The History of Antiquity, Vol. 1 (of 6)Duncker, Max
History
The History of Antiquity, Vol. 1 (of 6)
Duncker, Max
History, Ancient
date of this king cannot be ascertained: we only know that he must have
belonged to the old kingdom. Assyrian weights with inscriptions in the
Phenician alphabet, beside the cuneiform inscriptions, are found of the
eighth century B.C., the time of King Tiglath Pilesar II., Shalmanesar
IV., and Sennacherib.[392]
"It can be maintained with good reason," says Diodorus, "that the
Chaldæans are far before all other nations in their knowledge of the
heavens; and that they devoted the greatest attention and labour to this
science." At an early period, by comparing the course of the sun with
that of the moon, they had perceived that the sun returned to the same
position after passing through about twelve cycles of the moon; hence
they fixed the year at twelve months of thirty days, which they, by
intercalations of various kinds, brought into harmony with the
astronomical year of 365-1/4 days.[393] The observation, that the sun
after a course of twelve months returns to the same constellation, led
them on to determine the changing position of the sun in the other
months by constellations. Thus the Babylonians marked off the
constellations which seemed to touch nearest upon the course of the sun,
and arrived at the signs of the ecliptic or zodiac. Each of these twelve
stations through which the sun passed they again divided into thirty
parts. The week they fixed at seven days by the course of the moon; to
the day they allotted twelve hours, to correspond to the twelve months
of the year; the hours they divided into sixty parts, and each of these
sixtieths was again subdivided into sixty parts. Their measures were
also duodecimal. The cubit was twenty-four finger-breadths; and on the
same system, their numerals were based upon the _sossus_, or sixty,--a
derivative from twelve, and the _sarus_, or square of the _sossus_. When
they attempted to fix the position and intervals of the stars in the
sky, the basis taken for their measurements was the diameter of the sun.
They divided the daily course of the sun, like the ecliptic, into 360
parts, and then attempted to measure these at the equinox. At the moment
when the sun was seen in the sky on the morning of the equinox, a jar
filled with water was opened. From this the water was allowed to run
into a second small jar, till the orb of the sun was completely visible;
then it ran into a third and larger jar, till the sun was again seen on
the horizon on the following morning. They concluded that the diameter
of the sun must stand in the same proportion to the cycle it passed
through as the water in the small jar stood to the water in the large
one. Hence they found that the diameter of the sun was contained 720
times in its course, and this diameter they fixed at 1/30 of an
hour.[394] The observation that an active foot-courier could accomplish
a certain distance in the thirtieth part of an equinoctial hour, and
thirty times as much in the whole hour, supplied the Chaldæans with a
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