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). During Autumn 2009, the first three antennas were transported one-by-one to the Array Operations Site. ("Alma" means "soul" in Spanish and "learned" or "knowledgeable" in Arabic.) The American and European partners each provided twenty-five 12-meter diameter antennas, that compose the main array. ALMA is an international partnership among Europe, the United States, Canada, Japan, South Korea, Taiwan, and Chile. ALMA, a telescope so powerful it can see into the past . Research led by Durham University and with observations made with the Atacama Large Millimeter Array (ALMA) telescope of the European Southern Observatory reveals that after the collision, one of the galaxies ejects 10,000 Suns-worth of gas every year. The 130-ton ALMA antenna transporter "Otto" during its naming ceremony. Opening of Joint ALMA office, Santiago, Chile. The target of the observation was a pair of colliding galaxies with dramatically distorted shapes, known as the Antennae Galaxies. ALMA images of two molecular clouds. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA. ALMA … The antennas forming the Atacama Compact Array, four 12-meter antennas and twelve 7-meter antennas, were produced and delivered by Japan. [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. This video shows ISS astronauts congratulating the ALMA Partners on the occasion of its inauguration. May 09, 2014. Costing $1.4 billion, ALMA is the world’s most expensive ground based telescope. The final antenna for the project is here seen arriving to the high site at the observatory, 5000 meters above sea level. It also delayed the cycle 8 proposal submission deadline and suspended public visits to the site.[44]. By combining 54 parabolic antennas with 12 meter diameters and 12 parabolic antennas with diameters of 7 meters, ALMA creates one huge radio telescope consisting of 66 antennas in total. The telescope as we know it today has gone through several significant milestones since it was first patented way back in 1608. [2] Costing about US$1.4 billion, it is the most expensive ground-based telescope in operation. Calçada (ESO) & NASA/JPL-Caltech/WISE Team, 地球の生命のルーツは、いったいどこにあるのでしょうか? 生命の材料となる物質は、地球にしか存在しないのでしょうか?それとも、宇宙のいろんな場所にありうるのでしょうか?, アルマ望遠鏡は宇宙空間に漂う塵やガス、ガスのなかに含まれるアミノ酸などの有機物をとらえることもできます。それは、地球以外に生命が誕生する可能性を調べることにつながります。私たちの体はタンパク質でできていて、タンパク質はアミノ酸でできています。アミノ酸が宇宙に存在することがわかれば、地球以外で生命が発生する可能性があるかもしれません。アルマ望遠鏡は、アミノ酸をはじめとするさまざまな有機分子が放つ特有の電波をとらえることを目指しています。, アルマ望遠鏡の活躍により、惑星誕生の現場で複雑な有機分子がすでに何種類も発見されています。アミノ酸があれば必ず生命が生まれるわけではありませんが、少なくともその前提がどれくらいの確率で整っているのか、アルマ望遠鏡による観測で明らかになる日も遠くないでしょう。, ここまでに挙げたさまざまな宇宙の謎に迫るために重要なのが、宇宙からやってくる電波を望遠鏡でとらえることです。夜空に輝く恒星たちは、表面の温度が数千度~数万度という高温のため、私たちの目にも見える光(可視光)を発しています。すばる望遠鏡のような光学望遠鏡は、その恒星が放つ光をとらえることができます。しかし、惑星の材料となる塵やガス、ガスに含まれるアミノ酸はマイナス260℃程度と、とても低温なため、光を放つことができません。アルマ望遠鏡はこの塵やガスやアミノ酸が放つ電波をキャッチすることで、銀河や星、惑星の材料、そして生命の材料となる物質の分布や性質を明らかにしようとしています。, 下の画像は、2つの銀河が衝突しつつある「触角銀河」の画像です。アルマ望遠鏡が電波で観測した画像と、光学望遠鏡が可視光で観測した画像を重ねることで、可視光では見えなかった低温のガスの分布を見ることができます。アルマ望遠鏡が観測できるのは、「ミリ波・サブミリ波」と呼ばれる電波です。ミリ波・サブミリ波を観測する望遠鏡はほかにもいくつかありますが、非常に高い感度と解像度(視力)をあわせもつアルマ望遠鏡は、大きく抜きんでた存在であり、これまで見ることができなかった宇宙の姿を詳しく描き出すことができます。, 電波と可視光で観測した触角銀河。電波では、可視光では見ることのできないガスや塵の分布を知ることができます。, Credit:ALMA(ESO / NAOJ / NRAO), ESO, NASA / ESA Hubble Space Telescope, 世界最大級を誇るすばる望遠鏡の口径が8.2mもあるとおり、望遠鏡は、その口径が大きければ大きいほど弱い光や電波をとらえることができ、また解像度(視力)も向上します。このため、天文学者はより口径の大きな望遠鏡を作りだすことに力を注いできました。しかし、ある程度以上大きな望遠鏡は、技術的な限界から作ることが困難です。この限界を突破するためのアイデアが、「小さな望遠鏡を広い場所にたくさん並べ、それらを連動させて1つの巨大な望遠鏡として機能させる」というものです。この仕組みは「干渉計」と呼ばれ、アルマ望遠鏡もその技術を使っています。アルマ望遠鏡では、口径12mのパラボラアンテナ54台と、口径7mのパラボラアンテナ12台、合計66台を結合させることで、1つの巨大な電波望遠鏡を作りだします。