Zdjęcie tygodnia

28 września 2015: On the morning of Monday 28 September 2015 a spectacular total lunar eclipse was witnessed across Africa, the Americas, Europe and the Middle East. In Germany, it was photographed by Mahdi Zamani above the ESO Headquarters Extension and Technical Building. In this time-lapse sequence the Moon was visible between thin layers of cloud. It appeared bright to the upper-left and faded dramatically as it entered the Earth’s shadow and moved lower in the early morning sky. A lunar eclipse takes place when the Moon, Earth and Sun are exactly aligned. When the Moon passes through the shadow cast by the Earth, our planet blocks the path of direct sunlight to the lunar surface and a total eclipse occurs. This event can only happen on the night of a full Moon. This morning's total lunar eclipse took place during a supermoon — a full Moon which occurs at the same time ...

21 września 2015: This striking picture of the New Technology Telescope (NTT) was taken just after sunset at ESO's La Silla Observatory, located in the Norte Chico in outskirts of the Chilean Atacama Desert. The Moon has already begun its journey across the evening sky, and is shining brightly overhead. The Sun dips below the horizon to the left of the frame, soaking the clouds in a rich orange colour. The warm glow of the last rays of sunshine are caught by the reflective surface of the NTT walls. The purpose of this metallic dome is to stop the telescope’s enclosure from heating up during the day. This would affect the telescope’s observations, as rising warm air and turbulence blur images and worsen the astronomical seeing. It is not just the telescope's enclosure that is designed to reduce heat accumulation during the day; the concrete platforms and parking spaces around the site are ...

14 września 2015: The huge diffraction grating at the heart of the ultra-precise ESPRESSO spectrograph — the next generation in exoplanet detection technology — is pictured undergoing testing in the cleanroom at ESO Headquarters in Garching bei München, Germany. Engineers at ESO have recently completed the difficult process of aligning the grating. The production and alignment of this component is one of the key ESO contributions to the ESPRESSO project. The grating is the largest ever assembled at ESO, and its length matches the largest echelle grating ever made — the 1.2 x 0.3 metre grating for the HIRES spectrograph at the Keck 10-metre telescope. After its final alignment, the grating is fixed in a permanent mount. All its components are made of Zerodur (the same material that is used for the mirrors of the VLT) and will require no further adjustments, ever. This mounting technique was pioneered at ESO, and demonstrated to ...

7 września 2015: These images, taken two weeks apart, show the two hemispheres of Ceres and provide the best ground-based observations of the dwarf planet ever. They were taken using the SPHERE instrument on ESO's Very Large Telescope and form part of an effort undertaken since mid-July 2015 to compose a polarimetric map of the object's surface. Orbiting in the asteroid belt between Mars and Jupiter, a region known as the Main Belt, Ceres was the first asteroid to be discovered in 1801 and is the largest Main Belt asteroid. It is the largest reservoir of water in Earth's neighbourhood. Most of this water is thought to exist in the form of water ice in the object's mantle. The surface of the dwarf planet is about the size of India and several intriguing bright spots can be seen in these new images. These mysterious bright patches have also been looked at more closely ...

31 sierpnia 2015: To widowiskowe zdjęcie zostało wykonane za pomocą drona lecącego nad Atakamą. Razem Łączą się na nim razem ocean, chmury i pustynia, aby dać nam widok z lotu ptaka rozciągający się wzdłuż chilijskiego wybrzeża. Bardzo Duży Teleskop (VLT – Very Large Telescope), który należy do ESO, jest lekko oświetlony przez Słońce, które zachodzi na wieczornym niebie dając odcienie koloru pomarańczowego i morelowego na budynkach obserwatorium. Na sąsiednim wierzchołku po prawej stoi 4,1-metrowy teleskop Visible and Infrared Survey Telescope for Astronomy (VISTA), odgrywając bardziej samotną postać w tej scenie. Obszar przed VLT, wypełniony siecią szyn, jest używany przez cztery mniejsze, przesuwalne Teleskopy Pomocnicze (VLT Auxiliary Telescopes). Umieszczając je w różnych odległościach można zmieniać efektywny rozmiar Interferometru VLT, który działa jako pojedyncza, gigantyczne narzędzie obserwacyjne.

