MadSci Network: Astronomy |
Hello Alan! You present an interesting question. I'll start with a little history of high resolution images that I found. In June 1978, President Carter issued a Presidential Directive (37) that limited the spatial resolution within US Landsat images to 10 meters. In 1994, Clinton further decreased this maximum allowable resolution to 1 meter for commercial satellites. In fact, I saw an image with about 1 meter resolution at the American Astronomical Society meeting in Rochester, NY this past June. The detail was incredible--you could even make out lines painted in roads and helicopter blades, though they were not perfectly clear. These are legal limits imposed by the government on commercial satellites. They do not represent technological limits. Commercial satellites cannot therefore use images to identify individual people, for example. I found tantalizing hints that the highest resolution images obtained by American satellites were a few inches across, but of course those images are not publicly available. I did not find any indication that satellites with 1 inch resolution capability are currently in use or planned (though this information may be classified). The resolution of an image depends on the wavelength of light used in making the observation and the diameter of the telescope. This gives an angle. The actual physical measurement, in terms of inches or meters, depends on the distance between the observer and whatever is being imaged. So for imaging very small scales you would want a combination of a large telescope and a low orbit. A typical low earth orbit is 300-1000 miles. Lets take the lower limit of 300 miles for this demonstration. (Keep in mind that the lower the orbit of a satellite, the faster its orbit degrades so that these satellites have a lower lifetime than satellites in higher orbits.) To be able to image an object of 1 inch from this height, the telescope must have an angular resolution of 0.011 arc seconds (where an arc second is 1/3600 of a degree). The theoretical angular resolution of a telescope is given by theta(in arc seconds) = 1.22*206265*wavelength/(mirror diameter). If we take the wavelength to be 500 nm (visible light) then the mirror would have to be 11.4 meters in diameter (much too big to launch right now). On the other hand, to image a 1-meter object, the mirror would only have to be 0.3 meters--much more reasonable in terms of technology and cost. For a 1-meter telescope to resolve a 1 inch object, it would have to be a mere 26 miles away. Keep in mind these numbers are a theoretical minimum and do not take into account conditions which degrade the performance of an instrument. Interference due to the atmosphere itself--the bane of any ground based astronomer--will act to decrease resolution and image quality. Remarkable methods of improving image quality and resolution have been developed over the last few years. A method called adaptive optics (http://www.us-gemini.noao.edu/public/adaptive.html) is used by the Gemini telescopes to compensate for atmospheric degradation. Clever data reduction techniques also help to improve image quality. So while there is no technological reason why a 1 inch resolution cannot be obtained, it would be very difficult and expensive to do so. As for moving the aperture--the closer a satellite is to Earth, the faster it moves relative to the ground. While a satellite can track a stationary object, this fast motion means that (for low earth orbit satellites) the object is only visible for a couple minutes while the satellite is above the horizon. It is possible to point a satellite to image an area of interest using gyroscopes. To move the satellite itself is more of a problem and would not be done unless absolutely necessary. Erika
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