, アルマ望遠鏡の66台のアンテナは最大で直径16kmの範囲内に設置することができます。これは、東京の山手線の直径距離(田端〜品川間)に匹敵する大きさです。このときのアルマ望遠鏡の口径は実質16kmとなり、解像度は人間の視力に例えると「視力6000」、大阪に落ちている1円玉の大きさが東京から見分けられる能力に相当します。すばる望遠鏡やハッブル宇宙望遠鏡の視力と比べても10倍、これまでの電波望遠鏡と比べると数十倍から100倍高い性能になります。また、アンテナの位置を移動させることで、カメラのズームレンズのような働きを持たせることができます。広い視野で観測を行いたいときはアンテナを狭い範囲に集め、反対に高い解像度を得たいときにはアンテナを広い範囲に展開します。, Credit: ALMA (ESO/NAOJ/NRAO)/L. [1] The Very Large Telescope at the Paranal Observatory in Chile is a 27-foot (8.2-meter) interferometer. A groundbreaking ceremony was held on November 6, 2003 and the ALMA logo was unveiled.[8]. Working together, the separate ALMA telescopes become one giant telescope up to 11 miles (16 km) across. By using smaller antennas than the main ALMA array, larger fields of view can be imaged at a given frequency using ACA. ALMA can produce as many as 1,291 baselines, some up to 16 kilometers long. The array has much higher sensitivity and higher resolution than earlier submillimeter telescopes such as the single-dish James Clerk Maxwell Telescope or existing interferometer networks such as the Submillimeter Array or the Institut de Radio Astronomie Millimétrique (IRAM) Plateau de Bure facility. [28], ALMA participated in the detection of phosphine, a biomarker, in the atmosphere of Venus. Red and green show the distributions of molecular gas with different velocities mapped by 13 CO emissions. ALMA consists of 66 parabolic dishes, 54 of which are 12 metres (39 feet) in diameter and 12 of which are 7 metres (23 feet) in diameter. By using smaller antennas than the main ALMA array, larger fields of view can be imaged at a given frequency using ACA. ALMA (Atacama Large Millimeter/submillimeter Array) is a radio telescope inaugurated in 2013. The blue region in left panel shows the ionized hydrogen gas observed with the Hubble Space Telescope. European, North American & Japanese amend agreement on the Enhanced ALMA. Activates for operating the ARC have also divided into the three main regions involved (Europe, North America and East Asia). It has captured images of the most distant observations of water to date. [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. Red and green show the distributions of molecular gas with different velocities mapped by 13 CO emissions. In 1609 an Italian physicist and astronomer named Galileo became the first person to point a telescope skyward. Transporting the 115 tonne antennas from the Operations Support Facility at 2900 m altitude to the site at 5000 m, Costing $1.4 billion, ALMA is the world’s most expensive ground based telescope. Moonrise above the 12 meter wide access road to the ALMA High Site. 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 … ALMA was initially a 50-50 collaboration between the National Radio Astronomy Observatory and European Southern Observatory (ESO) and later extended with the help of the other Japanese, Taiwanese, and Chilean partners. ALMA … Thirty-two 12-m antennas in the 12-m array. Linking three antennas allows corrections of errors that can arise when only two antennas are used, thus paving the way for precise, high-resolution imaging. 09.12.03. Image of telescope in transit at the Site Erection Facility. Go inside the U. S. insurrection with a National Geographic photographer. [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. ALMA is being built by Europe, the United States, Canada, East Asia and the Republic of Chile. They are powered by twin turbocharged 500 kW Diesel engines. Sixteen 12-m antennas in the 12-m array. The Atacama Large Millimeter/submillimeter Array (ALMA) is a telescope array in Chile that includes 66 receivers. PROGRAM: (20 min talk + 5 min QA) 8:55-9:00 Daisuke Iono