alma telescope location
Testing of first prototype antenna begins at the ALMA Test Facility (ATF) site in Socorro, New Mexico. ALMA studies the building blocks of stars, planetary systems, galaxies and life itself. The first vehicle was completed and tested in July 2007. Call for shared-risk Early Science proposals. Il est ouvert d’un côté, celui que l’on pointe vers le ciel. The American and European partners each provided twenty-five 12-meter diameter antennas, that compose the main array. Time-lapse video at the ALMA Array Operations Site (AOS). During Autumn 2009, the first three antennas were transported one-by-one to the Array Operations Site. Thirty-two 12-m antennas in the 12-m array. This example image shows a comparison of Hubble and ALMA observations. ALMA is an international partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National … VLBA Global Locations; VLBA Global Locations . Location de télescopes. On 11 August 2014, astronomers released studies, using the Atacama Large Millimeter/submillimeter Array (ALMA) for the first time, that detailed the distribution of HCN, HNC, H2CO, and dust inside the comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON). IMAGE: (artist’s impression in post comments) ALMA image of the old star system W43A. A view across the plains of Chajnantor with the ALMA construction site at the center. La spécification la plus importante d’un télescope, ce n’est pas son grossissement, mais c’est sa capacité à collecter un maximum de lumière. ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust. ALMA began scientific observations in the second half of 2011 and the first images were released to the press on 3 October 2011. This location was chosen for its high elevation and low humidity, factors which are crucial to reduce noi… ALMA’s capabilities are world-renowned, but it’s not a place where tourists can go peer through a telescope to see the stars. The telescopes were provided by the European, North American and East Asian partners of ALMA. The components designed and manufactured across Europe were transported by specialist aerospace and astrospace logistics company Route To Space Alliance,[9] 26 in total which were delivered to Antwerp for onward shipment to Chile. L'instrument est capable grâce à sa haute résolution d'étudier le processus de formation des planètes autour des jeunes étoiles. Artist’s conception of the Very Long Baseline Array (VLBA), a continent-wide radio telescope system. [38][39][40][41] After 17 days an agreement was reached providing for reduced schedules and higher pay for work done at high altitude. European/U.S. One theory suggests that the faster accretion rate might be due to the complex magnetic field of the protoplanetary disk. The initial ALMA array is composed of 66 high-precision antennas, and operates at wavelengths of 3.6 to 0.32 millimeters (31 to 1000 GHz). Share the excitement of the inauguration ceremony and contemplate the breathtaking images from ALMA itself and views of its unique environment in the Atacama Desert. The ACA works together with the main array in order to enhance the latter's wide-field imaging capability. As no known non-biological source of phosphine on Venus could produce phosphine in the concentrations detected, this indicated the presence of biological organisms in the atmosphere of Venus. It also delayed the cycle 8 proposal submission deadline and suspended public visits to the site.[44]. In Carl Sagan’s Contact, a dramatic scene shows Dr. Ellie Arroway, played by Jodie Foster, looking out over the magnificent Arecibo Telescope. The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile, which observe electromagnetic radiation at millimeter and submillimeter wavelengths. ALMA Captures Stellar Fireworks in Orion. The array is located on the Chajnantor Plateau in the Atacama Desert. Video compilation showing various aspects of ALMA. ALMA is expected to help scientists understand how stars were created during the early universe. This video shows ISS astronauts congratulating the ALMA Partners on the occasion of its inauguration. Image of telescope in transit at the Site Erection Facility. [10] ALMA is the largest and most expensive ground-based astronomical project, costing between US$1.4 and 1.5 billion. Les locations de télescopes (matériel seul), sont proposées avec une initiation préalable et une mise en station pour un usage immédiat. This is why the ALMA antennas were located in one of the most arid areas in the world: the Atacama Desert. The VLBA is an interferometer consisting of 10 identical antennas on transcontinental baselines up to 8000 km (Mauna Kea, Hawaii to St. Croix, Virgin Islands). Thirty-four 12-m antennas in the 12-m array, nine 7-m antennas in the 7-m array, and two 12-m antennas in the TP array. At that size, ALMA can pinpoint small, hidden details deep inside galaxies or within giant star