![]() After each image is captured, a computer measures the apparent motion of one or more stars within the imaged area and issues the appropriate corrections to the telescope’s computerized mount. The device has a CCD or CMOS sensor that regularly takes short exposures of an area of sky near the object. To accomplish this automatically an autoguider is usually attached to either a guidescope or finderscope, which is a smaller telescope oriented in the same direction as the main telescope, or an off-axis guider, which uses a prism to divert some of the light originally headed towards the eyepiece. Even computer-tracked mounts and GoTo telescopes do not eliminate the need for tracking adjustments for exposures beyond a few minutes, as astrophotography demands an extremely high level of precision that these devices typically cannot achieve, especially if the mount is not properly polar aligned. In order for the resulting image to maintain usable clarity and sharpness during these exposures, the target must be held at the same position within the telescope’s field of view during the whole exposure any apparent motion would cause point sources of light (such as stars) to appear as streaks, or the object being photographed to appear blurry. Imaging of dim celestial targets, usually deep sky objects, requires exposure times of many minutes, particularly when narrowband images are being taken. This prevents the object from drifting across the field of view during long-exposures which would create a blurred or elongated image. An autoguider is an automatic electronic guidance tool used in astronomy to keep a telescope pointed precisely at an object being observed. ![]()
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