Welcome. The ALMA observatory itself is split into two facilities: at 3200 metres, the Operations Support Facility (OSF) which contains the administrative offices, maintenance facilities, and living quarters for … History. The inauguration ceremony took place in Chile’s high desert at an altitude of 16,500 feet, or 5,000 meters. [42][43], In March 2020, ALMA was shut down due to the COVID-19 coronavirus crisis. Two peacock-shaped gaseous clouds were revealed in the Large Magellanic Cloud (LMC) by observations with the Atacama Large Millimeter/submillimeter Array (ALMA). (in HD). 「私たちが住む太陽系は、どのように生まれたのだろう?」 ALMA, currently the largest telescope array in the world, just took a look at the Hubble Space Telescope’s deepest-ever image, the Hubble Ultra Deep Field. The blue region in left panel shows the ionized hydrogen gas observed with the Hubble Space Telescope. [21] In October 2012, 43 of the 66 antennas had been set up. A view across the plains of Chajnantor with the ALMA construction site at the center. The ALMA radio telescope array captures a ring of fire – the light from a remote, well-formed galaxy more than 12 billion light years away that was gravitationally magnified as it was bent around an intervening galaxy. The blue part in right panel shows the emissions from dust particles obtained with ALMA. 9:25-9:50 Tom Bakx The dust-obscured early Universe as probed by ALMA. 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. European, North American & Japanese draft agreement, with Japan providing new extensions to ALMA. A talk on the Atacama Large Millimeter/submillimeter Array (ALMA), by Leonardo Testi. ALMA is a premier telescope for studying the first stars and galaxies that emerged from the cosmic “dark ages” billions of years ago. (in HD). The Atacama Large Millimeter/submillimeter Array (ALMA) surveyed the Hubble Ultra Deep Field, uncovering new details of the star-forming history of the Universe. Start of Early Science Cycle 1. Start of Early Science Cycle 0. The ACA works together with the main array in order to enhance the latter's wide-field imaging capability. By using smaller antennas than the main ALMA array, larger fields of view can be imaged at a given frequency using ACA. This video shows the antenna being moved on the giant transporter called "Otto". [10] ALMA is the largest and most expensive ground-based astronomical project, costing between US$1.4 and 1.5 billion. The complex was built primarily by European, U.S., Japanese, and Canadian companies and universities. [38][39][40][41] After 17 days an agreement was reached providing for reduced schedules and higher pay for work done at high altitude. ESOcast 51: Video report about the ALMA correlator. Alma - the most complex ground-based telescope in existence - is officially opened during an inauguration ceremony in Chile's Atacama Desert. A merger between two galaxies led to something unique, as the news brought by Daily Mail reveals. On March 13, 2013, the ALMA Telescope in northern Chile officially went online. The criteria for the potential ALMA site include: (1) high atmospheric transparency at submillimeter wavelengths (2) good radio seeing to achieve sub-arcsec resolution (3) low wind velocity for a good pointing accuracy (4) flat and wide (> 3 km x 3 km) area to locate the array (5) easy accessibility to the site (6) existing infrastructure, etc. [14] The first antenna was delivered in 2008, the last in 2011.[15]. Testing of first prototype antenna begins at the ALMA Test Facility (ATF) site in Socorro, New Mexico. Here’s what it found. 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. 