The Submillimeter Array

The Submillimeter Array (SMA) is an advanced radio telescope located in Hawaii that observes celestial objects using submillimeter wavelengths, which are shorter than microwave but longer than infrared. By combining data from multiple dish antennas, it can capture detailed images and information about distant galaxies, star formation, and other astronomical phenomena. The SMA is particularly valuable for studying cool gas and dust in space, helping scientists understand the universe's structure and evolution, as well as the formation of stars and planets. Its unique capabilities enable researchers to explore areas of the cosmos that are often hidden from visible light.