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The Historians' History of the World 01 [Prolegomena; Egypt, Mesopotamia]
- Автор: Gutenberg
- Год: 1905
- Язык: английский
- Жанр: История
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“Those which we see, they assign to the living; and the other that do not appear, they conceive are Constellations for the Dead; and they term them Judges of all things. The Moon, they say, is in the lowest Orb; and being therefore next to the Earth (because she is so small,) she finishes her Course in a little time, not through the swiftness of her Motion, but the shortness of her Sphear. In that which they affirm (that she has but a borrow’d light, and that when she is eclips’d, it’s caus’d by the interposition of the shadow of the Earth) they agree with the Grecians.
“Their Rules and Notions concerning the Eclipses of the Sun are but weak and mean, which they dare not positively foretel, nor fix a certain time for them. They have likewise Opinions concerning the Earth peculiar to themselves, affirming it to resemble a Boat, and to be hollow, to prove which, and other things relating to the frame of the World, they abound in Arguments; but to give a particular Account of ’em, we conceive would be a thing foreign to our History. But this any Man may justly and truly say, That the Chaldeans far exceed all other Men in the Knowledge of Astrology, and have study’d it most of any other Art or Science: But the number of Years during which the Chaldeans say, those of their Profession have given themselves to the study of this natural Philosophy, is incredible; for when Alexander was in Asia, they reckon’d up Four Hundred and Seventy Thousand Years since they first began to observe the Motions of the Stars. But lest we should make too long a digression from our intended Design, let this which we have said concerning the Chaldeans suffice.”d
THE BABYLONIAN YEAR
The Babylonian year, according to Eduard Meyer, consisted of simple lunar months (twenty-nine or thirty days), which, as with the Greeks and the Mohammedans, was determined by the course of the moon itself.
To make this year coincide with the course of the sun, an extra month was intercalated; in olden times this seems to have been done after the first or the sixth month.
This year, with the names of its months, was adopted by the Jews at the time of the Exile, and is still in use with them. The commencement of their year (Nisan) falls at the time of the spring equinox. The Babylonians had no continuous chronology; they dated according to the years of the kings, or, rather, they marked the year according to any important event which took place in it. Thus we see dates like “on the 30th Adar in the Sixth year after the conquest of Nisin by King Rim-Sin.”
Later on in Babylon, and also in Assyria, they reckoned simply the years of the kings, from the day of their accession to the throne. The remainder of the year, in the course of which the predecessor had died, was therefore considered the first part of the first year of the new reign, and was very often called “the beginning of the reign” of the king in question.
Chronological calculations were reckoned from the same starting-point as in Egypt. They reckon the calendar year in which a king comes to the throne as his first year, and hence his death takes place in the first year of his successor. This is the method of the Ptolemaic canon, one of the most important chronological monuments of antiquity. It is the list beginning with Nabonassar (about 747 B.C.) of the native and Persian kings of Babylonia, to which the Egyptian rulers up to Alexander are added. It is an addition to the astronomical work of Ptolemy, and was intended to throw light on the passages relating to the Babylonian, and later on to the Alexandrian chronological methods. It is authentic, and is confirmed by the monuments. Yet, in using the same, it must be recollected that all dates of the Egyptian “vague” year (and the Egyptian months) are reduced. Therefore the first year of the Nabonassar era begins on the 1st Tehuti, the 26th February, 747 B.C.
In Assyria there is also a second and far more common form of specifying the years. Since a very early date (as far back as the fourteenth century) it was customary to name the year after some high official. The year, as such, is called limmu, “eponymic year.” Of course, they had continuous lists of these eponyms; and we have recovered several fragments. The lists for the years 893 to 666 are complete, and with fragments we can go still farther back. The kings frequently used this system, and private persons regularly used this eponym.
Some copies of the lists contain accounts of the changes of reigns, and give short statements of important internal and external events of the particular years. Thus an eclipse of the sun June 15, 763 B.C., mentioned therein can be astronomically fixed, and the dates arrived at thereby concur exactly with the accounts of the Ptolemaic canon. The chronological history of this epoch is therefore perfectly determined.e
THE BABYLONIAN DAY AND ITS DIVISION INTO HOURS
This being the Babylonian method of reckoning dates, it is interesting to note on what plan they subdivided the day. Investigations were made in this line by that indefatigable Irishman, Edward Hincks, from whose article “On the Assyrio-Babylonian Measures of Time,” in the Transactions of the Royal Irish Academy, we quote.a
I begin with the day and its divisions.
Our knowledge on this subject is mainly derived from a tablet in the British Museum, marked K. 15. A paper of mine was read before the Royal Irish Academy in 1854, and was published in the twenty-third volume of the Transactions in which this tablet was discussed. As that paper contained some slight philological errors, I will here repeat the substance of it, correcting those errors.
I now translate the inscription on the Tablet as follows, omitting the customary benedictory formula. “On the sixth day of the month Nisan the day and the night are equal; six kazabs [kashbu] are the day; six kazabs [kashbu] are the night.” It is evident that this inscription records the observation of an equinox; and I will return to the consideration of it with that view. At present I will only remark that it points to a double division of the day, or Nycthemeron; viz., the first into the day properly so called, and the night; which were in this instance equal, though not generally so; the second into twelve equal kazabs [kashbu].
I proceed to the second division of the day into twelve kazabs [kashbu]. Each of these was equivalent, putting out of sight errors of observation, to two hours of mean solar time, such as we use in ordinary life. The word kazab [kashbu] is from a Hebrew root meaning “to fail,” which is applied to streams that run dry. This suggests the primary signification, “runnings out,” namely, of the water which had been poured into a vessel with a small hole in the bottom. The Babylonians measured time by clepsydræ, which, when they had been filled, would be emptied in two hours of mean time. Such clepsydræ would maintain a sufficiently accurate division of the day into twelve kazabs [kashbu] if the first were set to run at apparent noon, the second when the first had run out, and so on till the thirteenth, which would be set to run at the next apparent noon, whether the twelfth was just running out, or had already run out, or had still a little water in it.