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by mapt
4769 days ago
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Optical band sensors are not fast and low-noise enough, by several orders of magnitude, to do the sort of digital interferometry available with radio telescopes. Optical interferometers so far require optical correlators. This geometric rather than data-analytical approach mandates knowing and controlling the delay distances between the beams of light down to the nanometer. Combined with adaptive optics, this is some of the highest resolution imagery we can produce; But it is extremely limited because of the practical difficulties of these hardware concerns, even in a situation where there is a massive underground lab connecting the telescopes like at the VLT. Satellites floating in free space on opposite sites of the Earth affected by differential atmospheric drag, geomagnetic and heliomagnetic effects, and even relativistic differences would present what appears to be an intractable problem for this technology. |
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