ASTROLABE (from Gr. liar pop, star, and Aa(3eiv, to take)

This article appears in Volume V02, Page 795 of the Encyclopedia Britannica.

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ASTROLABE (from Gr. liar pop, star, and Aa(3eiv, to take) , an

instrument

INSTRUMENT (Lat. instrumentum, from insincere, to build up, furnish, arrange, prepare)

used not only for stellar, but for solar and lunar altitude-taking. The principle of the astrolabe is explained in fig. 2. There were two kinds,spherical and planispheric.
P in the plane of the circle, the angle B 0 D will be the angle sub-tended by the two objects P and Q at the eye.
The earliest forms were " armillae " and spherical. Gradually, from Eratosthenes to Tycho, Hipparchus playing the most important part among ancient astronomers, the complex astrolabe was evolved, large specimens being among the

chief

CHIEF (from Fr. chef, head, Lat. caput)

observa-
-

ASTROLOGY

ASTROLOGY

795
tory

instruments

INSTRUMENTS

of the 15th, 16th and even r 7th centuries; while small ones were in use among travellers and learned men, not only for astronomical, but for astrological and topographical purposes. Nearly every one of the modem

instruments

INSTRUMENTS

used for the observations of physical astronomy is a part of the perfected astrolabe. A collection of circles such as is the armillary sphere, if each circle were fitted with a view-tube, might be considered a complete astrolabe. Tycho's armillae were astrolabes. In fact the modern equatorial, and the altitude and azimuth circle are astrolabes in the strictest and oldest meaning of the term; and Tycho in one of his astrolabes came so near the modern equatorial that it may be taken as the first of the kind.
The two forms of the planispheric astrolabe most widely known and used in the r5th, 16th and even 17th centuries were: (r) the portable astrolabe shown in fig. 1 (

Plate

PLATE

). This originated in the

East

EAST
EAST, ALFRED (1849- )

, and was in early use in India, Persia and Arabia, and was introduced into Europe by the Arabs, who had perfected it perhaps as early as A.D. 700. It combines the planisphere and armillae of Hipparchus and others, and the theodolite of Theon, and was usually of brass, varying in

diameter

DIAMETER (from the Cr. &a, through, µErpov, measure)

from a couple of inches to a foot or more. It was used for taking the altitudes of sun, moon and stars; for calculating

latitude

LATITUDE (Lat. latitudo, latus, broad)

; for determining the points of the compass, and time; for ascertaining heights of mountains, &c.; and for construction of horo-
scopes. The

instrument

INSTRUMENT (Lat. instrumentum, from insincere, to build up, furnish, arrange, prepare)

was a marvel of convenience and ingenuity, and was called " the mathematical

jewel

JEWEL, JOHN (1522-1571)

." Nevertheless it passed out of use, because incapable of any

great

GREAT

precision.
(2) The mariner's astrolabe, fig. 3, was adapted from that of astronomers by Martin Behaim, c. 1480. This was the instrument used by Columbus. With the tables of the sun's declination then available, he could calculate his

latitude

LATITUDE (Lat. latitudo, latus, broad)

by meridian altitudes of the sun taken with his astrolabe. The mariner's astrolabe was superseded by John Hadley's quadrant of 1731.

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