My object in the above discussion of the origin of the week (as distinguished from the origin of the Sabbath, which I considered in the essay on astrology), has been to show that the use of the twelve zodiacal signs was in every case preceded by the use of the twenty-eight lunar mansions. It has been supposed that those nations in whose astronomy the twenty-eight mansions still appear, adopted one system, while the use of the twelve signs implies that another system had been adopted. Thus the following passage occurs in Mr. Blake's version of Flammarion's 'History of the Heavens:'—'the Chinese have twenty-eight constellations, though the word sion does not mean a group of stars, but simply a mansion or hotel. In the Coptic and ancient Egyptian the word for constellations has the same meaning. They also have twenty-eight, and the same number is found among the Arabians, Persians, and Indians. Among the Chaldæans or Accadians we find no sign of the number twenty-eight. The ecliptic, or "yoke of the sky," with them, as we see in the newly-discovered tablet, was divided into twelve divisions, as now, and the only connection that can be imagined between this and the twenty-eight is the opinion of M. Biot, who thinks that the Chinese had originally only twenty-four mansions, four more being added by Chenkung, 1100 B.C., and that they corresponded with the twenty-four stars, twelve to the north and twelve to the south, that marked the twelve signs of the zodiac amongst the Chaldæans. But under this supposition the twenty-eight has no reference to the moon, whereas we have every reason to believe it has.' The last observation is undoubtedly correct—the twenty-eight mansions have been mansions of the moon from the beginning. But in this very circumstance, as also in the very tablets referred to in the preceding passage, we find all the evidence needed to show that originally the Chaldæans divided the zodiac into twenty-eight parts. For we find from the tablets that, like the other nations who had twenty-eight zodiacal mansions, the Chaldæans used a seven-day period, derived from the moon's motions, every seventh day being called sabbatu, and held as a day of rest. We may safely infer that the Chaldæan astronomers, advancing beyond those of other nations, recognised the necessity of dividing the zodiac with reference to the sun's motions instead of the moon's. They therefore discarded the twenty-eight lunar mansions, and adopted instead twelve solar signs; this number twelve, like the number twenty-eight itself, being selected merely as the most convenient approximation to the number of parts into which the zodiac was naturally divided by another period. Thus the twenty-eighth part of the zodiac corresponds roughly with the moon's daily motion, and the twelfth part of the zodiac corresponds roughly with the moon's monthly motion; and both the numbers twenty-eight and twelve admit of being subdivided, while twenty-nine (a nearer approach than twenty-eight to the number of days in a lunation) and thirteen (almost as near an approach as twelve to the number of months in a year) do not.

It seems to me highly probable that the date to which all inquiries into the origin of the constellations and the zodiacal signs seems to point—viz. 2170 B.C.—was the date at which the Chaldæan astronomers definitely adopted the new system, the lunisolar instead of lunar division of the zodiac and of time. One of the objects which the architects of the Great Pyramid (not the king who built it) may have had was not improbably this—the erection of a building indicating the epoch when the new system was entered upon, and defining in its proportions, its interior passages, and other features, fundamental elements of the new system. The great difficulty, an overwhelming difficulty it has always seemed to me, in accepting the belief that the year 2170 B.C. defined the beginning of exact astronomy, has been this, that several of the circumstances insisted upon as determining that date imply a considerable knowledge of astronomy. Thus astronomers must have made great progress in their science before they could select as a day for counting from, the epoch when the slow reeling motion of the earth (the so-called precessional motion) brought the Pleiades centrally south, at noon, at the time of the vernal equinox. The construction of the Great Pyramid, again, in all its astronomical features, implies considerable proficiency in astronomical observation. Thus the year 2170 B.C. may very well be regarded as defining the introduction of a new system of astronomy, but certainly not the beginning of astronomy itself. Of course we may cut the knot of this difficulty, as Prof. Smyth and Abbé Moigno do, by saying that astronomy began 2170 B.C., the first astronomers being instructed supernaturally, so that the astronomical Minerva came into full-grown being. But I apprehend that argument against such a belief is as unnecessary as it would certainly be useless.

