Parhaat 100 kuvaa

Tämä uusi, näyttävä tähtien lastentarhasta IC 2944 otettu kuva julkistetaan ESO:n VLT-teleskoopin 15-vuotisjuhlien kunniaksi. Kuva esittää myös joukkoa tummina vaaleanpunaista hohtavan kaasun pilveä vasten näkyviä tiheitä tomupilviä, jotka tunnetaan Thackerayn globuleina. Nämä globulit ovat kuumien, nuorten tähtien ultraviolettisäteilyn raivokkaassa pommituksessa. Ne sekä kuluvat loppuun että myös pirstaloituvat, aivan kuten kuumalle paistinpannulle pudotetut voimöykyt. On todennäköistä, että Thackerayn globulit tuhoutuvat ennen kuin luhistuvat ja muodostavat tähtiä.

The OmegaCAM imager on ESO’s VLT Survey Telescope has captured this glittering view of the stellar nursery called Sharpless 29. Many astronomical phenomena can be seen in this giant image, including cosmic dust and gas clouds that reflect, absorb, and re-emit the light of hot young stars within the nebula.

Tämä VLT-teleskoopin kuva Thorin kypärä -sumusta otettiin juhlistamaan ESO:n 50-vuotismerkkipäivää, 5. lokakuuta 2012. Kuvan ottamista avusti Brigitte Bailleul, Tviittaa itsesi VLT:lle! -kilpailun voittaja. Havainnot lähetettiin suorana Internetiin Paranalin observatoriolta, Chilestä. Myös nimellä NGC 2359 tunnettu kohde on tähtien lastentarha Ison koiran tähdistössä (Canis Major). Kypärän muotoinen kaasusumu on noin 15 000 valovuoden etäisyydellä Maasta ja on halkaisijaltaan yli 30 valovuotta. Kypärä on kosminen kupla, joka on muodostunut lähellä kuplan keskustaa sijaitsevan kirkkaan, massiivisen tähden aurinkotuulen puhaltaessa ympäröivän molekyylipilven halki.

Tämä hätkähdyttävä kuva on otettu VLT:n FORS2 instrumentilla ja se esittää kaunista galaksiparia NGC 4438 ja NGC 4435 lempinimeltään 'Silmät'. Kuvassa ylhäällä oleva suurempi galaksi NGC 4438 on luultavasti ollut aikoinaan spiraaligalaksi, mikä koki merkittävän muodonmuutoksen menneisyydessä tapahtuneen törmäyksen seurauksena. Galaksit kuuluvat Neitsyen galaksijoukkoon ja ovat noin 50 miljoonan valovuoden etäisyydellä.

The second of three images of ESO’s GigaGalaxy Zoom project is a new and wonderful 340-million-pixel vista of the central parts of our galactic home, a 34 by 20-degree wide image that provides us with a view as experienced by amateur astronomers around the world. Taken by Stéphane Guisard, an ESO engineer and world-renowned astrophotographer, from Cerro Paranal, home of ESO’s Very Large Telescope, this second image directly benefits from the quality of Paranal’s sky, one of the best on the planet. The image shows the region spanning the sky from the constellation of Sagittarius (the Archer) to Scorpius (the ...

This colour-composite image of the Helix Nebula (NGC 7293) was created from images obtained using the Wide Field Imager (WFI), an astronomical camera attached to the 2.2-metre Max-Planck Society/ESO telescope at the La Silla observatory in Chile. The blue-green glow in the centre of the Helix comes from oxygen atoms shining under effects of the intense ultraviolet radiation of the 120 000 degree Celsius central star and the hot gas. Further out from the star and beyond the ring of knots, the red colour from hydrogen and nitrogen is more prominent. A careful look at the central part of this ...

The central parts of our Galaxy, the Milky Way, as observed in the near-infrared with the NACO instrument on ESO's Very Large Telescope. By following the motions of the most central stars over more than 16 years, astronomers were able to determine the mass of the supermassive black hole that lurks there.

A reproduction of a composite colour image of the Horsehead Nebula and its immediate surroundings. It is based on three exposures in the visual part of the spectrum with the FORS2 multi-mode instrument at the 8.2-m KUEYEN telescope at Paranal. It was produced from three images, obtained on February 1, 2000, with the FORS2 multi-mode instrument at the 8.2-m KUEYEN Unit Telescope and extracted from the VLT Science Archive Facility . The frames were obtained in the B-band (600 sec exposure; wavelength 429 nm; FWHM 88 nm; here rendered as blue), V-band (300 sec; 554 nm; 112 nm; green) and ...

This spectacular image of the Orion Nebula star-formation region was obtained from multiple exposures using the HAWK-I infrared camera on ESO’s Very Large Telescope in Chile. This is the deepest view ever of this region and reveals more very faint planetary-mass objects than expected.

ESO:n Paranalin observatorion VST-teleskooppi on taltioinut näyttävän, tähtiä muodostavan Kölin sumun. Kuvaa ottamassa oli Chilen presidentti, Sebastián Piñera, tämän vieraillessa observatoriolla 5. kesäkuuta 2012. Se julkaistiin teleskoopin avajaisjuhlallisuuksissa Napolissa 6. joulukuuta 2012.

Outo galaksi Centaurus A esittäytyy uudessa Euroopan eteläisen observatorion tuottamassa kuvassa, joka on otettu MPG/ESO 2.2-metrin teleskoopin Wide Field Imager -havaintolaitteella ESO:n La Sillan observatoriolla, Chilessä. Yli 50 tunnin valotusajalla tämä on todennäköisesti syvin milloinkaan muodostettu kuva tästä erikoisesta ja näyttävästä kohteesta.

This broad image of the Carina Nebula, a region of massive star formation in the southern skies, was taken in infrared light using the HAWK-I camera on ESO’s Very Large Telescope. Many previously hidden features, scattered across a spectacular celestial landscape of gas, dust and young stars, have emerged.
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This VST image may be the best portrait of the globular star cluster Omega Centauri ever made. Omega Centauri, in the constellation of Centaurus (The Centaur), is the largest globular cluster in the sky, but the very wide field of view of VST and its powerful camera OmegaCAM can encompass even the faint outer regions of this spectacular object. This view includes about 300 000 stars. The data were processed using the VST-Tube system developed by A. Grado and collaborators at the INAF-Capodimonte Observatory.