forming regions, making it one of the most powerful telescopes ever made. La réalisation des 25 antennes européennes a été confiée à un consortium européen, dont Thales Alenia Space (TAS) assure la maîtrise d'œuvre, nous explique Vincenzo Giorgio, vice-président optique, observation et sciences pour TAS. The Arecibo radio telescope, the largest instrument of its type for decades, is now damaged beyond repair and set for demolition. Using a revolutionary telescope ALMA, various types of complex organic molecules have already been found in planet forming regions. The high velocity bipolar jets ejected from the central aged star are seen in blue, low velocity outflow is shown in green, and dusty clouds entrained by the jets are shown in orange. Cette caractéristique essentielle est déterminée par le diamètre de son ouverture (le diamètre du tube), et la surface de son … ESO/NRAO/NAOJ joint site testing with Chile. The radio telescope combines signals from each, working as an interferometer, in other words, a single giant telescope equal in size to the total array. They are powered by twin turbocharged 500 kW Diesel engines. This was mainly for political reasons. ESO and NRAO worked together in technical, science, and management groups to define and organize a joint project between the two observatories with participation by Canada and Spain (the latter became a member of ESO later). From Simple English Wikipedia, the free encyclopedia, Location of Atacama Large Millimeter Array, "At the End of the Earth, Seeking Clues to the Universe", https://simple.wikipedia.org/w/index.php?title=Atacama_Large_Millimeter_Array&oldid=6873890, Articles with infoboxes completely from Wikidata, Creative Commons Attribution/Share-Alike License, Atacama Large Millimeter and Submillimeter Array, National Institutes of Natural Sciences, Japan. On 30 September 2013 the final ALMA antenna was handed over to the ALMA Observatory. Update Location; SUNSET: MOON: 90% Waxing Gibbous; Interactive star Chart. Recently, observations from the ALMA radio telescope provided the first indication of the missing neutron star after the explosion. The guests are shown with one of the giant ALMA transporters as well as other components. This is not picked up by optic telescopes and is fundamental if we want to know how stars and planets are formed. It enables transformational research into the physics of the cold Universe, probes the first stars and galaxies, and directly images the formation of planets. Concept d'artiste via ALMA (ESO / NAOJ / NRAO). The ALMA (AL'-mah) telescope in Chile has captured a close-up of the glowing material spewing from a newborn star. The Essential Guide to Astronomy. Publié le 05/06/2012 par Musée Air Espace. Email … By the summer of 2011, sufficient telescopes were operational during the extensive program of testing prior to the Early Science phase for the first images to be captured. [3][4] ALMA began scientific observations in the second half of 2011 and the first images were released to the press on 3 October 2011. The 12-meter-diameter dish was manufactured by the European AEM Consortium and also marks the successful delivery of a total of 25 European antennas — the largest ESO contract so far. Avec l’Alma de Chajnantor et La Silla, Cerro Paranal est le troisième grand projet de l’Observatoire européen austral (ESO). Following mutual discussions over several years, the ALMA Project received a proposal from the National Astronomical Observatory of Japan (NAOJ) whereby Japan would provide the ACA (Atacama Compact Array) and three additional receiver bands for the large array, to form Enhanced ALMA. Opening of Joint ALMA office, Santiago, Chile. Costing more than a billion US dollars,[1] it is the worlds's most expensive ground-based telescope. The vehicles were made by Scheuerle Fahrzeugfabrik [de][17] in Germany and are 10 m wide, 20 m long and 6 m high, weighing 130 tonnes. ALMA is being built by Europe, the United States, Canada, East Asia and the Republic of Chile. [18] Both transporters were delivered to the ALMA Operations Support Facility (OSF) in Chile on 15 February 2008. Choisissez parmi des contenus premium Atacama Large Millimeter Array de la plus haute qualité. For the first time, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have witnessed 3D motions of gas in a planet-forming disk. [28], ALMA participated in the detection of phosphine, a biomarker, in the atmosphere of Venus. This is one baby picture you won't want to miss. The participating East Asian countries are contributing 16 antennas (four 12-meter diameter and twelve 7-meter diameter antennas) in the form of the Atacama Compact Array (ACA), which is part of the enhanced ALMA. The target of the observation was a pair of colliding galaxies with dramatically distorted shapes, known as the Antennae Galaxies. News Observing Tools. A drone camera flies overhead the