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There is a simple relationship between mirror size and resolving power: R = 11.6 / D. First, R = the angular size of the object in arcseconds.
An arcsecond is a measure of angular size (how big an object appears to be — if two objects are the same size).
Over the course of three more years, we did it five more times.
Plugging that into the formula, we see that Hubble’s resolution is 11.6 / 240 = 0.05 arcseconds. The first is that there’s a wavelength dependence too; for a given telescope size, the shorter the wavelength the more resolution you get (a telescope will resolve blue objects better than red ones, since blue has a shorter wavelength).So really, Hubble’s working resolution limit is about 0.1 arcseconds.There are tricks you can do to get slightly higher resolution, but that’s getting too picky. So what does this mean if you want to look at the lunar artifacts?That includes all the pictures taken by the astronauts themselves. Check out the hottest cyber sex game in the world and experience real-time breathtaking 3D hardcore virtual sex!