The first released VST image shows the spectacular star-forming region Messier 17, also known as the Omega Nebula or the Swan Nebula, as it has never been seen before. This vast region of gas, dust and hot young stars lies in the heart of the Milky Way in the constellation of Sagittarius (The Archer). The VST field of view is so large that the entire nebula, including its fainter outer parts, is captured — and retains its superb sharpness across the entire image. The data were processed using the Astro-WISE software system developed by E.A. Valentijn and collaborators at Groningen ...

This new image of the reflection nebula Messier 78 was captured using the Wide Field Imager camera on the MPG/ESO 2.2-metre telescope at the La Silla Observatory, Chile. This colour picture was created from many monochrome exposures taken through blue, yellow/green and red filters, supplemented by exposures through a filter that isolates light from glowing hydrogen gas. The total exposure times were 9, 9, 17.5 and 15.5 minutes per filter, respectively.
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This composite image shows an exoplanet (the red spot on the lower left), orbiting the brown dwarf 2M1207 (centre). 2M1207b is the first exoplanet directly imaged and the first discovered orbiting a brown dwarf (see the press release). It was imaged the first time by the VLT in 2004. Its planetary identity and characteristics were confirmed after one year of observations in 2005. 2M1207b is a Jupiter-like planet, 5 times more massive than Jupiter. It orbits the brown dwarf at a distance 55 times larger than the Earth to the Sun, nearly twice as far as Neptune is from the ...

This image, the first to be released publicly from VISTA, the world’s largest survey telescope, shows the spectacular star-forming region known as the Flame Nebula, or NGC 2024, in the constellation of Orion (the Hunter) and its surroundings. In views of this evocative object in visible light the core of the nebula is completely hidden behind obscuring dust, but in this VISTA view, taken in infrared light, the cluster of very young stars at the object’s heart is revealed. The wide-field VISTA view also includes the glow of the reflection nebula NGC 2023, just below centre, and the ghostly outline ...

This magnificent 360-degree panoramic image, covering the entire southern and northern celestial sphere, reveals the cosmic landscape that surrounds our tiny blue planet. This gorgeous starscape serves as the first of three extremely high-resolution images featured in the GigaGalaxy Zoom project, launched by ESO within the framework of the International Year of Astronomy 2009 (IYA2009). The plane of our Milky Way Galaxy, which we see edge-on from our perspective on Earth, cuts a luminous swath across the image. The projection used in GigaGalaxy Zoom place the viewer in front of our Galaxy with the Galactic Plane running horizontally through the ...

Three-colour composite image of the Omega Nebula (Messier 17, or NGC 6618), based on images obtained with the EMMI instrument on the ESO 3.58-metre New Technology Telescope at the La Silla Observatory. North is down and East is to the right in the image. It spans an angle equal to about one third the diameter of the Full Moon, corresponding to about 15 light-years at the distance of the Omega Nebula. The three filters used are B (blue), V ("visual", or green) and R (red).
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This colour image of the region known as NGC 2264 — an area of sky that includes the sparkling blue baubles of the Christmas Tree star cluster and the Cone Nebula — was created from data taken through four different filters (B, V, R and H-alpha) with the Wide Field Imager at ESO's La Silla Observatory, 2400 m high in the Atacama Desert of Chile in the foothills of the Andes. The image shows a region of space about 30 light-years across.
This image is available as a mounted image in the ESOshop.
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This spectacular image of the large spiral galaxy NGC 1232 was obtained on September 21, 1998, during a period of good observing conditions. It is based on three exposures in ultra-violet, blue and red light, respectively. The colours of the different regions are well visible : the central areas contain older stars of reddish colour, while the spiral arms are populated by young, blue stars and many star-forming regions. Note the distorted companion galaxy on the left side, shaped like the greek letter "theta".
NGC 1232 is located 20º south of the celestial equator, in the constellation Eridanus (The River). ...

OmegaCAM — the wide-field optical camera on ESO’s VLT Survey Telescope (VST) — has captured the spectacular Orion Nebula and its associated cluster of young stars in great detail, producing this beautiful new image. This famous object, the birthplace of many massive stars, is one of the closest stellar nurseries, at a distance of about 1350 light-years.

Antennas of the Atacama Large Millimeter/submillimeter Array (ALMA), on the Chajnantor Plateau in the Chilean Andes. The Large and Small Magellanic Clouds, two companion galaxies to our own Milky Way galaxy, can be seen as bright smudges in the night sky, in the centre of the photograph.

Tämä häikäisevä kuva Linnunradan keskiosista otettiin ESO:n Chilessä sijaitsevalla Paranalin observatorion VISTA-kartoitusteleskoopilla. Tämä suunnaton kuva on kooltaan 108 500 kertaa 81 500 pikseliä ja koostuu lähes yhdeksästä miljardista pikselistä. Se koostettiin yhdeksi monumentaaliseksi mosaiikkikuvaksi yhdistämällä tuhansia yksittäisiä VISTA:n kuvia, jotka oli otettu kolmella eri infrapunasuotimella. Tämä aineisto muodostaa osan julkista VVV-kartoitusta ja sitä on käytetty tutkimaan paljon suurempaa määrää Linnunradan keskustan tähtiä kuin milloinkaan aikaisemmin. Koska VISTA:n kamera on herkkä infrapunavalolle, se näkee läpi suurimmasta osasta näkyvän valon teleskooppeja haittaavaa tomua, joskin useita läpinäkymättömiä tomuarihmastoja on yhä hyvin näkyvissä tässä kuvassa.
Tämä kuva on liian suuri näytettäväksi täydellä resoluutiolla ja ...

ESO Photo Ambassador Babak Tafreshi snapped this remarkable image of the antennas of the Atacama Large Millimeter/submillimeter Array (ALMA), set against the splendour of the Milky Way. The richness of the sky in this picture attests to the unsurpassed conditions for astronomy on the 5000-metre-high Chajnantor plateau in Chile’s Atacama region.
This view shows the constellations of Carina (The Keel) and Vela (The Sails). The dark, wispy dust clouds of the Milky Way streak from middle top left to middle bottom right. The bright orange star in the upper left is Suhail in Vela, while the similarly orange star in ...