ALMA observatory, showing the 66 telescopes that make up the array in the wilderness of Chile's Atacama desert. Répondre. [31], The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile. A follow-up to radio telescopes such as ALMA is a telescope capable of collecting data over one square kilometer. The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile, which observe electromagnetic radiation at millimeter and submillimeter wavelengths. The high sensitivity is mainly achieved through the large numbers of antenna dishes that will make up the array. The project is should be fully operational by March 2013. Stellar Science. Due to … The 130-ton ALMA antenna transporter "Otto" during its naming ceremony. This video shows the antenna being moved on the giant transporter called "Otto". Placing the antennas closer together enables the imaging of sources of larger angular extent. ALMA has 66 antennas: fifty-four 12-meter diameter antennas and twelve 7-meter diameter antennas. This was the number of antennas specified for ALMA to begin its first science observations, and was therefore an important milestone for the project. L'entreprise est surtout recon… Taiwan joins the ALMA Project through Japan. General Dynamics C4 Systems and its SATCOM Technologies division was contracted by Associated Universities, Inc. to provide twenty-five of the 12 m antennas,[12] while European manufacturer Thales Alenia Space provided the other twenty-five principal antennas[13] (in the largest-ever European industrial contract in ground-based astronomy). La signature du contrat de location et la remise du chèque de caution est faite à la présentation du matériel. In 2013, the Atacama Compact Array was named the Morita Array after Professor Koh-ichiro Morita, a member of the Japanese ALMA team and designer of the ACA, who died on 7 May 2012 in Santiago. Extremely high-resolution images revealed a hot “blob” in the dusty core of SN 1987A, which is brighter than its surroundings and matches the suspected location of the neutron star. A groundbreaking ceremony was held on November 6, 2003 and the ALMA logo was unveiled.[8]. Credit:NRAO | Download image in HD The Essential Guide to Astronomy . It will also provide detailed imaging of local star and planet formation. [16] The solution chosen is to use two custom 28-wheel self-loading heavy haulers. [14] The first antenna was delivered in 2008, the last in 2011.[15]. MENU. L’ALMA, situé dans le désert d’Atacama, plus précisément sur le Llano de Chajnantor (à une cinquantaine de kilomètres de San Pedro de Atacama), est le plus grand radio-téléscope du monde. Transporting the 115 tonne antennas from the Operations Support Facility at 2900 m altitude to the site at 5000 m, Start of Early Science Cycle 1. The work stoppage began after the observatory failed to reach an agreement with the workers' union. This 16-minute video presents the history of ALMA from the origins of the project several decades ago to the recent first science results. In addition, the surface area should be large and flat enough for distribution of the antennas. (in HD). By: Monica Young April 11, 2017 2. Login Shop at Sky SEARCH. [42][43], In March 2020, ALMA was shut down due to the COVID-19 coronavirus crisis. Interestingly, the region’s indigenous people were observing dark space long before the observatory was built. First move of an ALMA antenna to Chajnantor. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA. ALMA has 66 antennas: fifty-four 12-meter diameter antennas and twelve 7-meter diameter antennas. The Atacama Large Millimeter/submillimeter Array (ALMA) -the largest astronomical project in existence- is a single telescope of revolutionary design, composed of 66 high precision antennas located on the Chajnantor Plateau, 5000 meters altitude in northern Chile. Pourquoi parle-t-on du télescope Alma ? ALMA is funded in Europe by the European Southern Observatory (ESO), in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and in East Asia by the National Institutes of Natural Sciences of Japan (NINS) in cooperation with the Academia Sinica (AS) in Taiwan. Les astronomes ont utilisé le télescope ALMA du nord du Chili pour visualiser un tore gazeux en rotation autour d’un trou noir supermassif actif dans une galaxie lointaine. Moonrise above the 12 meter wide access road to the ALMA High Site. On 7 July 2008, an ALMA transporter moved an antenna for the first time, from inside the antenna assembly building (Site Erection Facility) to a pad outside the building for testing (holographic surface measurements).