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). [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. [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. or moving antennas around the site to change the array size, presents enormous challenges; as portrayed in the television documentary Monster Moves: Mountain Mission. [16] The solution chosen is to use two custom 28-wheel self-loading heavy haulers. Time-lapse video at the ALMA Array Operations Site (AOS). On 30 September 2013 the final ALMA antenna was handed over to the ALMA Observatory. Costing more than a billion US dollars, it is the worlds's most expensive ground-based telescope. ALMA began scientific observations in the second half of 2011 and the first images were released to … 66th and final antenna arrived and accepted. Image of the dust ring around the bright star Fomalhaut from the ALMA, and underlying blue image obtained by the NASA/ESA Hubble Space Telescope. It is composed of 66 antennas, each several metres in diameter, and works in synergy as a single giant telescope thanks to the interferometry technique. It is also one of our most important scientific inventions for exploring our galaxies. 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. 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. A history of telescopes Mirrors of creation. This new version of ALMA allows its 66 antennas to function as a single radio dish 85 meters in diameter. Featured Videos Related A Hundred Million ... History. 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. 01:32. Go inside the U. S. insurrection with a National Geographic photographer. In 1609 an Italian physicist and astronomer named Galileo became the first person to point a telescope skyward. 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). 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. It was this period that the scientists in the ALPINE project focused on when they used ESO's ALMA telescope to carry out the first ever large survey of distant galaxies. 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. This 16-minute video presents the history of ALMA from the origins of the project several decades ago to the recent first science results. Calçada (ESO), アルマ望遠鏡が観測するミリ波・サブミリ波は、地球の大気に含まれる水蒸気によって激しく吸収されてしまうため、空気が薄く乾燥した高地に建設する必要がありました。また、複数の電波望遠鏡を協働させる干渉計の技術を活用するためには、たくさんのアンテナを設置するための広い平坦な場所が必要です。野心的なアルマ望遠鏡を設置するにふさわしい「観測最適地」を求めて、天文学者は世界中の高地を調査しました。, その答えとして見出されたのが、南米チリ北部、アタカマ砂漠の標高5,000mの高原です。アタカマ砂漠は年間降水量が100mm以下で、世界でもっとも乾燥した場所のひとつといわれています。日本からアルマ望遠鏡施設までは、飛行機の乗り継ぎ時間を含めると40時間ほどかかりますが、アルマ望遠鏡設置に理想的な条件を備えた、地球上で究極の場所といえます。, アルマ望遠鏡のような巨大プロジェクトは、一国だけで開発・運用できるものではありません。世界中の国々が手を取りあい、人と技術と資金を出しあうことでアルマ望遠鏡は生まれました。, 一般的に学術研究は熾烈な国際競争の場でもありますが、同時に研究者が国々を自由に行き来したり、国際協力が当たり前のように行われたりもする平和な分野でもあります。1980年代から1990年代にかけて、日米欧のそれぞれが独自の巨大電波望遠鏡を計画していました。これらの状況は国際会議でお互いに共有されていたため、お互いの良いところを取り入れていくにつれて、計画はどれも似たものになっていきました。そして、「それぞれの計画を合体させ、1つの国や地域では実現できない理想の望遠鏡を作ってはどうか」という構想が日米欧の研究者たちのなかから生まれたのです。アルマ望遠鏡計画の誕生です。, 現在のアルマ望遠鏡の運用は、日本・台湾・韓国の東アジア、アメリカとカナダからなる北米、欧州南天天文台を構成する16か国と建設地のチリ共和国の協力で行われています。日本の国立天文台のスタッフ十数名も現地に赴任し、世界中から集まってきた研究者や技術者・事務職員と協力してアルマ望遠鏡の運用にあたっています。また日本・アメリカ・ドイツに設置されたアルマ地域支援センターでは、それぞれ東アジア・北米・欧州地域にいる天文学者がアルマ望遠鏡で研究を行うためのサポートを担当しています。, 国際協力で生まれたアルマ望遠鏡プロジェクトのなかで、日本は全体のおよそ4分の1の貢献をしています。パラボラアンテナは66台のうちの16台、電波をとらえる受信機は10種類のうち3種類を日本が開発しました。日本製の16台のアンテナで集められた信号を処理するためのスーパーコンピューターも、日本が開発したものです。アルマ望遠鏡には、日本の最先端技術が惜しみなく投入されているのです。, パラボラアンテナは、はるかかなたの天体からやってくる電波が最初に触れる人工物です。微弱な電波をもれなく集めるため、アンテナの表面はできるだけ滑らかにしておく必要があります。アルマ望遠鏡では、その誤差を人間の髪の毛の太さの約3分の1、25ミクロン以下という高い精度で実現しました。, パラボラアンテナには、観測対象の天体を高い精度で追尾できる性能が求められます。アタカマ砂漠の強い日射や昼夜の大きな温度差、強い風など、厳しい自然環境のもとでこれを実現するのは簡単なことではありませんでした。, 日本製のアンテナには、アンテナ自身の微妙なゆがみを自ら計測してリアルタイムで補正する最先端の技術をはじめ、さまざまな工夫が凝らされています。