This panoramic view of the Chajnantor plateau, spanning about 180 degrees from north (on the left) to south (on the right) shows the antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) ranged across the unearthly landscape. Some familiar celestial objects can be seen in the night sky behind them. These crystal-clear night skies explain why Chile is the home of not only ALMA, but also several other astronomical observatories. This image is just part of an even wider panorama of Chajnantor.
In the foreground, the 12-metre diameter ALMA antennas are in action, working as one giant telescope, during the observatory’s ...

The nearby star-forming region around the star R Coronae Australis imaged by the Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile. This picture, which covers a field of 33.7 x 31.9 arcminutes (about the diameter of the full Moon), is a combination of twelve CCD frames, 67 megapixels each, taken through B, V and R filters, with four exposures of five minutes each.
This image is available as a mounted image in the ESOshop.
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Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimetre data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the stars and the galaxy’s characteristic dust lane in close to "true colour".
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The Chandra Deep Field South, observed in the U-, B-, and R-bands with ESO''s VIMOS and WFI instruments. The U-band VIMOS observations were made over a period of 40 hours and constitute the deepest image ever taken from the ground in the U-band. The image covers a region of 14.1 x 21.6 arcminutes on the sky and shows galaxies that are 1 billion times fainter than can be seen by the unaided eye. The VIMOS R-band image was assembled by the ESO/GOODS team from archival data, while the WFI B-band image was produced by the GABODS team.
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This spectacular panoramic view combines a new image of the field around the Wolf–Rayet star WR 22 in the Carina Nebula (right) with an earlier picture of the region around the unique star Eta Carinae in the heart of the nebula (left). The picture was created from images taken with the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile.
This image is available as a mounted image in the ESOshop.
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It’s a real treat for photographers and astronomers alike: our skies are currently witnessing a phenomenon known as a syzygy — when three celestial bodies (or more) nearly align themselves in the sky. When celestial bodies have similar ecliptic longitude, this event is also known as a triple near-conjunction. Of course, this is just a trick of perspective, but this doesn't make it any less spectacular. In this case, these bodies are three planets, and the only thing needed to enjoy the show is a clear view of the sky at sunset.
Luckily, this is what happened for ESO photo ...

Sunset is typically a sign that another working day is over. City lights are slowly switched on as people return home eager to enjoy the evening and a good night’s sleep. However, this does not apply to astronomers working at an observatory such as ESO’s Paranal Observatory in Chile. Observing starts as soon as the Sun has disappeared below the horizon. Everything needs to be ready before dusk.
This panoramic photograph captures the ESO Very Large Telescope (VLT) against a beautiful twilight on Cerro Paranal. The enclosures of the VLT stand out in the picture as the telescopes in them ...

The Antennae Galaxies (also known as NGC 4038 and 4039) are a pair of distorted colliding spiral galaxies about 70 million light-years away, in the constellation of Corvus (The Crow). This view combines ALMA observations, made in two different wavelength ranges during the observatory’s early testing phase, with visible-light observations from the NASA/ESA Hubble Space Telescope.
The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution. ALMA observes at much longer wavelengths which makes it much harder to obtain comparably sharp images. However, when the full ALMA array ...

Infrared view of the Cat’s Paw Nebula (NGC 6334) taken by VISTA. NGC 6334 is a vast region of star formation about 5500 light-years from Earth in the constellation of Scorpius. The whole gas cloud is about 50 light-years across. NGC 6334 is one of the most active nurseries of young massive stars in our galaxy, some nearly ten times the mass of our Sun and most born in the last few million years. The images were taken through Y, J and Ks filters (shown as blue, green and red respectively) and the exposure time was five minutes per filter. ...

This wide-field view of the Orion Nebula (Messier 42), lying about 1350 light-years from Earth, was taken with the VISTA infrared survey telescope at ESO’s Paranal Observatory in Chile. The new telescope’s huge field of view allows the whole nebula and its surroundings to be imaged in a single picture and its infrared vision also means that it can peer deep into the normally hidden dusty regions and reveal the curious antics of the very active young stars buried there. This image was created from images taken through Z, J and Ks filters in the near-infrared part of the spectrum. ...

Yhden neliöasteen kuva Tarantellasumusta ja sen ympäristöstä. Hämähäkkimäinen sumu näkyy ylhäällä kuvan keskellä. Hieman alas ja oikealle sijaitseva rihmojen verkosto pitää sisällään kuuluisan supernovan SN 1987A. Monet muut punertavat sumut näkyvät kuvassa, kuten myös nimellä NGC 2100 tunnettu nuorten tähtien joukko vasemmalla. Teknistä tietoa: kuva perustuu havaintoihin, jotka tekivät Joao Alves (Calar Alto, Espanja), Benoit Vandame ja Yuri Beletsky (ESO) La Sillan 2.2-metrin teleskoopin WFI-havaintolaitteella (Wide Field Imager). Havaintoaineisto koostuu 2x2 WFI-mosaiikista B- ja V-kaistoilla sekä H-alfa- ja [OIII]-kapeakaistakuvista. Aineiston käsitteli ensin ESO/MVM-ohjelmistolla ESOn ADP-ryhmä (Advanced Data Products).
Kuva on saatavana kehystettynä ESOshopista.

While ALMA is currently under construction, astronomers are already doing millimetre and submillimetre astronomy at Chajnantor, with the Atacama Pathfinder Experiment (APEX). This is a new-technology 12-m telescope, based on an ALMA prototype antenna, and operating at the ALMA site. It has modified optics and an improved antenna surface accuracy, and is designed to take advantage of the excellent sky transparency working with wavelengths in the 0.2 to 1.4 mm range.
This image is available as a mounted image in the ESOshop

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 ...

Tässä uudessa, hätkähdyttävässä kuvassa Chilessä sijaitsevalta ESOn La Sillan obsrvatoriolta nuoret tähdet värjöttelevät yhdessä taustan hohtavia kaasupilviä ja tomuväyliä vasten. Nimellä NGC 3293 tunnettu tähtijoukko olisi itse ollut vain kaasu- ja tomupilvi noin kymmenen miljoonaa vuotta sitten, mutta tähtien alkaessa muodostua siitä tuli tässä näkemämme kirkas tähtijoukko. Tämänkaltaiset joukot ovat taivaallisia laboratorioita, joiden avulla tähtitieteilijät voivat oppia lisää siitä kuinka tähdet kehittyvät.

