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IR Astronomy Pioneer Dies

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TUCSON, Ariz., June 22, 2009 -- Infrared astronomy pioneer Frank J. Low died June 11, according to the University of Arizona, his employer since 1965. He was 75. Low was a solid-state physicist who became a leader in the new field of infrared astronomy after inventing the gallium-doped germanium bolometer in 1961. After receiving his PhD from Rice University in 1959, Low developed a low temperature thermometer at Texas Instruments but realized that the device had much greater potential as an infrared bolometric detector. He moved to the National Radio Astronomy Observatory to explore use of his bolometer in...Read full article

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    Published: June 2009
    Glossary
    astronomy
    The scientific observation of celestial radiation that has reached the vicinity of Earth, and the interpretation of these observations to determine the characteristics of the extraterrestrial bodies and phenomena that have emitted the radiation.
    bolometer
    A thermometric instrument used for the detection and measurement of radiant energy. Its essential component is a short narrow strip covered with a dead black absorbing coating and mounted at the lower end of a long cylindrical tube having a stop across it to exclude unwanted radiation. The electrical resistance of the strip changes with the changes in temperature that arise from absorbing varying amounts of radiant energy.
    infrared
    Infrared (IR) refers to the region of the electromagnetic spectrum with wavelengths longer than those of visible light, but shorter than those of microwaves. The infrared spectrum spans wavelengths roughly between 700 nanometers (nm) and 1 millimeter (mm). It is divided into three main subcategories: Near-infrared (NIR): Wavelengths from approximately 700 nm to 1.4 micrometers (µm). Near-infrared light is often used in telecommunications, as well as in various imaging and sensing...
    infrared astronomy
    The study and the interpretation of the infrared emittances of celestial bodies and phenomena.
    photonics
    The technology of generating and harnessing light and other forms of radiant energy whose quantum unit is the photon. The science includes light emission, transmission, deflection, amplification and detection by optical components and instruments, lasers and other light sources, fiber optics, electro-optical instrumentation, related hardware and electronics, and sophisticated systems. The range of applications of photonics extends from energy generation to detection to communications and...
    telescope
    An afocal optical device made up of lenses or mirrors, usually with a magnification greater than unity, that renders distant objects more distinct, by enlarging their images on the retina.
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