they only cover 10 square degrees of sky"only", heh (BTW, it's 12 linear degrees, 105 square degrees)
It's hard to make instruments that provide good images across wide angles. Many visual telescopes, both amateur and professional, stay at 1 degree and less of true field of view for medium and high magnification; 2 degrees true field is already pretty good and it's usually obtained at low magnification.
Astrographs can produce wider fields of view, 10 degrees being considered pretty studly, to borrow a quote from Linus. But normally you don't get that "for free". You force an optical element to work at such a wide angle, and then correct the inevitable distortions with various correctors, which are usually lenses or combinations thereof.
The Kepler mission is essentially a Schmidt camera, an old, true and tested design:
http://en.wikipedia.org/wiki/Schmidt_camera
Its almost 1 meter aperture would allow a theoretical resolving power of almost 0.1 arcsec (which is my full height as an average guy, standing in Los Angeles, as seen from New York), which could be exploited freely in space since there's no atmosphere to reduce it. Unfortunately, for the type of measurements they do, the image is softened intentionally back to 10 arcsec, which is the theoretical resolution of a 1 cm aperture, or the lens in your digital camera (assuming your camera is a true diffraction-limited system, which it very likely isn't). However, the light gathering power of Kepler is, of course, 10k greater than your camera's; and, again, it's unimpeded by messy and light-polluted Earth atmosphere.
Sorry for the pop-sci journalism comparisons, but the numbers really are kind of mind-boggling.
http://kepler.nasa.gov/Mission/QuickGuide/MissionDesign/Phot...
Please note the curved sensor array, which is due to the fact that a Schmidt scope actually does have a curved field (the light comes to true focus not in a plane, but in a segment of sphere). In fact, flat fields are something you strive for, you don't get for free; even common types of instruments have curved fields, but in most cases the radius of curvature is so big you can ignore it.
Optical instruments are tricksy.