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What barriers - of technology, physics and possibly economy (things that would be possible technologically but are simply too expensive) sets the upper bound on quality of telescopes for observation of the sky in visible spectrum - observing surface of distant objects at maximum resolution/detail?

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"Zoom" is a poor word in the question. Telescopes don't "zoom" like consumer cameras. They tend to have a fixed focal length. "Zoom" might mean "how high can the telescope magnify" but telescopes typically aren't designed for high magnifications, as that is not the primary consideration. Suggest replacing "zoom" with "quality" as used in the detail... –  Jeremy Oct 7 '13 at 5:23
"Quality" is rather arbitrary metrics. I replaced "Zoom" with "Usable focal length" ("Usable" - because there are cameras of infinite focal length used commonly in machine vision systems in industry, but the brightness of observed objects drops with distance in them, so a couple meters away everything is entirely dark. They are good for automatic image recognition though, removing perspective effects from image to be analyzed, e.g. in QA of machined parts. Obviously not usable at multi-parsec distances) –  SF. Oct 7 '13 at 6:56

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Visual resolution of a telescope is directly proportional to the aperture of the telescope. The focal length, and hence the magnification that can be achieved, is then just following on the visual resolution.

The telescopes today are usually so well build that they are diffraction limited, which means optical resolution due to diffraction is the limiting factor. If you want to have "higher magnification" in a telescope, you always want to have a larger aperture. The longer focal length may help, but is not quite necessary.

And, as Jeremy said, the limiting resource in this is money. There are some engineering problems with building extremely large telescopes, but most of these can be solved, given enough money, time and resources.

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To answer the question reworded as: "What limits the quality of telescopes currently?" The answer is mostly: money.

It used to be: atmosphere. But with advances in adaptive optics, ground-based telescopes are achieving what used to require a space telescope. Plus, we have the technology for space telescopes if we want, like the pending JWST.

So pretty much, it boils down to funding. Who is going to spend the money on the expensive technology to see better and further, when science is being squeezed for funding from all quarters, and astronomers can't put forward a business case for a return on investment like a biotech company can for developing a grass that will result in cows burping less methane.

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Thanks to whoever -1'd my answer here without leaving a comment. When I wrote this, the question was NOT about focal length but what limits a telescope's "zoom" –  Jeremy Jul 2 at 21:16

Comparing telescopes that observe the visible spectrum to the radio spectrum, radio astronomers have been able to create telescopes with apertures of the order of kms, thanks to aperture synthesis. This is extremely hard in optical telescopes and the only telescope (afaik) that does so is the Large Binocular Telescope. The reason this is possible in radio astronomy is because we can measure the phase of the incoming wave using radio telescopes where as information about the phase is not captured by optical telescopes. Maybe in the future, technology will help us make optical detectors that can measure the phase of the wave.

coming to the size of the aperture itself, larger and larger sizes doesn't help as long as we don't account for the atmospheric seeing. the reason stars twinkle is because of atmospheric seeing. effects seeing can be negated using adaptive and active optics and advancement of these technologies will help astronomy move ahead.

coming to the actual detectors, the intrinsic noise from radio detectors (eg. bolometers) is much smaller than that in optical detectors (eg. CCDs). so again, maybe in the future, we have better detectors with extremely low noise.

(sorry coulnd't add more links. needed more rep :D)

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I wonder, radio waves, optical waves, that's all electromagnetic radiation, just different wavelengths. What's with optical waves that prevents radio waves tech to be adapted to that spectrum? –  SF. Mar 23 at 18:55
the detectors used in optical and radio astronomy are different. in radio astronomy, we detect the E and B fields of the propagating wave using antenna where as in optical astronomy, we absorb the photons and only measure the flux of photons and their energy. it's the wavelength/photon energy that makes the difference. similarly, can you think of how x-rays are studied though they pass through most metals? by the use of photo-multiplier tubes. –  rahul.poruri Mar 24 at 6:34

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