[19]. ALMA is being built on the Chajnantor plateau at 5000 metres altitude. Pour l'astronome amateur qui réside dans nos lodges, nous pouvons louer du matériel astronomique, aux conditions suivantes: Vous devez être capable d'utiliser le télescope seul, sans mettre en risque les équipements. Array configurations from approximately 150 m to 14 km, Faster and more flexible imaging instrument than the Very Large Array, Largest and most sensitive instrument in the world at millimeter and submillimeter wavelengths, Point source detection sensitivity 20 times better than the Very Large Array, Data reduction system will be CASA (Common Astronomy Software Applications) which is a new software package based on, This page was last edited on 29 December 2020, at 02:01. Il contient 66 antennes, c'est-à-dire 66 gros télescopes tournés vers le ciel pour faire des observations dans l'espace. The antennas can be moved across the desert plateau over distances from 150 m to 16 km, which will give ALMA a powerful variable "zoom", similar in its concept to that employed at the centimetre-wavelength Very Large Array (VLA) site in New Mexico, United States. Although very different approaches have been chosen by the providers, each of the antenna designs appears to be able to meet ALMA's stringent requirements. Trouvez les Atacama Large Millimeter Array images et les photos d’actualités parfaites sur Getty Images. The first step toward the creation of what would become ALMA came in 1997, when the National Radio Astronomy Observatory (NRAO) and the European Southern Observatory (ESO) agreed to pursue a common project that merged the MMA and LSA. The Atacama Large Millimeter/sub-millimeter Array (ALMA) is an array of radio telescopes in the Atacama Desert of northern Chile. Several areas in New México, Hawaii (Mauna-Kea), France (Plateau de Bure) and northern … The ALMA regional centre (ARC) has been designed as an interface between user communities of the major contributors of the ALMA project and the JAO. or moving antennas around the site to change the array size, presents enormous challenges; as portrayed in the television documentary Monster Moves: Mountain Mission. A series of resolutions and agreements led to the choice of "Atacama Large Millimeter Array", or ALMA, as the name of the new array in March 1999 and the signing of the ALMA Agreement on 25 February 2003, between the North American and European parties. The array has been constructed on the 5,000 m (16,000 ft) elevation Chajnantor plateau - near the Llano de Chajnantor Observatory and the Atacama Pathfinder Experiment. The core purpose of the ARC is to assist the user community with the preparation of observing proposals, ensure observing programs meet their scientific goals efficiently, run a help-desk for submitting proposals and observing programs, delivering the data to principal investigators, maintenance of the ALMA data archive, assistance with the calibration of data and providing user feedback. [29][30] However, this theory has since been overturned, and there has been a new study indicating that there is no phosphine in the atmosphere of Venus. Activates for operating the ARC have also divided into the three main regions involved (Europe, North America and East Asia). This artist's rendering of the ALMA array on the Chajnantor plateau shows how, as an interferometer, ALMA acts like a single telescope with a diameter as large as the distance between its individual antennas (represented by the blue circle). Grâce à ses 66 antennes - ou radio téléscopes, les ingénieurs et astronomes à l’origine de ce projet espèrent qu’il apportera de nouveaux éléments-clé sur la formation de l’univers . [23] These early images give a first glimpse of the potential of the new array that will produce much better quality images in the future as the scale of the array continues to increase. Ainsi, non seulement il capte la lumière, mais également les ondes millimétriques et submillimétriques , de sorte que le dispositif astronomique peut fonctionner de jour comme de nuit. Here’s what made it so great. [21] In October 2012, 43 of the 66 antennas had been set up. ALMA observes light that is invisible to the naked eye, a light that emanates naturally from the Universe in long waves, a portion of the electromagnetic spectrum that lets us explore the “cold Universe”. The final antenna for the project is here seen arriving to the high site at the observatory, 5000 meters above sea level. Location of Atacama Large Millimeter Array. ALMA construction and operations are led on behalf of Europe by ESO, on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc (AUI) and on behalf of East Asia by the National Astronomical Observatory of Japan (NAOJ). Although ALMA did not observe the entire galaxy merger, the result is the best submillimeter-wavelength image ever made of the Antennae Galaxies, showing the clouds of dense cold gas from which new stars form, which cannot be seen using visible light. La mise en service progressive de ses 66 antennes se poursuit. First interferometry with two antennas at the Operations Support Facility (OSF). This video begins near the ground of the Chajnantor Plateau, at 5000 meters altitude in