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intensity interferometry

astronomy

Quick Summary

Intensity interferometry is a technique in astronomy used to measure the angular size of bright visible stars. Developed by Robert Hanbury Brown and Richard Q. Twiss, it applies principles of radio interferometry to visible light. This method allows astronomers to overcome atmospheric distortion and resolve details of stars that would otherwise be blurred. An intensity interferometer was set up in Narrabri, Australia, to measure the sizes of hot stars. A stellar interferometer, a related device, is an attachment to a telescope used for measuring objects that subtend very small angles, such as close double stars.12

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