Tässä kuvassa on Barnard 59, osa valtavaa tähtienvälisen tomun muodostamaa pimeää pilveä, jota kutsutaan Piippusumuksi. Tämä uusi ja hyvin yksityiskohtainen kuva pimeänä sumuna tunnetusta kohteesta taltioitiin ESO:n La Sillan observatorion MPG/ESO 2.2 metrin teleskoopin Wide Field Imager -havaintolaitteella. Kuva on niin suuri, että on suositeltavaa käyttää zoomattavaa versiota, jotta sen piirteet tulevat parhaiten näkyviin.

ESO Photo Ambassador Stéphane Guisard captured this astounding panorama from the site of ALMA, the Atacama Large Millimeter/submillimeter Array, in the Chilean Andes. The 5000-metre-high and extremely dry Chajnantor plateau offers the perfect place for this state-of-the-art telescope, which studies the Universe in millimetre- and submillimetre-wavelength light.
Numerous giant antennas dominate the centre of the image. When ALMA is complete, it will have a total of 54 of these 12-metre-diameter dishes. Above the array, the arc of the Milky Way serves as a resplendent backdrop. When the panorama was taken, the Moon was lying close to the centre of the ...

A total eclipse of the Moon is an impressive spectacle. But it also provides another viewing opportunity: a dark, moonlight-free starry sky. At Cerro Paranal in the Chilean Atacama Desert, one of the most remote places in the world, the distance from sources of light pollution makes the night sky all the more remarkable during a total lunar eclipse.
This panorama photo, taken by ESO Photo Ambassador Yuri Beletsky, shows the view of the starry sky from the site of ESO’s Very Large Telescope (VLT) at Cerro Paranal during the total lunar eclipse of 21 December 2010. The reddish disc ...

This dramatic infrared image shows the nearby star formation region Monoceros R2, located some 2700 light-years away in the constellation of Monoceros (the Unicorn). The picture was created from exposures in the near infrared bands Y, J and Ks taken by the VISTA survey telescope at ESO’s Paranal Observatory. Monoceros R2 is an association of massive hot young stars illuminating a beautiful collection of reflection nebulae, embedded in a large molecular cloud.
This image is available as a mounted image in the ESOshop.

The ESO Very Large Telescope (VLT) during observations. In this picture, taken from the VLT platform looking north-northwest at twilight, the four 8.2-metre Unit Telescopes (UTs) are visible. From left to right, Antu, Kueyen, Melipal and Yepun, the Mapuche names for the VLT's giant telescopes. In front of the UTs are the four 1.8-metre Auxiliary Telescopes (ATs), entirely dedicated to interferometry, a technique which allows astronomers to see details up to 25 times finer than with the individual telescopes. The configuration of the ATs can be changed by moving them across the platform between 30 different observing positions. One of ...

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 ...

Three-colour composite mosaic image of the Eagle Nebula (Messier 16, or NGC 6611), based on images obtained with the Wide-Field Imager camera on the MPG/ESO 2.2-metre telescope at the La Silla Observatory. At the centre, the so-called “Pillars of Creation” can be seen. This wide-field image shows not only the central pillars, but also several others in the same star-forming region, as well as a huge number of stars in front of, in, or behind the Eagle Nebula. The cluster of bright stars to the upper right is NGC 6611, home to the massive and hot stars that illuminate the ...

Using ESO's Very Large Telescope, an international team of astronomers has discovered a stunning rare case of a triple merger of galaxies. This system, which astronomers have dubbed 'The Bird' - although it also bears resemblance with a cosmic Tinker Bell - is composed of two massive spiral galaxies and a third irregular galaxy.
In this image, a 30-min VLT/NACO K-band exposure has been combined with archive HST/ACS B and I-band images to produce a three-colour image of the 'Bird' interacting galaxy system. The NACO image has allowed astronomers to not only see the two previously known galaxies, but to ...

This is the sharpest image ever taken by ALMA — sharper than is routinely achieved in visible light with the NASA/ESA Hubble Space Telescope. It shows the protoplanetary disc surrounding the young star HL Tauri. These new ALMA observations reveal substructures within the disc that have never been seen before and even show the possible positions of planets forming in the dark patches within the system.

This view shows several of the ALMA antennas and the central regions of the Milky Way above. In this wide field view, the zodiacal light is seen upper right and at lower left Mars is seen. Saturn is a bit higher in the sky towards the centre of the image. The image was taken during the ESO Ultra HD (UHD) Expedition.

This beautiful new image, taken during a time-lapse set at the Atacama Large Millimeter/submillimeter Array (ALMA) is another dramatic Ultra High Definition photograph from the ESO Ultra HD Expedition. ALMA, located at 5000 metres above sea level on the remote and empty Chajnantor Plateau in the Chilean Andes, marks the second destination for the four ESO Photo Ambassadors [1] on their 17-day trip. The ambassadors are equipped with state-of-the-art Ultra HD tools to help them capture the true majesty of sights like the one pictured here [2] [3].
Some of the 66 high-precision antennas that comprise ALMA are visible here, ...

Tämä eloisa uusi kuva esittää uusia tähtiä muodostavaa pimeää pilveä sekä ryhmää kirkkaita tähtiä, jotka ovat jo tulleet esille pölyisästä tähtien lastentarhastaan. Tämä pilvi tunnetaan nimellä Lupus 3 ja se sijaitsee noin 600 valovuoden etäisyydellä Maasta Skorpionin tähdistössä (Scorpius). On todennäköistä, että Aurinko muodostui samanlaisessa tähtienmuodostusalueessa yli neljä miljardia vuotta sitten. Tämä kuva otettiin La Sillan observatoriolla Chilessä sijaitsevalla MPG/ESO 2.2-metrin teleskoopilla. Se on paras näkyvällä valolla tästä vähän tunnetusta kohteesta otettu kuva.

Tämä kirkas kokoelma tähtiä on 47 Tucanae (NGC 104), tässä ESO:n Paranalin observatoriolla Chilessä sijaitsevan VISTA-teleskoopin (Visible and Infrared Survey Telescope for Astronomy) kuvaamana. Tämä tähtijoukko sijaitsee noin 15 tuhannen valovuoden etäisyydellä meistä ja käsittää miljoonia tähtiä, joista osa on epätavallisia ja eksoottisia. Kuva otettiin osana VISTA:n Magellanin pilvien kartoitusta, joka on Linnunrataamme lähellä sijaitsevien kahden pienen galaksin, Magellanin pilvien, aluetta kartoittava projekti.