the Chilean Andes, and later takes in views of the 58 antennae that make up the Atacama Large Millimeter/submillimeter Array. Start of Early Science Cycle 0. Working together, the separate ALMA telescopes become one giant telescope up to 11 miles (16 km) across. ALMA has its conceptual roots in three astronomical projects — the Millimeter Array (MMA) of the United States, the Large Southern Array (LSA) of Europe, and the Large Millimeter Array (LMA) of Japan. ALMA se compose d’un réseau de 66 radiotélescopes, qui reliés entre eux équivalent à un télescope de 16 km de diamètre. Japan constructed 16 Antennas. European, North American & Japanese draft agreement, with Japan providing new extensions to ALMA. Premiers résultats pour le télescope ALMA. This model of the ALMA array on the Chajnantor plateau shows how ALMA acts like a single telescope with a diameter as large as the distance between its individual antennas (represented by the blue circle). That's a huge, light-gathering eyeball! The transporters, which feature a driver's seat designed to accommodate an oxygen tank to aid breathing the thin high-altitude air, place the antennas precisely on the pads. Login Shop at Sky. By using smaller antennas than the main ALMA array, larger fields of view can be imaged at a given frequency using ACA. ALMA is a 66-dish array in Chile capable of spying cool gas and dust in galaxies whose light has been traveling for up to 12 billion years. L'actu du jour : Voici un objet unique sur notre planète. Start of Early Science Cycle 2. After its design, one of the most important success factors for this type of radioastronomy project lies in its location. Alma est l' observatoire radio millimétrique et submillimétrique le plus grand et le plus moderne au monde. [35], The Atacama Compact Array, ACA, is a subset of 16 closely separated antennas that will greatly improve ALMA's ability to study celestial objects with a large angular size, such as molecular clouds and nearby galaxies. [2] Costing about US$1.4 billion, it is the most expensive ground-based telescope in operation. The Atacama Large Millimeter/submillimeter Array (ALMA) is a telescope array in Chile that includes 66 receivers. The merged array combined the sensitivity of the LSA with the frequency coverage and superior site of the MMA. [24][25], An image of the protoplanetary disk surrounding HL Tauri (a very young T Tauri star[26] in the constellation Taurus) was made public in 2014, showing a series of concentric bright rings separated by gaps, indicating protoplanet formation. ALMA identified 39 faint galaxies that are not seen with the Hubble Space Telescope’s deepest view of the Universe 10 billion light-years away. Sixteen 12-m antennas in the 12-m array. ; Le bijou du Paranal est le très grand télescope (Very large telescope, VLT), un instrument extrêmement performant qui compte 4 miroirs de 8,2 m de diamètre. Alors même que son installation n’est pas entièrement terminée, le télescope ALMA, situé au Chili, commence à donner ses premiers résultats. A talk on the Atacama Large Millimeter/submillimeter Array (ALMA), by Leonardo Testi. A high and dry site is very important for millimeter wavelength work. [37], In August 2013, workers at the telescope went on strike to demand better pay and working conditions. ALMA (Atacama Large Millimeter/submillimeter Array) is the world's largest ground-based facility for observations in the millimeter/submillimeter regime located on the Chajnantor plateau, 5000 meters altitude in northern Chile. European, North American & Japanese amend agreement on the Enhanced ALMA. At three locations in the disk around a young star called HD 163296, gas is flowing like a waterfall into gaps that … ALMA is an international partnership among Europe, the United States, Canada, Japan, South Korea, Taiwan, and Chile. Low frequency waves are better received at high altitudes and in dry climates, as this reduces the amount of noise. Further discussions between ALMA and NAOJ led to the signing of a high-level agreement on 14 September 2004 that makes Japan an official participant in Enhanced ALMA, to be known as the Atacama Large Millimeter/submillimeter Array. The instruments at ALMA observe long waves of invisible light, a portion of electromagnetic spectrum that reveals the dark universe. Arrival of the two ALMA transporters in Chile. (in HD). The squares numbered from 1 to 4 are the locations of faint galaxies unseen in … Community Tours Magazine. memorandum of understanding for design & development. The array has been constructed on the 5,000 m (16,000 ft) elevation Chajnantor plateau - near the Llano de Chajnantor Observatory and the Atacama Pathfinder Experiment. The European ARC (led by ESO) has been further subdivided into ARC-nodes[34] located across Europe in Bonn-Bochum-Cologne, Bologna, Ondřejov, Onsala, IRAM (Grenoble), Leiden and JBCA (Manchester). [1] ALMA