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23. marts 2009: Located inside the Large Magellanic Cloud (LMC) – one of our closest galaxies – in what some describe as a frightening sight, the Tarantula nebula is worth looking at in detail. Also known as 30 Doradus or NGC 2070, the nebula owes its name to the arrangement of its bright patches that somewhat resemble the legs of a tarantula. Taking the name of one of the biggest spiders on Earth is very fitting in view of the gigantic proportions of this celestial nebula — it measures nearly 1,000 light years across ! Its proximity, the favourable inclination of the LMC, and the absence of intervening dust make this nebula one of the best laboratories to better understand the formation of massive stars. This spectacular nebula is energised by an exceptionally high concentration of massive stars, often referred to as super star clusters. This image is based on data acquired with ...

9. marts 2009: The 40-metre-class primary mirror of the European Extremely Large Telescope (E-ELT) will be composed of 984 individual segments, which must be aligned with incredible precision. The position of the individual hexagonal mirrors needs to be controlled with nanometre precision (1 nanometre is 1 millionth of a mm). This can only be achieved with the help of new technologies and a prototype component for this high-tech alignment of segmented mirrors is seen in this image. The so-called Active Phasing Experiment achieved its First Light during the night of 6 December 2008 on the visitor focus of Melipal, one of the 8.2 m Unit Telescopes of ESO’s Very Large Telescope at Paranal. Made in collaboration with several European partners, the current active segmented mirror is composed of 61 hexagonal segments. You can move around the experiment in this Quicktime VTR animation.

2. marts 2009: One of most famous spiral galaxies is Messier 104, widely known as the "Sombrero" (the Mexican hat) because of its particular shape. It is located towards the constellation Virgo (the ‘virgin’), at a distance of about 30 million light-years and is the 104th object in the famous catalogue of deep-sky objects by French astronomer Charles Messier (1730 - 1817).This luminous and massive galaxy has a total mass of about 800 billion suns, and is notable for its dominant nuclear bulge, composed mainly of mature stars, and its nearly edge-on disc composed of stars, gas, and dust. The complexity of this dust is apparent directly in front of the bright nucleus, but is also evident in the dark absorbing lanes throughout the disc. A large number of small, diffuse objects can be seen as a swarm in the halo of Messier 104. Most of these are globular clusters, similar to those ...

23. februar 2009: A view of Paranal from May 1987.

16. februar 2009: The Bug Nebula, NGC 6302, is one of the brightest and most extreme planetary nebulae known. It is located about 4,000 light-years away, towards the Scorpius constellation (the Scorpion). The nebula is the swansong of a dying solar-like star lying at its centre. At about 250,000 degrees Celsius and smothered in a blanket of hailstones, the star itself has never been observed as it is surrounded by a dense disc of gas and dust, opaque to light. This dense disc may be the origin of the hourglass structure of the nebula. This colour image, which nicely highlights the complex structure of the nebula, is a composite of three exposures through blue, green and red filters. It was made using the 1.5-metre Danish telescope at the ESO La Silla Observatory, Chile.

9. februar 2009: Dette billede, taget en tidlig morgen i december måned 2009, viser al ønskelig tydelighed den fantastiske himmel over Paranal, hjemsted for ESO Very Large Telescope (VLT) i Chile.Man fornemmer det vidunderlige landskab med Mælkevejen, der hænger i al sin pragt over tre af de fire 1,8 meter VLT hjælpeteleskoper (Auxiliary Teleskopes (ATs)).De fire teleskoper observerer samtidigt, ved hjælp af interferometri for at få en opløsning så stor som hvis de brugte et teleskop med en diameter svarende til den største afstand mellem teleskoperne, i dette tilfælde, 48 meter.Da de større 8,2-meter Unit Teleskoper i VLT normalt anvendes individuelt, er de fire ATs blevet tilføjet til systemet for at gøre fuld brug af det interferometriske laboratorium.Det bemærkelsesværdige foto, som er taget i retning mod øst, viser konstellationerne Ophiuchus (Slangebæreren), Sagittarius (Skytten), Scorpius (Skorpionen), og Triangulum Australe (Sydlige trekant).Mælkevejens centrum befinder sig lige under midten af ​​billedet.Dette billede er tilgængelig som et ...

