Alexandria and Her Schools: Four Lectures Delivered at the Philosophical Institution, EdinburghKingsley, Charles
Philosophy
Alexandria and Her Schools: Four Lectures Delivered at the Philosophical Institution, Edinburgh
Kingsley, Charles
Alexandrian school
But such schools of science, founded on such a ground as this, on the
mere instinct of curiosity, had little chance of originality or vitality.
All the great schools of the world, the elder Greek philosophy, the
Alexandrian, the present Baconian school of physics, have had a deeper
motive for their search, a far higher object which they hope to discover.
But indeed, the Mussulmans did not so much wish to discover truth, as to
cultivate their own intellects. For that purpose a sharp and subtle
systematist, like Aristotle, was the very man whom they required; and
from the destruction of Alexandria may date the rise of the Aristotelian
philosophy. Translations of his works were made into Arabic, first, it
is said, from Persian and Syriac translations; the former of which had
been made during the sixth and seventh centuries, by the wreck of the
Neoplatonist party, during their visit to the philosophic Chozroos. A
century after, they filled Alexandria. After them Almansoor, Hairoun
Alraschid, and their successors, who patronised the Nestorian Christians,
obtained from them translations of the philosophic, medical, and
astronomical Greek works; while the last of the Omniades, Abdalrahman,
had introduced the same literary taste into Spain, where, in the
thirteenth century, Averroës and Maimonides rivalled the fame of
Avicenna, who had flourished at Bagdad a century before.
But, as I have said already, these Arabs seem to have invented nothing;
they only commented. And yet not only commented; for they preserved for
us those works of whose real value they were so little aware. Averroës,
in quality of commentator on Aristotle, became his rival in the minds of
the mediæval schoolmen; Avicenna, in quality of commentator on
Hippocrates and Galen, was for centuries the text-book of all European
physicians; while Albatani and Aboul Wefa, as astronomers, commented on
Ptolemy, not however without making a few important additions to his
knowledge; for Aboul Wefa discovered a third inequality of the moon’s
motion, in addition to the two mentioned by Ptolemy, which he did,
according to Professor Whewell, in a truly philosophic manner—an
apparently solitary instance, and one which, in its own day, had no
effect; for the fact was forgotten, and rediscovered centuries after by
Tycho Brahe. To Albatani, however, we owe two really valuable heirlooms.
The one is the use of the sine, or half-chord of the double arc, instead
of the chord of the arc itself, which had been employed by the Greek
astronomers; the other, of even more practical benefit, was the
introduction of the present decimal arithmetic, instead of the
troublesome sexagesimal arithmetic of the Greeks. These ten digits,
however, seem, says Professor Whewell, by the confession of the Arabians
themselves, to be of Indian origin, and thus form no exception to the
sterility of the Arabian genius in scientific inventions. Nevertheless
Public-domain text, read in full here on John Shaqi.
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