A
sextant is an instrument used to measure the angle between any two visible objects. Its primary use is to determine the angle between a celestial object and the horizon which is known as the object's
altitude. Using this measurement is known as
sighting the object,
shooting the object, or
taking a sight and it is an essential part of celestial navigation. The angle, and the time when it was measured, can be used to calculate a position line on a nautical or aeronautical chart. Common uses of the
sextant include sighting the sun at solar noon and sighting Polaris at night (in the Northern Hemisphere), to find one's latitude. Sighting the height of a landmark can give a measure of
distance off and, held horizontally, a
sextant can measure angles between objects for a position
[1] A
sextant can also be used to measure the lunar distance between the moon and another celestial object (e.g., star, planet) in order to determine Greenwich time which is important because it can then be used to determine the longitude
on a chart.The scale of a
sextant has a length of
⅙ of a turn (60°); hence the
sextant's name (
sextāns, -antis is the Latin word for "one sixth"). An octant is a similar device with a shorter scale (
⅛ turn, or 45°), where as a quintant (
⅕ turn, or 72°) and a quadrant (
¼ turn, or 90°) have longer scales.
Sir Isaac Newton (1643–1727) invented the principle of the doubly reflecting navigation instrument (a reflecting quadrant—see Octant (instrument)), but never published it. Two men independently developed the octant around 1730: John Hadley (1682–1744), an English mathematician, and Thomas Godfrey (1704–1749), a glazier in Philadelphia. John Bird made the first
sextant in 1757. The octant and later the
sextant, replaced the Davis quadrantas the main instrument for navigation.
Advantages
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Nautical sextant manufacturer |
Like the Davis quadrant (also called backstaff), the
sextant allows celestial objects to be measured relative to the horizon, rather than relative to the instrument. This allows excellent precision. However, unlike the backstaff, the
sextant allows direct observations of stars. This permits the use of the
sextant at night when a backstaff is difficult to use. For solar observations, filters allow direct observation of the sun.
Since the measurement is relative to the horizon, the measuring pointer is a beam of light that reaches to the horizon. The measurement is thus limited by the angular accuracy of the instrument and not the sine error of the
length of an alidade, as it is in a mariner's astrolabe or similar older instrument.
A
sextant does not require a completely steady aim, because it measures a relative angle. For example, when a
sextant is used on a moving ship, the image of both horizon and celestial object will move around in the field of view. However, the relative position of the two images will remain steady, and as long as the user can determine when the celestial object touches the horizon the accuracy of the measurement will remain high compared to the magnitude of the movement.
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Nautical sextant manufacturer |
The
sextant is not dependent upon electricity (unlike many forms of modern navigation) or anything human-controlled (like GPS satellites). For these reasons, it is considered an eminently practical back-up navigation tool for ships.