2. februar 2009: Galakseparret NGC 1531/2, i en engageret livlig vals, ligger omkring 70 millioner lysår borte i retning mod det sydlige stjernebillede Eridanus (Floden).Den deformerede forgrundsspiralgalakse med fint svungne støvbaner NGC 1532, er så tæt på sin følgesvend - baggrundsgalaksen, også en spiral, NGC 1531, med sin lyse kerne lige over midten af ​​NGC 1532 - at den bliver forvrænget: En af ​​dens spiralarme er skæv og faner af støv og gas er synlige over skiven.Den kosmiske dans fører til en anden dramatisk effekt: En helt ny generation af massive stjerner er blevet dannet i NGC 1532 på grund af denne interaktion.De unge stjerner er synlige som lilla objekter i spiralarmene.Dette udsøgte billede blev lavet ved hjælp af det danske 1,52-meter teleskop på ESOs La Silla-observatorium i Chile.Det er baseret på data indsamlet gennem tre forskellige filtre: B, V og R.Synsfeltet er 12x12 bueminutter.

26. januar 2009: The 8.2m diameter main mirror of Antu, the first Unit Telescope of ESO's Very Large Telescope, is being cleaned using carbon dioxide snow. While the telescope enclosure is maintained extremely clean, the mirrors are exposed to the elements during the observations. Consequently, dust from the desert slowly accumulates over the surface of the mirror, making it less reflective over time. The mirror's surface is so delicate that normal cleaners used for household mirrors are not appropriate for telescopes. Observatories have developed other methods, such as this one using carbon dioxide snow. The tiny CO2 snowflakes in the white plume have a temperature of almost minus 80 degrees Celsius; when they land on the mirror, which is at room temperature, they cause minuscule 'explosions' that detach the dust grains from the surface. The dust then floats away, leaving the mirror clean. The process is nevertheless very delicate: should Alain Gilliotte, the ...

12. januar 2009: The Orion Nebula is arguably the finest of all nebulae within the Milky Way visible from the Northern Hemisphere. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of Messier 42 — as it is also known — glow with fantastic colours and shapes, giving us a bird’s eye view of one of the greatest star forming nurseries in our part of the Milky Way. Messier 42 is a complex of glowing gas, mostly hydrogen but also helium, carbon, nitrogen, and oxygen in decreasing amounts, located 1,500 light-years away. At its very heart, we find the Trapezium, a group of four very hot stars that illuminate the nebula. They are the brightest of an extended cluster of several thousand young stars many of which lie unseen within the opaque gas and dust. Amazingly, whilst the Orion Nebula is easy to identify ...

15. december 2008: The striking, large spiral galaxy NGC 1232, and its distorted companion shaped like the greek letter "theta". The pair is located roughly 60 million light-years away in the constellation Eridanus (The River). Billions of stars and dark dust are caught up in this beautiful gravitational swirl. The blue spiral arms with their many young stars and star-forming regions make a striking contrast with the yellow-reddish core of older stars. This image is based on data acquired with the 1.5 m Danish telescope at the ESO La Silla Observatory in Chile, through three filters (B: 900 s, V: 400 s, R: 400 s).

8. december 2008: About a year ago, ESO kindly agreed to donate a surplus van to the Colegio Hellen Keller, a school for children with visual disabilities, located in Santiago, Chile. The school was in desperate need of some form of transport as there were many children who could either not attend school at all, or had to spend the weekdays away from their family, simply because they could not make the daily journey on public transport, due to their disabilities. The initial idea was to donate one of the bus used to carry staff to Paranal. However, it became clear that this big van was not ideal for the school, especially with rising fuel prices. ESO kindly offered to donate the proceeds from the sale of the van instead, which was in excess of 4.000.000 Chilean Pesos (about 5,000 EUR). The school set up a fund to raise the rest of the ...

1. december 2008: Supernova 2008bk in the spiral galaxy NGC 7793 was discovered at the end of March 2008 by amateur astronomer Berto Monard from South Africa. The galaxy is 13 million light-years away in the direction of Sculptor constellation. This supernova is a typical example of a massive star that exploded at the end of its life. But this time, the astronomers were able not only to see the explosion, but to precisely pinpoint the star that exploded, a rather rare achievement. This was made possible because the explosion site had been observed several times with the help of ESO's Very Large Telescope, the latest images having been observed only a few months before the explosion with the new HAWK-I instrument. An European team of astronomers, led by Seppo Mattila of University of Turku, Finland, then observed the explosion site again two months after the supernova's discovery, this time with the VLT's ...

25. november 2008: ESOs Very Large Telescope (VLT) på det 2600 meter høje Cerro Paranal i den chilenske Atacama-ørkenen, er ESOs primære observatorium til observationer i synligt og infrarødt lys.Alle fire enhedsteleskoper (Unit Telescopes (UTs)) med primær-spejle på 8,2 meter i diameter er individuelt i drift med en stor samling af instrumenter og har allerede gjort forbløffende videnskabelige opdagelser.VLT giver også mulighed for at kombinere lyset fra de fire enhedsteleskoper til at arbejde sammen som et interferometer kaldet Very Large Telescope Interferometer (VLTI)VLTI, med sin egen suite af instrumenter, giver en billedopløsning på milli-buesekund-niveau samt astrometri med en præcision på 10 mikro-buesekunder.Udover 8,2 meter-teleskoperne, er VLTI suppleret med fire hjælpeteleskoper (Auxiliary Telescopes (AT)) hver på 1,8 meter i diameter, til at forbedre instrumentets kapacitet og muliggøre fuld natlig brug året rundt.Den teleskopbygning, der indeholder VLT Survey Telescope (2,6-meter i diameter), er synlig i midten af billedet.

