the power of a professional telescope to reveal the details of a famous nebula. In this way, the project links the sky we can all see with the deep, “hidden” cosmos that astronomers study on a daily basis and allows the viewers to take a breathtaking dive into our Milky Way. The wonderful quality of the images is a testament to the splendour of the night sky at ESO’s sites in Chile, which are the most productive astronomical observatories in the world.

21 September 2009: Cerro Paranal, in the Chilean Atacama Desert, is considered one of the best astronomical observing sites in the world. It is home to ESO’s Very Large Telescope (VLT), the flagship facility for European ground-based astronomy. The humidity at Paranal is generally below five percent and the overall precipitation is only 4 mm per year — a rather dry place indeed. It does, on very rare occasions, snow on this 2600-metre-high peak as illustrated by this beautiful image taken in 2002. The snow-covered terrain gleams under a bright blue sky as the snow storm passes.

14 September 2009: In this image, two spiral galaxies, similar in looks to the Milky Way, are participating in a cosmic ballet, which, in a few billion years, will end up in a complete galactic merger — the two galaxies will become a single, bigger one. Located about 150 million light-years away in the constellation of Canis Major (the Great Dog), NGC 2207 — the larger of the two — and its companion, IC 2163, form a magnificent pair. English astronomer John Herschel discovered them in 1835. The fatal gravitational attraction of NGC 2207 is already wreaking havoc throughout its smaller partner, distorting IC 2163’s shape and flinging out stars and gas into long streamers that extend over 100,000 light-years. The space between the individual stars in a galaxy is so vast, however, that when these galaxies collide, virtually none of the stars in them will actually physically smash into each other. This ...

7 September 2009: In this photograph taken on 18 August 2009, a European ALMA antenna takes shape at the observatory's Operations Support Facility (OSF). ALMA, the Atacama Large Millimeter/submillimeter Array, is a revolutionary astronomical telescope, comprising an array of 66 giant 12-metre and 7-metre diameter antennas observing at millimetre and submillimetre wavelengths. The telescope is being built on the breathtaking location of the Chajnantor plateau, at 5000 metres altitude in the Chilean Andes. The OSF, at which the antennas are being assembled and tested, is at an altitude of 2900 metres. ESO has contracted with the AEM (Alcatel Alenia Space France, Alcatel Alenia Space Italy, European Industrial Engineering S.r.L., MT Aerospace) Consortium for the supply of 25 of the 12-metre diameter ALMA antennas, with options to increase the number to 32. ALMA is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile.

31 August 2009: Stars such as our Sun do not contain enough mass to finish their lives in the glorious explosions known as supernovae. However, they are still able to salute their imminent demise into dense, Earth-sized embers called white dwarfs by first expelling colourful shells of gas known as planetary nebulae. This misnomer comes from the similarity in appearance of these spherical mass expulsions to giant planets when seen through small telescopes. NGC 6781 is a nice representative of these cosmic bubbles. The planetary nebula lies a few thousand light-years away towards the constellation of Aquila (the Eagle) and is approximately two light-years across. Within NGC 6781, shells of gas blown off from the faint, but very hot, central star’s surface expand out into space. These shells shine under the harsh ultraviolet radiation from the progenitor star in intricate and beautiful patterns. The central star will steadily cool down and darken, eventually ...

24 August 2009: The great hunter Orion hangs above ESO’s Very Large Telescope (VLT), in this stunning, previously unseen, image. As the VLT is in the Southern Hemisphere, Orion is seen here head down, as if plunging towards the Chilean Atacama Desert. At night the four giant 8.2-metre Unit Telescopes of the VLT are all turned skywards to help astronomers in their quest to understand the Universe. The band of the Milky Way, crisscrossed by contrasting dark dust lanes, stretches up over the VLT’s Unit Telescope 3 (Melipal), with the bright star Capella glinting just above the telescope. Up and to the left, Orion’s belt and sword, containing the Orion Nebula, lie between the blue star Rigel and the orange Betelgeuse. The red Rosetta Nebula is seen in the middle part of the Milky Way, while Sirius, the brightest star in the night sky, hangs above the scene. The red patch just above ...

