Sextant (astronomical)

Sextants for astronomical observations were devices depicting a sixth of a circle, used primarily for measuring the positions of stars. They are of significant historical importance, but have been replaced over time by transit telescopes, astrometry techniques, and satellites such as Hipparcos.

There are two types of astronomical sextants, mural instruments and frame-based instruments.

Mural sextants are a special case of a mural instrument. Many were made that were quadrants rather than sextants. They were a kind of specialty of medieval Muslim astronomers, to whom the credit of building the first mural sextants is attributed.

The first known mural sextant was constructed in Ray, Iran, by Abu-Mahmud al-Khujandi in 994. To measure the obliquity of the ecliptic, al-Khujandī invented a device that he called al-Fakhri sextant (al-suds al Fakhrī), a reference to his patron, Buwayhid ruler, Fakhr al Dawla (976-997). This instrument was a sixty-degree arc on a wall aligned along a meridian arc (north-south line). Al Khujandi’s instrument was larger than previous instruments; it had a radius of about twenty meters. The main improvement incorporated in al-Fakhri sextants over earlier instruments was bringing the precision of reading to seconds while older instruments could only be read in degrees and minutes. This was confirmed by al-Birūni, al-Marrākushī and al-Kāshī. Al-Khujandī used his device to measure the sun's angle above the horizon at the summer and winter solstices; these two measurements allow computation of the latitude of the sextant's location and the obliquity of the ecliptic.

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