Generated by DeepSeek V3.2| Atacama Large Millimeter Array | |
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| Name | Atacama Large Millimeter Array |
| Caption | A view of the ALMA array on the Chajnantor Plateau. |
| Organization | European Southern Observatory, National Radio Astronomy Observatory, National Astronomical Observatory of Japan |
| Location | Chajnantor Plateau, Atacama Desert, Chile |
| Wavelength | 0.32 to 3.6 mm (radio) |
| Built | 2003–2013 |
| Website | almaobservatory.org |
Atacama Large Millimeter Array. It is the world's most powerful observatory for studying the universe in millimeter and submillimeter wavelengths. This international astronomy facility is situated on the high Chajnantor Plateau in the Atacama Desert of northern Chile. The collaboration behind it involves Europe, North America, and East Asia through partners like the European Southern Observatory and the National Radio Astronomy Observatory.
The facility is a transformative interferometer consisting of 66 high-precision antennas that work together as a single, enormous telescope. Its primary location on the Chajnantor Plateau was chosen for its extreme altitude, exceeding 5,000 meters, and the unparalleled dryness of the Atacama Desert, which is critical for observing faint signals in this part of the electromagnetic spectrum. By combining signals from its widely spaced antennas, it achieves extraordinary angular resolution, allowing it to peer into regions such as protoplanetary disks and distant galaxies with unprecedented detail. The project represents an unprecedented partnership between global scientific communities.
The array's technical backbone comprises fifty-four 12-meter diameter antennas and twelve 7-meter antennas, which form the Atacama Compact Array. These antennas can be repositioned across the Chajnantor Plateau along a specially designed transporter system, allowing the configuration to be adjusted from a compact 150-meter layout to a sprawling baseline extending over 16 kilometers. This mobility enables astronomers to tailor the instrument's resolution and field of view for specific observations. The receivers cover a wide range of frequencies from 84 to 950 GHz, sensitive to the cold universe, including molecular clouds and cosmic dust. Sophisticated correlator hardware, like the ALMA Correlator, combines the data from all antennas in real time.
Its core mission is to investigate cosmic origins, from the formation of stars and planets to the evolution of galaxies across cosmic time. Key early targets included the detailed structure of the protoplanetary disk around the young star HL Tauri, where it revealed stunning gaps indicative of planet formation. It has made landmark observations of the Event Horizon Telescope target, the supermassive black hole at the center of Messier 87, and has detected complex organic molecules in distant star-forming regions. The observatory has also studied the atmosphere of exoplanets and provided critical data on the Solar System, including comets like 67P/Churyumov–Gerasimenko.
The concept for a large millimeter array in the southern hemisphere emerged from separate planning efforts in the United States, Europe, and Japan during the 1990s. These projects eventually merged into a single global initiative, with the National Radio Astronomy Observatory leading the North American contribution and the European Southern Observatory managing the European part. Construction began in 2003 with major milestones including the installation of the first antenna in 2009 and the beginning of Early Science operations in 2011. The site inauguration was formally held in March 2013, presided over by the President of Chile, Sebastián Piñera. The total cost exceeded one billion United States dollars.
The observatory is operated under a tripartite agreement by the European Southern Observatory, the National Radio Astronomy Observatory (on behalf of North America), and the National Astronomical Observatory of Japan (representing East Asia). The Joint ALMA Observatory, headquartered in Santiago, Chile, oversees day-to-day scientific and technical operations. Observing time is allocated through competitive proposals reviewed by international panels from the partner regions. The facility supports a vast international community of astronomers, with data processed and archived at centers including the ALMA Regional Centres in Garching, Charlottesville, and Tokyo.
Category:Radio telescopes Category:Astronomical observatories in Chile Category:European Southern Observatory