, アンテナで集められた電波をコンピューターで処理するための電気信号に変換するのが、受信機です。アルマ望遠鏡では、観測した電波を10の周波数帯(バンド)に分けて電気信号に変換するため、それぞれに最適な設計で受信機を開発しました。受信する波長が短くなるほど精度の要求も高くなります。, 日本は、超伝導技術や精密機械加工技術など、最先端技術の粋を集め、もっとも波長の短いバンド10受信機を含む3種類の受信機を開発し、全66台のアンテナに搭載される受信機を量産しました。, たくさんのアンテナからやってくる電気信号を処理するのが、「相関器」と呼ばれるスーパーコンピューターです。, 日本が開発した相関器は、日本製の16台のアンテナから届けられる膨大なデータを即座に処理する必要があります。そのデータ処理能力は、1秒間に256ギガバイト。DVD54枚(片面一層)のデータを毎秒処理することが可能です。, アルマ望遠鏡を構成する66台のアンテナのなかで、日本が開発した16台のアンテナ群と受信機、相関器からなるシステムを、「アタカマコンパクトアレイ(愛称:モリタアレイ)」と呼びます。たくさんのアンテナを連動させて、巨大な1つの望遠鏡とする「干渉計」方式の電波望遠鏡では、アンテナの間隔を広げれば広げるほど解像度が上がりますが、逆に視野は狭くなります。逆に、大きく広がった天体を広い視野で観測するためには、アンテナの間隔を小さくする必要があります。モリタアレイは、口径の小さなアンテナを狭い範囲にまとめることで、それを実現しました。, つまりアルマ望遠鏡を使う天文学者たちは、広い範囲に展開される米欧のアンテナ群と、モリタアレイの両方を組み合わせて観測することで、広がった天体のなかの細かい構造まではっきりと描き出すことができるのです。なおモリタアレイの名は、その設計に大きな貢献を残した、故・森田耕一郎 国立天文台教授にちなんでつけられたものです。アルマ望遠鏡が世界の天文学研究を今後もリードし続けるために、パワーアップのための将来開発計画も検討されています。日本の高い技術力をアルマ望遠鏡に投入することで、これからも天文学の発展に貢献していきます。, Credit:ALMA(ESO / NAOJ / NRAO)/ L. Calçada, アリゾナ大学のフェイジ・ワン氏らの国際研究チームは、観測史上最も遠くに位置するクエーサーを発見しました。このクエーサー…, イギリス・ダーラム大学/フランス原子力・代替エネルギー庁(CEA)のアナガラジア・プグリシ(Annagrazia Puglisi)氏らの研究…, チリでは、2019年に引き続き、2020年12月14にも皆既日食を観察できる機会が巡ってきました。この天文学の一大イベントに乗って…, © 2005 - 2017 National AstronomicalObservatory of Japan, © 2005 - 2017 National Astronomical Observatory of Japan. The telescopes were provided by the European, North American and East Asian partners of ALMA. 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). Dec 11, 2012. 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. The project began when Europe, North America and Eastern Asia each worked in isolation to propose a telescope that would receive light in millimeter and submillimeter wavelengths in large magnitudes. 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. That's a huge, light-gathering eyeball! [37], In August 2013, workers at the telescope went on strike to demand better pay and working conditions. This location was chosen for its high elevation and low humidity, factors which are crucial to reduce noise and decrease signal attenuation due to Earth's atmosphere. 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. Final European / North American agreement, with 50% of funding from ESO, and 50% of funding shared between USA and Canada. 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. One theory suggests that the faster accretion rate might be due to the complex magnetic field of the protoplanetary disk. This video clip shows the distinguished guests, including the President of Chile, Sebastián Piñera, arriving at the ALMA Operations Support Facility (OSF), located at an altitude of 2900 meters in the Atacama Desert in Chile for the inauguration of the giant telescope. The guests are shown with one of the giant ALMA transporters as well as other components. ESO/NRAO/NAOJ joint site testing with Chile. Arrival of the two ALMA transporters in Chile. The blue features are galaxies imaged by Hubble. 01:32. The blue part in right panel shows the emissions from dust particles obtained with ALMA. 9:00-9:25 Tomoko Suzuki Gas contents in star-forming galaxies around Cosmic High Noon. The array is located on the Chajnantor Plateau in the Atacama Desert. Share Link. The high sensitivity is mainly achieved through the large numbers of antenna dishes that will make up the array. 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. A Panchromatic View of Galaxy Build-up in the First 2 Gyrs of Cosmic History-----Venue: Online Date: December 15, 2020. First antenna movement with a transporter. European/U.S. 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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