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Slide 1Slide 2Slide 3Slide 4Slide 5Slide 6Slide 7Slide 8Issues with the use of telescopesLong wavelength (Radio) AstronomyResolution RevisitedRadio telescopes have relatively poor ability to resolve objects because of the long wavelength of the EM waves.Issues with the use of telescopesResolutionFor the National Radio Astronomical Observatory Robert C. Byrd Radio Telescope, wavelength ≈ 1 m = 1 x 106 μm Diameter of the aperture (the objective) = 100 mΘmin ≈ 2500” = 41’ = .69o The angular diameter of the moon = 30’ The angular diameter of the Andromeda Galaxy ≈ 178’The NRAO telescope would be able (roughly) to resolve radio sources of these angular diametersThis is the worlds largest fully steerable radio telescope Θmin (in arc sec) = .25λ (in μm )D (in m)Issues with the use of telescopesLong wavelength (Radio) AstronomyInterferometrySolution: Use multiple radio telescopes separated by a large distance.The separation between the telescopes is called the baseline.Signals are then collected from the two sources and then combined. In effect, the separated telescopes increase the effective diameter of the objective. The process of combining the signals from two (or more) receivers is called interferometry.Issues with the use of telescopesInterferometryDΘmin (in arc sec) = .25λ (in μm )D (in m)D Signal CombinedΘmin (in arc sec) = .25λ (in μm )D (in m)Issues with the use of telescopesInterferometryVery high resolutions can be obtained even if the wavelengths are very


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Dayton PHY 250 - Interferometry

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