11. november 2008: The Carina Nebula is a large bright nebula that surrounds several clusters of stars. It contains two of the most massive and luminous stars in our Milky Way galaxy, Eta Carinae and HD 93129A. Located 7500 light years away, the nebula itself spans some 260 light years across, about 7 times the size of the Orion Nebula, and is shown in all its glory in this mosaic. It is based on images collected with the 1.5-m Danish telescope at ESO's La Silla Observatory. Being brighter than one million Suns, Eta Carinae (the brightest star in this image) is the most luminous star known in the Galaxy, and has most likely a mass over 100 times that of the Sun. It is the closest example of a luminous blue variable, the last phase in the life of a very massive star before it explodes in a fiery supernova. Eta Carinae is ...

4. november 2008: M1-67 is the youngest wind-nebula around a Wolf-Rayet star, called WR124, in our Galaxy. These Wolf-Rayet stars start their lives with dozens of times the mass of our Sun, but loose most of it through a powerful wind, which is ultimately responsible for the formation of the nebula. Ten years ago, Hubble Space Telescope observations revealed a wealth of small knots and substructures inside the nebula. The same team, led by Cédric Foellmi (ESO), has now used ESO's Very Large Telescope (VLT) to watch how these structures have evolved and what they can teach us about stellar winds, their chemistry, and how they mix with the surrounding interstellar medium, before the star will eventually blow everything away in a fiery supernova explosion. The image is based on FORS1 data obtained by the Paranal Science team with the VLT through 2 wide (B and V) and 3 narrow-band filters.

30. september 2008: A night of work for the Paranal Observatory, in the Chilean Atacama Desert. This picture, taken on 20 September, shows the incredible beauty of the night sky above the most advanced telescope in the world, ESO's Very Large Telescope. The Milky Way is clearly seen in this superb image.

22. september 2008: Composite colour-coded image of another magnificent spiral galaxy, NGC 7424, at a distance of 40 million light-years. It is based on images obtained with the multi-mode VIMOS instrument on the ESO Very Large Telescope (VLT) in three different wavelength bands. The image covers 6.5 x 7.2 square arcminutes on the sky. North is up and East is to the right. Read more about this superb object in the ESO Press Release eso0436.

21. august 2008: Billede af kuglehoben NGC 3201 i 'falske farver', optaget med instrumentet WFI på teleskopet ESO/MPG 2,2 m på La Silla. Kugleformede stjernehobe er store stjernesamlinger med op mod flere millioner stjerner. Det er nogle af de ældste objekter i Universet, og de er formentlig dannetsamtidig med Mælkevejen, tidligt efter Big Bang. Kuglehoen her befinder sig omkring 16 000 lysår fra Jorden i retning mod stjernebilledet Vela. De data, som er anvendt, er indhøstet som en del af ESO Imaging Survey - et offentligt tilgængeligt dataset, som udføres af ESO og medlemstaterne i forberedelse til VLT First Light. Det originale billede og de tilhørende astronomiske data kan hentes i dette link, hvor der også kan findes mange andre flotte billeder: EIS Pre-Flames Survey Data Release pages.

14. august 2008: The centre of our Milky Way galaxy is located in the southern constellation Sagittarius (The Archer) and is "only" 26,000 light-years away. On high-resolution images, it is possible to discern thousands of individual stars within the central, one light-year wide region. Using the motions of these stars to probe the gravitational field, observations over the last decade have shown that a mass of about 3 million times that of the Sun is concentrated within a radius of only 10 light-days of the compact radio and X-ray source SgrA* (Sagittarius A) at the centre of the star cluster. This means that SgrA* is the most likely counterpart of the black hole believed to exist at the centre of our Galaxy. This image was obtained in mid-2002 with the NACO instrument at the 8.2-m VLT Yepun telescope. It combines frames in three infrared wavebands between 1.6 and 3.5 µm. The compact objects ...

7. august 2008: Paranal, the site of the VLT, was chosen for its unique characteristics: extreme dryness, very low cloud coverage, high altitude, and distant from any source of pollution. This wide-angle shot of the Atacama desert around Paranal, which shows the VLT and, in foreground, VISTA, summarizes it all. Photo taken in November 2007.