24 sierpnia 2015: To zdjęcie, które wykonał Fotograficzny Ambasador ESO Alexandre Santerne, jest nieco dezorientujące na pierwszy rzut oka! Przypomina optyczną iluzję albo abstrakcyjny obraz, a przedstawia gwiezdne okręgi wokół bieguna południowego na niebie widziane nad należącym do ESO Obsewratorium La Silla w Chile. Każdy kołowy ślad odpowiada pojedynczej gwieździe fotografowanej przez długo okres czasu, aby uchwycić ruch gwiazd po niebie spowodowany obrotem Ziemi dookoła swojej osi. La Silla znajduje się na obrzeżach chilijskiej pustyni Atakama na wysokości 2400 metrów nad poziomem morza i oferuje idealne warunki obserwacyjne dla długoczasowych ekspozycji takich jak ta. Na dodatek w tym miejscu występuje ponad 300 pogodnych nocy w roku! Miejsce to stanowi dom dla teleskopów ESO i dla projektów krajowych prowadzonych przez poszczególne Kraje Członkowskie ESO. Niektóre z teleskopów są widoczne na dole fotografii. 3,6-metrowy teleskop ESO, który stoi na szczycie po lewej stronie, jest obecnie domem dla czołowego łowcy planet pozasłonecznych: High Accuracy Radial velocity ...

17 sierpnia 2015: Na panoramicznym zdjęciu, które wykonał Babak Tafreshi — członek zespołu ESO Ultra HD Expedition — anteny Obserwatorium ALMA wydają się być połączone Drogą Mleczną, wyginającą się jak galaktyczna tęcza z pyłu i gwiazd nad płaskowyżem Chajnantor w Andach Chilijskich. Płaskowyż Chajantor, położony 5000 metrów nad poziomem morza, jest idealny miejscem na polowania ALMA. Sieć używa obserwacji na falach milimetrowych i submilimetrowych, aby badań najchłodniejsze części Wszechświata. Niesamowita suchość płaskowyżu oznacza, że absorbowane i osłabiane przez parę wodną jest dużo mniej promieniowania submilimetrowego niż na obszarach bliższych poziomowi morza. Tak jak ALMA próbuje uchwycić sekrety Wszechświata, Babak Tafreshi i inni członkowie zespołu, próbują zarejestrować piękno i wielkość obserwatoriów ESO i ich nietypowego otoczenia. Składająca się z czterech znanych astrofotografów i ESO Fotograficznych Ambasadorów ESO, ESO Ultra HD Expedition ma na celu zwiększenie w społeczeństwie świadomości wykonywanej w Chile pracy, poprzez zadziwiające zdjęcie i filmy Ultra HD.

10 sierpnia 2015: This view shows La Residencia, the hotel that provides an oasis for the astronomers and staff working at ESO’s Paranal Observatory in Chile. The image is taken from the south corner of the building, looking north towards the Very Large Telescope (VLT) sitting atop the summit of Cerro Paranal at some 2635 metres above sea level. The VLT is the flagship facility for European ground-based optical astronomy, and is the world’s most advanced optical observatory. The windows of the 108 rooms of La Residencia look west (left on the photo) towards the Pacific Ocean. Designed by the German architects Auer+Weber+Assoziierte, this award-winning building was featured as a backdrop for part of the James Bond film Quantum of Solace. It was built in a partially subterranean L-shape, making use of natural materials to allow it to blend in with the colours of the desert’s Mars-like landscape. It is little surprise that ...

3 sierpnia 2015: The bright star in the centre of this image is not the star of this show. At the bottom centre is a rather unremarkable smudge of red which is in fact a rare and valuable object. First discovered by amateur Japanese astronomer, Yukio Sakurai, in 1996, and noted as a nova-like object, Sakurai’s discovery turned out to be far more interesting than the supernova he initially supposed it to be. The object is actually a small white dwarf star undergoing a helium flash — one of only a handful of examples of such an event ever witnessed by astronomers. Normally, the white dwarf stage is the last in the life cycle of a low-mass star. In some cases, however, the star reignites in a helium flash and expands to return to a red giant state, ejecting huge amounts of gas and dust in the process, before once again shrinking to ...

27 lipca 2015: This photograph shows the road to the Atacama Large Millimeter/submillimeter Array (ALMA)’s Operations Support Facility (OSF) and then on further to the breathtaking Chajnantor Plateau at 5000 metres above sea level. The plateau, situated in Chilean Puna in the Atacama region, is home to the Array Operations Site (AOS) and is the site of the highest and driest astronomical observatory on Earth. The OSF is the centre of activities for the ALMA project and is where all staff and contractors are accommodated — only 2900 metres above sea level. This is where all the scientific operations related to the daily operation of the observatory take place. The AOS houses a technical building — the second highest building on Earth — along with the ALMA correlator, the highest and fastest computer ever used at an astronomical site. Due to the high altitude, human operations are kept to a minimum. ALMA will ...