This panoramic view of the Chajnantor Plateau shows the site of the Atacama Large Millimeter/submillimeter Array (ALMA), taken from near the peak of Cerro Chico. Babak Tafreshi, an ESO Photo Ambassador, has succeeded in capturing the feeling of solitude experienced at the ALMA site, 5000 metres above sea level in the Chilean Andes. Light and shadow paint the landscape, enhancing the otherworldly appearance of the terrain. In the foreground of the image, clustered ALMA antennas look like a crowd of strange, robotic visitors to the plateau. When the telescope is completed in 2013, there will be a total of 66 ...

In the search for distant worlds, few telescopes have had as much success as ESO's 3.6-metre telescope and the Swiss 1.2-metre Leonhard Euler Telescope, both of which are shown in this image.
The 3.6-metre telescope is home to HARPS (High Accuracy Radial velocity Planet Searcher), a spectrograph with unrivalled precision, and holder of many records in the field of exoplanet research, including the discovery of the least massive exoplanet, as well as of the smallest ever measured. Together with HARPS, the Leonhard Euler Telescope has allowed astronomers to find that six exoplanets from a larger sample of 27 were orbiting ...

This impressive panoramic image depicts the Chajnantor Plateau — home of the Atacama Large Millimeter/submillimeter Array (ALMA) — with the majestic Licancabur volcano in the background. Watched over by Licancabur, a icy forest of penitentes (Spanish for “penitents”) cluster in the foreground. The penitentes are a curious natural phenomenon found in high-altitude regions. They are thin spikes of hardened snow or ice, with sharp edges pointing towards the Sun, reaching heights from a few centimetres up to several metres. You can read more about penitentes in a previous Picture of the Week (potw1221).
The Licancabur volcano, with an altitude of ...

On a cold dark night on Mars, in the middle of an arid desert, a narrow road lit by artificial lights winds its way up to a lonely human outpost on the top of an old mountain. Or at least, that’s what a science fiction fan might make of this almost unearthly view.
The photograph actually shows ESO’s Paranal Observatory, home to the Very Large Telescope (VLT), on Earth. Nevertheless, it’s easy to imagine it as a future view of Mars, perhaps at the end of the century. Which is why Julien Girard, who took this photograph, calls it “Mars ...

One of the major enemies of astronomers is the Earth’s atmosphere, which makes celestial objects appear blurry when observed by ground-based telescopes. To counteract this, astronomers use a technique called adaptive optics, in which computer-controlled deformable mirrors are adjusted hundreds of times per second to correct for the distortion of the atmosphere.
This spectacular image shows Yepun [1], the fourth 8.2-metre Unit Telescope of ESO’s Very Large Telescope (VLT) facility, launching a powerful yellow laser beam into the sky. The beam creates a glowing spot — an artificial star — in the Earth’s atmosphere by exciting a layer of sodium ...

Babak Tafreshi, one of the ESO Photo Ambassadors, has captured a curious phenomenon on the Chajnantor plateau, the site of the Atacama Large Millimeter/submillimeter array (ALMA).
These bizarre ice and snow formations are known as penitentes (Spanish for “penitents”). They are illuminated by the light of the Moon, which is visible on the right on the photograph. On the left, higher in the sky, the Large and Small Magellanic Clouds can be faintly seen, while the reddish glow of the Carina Nebula appears close to the horizon on the far left.
The penitentes are natural marvels found in high-altitude regions, ...

This panorama photograph shows the European Southern Observatory’s Headquarters in Garching, near Munich, Germany. The image shows the view from the roof of the main building just after sunset. This is the scientific, technical and administrative centre for ESO’s operations, and the base from which many astronomers conduct their research. The scientists, technicians and administrators who work here come from many different backgrounds, but all have one thing in common: a passion for astronomy.
ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive astronomical observatory. ESO operates telescopes at three observing sites in Chile: La ...

This very detailed enhanced-colour image from ESO’s Very Large Telescope shows the dramatic effects of very young stars on the dust and gas from which they were born in the star-forming region NGC 6729. The baby stars are invisible in this picture, being hidden behind dust clouds at the upper left of the picture, but material they are ejecting is crashing into the surroundings at speeds of that can be as high as one million kilometres per hour. This picture was taken by the FORS1 instrument and records the scene in the light of glowing hydrogen and sulphur.

A bird soaring over the remote, sparsely populated Atacama Desert in northern Chile — possibly the driest desert in the world — might be surprised to come upon the technological oasis of ESO’s Very Large Telescope (VLT) at Paranal. The world’s most advanced ground-based facility for astronomy, the site hosts four 8.2-metre Unit Telescopes, four 1.8-metre Auxiliary Telescopes, the VLT Survey Telescope (VST), and the 4.1-metre Visible and Infrared Survey Telescope for Astronomy (VISTA), seen in the distance on the next mountain peak over from the main platform.
This aerial view also shows other structures, including the Observatory Control Room ...

This marvellous aerial photograph of the home of ESO’s Very Large Telescope (VLT), fully demonstrates the superb quality of the observing site. In the foreground we see the Paranal Observatory, located at an altitude of 2,600 metres on mount Paranal in Chile. In the background we can see the snow-capped, 6,720 meter-high volcano Llullaillaco, located a mind-boggling 190 km further East on the Argentinean border. This image is a testimony of the magnificent quality of the air and the ideal conditions for observing at this remote site.
Clearly visible in the image are the domes of the four giant 8.2-metre ...

The third image of ESO’s GigaGalaxy Zoom project is an amazing vista of the Lagoon Nebula taken with the 67-million-pixel Wide Field Imager attached to the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. The image covers more than one and a half square degree — an area eight times larger than that of the Full Moon — with a total of about 370 million pixels. It is based on images acquired using three different broadband filters (B, V, R) and one narrow-band filter (H-alpha).
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The massive star factory known as the Trifid Nebula was captured in all its glory with the Wide-Field Imager camera attached to the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in northern Chile. So named for the dark dust bands that trisect its glowing heart, the Trifid Nebula is a rare combination of three nebulae types that reveal the fury of freshly formed stars and point to more star birth in the future. The field of view of the image is approximately 13 x 17 arcminutes.
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Measuring 70 000 light-years across and laying 13 million light-years away, the nearly edge-on spiral galaxy NGC 253 is revealed here in an image from the Wide Field Imager (WFI) on the MPG/ESO 2.2-metre telescope at the La Silla Observatory. The image is based on data obtained through four different filters (R, V, H-alpha and OIII). North is up and East to the left. The field of view is 30 arcminutes.

