Stellar Interferometer Part 1

the same technique to measure the diameter of Jupiter's moons in 1890. For smaller stars, a much longer baseline is needed such as the Mark III long baseline (12 m) interferometer at Palomar that is designed, and run by JPL. The large Binocular Telescope (LBT) is also suitable for stellar interferometry with its 22.8 m combined aperture (two 8.4 m mirrors). ... Optoform stellar interferometer opto mechanical assembly optics Palomar Mount Wilson Michaelson experiment fourier transform LBT ...

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