is expected to provide insight on star birth during the early Stelliferous era and detailed imaging of local star and planet formation. Although the existence of amino acids does not necessarily lead to the birth of life, ALMA observations may clarify the probability of the occurrence of life in the universe. Parce que mercredi, l'un des projets astronomiques les plus gros du monde a été inauguré en grande pompe au Chili : il s'agit d'un télescope hors du commun. At the end of 2009, a team of ALMA astronomers and engineers successfully linked three antennas at the 5,000-metre (16,000 ft) elevation observing site thus finishing the first stage of assembly and integration of the fledgling array. ALMA doit également observer les trous no As of 2014[update], most theories did not expect planetary formation in such a young (100,000-1,000,000-year-old) system, so the new data spurred renewed theories of protoplanetary development. Phase closure with three antennas at Chajnantor. The radio telescope combines signals from each, working as a single giant telescope … Locations of the EHT Telescopes This diagram shows the location of the telescopes used in the 2017 EHT observations of M87. “This is one of the largest programs executed at ALMA,” Walter says, adding that the program used almost 200 hours of ALMA observing time. Three prototype antennas have undergone evaluation at the Very Large Array since 2002. 66 radio telescopes in the Atacama Desert of northern Chile, Location of Atacama Large Millimeter Array, The first two ALMA antennas linked together as an, Three ALMA antennas linked together as an interferometer for the first time, ALMA prototype-antennas at the ALMA test facility, July 2008 NRAO ALMA newsletter article by Dr. Al Wootten, National Institutes of Natural Sciences, Japan, Institut de Radio Astronomie Millimétrique, National Astronomical Observatory of Japan, After a Tough Year, ALMA's Star Begins to Rise at Last, removing excessive or indiscriminate images, Learn how and when to remove this template message, Atacama Submillimeter Telescope Experiment, "Alma telescope peers into space from Chile's mountains", "ALMA Inauguration Heralds New Era of Discovery", "At the End of the Earth, Seeking Clues to the Universe", "Alma telescope: Ribbon cut on astronomical giant", "ALMA - Atacama Large Millimeter/submillimeter Array", "Ground breaking ceremony for the Atacama Large Millimeter Array (ALMA)", "National Radio Astronomy Observatory - Legacy Content - ALMA (CV)", Chile's ALMA probes for origins of universe, "General Dynamics Receives $169 Million to Build 12-Meter Antennas for Advanced Radio Telescope", https://www.almaobservatory.org/en/announcement/result-of-the-initial-testing-of-the-japanese-aca-12-m-antenna-to-be-delivered-to-alma-2/, https://www.almaobservatory.org/en/press-release/alma-observatory-equipped-with-its-first-antenna/, "Monster Moves, Season 5, Episode 6: Mountain Mission", "European ALMA antenna brings total on Chajnantor to 16", "Birth of Planets Revealed in Astonishing Detail in ALMA's 'Best Image Ever' - NRAO: Revealing the Hidden Universe", "RELEASE 14-038 - NASA's 3-D Study of Comets Reveals Chemical Factory at Work", "Event Horizon Telescope Captures First Image of Black Hole | Astronomy | Sci-News.com", "Phosphine gas in the cloud decks of Venus", "Scientists find gas linked to life in atmosphere of Venus", "First Light for Band 5 at ALMA - New receivers improve ALMA's ability to search for water in the Universe", Creative Commons Attribution 4.0 International License, ALMA Observatory: ALMA Selects New Director, "New 2012 ALMA Video Compilation Released", "ALMA Compact Array Completed and Named After Japanese Astronomer", "Workers at Earth's largest radio telescope in Chile strike over pay, working conditions", "Workers strike at world's largest radio telescope", "ALMA resumes operations after end of workers' strike", "COVID-19 (coronavirus) Measures at ALMA", "ALMA Residencia Handed Over - New accommodation for staff and visitors at ALMA site in Chile", How the Huge ALMA Radio Telescope Works (Infographic), An optical system design for the Atacama Large Millimeter Array, Australian Square Kilometre Array Pathfinder, Canadian Hydrogen Intensity Mapping Experiment, Combined Array for Research in Millimeter-wave Astronomy, Multi-Element Radio Linked Interferometer Network, Special Astrophysical Observatory of the Russian Academy of Science, Space Telescope European Coordinating Facility, https://en.wikipedia.org/w/index.php?title=Atacama_Large_Millimeter_Array&oldid=996886963, Articles with infoboxes completely from Wikidata, Articles containing potentially dated statements from 2014, All articles containing potentially dated statements, Creative Commons Attribution-ShareAlike License, Atacama Large Millimeter and Submillimeter Array. 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