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An equatorial mounting is a telescope mount that aligns its polar axis parallel to Earth's axis. This allows the telescope to track celestial objects by rotating along this axis, compensating for Earth's rotation. The mounting supports a declination axis, which enables pointing to various angles north or south of the celestial equator. Declination and right ascension are the two coordinates used to locate objects in the sky, similar to latitude and longitude. By driving the polar axis at a sidereal rate (Earth's rotation rate relative to stars), telescopes with equatorial mountings can follow objects for extended periods, which is crucial for accurate astronomical observations.1

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