20 lipca 2015: Here we see the now-obsolete Swedish–ESO Submillimetre Telescope (SEST), watching vigilantly over the horizon at ESO’s La Silla Observatory like a sentinel. Below, stratus clouds blanket the valley. SEST was installed at La Silla in 1987, and at the time of its first light was the only large submillimetre telescope operating in the southern hemisphere. Although it was decommissioned in 2003, the 15-metre diameter dish remains at La Silla Observatory and serves as a tribute to the groundbreaking work it accomplished — both as a standalone telescope, and also as a testbed for later projects such as the Atacama Pathfinder Experiment telescope (APEX) and the Atacama Large Millimeter/submillimeter Array (ALMA). During its tenure, SEST made several big discoveries, including, in 1995, finding the Boomerang Nebula to be the coldest place in the Universe at just one degree above absolute zero, and discovering the first extragalactic silicon monoxide maser. This beautiful ...

13 lipca 2015: Not all regions of Chile are as stark and barren as the ESO observing sites at Paranal, La Silla, and Chajnantor. ESO’s Santiago office, located in Vitacura, is sometimes visited by passing rainclouds and plays host to astronomers, technicians and administrative staff. Some 15 kilometres off in the background of this image, the beautiful snow-capped peaks of the Chilean Andes are visible. On a clear day the peaks can be viewed from almost anywhere in the city. They serve as a constant reminder of the natural boundaries of the busy city and its proximity to nature, should anyone require a break from the hustle and bustle of city life. Visitors to the area can take an easy hike in the Parque Natural Aguas de Ramón or fans of local flora and fauna may like to visit the Santuario de La Naturaleza El Arrayán (nature sanctuary), both located close to the ...

6 lipca 2015: This image by ESO Photo Ambassador Alexandre Santerne shows the Swedish–ESO Submillimetre Telescope (SEST) on the left, alongside the ESO 3.6-metre telescope on the right. In the background bright star trails circle the La Silla Observatory where the telescopes are situated, in the outskirts of the Atacama Desert in Chile. Star trails like these are created by using a long exposure to capture the apparent motion of the stars in the night sky as the Earth rotates. This image is a composite of 250 consecutive one-minute exposures, spanning four hours. A flipped version of the star trails is also visible as a reflection in the dish of the telescope. The reflection also includes the red lights of a car passing by. La Silla is ESO’s first observatory and has been a major ESO stronghold since the 1960s. SEST was, at the time of construction, the only large submillimetre telescope in ...

29 czerwca 2015: On 27 June 2015, the ESO Headquarters in Garching, Germany, opened its doors to the public as part of the Long Night of Science (Lange Nacht der Wissenschaften), along with the other facilities based at the science campus in Garching. ESO invited visitors to experience the work of this world-leading ground-based astronomy organisation at first hand with eighteen different activities to take part in. In the picture ESO astronomer Vinod Arumugam is making a comet out of dry ice. Before the doors had even opened at six in the evening people were waiting outside, eager to look around the Headquarters and take part in the activities within. In total, 3800 people attended the events and had the chance to have their questions answered by experienced astronomers; see live experiments; join guided tours through the new office and technical buildings; listen to talks about ongoing astronomical research; visit the exhibition LIGHT: ...

22 czerwca 2015: Illuminated by the stars of the Milky Way, the majestic fourth Unit Telescope (UT4) of the Very Large Telescope (VLT) sits atop Cerro Paranal, ready to observe the night sky. The Paranal Observatory, at an altitude of 2635 metres above sea level, is the world”s most advanced ground-based astronomical observatory and ESO’s flagship facility. UT4 — also known as Yepun (Venus) — has a main mirror 8.2 metres diameter, and is one of four Unit Telescopes that comprise the VLT. The others are known as Antu (Sun), Kueyen (Moon) and Melipal (Southern Cross). The names of the telescopes are words from the language of the Mapuche people who live some 500 kilometres south of Santiago de Chile. The four Unit Telescopes can work together to form the ESO Very Large Telescope Interferometer (VLTI). The VLTI allows astronomers to measure details up to 16 times finer than with the individual telescopes. ...