And now let us consider how this theory accords with the result to which we were led by the position of the great vacant space around the southern pole. So far as the date is concerned, we have already seen that the epoch 2170 B.C. accords excellently with the evidence of the vacant space. But this evidence, as I mentioned at the outset, establishes more than the date; it indicates the latitude of the place where the most ancient of Ptolemy's forty-eight constellations were first definitely adopted by astronomers. If we assume that at this place the southernmost constellations were just fully seen when due south, we find for the latitude about thirty-eight degrees north. (The student of astronomy who may care to test my results may be reminded here that it is not enough to show that every star of a constellation would when due south be above the horizon of the place—what is wanted is, that the whole constellation when towards the south should be visible at a single view. However, the whole constellation may not have included all the stars now belonging to it.) The station of the astronomers who founded the new system can scarcely have been more than a degree or two north of this latitude. On the other side, we may go a little further, for by so doing we only raise the constellations somewhat higher above the southern horizon, to which there is less objection than to a change thrusting part of the constellations below the horizon. Still it may be doubted whether the place where the constellations were first formed was less than 32 or 33 degrees north of the equator. The Great Pyramid, as we know, is about 30 degrees north of the equator; but we also know that its architects travelled southwards to find a suitable place for it. One of their objects may well have been to obtain a fuller view of the star-sphere south of their constellations. I think from 35 to 39 degrees north would be about the most probable limits, and from 32 to 41 degrees north the certain limits of the station of the first founders of solar zodiacal astronomy.

What their actual station may have been is not so easily established. Some think the region lay between the sources of the Oxus (Amoor) and Indus, others that the station of these astronomers was not very far from Mount Ararat—a view to which I was led long ago by other considerations discussed in the first appendix to my treatise on 'Saturn and its System.'

At the epoch indicated, the first constellation of the zodiac was not, as now, the Fishes, nor, as when a fresh departure was made by Hipparchus, the Ram, but the Bull, a trace of which is found in Virgil's words—

Candidus auratis aperit cum cornibus annum Taurus.

The Bull then was the spring sign, the Pleiades and ruddy Aldebaran joining their rays with the sun's at the time of the vernal equinox. The midsummer sign was the Lion (the bright Cor Leonis nearly marking the sun's highest place). The autumn sign was the Scorpion, the ruddy Antares and the stars clustering in the head of the Scorpion joining their rays with the sun's at the time of the autumnal equinox. And lastly the winter sign was the Water Bearer, the bright Fomalhaut conjoining his rays with the sun's at midwinter. It is noteworthy that all these four constellations really present some resemblance to the objects after which they are named. The Scorpion is in the best drawing, but the Bull's head is well marked, and, as already mentioned, a leaping lion can be recognised. The streams of stars from the Urn of Aquarius and the Urn itself are much better defined than the Urn Bearer.

I have not left myself much space to speak of the finest of all the constellations, the glorious Orion—the Giant in his might, as he was called of old. In this noble asterism the figure of a giant ascending a slope can be readily discerned when the constellation is due south. At the time to which I have referred the constellation Orion was considerably below the equator, and instead of standing nearly upright when due south high above the horizon, as now in our northern latitudes, he rose upright above the south-eastern horizon. The resemblance to a giant figure must then have been even more striking than it is at present (except in high northern latitudes, where Orion, when due south, is just fully above the horizon). The giant Orion has long been identified with Nimrod; and those who recognise the antitypes of the Ark in Argo, of the old dragon in Draco, and of the first and second Adams in the kneeling Hercules defeated by the serpent and the upright Ophiuchus triumphant over the serpent, may, if they so please, find in the giant Orion, the Two Dogs, the Hare, and the Bull (whom Orion is more directly dealing with), the representations of Nimrod, that mighty hunter before the Lord, his hunting dogs, and the animals he hunted. Pegasus, formerly called the Horse, was regarded in very ancient times as the Steed of Nimrod.

In modern astronomy the constellations no longer have the importance which once attached to them. They afford convenient means for naming the stars, though I think many observers would prefer the less attractive but more business-like methods adopted by Piazzi and others, according to which a star rejoices in no more striking title than 'Piazzi XIIIh. 273,' or 'Struve, 2819.' They still serve, however, to teach beginners the stars, and probably many years will pass before even exact astronomy dismisses them altogether to the limbo of discarded symbolisms. It is, indeed, somewhat singular that astronomers find it easier to introduce new absurdities among the constellations than to get rid of these old ones. The new and utterly absurd figures introduced by Bode still remain in many charts despite such inconvenient names as Honores Frederici, Globum Ærostaticum and Machina Pneumatica; and I have very little doubt that a new constellation, if it only had a specially inconvenient title, would be accepted. But when Francis Baily tried to simplify the heavens by removing many of Bode's absurd constellations, he was abused by many as violently as though he had proposed the rejection of the Newtonian system. I myself tried a small measure of reform in the three first editions of my 'Library Atlas,' but have found it desirable to return to the old nomenclature in the fourth.