17 August 2009: This image shows the platform on the summit of Cerro Paranal, in Northern Chile that houses the ESO Very Large Telescope (VLT). Three of the enclosures protecting the 8.2-metre diameter VLT Unit Telescopes (UTs) are shown and the photographer was on the top of the fourth one, about 35 metres above the platform. At night the huge doors in the enclosures slide open and the 275-tonne top parts of these buildings rotate so that the telescope can observe any part of the sky. The pick-up truck in front of the first UT helps give the scale of this 10-story high building. On the left of the image the rails on which the 1.8-metre Auxiliary Telescopes (ATs) can be moved to different observing stations are visible. Two of the four ATs are visible in the picture. The low building in the lower left corner houses the VLT Interferometer laboratory, where the ...

10 August 2009: This new image of the galaxy NGC 2280 shows the extent of its massive spiral arms that reach far into the surrounding space. These star-filled tentacles taper off into wispy blue clouds of illuminated and glowing gas well away from the central, bright bulge of the galaxy. Found towards the constellation of Canis Major (the Greater Dog), NGC 2280 is thought to be similar in shape to our own Milky Way galaxy. NGC 2280 whirls in the cosmos about 75 million light-years from us; this snapshot therefore shows the galaxy as it appeared when dinosaurs still roamed the Earth. The very bright stars that sparkle like diamonds in the image, as well as the many other stars of various colours, are all in the foreground of our view, as they lie much closer to us than NGC 2280. The image was captured with the ESO Faint Object Spectrograph and Camera ...

3 August 2009: The Milky Way blazes above the European Southern Observatory (ESO) facilities at Mount Paranal in northern Chile’s Atacama Desert. Paranal hosts the world’s most advanced ground-based astronomical observatory, the Very Large Telescope (VLT), and is home to two new telescopes for large imaging surveys currently under construction, the VLT Survey Telescope (VST) and the Visible and Infrared Survey Telescope for Astronomy (VISTA). Both are expected to “take up duty” in the 2009-2010 timeframe. This photograph shows an edge-on view of the Milky Way’s glowing plane slicing across the night sky, laced by bands of dust and dark gas. Taken with a digital camera using a three-minute exposure, the photograph also reveals a bit of action on the ground. To the left, a vehicle with its parking lights on stops lets out a passenger. Though bathed by the light of the Milky Way, the high-altitude desert remains quite dark. To illuminate ...

27 July 2009: This image shows how ESO’s Very Large Telescope (VLT) facility looks through the eyes of Google Earth. This popular software allows users to see the world from above, ranging from a satellite to a bird’s eye view. Now, Google Earth users can swoop around detailed 3-D models of the massive structures housing the four 8.2-metre Unit Telescopes (UTs) atop Mount Paranal in the Chilean Atacama Desert. Also visible in this sample image are the four 1.8-metre movable Auxiliary Telescopes (ATs), the enclosure of the 2.4-metre VLT Survey Telescope (VST), and technical and support buildings. The models can be downloaded from ESO’s VLT page, and opened using Google Earth.

20 July 2009: This new artist’s impression shows the future Extremely Large Telescope (ELT), which is currently being planned by ESO. This revolutionary new ground-based telescope will be the largest optical/near-infrared telescope ever conceived, and will serve as “the world’s biggest eye on the sky”. The present concept is for a telescope with a mirror 39 metres in diameter, able to capture images of the sky about a tenth the size of the full Moon. The telescope will contain five mirrors, a novel configuration that results in exceptional image quality. The largest (primary) mirror will consist of almost 800 segments, each 1.4 metres wide but only 50 mm thick. The optical system’s design also calls for an immense secondary mirror measuring 4.2 metres in diameter, which is almost as large as the biggest primary mirrors used in today’s telescopes. With the start of operations planned early in the next decade, the ELT will ...