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Radio telescopes are much larger than optical telescopes because of wavelength.

Earth's atmosphere has two major "windows" where it is transparent to photons:

300 nm - 800 nm: optical wavelength window (approximate)

30 mm - 30 m: radio wavelength window (approximate)

Even the shortest-wavelengths used by radio telescopes at around 30 mm are still thousands of times longer than the longest wavelengths used by optical telescopes.

The wavelength has 2 effects on the size of a telescope:

* The angular resolution (in order to distinguish 2 nearby stars, FWHM) depends on the wavelength/aperture ratio. Radio-frequency photons require a wider aperture to focus than visible-light-frequency photons, so radio telescopes *must* be larger to get a reasonable resolution.

* A telescope typically requires the collecting area to be aligned within 1/10 of the wavelength it is designed for. Because it is almost impossible to get all the parts of a sufficiently large telescope aligned to within 80 nm, radio telescopes *can* be built much larger.

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