Atacama Large Millimeter Array
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 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 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. ALMA provides insight on star birth during the early Stelliferous era and detailed imaging of local star and planet formation.
| Alternative names | Atacama Large Millimeter and Submillimeter Array |
|---|---|
| Part of | Event Horizon Telescope Llano de Chajnantor Observatory |
| Location(s) | Atacama Desert, Antofagasta Region, Atacama Desert, Chile |
| Coordinates | 23°01′09″S 67°45′12″W |
| Organization | European Southern Observatory National Institutes of Natural Sciences, Japan National Science Foundation |
| Altitude | 5,058.7 m (16,597 ft) |
| Built | March 2013 |
| Telescope style | radio interferometer |
| Website | www |
Location of Atacama Large Millimeter Array | |
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ALMA is an international partnership amongst Europe, the United States, Canada, Japan, South Korea, Taiwan, and Chile. Costing about US$1.4 billion, it is the most expensive ground-based telescope in operation. ALMA began scientific observations in the second half of 2011 and the first images were released to the press on 3 October 2011. The array has been fully operational since March 2013.