Colour composite image of RCW120. It reveals how an expanding bubble of ionised gas about ten light-years across is causing the surrounding material to collapse into dense clumps where new stars are then formed. The 870-micron submillimetre-wavelength data were taken with the LABOCA camera on the 12-m Atacama Pathfinder Experiment (APEX) telescope. Here, the submillimetre emission is shown as the blue clouds surrounding the reddish glow of the ionised gas (shown with data from the SuperCosmos H-alpha survey). The image also contains data from the Second Generation Digitized Sky Survey (I-band shown in blue, R-band shown in red).
This image ...

Two of the sky’s more famous residents share the stage with a lesser-known neighbour in this enormous three gigapixel image from ESO’s VLT Survey Telescope (VST). On the right lies the faint, glowing cloud of gas called Sharpless 2-54, the iconic Eagle Nebula (Messier 16) is in the centre, and the Omega Nebula (Messier 17) to the left. This cosmic trio makes up just a portion of a vast complex of gas and dust within which new stars are springing to life and illuminating their surroundings.

This artist’s impression shows the view from the surface of one of the planets in the TRAPPIST-1 system. At least seven planets orbit this ultra cool dwarf star 40 light-years from Earth and they are all roughly the same size as the Earth. They are at the right distances from their star for liquid water to exist on the surfaces of several of them.
This artist’s impression is based on the known physical parameters for the planets and stars seen, and uses a vast database of objects in the Universe.

Tämä ESO:n valokuvalähettilään Yuri Beletskyn loistelias otos, joka on kuvattu ESO:n VLT-teleskoopin (Very Large Telescope) suojakuvun sisältä, näyttää VLT:n laserohjaustähden (LGS, Laser Guide Star) toiminnassa.
LGS, joka sijaitsee Yksikköteleskooppi 4:n 1.2 metrin sekundääripeilin päällä, on osa VLT:n adaptiivisen optiikan järjestelmää. Laserin Maan ilmakehään 90 kilometrin korkeuteen luomasta hehkuvasta pisteestä – keinotekoisesta tähdestä – takaisin tulevaa valoa voidaan käyttää vertailukohteena, jonka avulla poistetaan ilmakehän aiheuttamat vääristymät. Tämän ansiosta teleskooppi voi tuottaa lähes yhtä teräviä tähtitieteellisiä kuvia kuin jos se olisi avaruudessa.
Linnunradan taso, joka näyttää laserin puhkaisemalta sen kohotessa teleskoopin avoimen kuvun yllä, on tummien, näkyvän valon taakseen peittävien, tähtienvälisen pölyn ...

Our magnificent Milky Way galaxy is radiant over La Silla Observatory. The ESO 3.6-metre telescope is shown to the right, now home to the world's foremost extrasolar planet hunter: High Accuracy Radial velocity Planet Searcher (HARPS), a spectrograph with unrivalled precision.

Käyttäen 39:ää ALMA:n (Atacama Large Millimeter/submillimeter Array) 66:sta antennista, jotka sijaitsevat 5000 metrin korkeudessa Chajnantorin ylätasangolla Chilen Andeilla, tähtitieteilijät ovat pystyneet havaitsemaan hiilimonoksidia (CO) F-tyypin tähden ympärillä olevassa pölykiekossa. Vaikka hiilimonoksidi on toiseksi yleisin molekyyli tähtienvälisessä aineessa heti molekulaarisen vedyn jälkeen, kyseessä on ensimmäinen kerta, kun CO:ta on havaittu tämäntyyppisen tähden ympärillä. Tähti, nimeltään HD 181327, kuuluu Beta Pictoriksen liikkuvaan joukkoon, joka sijaitsee lähes 170 valovuoden etäisyydellä Maasta.
Tähän asti CO:ta on havaittu vain muutaman A-tyypin tähden ympärillä, jotka ovat paljon suurempia ja kirkkaampia kuin HD 181327. Käyttäen ALMA-observatorion tarjoamaa upeaa paikkaresoluutiota ja herkkyyttä, tähtitieteilijät onnistuivat kuvaamaan tämän häikäisevän savurenkaan ...

ESO’s Very Large Telescope in Chile has captured the most detailed image ever taken of the Medusa Nebula (also known Abell 21 and Sharpless 2-274). As the star at the heart of this nebula made its final transition into retirement, it shed its outer layers into space, forming this colourful cloud. The image foreshadows the final fate of the Sun, which will eventually also become an object of this kind.

Like the gaping mouth of a gigantic celestial creature, the cometary globule CG4 glows menacingly in this image from ESO’s Very Large Telescope. Although it looks huge and bright in this image it is actually a faint nebula and not easy to observe. The exact nature of CG4 remains a mystery.

The VLT Survey Telescope (VST) at ESO’s Paranal Observatory in Chile has captured this beautifully detailed image of the galaxy Messier 33, often called the Triangulum Galaxy. This nearby spiral, the second closest large galaxy to our own galaxy, the Milky Way, is packed with bright star clusters, and clouds of gas and dust. This picture is amongst the most detailed wide-field views of this object ever taken and shows the many glowing red gas clouds in the spiral arms with particular clarity.

This new view of Comet C/2012 S1 (ISON) was taken with the TRAPPIST–South national telescope at ESO's La Silla Observatory on the morning of Friday 15 November 2013. Comet ISON was first spotted in our skies in September 2012, and will make its closest approach to the Sun in late November 2013.
TRAPPIST–South has been monitoring comet ISON since mid-October, using broad-band filters like those used in this image. It has also been using special narrow-band filters which isolate the emission of various gases, allowing astronomers to count how many molecules of each type are released by the comet.
Comet ...

