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The antennas, which are located at an altitude of 5,000 meters in the Atacama Desert of the Andes Mountains, incorporate innovative correction technologies and bespoke structural designs to minimize deformation due to heat or wind, and are driven with a direct-drive method using linear motors, resulting in the achievement of 25μm mirror accuracy and 0.6 arc-second pointing accuracy despite the harsh conditions of their operating environment.

Since the launch of the first-phase observations in September 2011, the ALMA project already has discovered a simple sugar molecule in a planet-forming region, measured the chemical composition of a very distant galaxy and found planet-forming gas streams that feed gas-guzzling giant planets. Going forward, Mitsubishi Electric will continue contributing to the project through training to local engineers and support in equipment maintenance.

About the ALMA project
ALMA is an international astronomical project involving the participation of Japan, the United States, Europe, Chile and other countries. Combining 66 telescopes using an interferometer array, the multiple antennas is equal to a massive radio telescope that would measure 18.5 kilometers in diameter, achieving a resolution equivalent to visualizing a small coin from a distance of 400 kilometers. The three major goals of the ALMA project are to investigate the birth of planets, the birth of galaxies and the evolution of matter in the universe.

Mitsubishi Electric's involvement in large telescopes for NAOJ
Since the 1980s, Mitsubishi Electric has been involved in numerous NAOJ-related projects for large telescopes, including the Nobeyama 45m radio telescope in Japan, the Subaru Telescope in Hawaii and the VLBI Exploration of Radio Astrometry (VERA) telescope in Japan.