15 czerwca 2015: ESO’s Paranal Observatory is one of the best places on Earth to take in the night sky. This panorama of ESO’s Very Large Telescope (VLT) atop the platform of Chile’s Cerro Paranal was taken by Babak Tafreshi, one of the ESO Photo Ambassadors. A mix of colours sweeps across the sky in this image. From the fiery red sunset up to the dusty purple band of the Milky Way. Although the VLT site is one of the best places on Earth for astronomy, the telescope must still overcome the natural distortions caused by our atmosphere. This is done through a process known as adaptive optics. Astronomers can make use of an artificial star by shining a powerful laser — seen here projected from the telescope on the far right — to correct for the blurring caused by the atmosphere. The VLT, as a flagship facility for European astronomy, has opened ...

8 czerwca 2015: The Crab Nebula, which also goes by the names Messier 1, NGC 1952 and Taurus A, is one of the best studied astronomical objects in the sky. It is the remnant of a supernova explosion which was observed by Chinese astronomers in 1054. The tangled filaments visible in this image are the remains of the exploded star, which are still expanding outwards at about 1500 kilometres per second. Although not visible to the naked eye due to foreground filaments of helium and hydrogen the heart of the nebula hosts two faint stars. It is one of these that is responsible for the nebula that we see today — a star that is known as the Crab Pulsar, or CM Tau. This is the small, dense, corpse of the original star that caused the supernova. It is now only about 20 kilometres in diameter and rotates around its axis 30 times ...

1 czerwca 2015: The brilliant starry sky, the red sand and the ice structures piercing the foreground of this image combine to give the impression of a desert far from the reach of human footprints. A landscape that could easily be mistaken for the polar regions of our distant neighbour Mars. The jagged tooth-like formations are not on the Red Planet however, but on the sloping hills of the Atacama Desert. The formations are called penitentes — structures made of snow and ice that form mostly at high altitudes. The low pressure, moisture and temperature at these altitudes help to create this interesting and rare behaviour in the freezing of ice. The strange structures also have a tendency to orient themselves towards the Sun, which is why they are all perfectly aligned like a carefully tended garden of ice. As if this beautiful quirk of nature wasn’t enough, above the structures lies an ...

25 maja 2015: In this image, taken by ESO Photo Ambassador Yuri Beletsky, the control building at the Paranal Observatory can be seen below a rising Milky Way, like the proverbial pot of gold at the end of a celestial rainbow. This building is a hub for the observatory’s operations, and it is from here that the Very Large Telescope (VLT), the VLT interferometer (VLTI), the VLT Survey Telescope (VST) and VLT Infrared Survey Telescope for Astronomy (VISTA) are controlled and maintained. The team of astronomers, telescope and instrument operators, and engineers is on site 24 hours a day to to run these telescopes and to keep them in top condition. The control building is located on a “shelf” below the main observing platform at the top of the Paranal Mountain. All functions of the four Unit Telescopes (UTs), the four Auxiliary Telescopes (ATs), the two survey telescopes are controlled from their own ...

18 maja 2015: Widoczna tutaj sieć Atacama Large Millimeter/submillimeter Array (ALMA), położona jest wysoko na płaskowyżu Chajnantor w Andach Chilijskich na 5000 metrach and poziomem morza. Skalisty brzeg widoczny na pierwszym planie zdjęcia jest górą, która rozciąga się powyżej ALMA. To tutaj umiejscowiony jest 1-metrowy teleskop testowy o nazwie MiniTAO. MiniTAO jest częścią projektu University of Tokyo Atacama Observatory (TAO), w ramach którego powstanie później w tym miejscu większy, 6,5-metrowy teleskop zoptymalizowany na podczerwień. NAOJ, ESO i inni partnerzy zaangażowani w ALMA wybrali to miejsce, ponieważ jest jednym z najwyżej położonych i najsuchszych obserwatoriów astronomicznych na Ziemi. ALMA składa się z 66 precyzyjnych anten rozmieszczonych na przestrzeni do 16 kilometrów. Anteny używają techniki znanej jako interferometria, aby łączyć swoje sygnały, co pozwala działać im jako jedna gigantyczna antena, Sygnały od każdej z anten muszą zostać połączone z idealną synchronizacją - z precyzją do jednej bilionowej części sekundy. Są zbierane przez korelator ALMA (tuż ...