ESO’s Paranal Observatory — located in Chile’s Atacama region — is most well known for the Very Large Telescope (VLT), ESO’s flagship telescope facility. However, over the last few years, the site has also become home to two state-of-the-art survey telescopes. These new members of the Paranal family are designed to image large areas of the sky quickly and deeply.
One of them, the 4.1-metre Visible and Infrared Survey Telescope for Astronomy (VISTA), is located on a neighbouring peak not far from the Paranal summit. It is shown in this beautiful photograph taken from Paranal by ESO Photo Ambassador, Babak ...

Oudonmuotoinen Kynäsumu (NGC 2736) esittäytyy tässä ESO:n Chilessä sijaitsevan La Sillan observatorion kuvassa. Kaasusumu on pieni osa valtavaa jäännöstä, joka muodostui supernovaräjähdyksessä noin 11 000 vuotta sitten. Kuvan tuotti tuotti ESO:n Chilessä sijaitsevan La Sillan observatorion MPG/ESO 2.2-metrin teleskoopin Wide Field Imager -havaintolaite.

The Atacama Pathfinder Experiment (APEX) telescope looks skyward during a bright, moonlit night on Chajnantor, one of the highest and driest observatory sites in the world. Astronomical treasures fill the sky above the telescope, a testament to the excellent conditions offered by this site in Chile’s Atacama region.
On the left shine the stars that make up the tail of the constellation of Scorpius (The Scorpion). The scorpion’s “stinger” is represented by the two bright stars that are particularly close to each other. Reaching across the sky and looking like a band of faint, glowing clouds is the plane of ...

The VLT Survey Telescope (VST) is the latest telescope to be added to ESO’s Paranal Observatory in the Atacama Desert of northern Chile. It is housed in an enclosure immediately adjacent to the four VLT Unit Telescopes on the summit of Cerro Paranal. The VST is a 2.6-metre wide-field survey telescope with a field of view twice as broad as the full Moon. It is the largest telescope in the world dedicated to sky surveys in visible light. The VST was designed and built by the INAF–Osservatorio Astronomico di Capodimonte, Naples, Italy as part of a joint venture between INAF ...

NGC 3603 is a starburst region : a cosmic factory where stars form frantically from the nebula’s extended clouds of gas and dust. Located 22,000 light-years away from the Sun, it is the closest region of this kind known in our galaxy, providing astronomers with a local test bed for studying the intense star formation processes, very common in other galaxies, but hard to observe in detail because of their large distance.
The newly released image, obtained with the FORS instrument attached to one of the four 8.2-metre VLT Unit Telescopes at Cerro Paranal, Chile, is a three-colour combination of ...

With this remarkable VISTA mosaic we look deep into the dusty heart of our own Milky Way galaxy in the constellation of Sagittarius (the Archer). About one million stars are revealed in this picture, most of them not seen in visible light pictures. As well as absorbing light, the dust also scatters blue light from the distant stars and makes the central part of this huge starscape appear very red. This image is a mosaic created from VISTA images taken through Y, J and Ks filters in the near-infrared part of the spectrum. The image is about 2 degrees by ...

In the night sky over ESO’s Very Large Telescope (VLT) observatory at Paranal, the Moon shines along with two bright companions : already aloft in the heavens and glowing in the centre of the image is Venus, Earth’s closest planetary neighbour, and, to its right, the giant, though more distant planet, Jupiter. 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 this night view at Paranal : the radiant, reddish plane of the Milky Way, smouldering on the horizon, and an ...

The Milky Way, shining in its full splendour on top of the four Unit Telescopes and one of the Auxiliary Telescopes of ESO’s Very Large Telescope (VLT).

Seen edge-on, observations of NGC 4945 suggest that this hive of stars is a spiral galaxy much like our own Milky Way, with swirling, luminous arms and a bar-shaped centre. Sites of active star formation, known as HII regions, are seen prominently in the image, appearing bright pink. These resemblances aside, NGC 4945 has a brighter centre that likely harbours a supermassive black hole, which is devouring reams of matter and blasting energy out into space. NGC 4945 is about 13 million light-years away in the constellation of Centaurus (the Centaur) and is beautifully revealed in this image taken with ...

Neljä lasersädettä sojottaa kohti pimeyttä VLT-teleskoopin (Very Large Telescope) Yksikköteleskooppi 4:stä (UT4) ja kimaltavat yötaivaan uskomatonta taustaa vasten ESO:n Paranalin observatorion yllä. Ne todistavat ensimmäistä usean laserin käyttöä ESO:lla ja ovat voimakkaimmat laserohjaustähdet, joita tähtitieteessä on koskaan käytetty. Laserit virittävät natriumatomeja noin 90 kilometrin korkeudessa ilmakehässä luoden keinotekoisia tähtiä teleskoopin adaptiivisen optiikan järjestelmiä varten.
Nykyaikaiset teleskoopit käyttävät adaptiivisen optiikan järjestelmiä korjatakseen Maan ilmakehän sumentavan vaikutuksen. Tässä onnistuakseen teleskoopin täytyy kyetä näkemään kirkas referenssitähti samanaikaisesti pääkohdetta havaitessaan. Riittävän kirkasta tähteä ei aina kuitenkaan ole lähistöllä, joten tähtitieteilijät käyttävät lasereita luodakseen keinotekoisia tähtiä juuri sinne, missä niitä tarvitaan. Natriumatomit korkealla ilmakehässä saadaan ...

This extraordinary bubble, glowing like the ghost of a star in the haunting darkness of space, may appear supernatural and mysterious, but it is a familiar astronomical object: a planetary nebula, the remnants of a dying star. This is the best view of the little-known object ESO 378-1 yet obtained and was captured by ESO’s Very Large Telescope in northern Chile.

Tässä uudessa ESO:n kuvassa yön laskeutuminen nostaa esiripun La Sillan pilvettömällä taivaalla tapahtuvan näytöksen edestä.
Toimintaa huokuvassa näkymässä pääosan esittäjät ovat komeetta Lovejoy, joka hohtaa vihreänä keskellä kuvaa, Seulaset siitä yläoikealla, ja Lovejoyn oikealla puolella Kalifornia-sumu, jonka punainen kaari tuo kuvaan kontrastia.
Meteori lisää näkymään oman valoviirunsa ja näyttää sukeltavan horisonttia myötäilevään utumaiseen vihreän valon lammikkoon.
Taivaallisen näytöksen yleisönä ovat La Sillan teleskoopit. Ohut alapilviverho liimautuu observatorion alapuolella olevaan tasankoon, jota pitkin kulkee Panamericana-moottoritien piirtämä viiru.
Aurinkotuuli saa aikaan Lovejoy-komeetan pitkän pyrstön ja puhaltaa sitä poispäin komeetasta. Se saa vihreän värinsä Auringon ultraviolettisäteilyn virittämistä hiiliyhdisteistä.
Aurinkokunnan sisäosien läpi kulkeva komeetta ...

