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> In other words, it's got a giant steel mounting that needs an entire building foundation to support it. This is still the case for the Alt-Az telescopes. For stability, telescopes are built on a foundation that is independent from the building's foundation and, ideally, that goes to bedrock. > Modern (giant) telescopes use alt-azimuth mounts (similar to a normal camera mount), which require two axes to be adjusted simultaneously with computer control. This causes the projected image to rotate and is not suitable for photographic plates but can be compensated with digital image processing. Actually, there's usually a third rotation axis often added to instruments (or their mount points) for Alt-Az telescopes, called a field rotator. As one might expect, this counteracts the apparent rotation of the field and maintains the same image orientation on the detector. Note that this is also important for spectroscopy and not just imaging. For spectroscopy, you may also want to ensure the position angle of your slit is constant relative to your source of interest, particularly if the source is not point-like. In principle, one could correct for the field rotation with image processing. But for many observing programs, the individiual exposures can be in excess of 15 minutes. For crowded fields or extended sources, it would be non-trivial to deconvolve the field rotation. In practice, it's much easier to just add a third axis to the instrument which counteracts the field rotation. |