Astrolabe
\n\n | \n
\n
From the 16th century to the 18th century (when the
sextant was invented) the
astrolabe was the chief navigational instrument.
An astrolabe consists of a circle marked in degrees (similar to a protractor) with a rotating arm attached at its center. When the 0° mark on the circle is aligned with the horizon, and a star (or other celestial body) "sighted" at the end of the movable arm, the position (in degrees) of the star can be read ("taken") off the calibrated circle (hence, "astro" = star + "labe" = to take).
On the plate (
mater) are engraved coordinate lines which represent a
stereographic projection of the
celestial sphere (
climate), valid for places at a specific geographic latitude. Over this coordinate grid rotates the
rete, which is a framework with spikes whose points represent fixed stars. After adjusting the instrument for the current time, the position of a star can be read from the coordinate grid. Conversely, the instrument can be adjusted to fit the measured position, and the time can be read off the scale.
The astrolabe therefore is a predecessor of the modern
planisphere.
The astrolabe was probably invented by
Hipparchus (
2nd century BC). Stereographical projection is first described by
Ptolemy (
2nd century). The astrolabe reaches the islamic world in the 8th or
9th century and it is re-introduced to Europe via islamic
Spain in the
11th century (early christian recipients of arab astronomy are
Gerbert of Aurillac and
Hermannus Contractus). The mathematical background was established by
Al-Battani in his treatise
Kitab az-Zij (ca. 920), which is translated into latin in by Plato Tiburtinus (
De Motu Stellarum).
The English author
Geoffrey Chaucer (ca. 1343 -
1400) wrote a treatise on the astrolabe for his son. \nIn the 15th century, the French instrument-maker Jean Fusoris (~1365 - 1436) started selling them in his shop in Paris, along with portable sundials and other popular scientific
gadgets of the day.
See also
Category:Navigation
\n\n