The smokey black silhouette in this new image is part of a large, sparse cloud of partially ionised hydrogen — an HII region — known as Gum 15. In wide-field images this nebula appears as a striking reddish purple clump dotted with stars and slashed by opaque, weaving dust lanes. This image homes in on one of these dust lanes, showing the central region of the nebula.
These dark chunks of sky have seemingly few stars because lanes of dusty material are obscuring the bright, glowing regions of gas beyond. The occasional stars that do show up in these patches ...

This richly detailed new view from the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile shows the star formation region Gum 15. This little-known object is located in the constellation of Vela (The Sails), some 3000 light-years from Earth. The glowing cloud is a stunning example of an HII region. It also has a similarity to a more famous HII region, the Trifid Nebula (Messier 20).

This image of the Paranal platform was taken right after sunset. The four Unit Telescopes are ready to start the observations.

The Milky Way glitters brightly over ALMA antennas, in this image taken by the ESO Ultra High Definition Expedition team as they capture the site in 4K quality.

Chilessä sijaitsevaa ESO:n VLT-teleskooppia käyttäneet tähtitieteilijät ovat taltioineet tämän silmiinpistävän kuvan planetaarisesta sumusta Abell 33. Vanhenevasta tähdestä ulos avaruuteen vuotaneiden uloimpien kaasukerrosten muodostama kaunis sininen kupla on sattumalta linjautunut etualan tähden kanssa ja saanut aikaan hämmentävän vastaavuuden timanttivihkisormuksen kanssa. Tämä kosminen jalokivi on epätavallisen symmetrinen ja vaikuttaa taivaalla lähes pyöreältä.

Chilessä sijaitsevan, ESO:n La Sillan observatorion tanskalainen 1.54-metrin teleskooppi on taltioinut hätkähdyttävän kuvan kohteesta NGC 6559, joka esittelee tähtienvälisessä pilvessä muodostuvien tähtien anarkiaa. Tämä taivaan alue käsittää punaisena hehkuvia, pääasiassa vetykaasusta koostuvia pilviä, sinisiä alueita, joissa tähtien valo heijastuu pikkuruisista tomuhiukkasista sekä myös tummia alueita, joissa tomu on tiheää ja läpinäkymätöntä.

ALMA:lla (Atacama Large Millimetre/submillimetre Array) tehdyt havainnot ovat paljastaneet odottamattoman spiraalirakenteen vanhaa R Sculptoris -tähteä ympäröivässä materiassa. Tätä rakennetta ei ole milloinkaan nähty ennen ja sen aiheuttaa todennäköisesti tähteä kiertävä näkymätön tähtikumppani. Tämä uuden ALMA-aineiston poikkileikkaus paljastaa tähden ympärillä olevan kuoren, joka näkyy ulompana pyöreänä renkaana, sekä hyvin selvän spiraalirakenteen sisemmässä materiassa.

Four antennas of the Atacama Large Millimeter/submillimeter Array (ALMA) gaze up at the star-filled night sky, in anticipation of the work that lies ahead. The Moon lights the scene on the right, while the band of the Milky Way stretches across the upper left.
ALMA is being constructed at an altitude of 5000 m on the Chajnantor plateau in the Atacama Desert in Chile. This is one of the driest places on Earth and this dryness, combined with the thin atmosphere at high altitude, offers superb conditions for observing the Universe at millimetre and submillimetre wavelengths. At these long wavelengths, ...

The night sky above Cerro Paranal, the home of ESO’s Very Large Telescope (VLT), is dark and dotted with the bright stars of the Milky Way, and more distant galaxies. But it is very rare to see the ground contrasting with the sky as markedly as in this photograph, which shows a gentle layer of white snow dotted with darker spots of the desert terrain beneath. The picture was taken last week, shortly before sunrise, by ESO Photo Ambassador Yuri Beletsky, who works as an astronomer at the La Silla Paranal Observatory. He captured not only the beautiful snowy landscape ...

In mid-August 2010 ESO Photo Ambassador Yuri Beletsky snapped this amazing photo at ESO’s Paranal Observatory. A group of astronomers were observing the centre of the Milky Way using the laser guide star facility at Yepun, one of the four Unit Telescopes of the Very Large Telescope (VLT).
Yepun’s laser beam crosses the majestic southern sky and creates an artificial star at an altitude of 90 km high in the Earth's mesosphere. The Laser Guide Star (LGS) is part of the VLT’s adaptive optics system and is used as a reference to correct the blurring effect of the atmosphere on ...

This picture of the spiral galaxy NGC 247 was taken using the Wide Field Imager (WFI) at ESO’s La Silla Observatory in Chile. NGC 247 is thought to lie about 11 million light-years away in the constellation of Cetus (The Whale). It is one of the closest galaxies to the Milky Way and a member of the Sculptor Group.

The stars rotate around the southern celestial pole during a night at ESO’s La Silla Observatory in northern Chile. The fuzzy parts in the trails on the right are due to the Magellanic Clouds, two small galaxies neighbouring the Milky Way. The dome seen in the image hosts ESO’s 3.6-metre telescope and is home to HARPS (High Accuracy Radial velocity Planet Searcher), the world’s foremost exoplanet hunter. The rectangular building seen in the lower right of the image contains the 0.25-metre TAROT telescope, designed to react very quickly when a gamma-ray burst is detected. Other telescopes at La Silla include ...

This VISTA image shows the spectacular 30 Doradus star-forming region, also called the Tarantula Nebula. At its core is a large cluster of stars known as R 136, in which some of the most massive stars known are located. This infrared image, made with ESO’s VISTA survey telescope, is from the VISTA Magellanic Cloud Survey. The project will scan a vast area — 184 square degrees of the sky (corresponding to almost one thousand times the apparent area of the full Moon), including our nearby neighbouring galaxies, the Large and Small Magellanic Clouds. The end result will be a detailed ...