In the first place, it is almost an utter impossibility to
calculate with a fair degree of accuracy the days of the year and
the movements of the sun. To the three hundred and sixty-five days
there are still to be added the intercalary days, the
result of the additional quarters of a day and night: hence it
is, that it is found impossible to ascertain with exactness the
proper periods for the appearance of the stars. To this we
must add, too, a certain degree of uncertainty connected with
these matters, that is universally admitted; thus, for instance,
bad and wintry weather will often precede, by several days,
the proper period for the advent of that season, a state of things
known to the Greeks as
There are some who look upon the appearance of the butterfly as the surest sign of spring, because of the extreme delicacy of that insect. In this present year,[6] however, in which I am penning these lines, it has been remarked that the flights of butterflies have been killed three several times, by as many returns of the cold; while the foreign birds, which brought us by the sixth of the calends of February[7] every indication of an early spring, after that had to struggle against a winter of the greatest severity. In treating of these matters, we have to meet a twofold difficulty: first of all, we have to ascertain whether or not the celestial phænomena are regulated by certain laws, and then we have to seek how to reconcile those laws with apparent facts. We must, however, be more particularly careful to take into account the convexity of the earth, and the differences of situation in the localities upon the face of the globe; for hence it is, that the same constellation shows itself to different nations at different times, the result being, that its influence is by no means perceptible everywhere at the same moment. This difficulty has been considerably enhanced, too, by various authors, who, after making their observations in different localities, and indeed, in some instances, in the same locality, have yet given us varying or contradictory results.
There have been three great schools of astronomy, the Chaldæan,
the Ægyptian, and the Grecian. To these has been
added a fourth school, which was established by the Dictator
Cæsar among ourselves, and to which was entrusted the duty
of regulating the year in conformity with the sun's revolution,[8]
under the auspices of Sosigenes, an astronomer of considerable
learning and skill. His theory, too, upon the discovery of certain
errors, has since been corrected, no intercalations having
As for ourselves, we shall follow the calculations made by
Julius Cæsar,[12] which bear reference more particularly to Italy;
though at the same time, we shall set forth the dicta of various
other writers, bearing in mind that we are treating not of an
individual country, but of Nature considered in her totality.
In doing this, however, we shall name, not the writers themselves,
for that would be too lengthy a task, but the countries
in reference to which they speak. The reader must bear in
mind, then, that for the sake of saving space, under the head
of Attica, we include the islands of the Cyclades as well; under
that of Macedonia, Magnesia and Thracia; under that of Egypt,
My silence as to Africa,[14] Spain, and the provinces of Gaul, will occasion no surprise, from the fact that no one has published any observations made upon the stars in those countries. Still, however, there will be no difficulty in calculating them, even for these regions as well, on reference being made to the parallels which have been set forth in the Sixth Book.[15] By adopting this course, an accurate acquaintance may be made with the astronomical relations, not only of individual nations, but of cities even as well. By taking the circular parallels which we have there appended to the several portions of the earth respectively, and applying them to the countries in question, that are similarly situate, it will be found that the rising of the heavenly bodies will be the same for all parts within those parallels, where the shadows projected are of equal length. It is also deserving of remark, that the seasons have their periodical recurrences, without any marked difference, every four years, in consequence of the influence[16] of the sun, and that the characteristics of the seasons are developed in excess every eighth year, at the revolution of every hundredth moon.
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13. I. e. Asia Minor.
14. I. e. the north-west parts of Africa.
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