Theodor Mommsen

The History of Rome, Book I


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to mark the alterations introduced in the more recent editions of the original, I thought it due to him and to the favour with which the translation had been received that I should subject it to such a fresh revision as should bring it into conformity with the last form (eighth edition) of the German, on which, as I learn from him, he hardly contemplates further change. As compared with the first English edition, the more considerable alterations of addition, omission, or substitution amount, I should think, to well-nigh a hundred pages. I have corrected various errors in renderings, names, and dates (though not without some misgiving that others may have escaped notice or been incurred afresh); and I have still further broken up the text into paragraphs and added marginal headings.

      The Index, which was not issued for the German book till nine years after the English translation was published, has now been greatly enlarged from its more recent German form, and has been, at the expenditure of no small labour, adapted to the altered paging of the English. I have also prepared, as an accompaniment to it, a collation of pagings, which will materially facilitate the finding of references made to the original or to the previous English editions.

      I have had much reason to be gratified by the favour with which my translation has been received on the part alike of Dr. Mommsen himself and of the numerous English scholars who have made it the basis of their references to his work.1 I trust that in the altered form and new dress, for which the book is indebted to the printers, it may still further meet the convenience of the reader.

      September 1894.

      INTRODUCTORY NOTE BY DR. MOMMSEN

      The Varronian computation by years of the City is retained in the text; the figures on the margin indicate the corresponding year before the birth of Christ.

      In calculating the corresponding years, the year 1 of the City has been assumed as identical with the year 753 B.C., and with Olymp. 6, 4; although, if we take into account the circumstance that the Roman solar year began with the 1st day of March, and the Greek with the 1st day of July, the year 1 of the City would, according to more exact calculation, correspond to the last ten months of 753 and the first two months of 752 B.C., and to the last four months of Ol. 6, 3 and the first eight of Ol. 6, 4.

      The Roman and Greek money has uniformly been commuted on the basis of assuming the libral as and sestertius, and the denarius and Attic drachma, respectively as equal, and taking for all sums above 100 denarii the present value in gold, and for all sums under 100 denarii the present value in silver, of the corresponding weight. The Roman pound (=327.45 grammes) of gold, equal to 4000 sesterces, has thus, according to the ratio of gold to silver 1:15.5, been reckoned at 304 1/2 Prussian thalers [about 43 pounds sterling], and the denarius, according to the value of silver, at 7 Prussian groschen [about 8d.].2

      Kiepert's map will give a clearer idea of the military consolidation of Italy than can be conveyed by any description.

      DEDICATIONS

      The First Volume of the original bears the inscription:—

To My FriendMORIZ HAUPT Of BerinThe Second:—To My Dear AssociatesFERDINAND HITZIG Of ZurichAndKARL LUDWIG Of Vienna 1852, 1853, 1854And the Third:—Dedicated With Old And Loyal Affection ToOTTO JAHN Of Bonn

      BOOK FIRST

      The Period Anterior to the Abolition of the Monarchy

      —Ta palaiotera saphos men eurein dia chronou pleithos adunata ein ek de tekmeirion on epi makrotaton skopounti moi pisteusai xumbainei ou megala nomizo genesthai oute kata tous polemous oute es ta alla.—

Thucydides.

      CHAPTER I

      Introduction

      Ancient History

      The Mediterranean Sea with its various branches, penetrating far into the great Continent, forms the largest gulf of the ocean, and, alternately narrowed by islands or projections of the land and expanding to considerable breadth, at once separates and connects the three divisions of the Old World. The shores of this inland sea were in ancient times peopled by various nations belonging in an ethnographical and philological point of view to different races, but constituting in their historical aspect one whole. This historic whole has been usually, but not very appropriately, entitled the history of the ancient world. It is in reality the history of civilization among the Mediterranean nations; and, as it passes before us in its successive stages, it presents four great phases of development—the history of the Coptic or Egyptian stock dwelling on the southern shore, the history of the Aramaean or Syrian nation which occupied the east coast and extended into the interior of Asia as far as the Euphrates and Tigris, and the histories of the twin-peoples, the Hellenes and Italians, who received as their heritage the countries on the European shore. Each of these histories was in its earlier stages connected with other regions and with other cycles of historical evolution; but each soon entered on its own distinctive career. The surrounding nations of alien or even of kindred extraction—the Berbers and Negroes of Africa, the Arabs, Persians, and Indians of Asia, the Celts and Germans of Europe—came into manifold contact with the peoples inhabiting the borders of the Mediterranean, but they neither imparted unto them nor received from them any influences exercising decisive effect on their respective destinies. So far, therefore, as cycles of culture admit of demarcation at all, the cycle which has its culminating points denoted by the names Thebes, Carthage, Athens, and Rome, may be regarded as an unity. The four nations represented by these names, after each of them had attained in a path of its own a peculiar and noble civilization, mingled with one another in the most varied relations of reciprocal intercourse, and skilfully elaborated and richly developed all the elements of human nature. At length their cycle was accomplished. New peoples who hitherto had only laved the territories of the states of the Mediterranean, as waves lave the beach, overflowed both its shores, severed the history of its south coast from that of the north, and transferred the centre of civilization from the Mediterranean to the Atlantic Ocean. The distinction between ancient and modern history, therefore, is no mere accident, nor yet a mere matter of chronological convenience. What is called modern history is in reality the formation of a new cycle of culture, connected in several stages of its development with the perishing or perished civilization of the Mediterranean states, as this was connected with the primitive civilization of the Indo-Germanic stock, but destined, like the earlier cycle, to traverse an orbit of its own. It too is destined to experience in full measure the vicissitudes of national weal and woe, the periods of growth, of maturity, and of age, the blessedness of creative effort in religion, polity, and art, the comfort of enjoying the material and intellectual acquisitions which it has won, perhaps also, some day, the decay of productive power in the satiety of contentment with the goal attained. And yet this goal will only be temporary: the grandest system of civilization has its orbit, and may complete its course but not so the human race, to which, just when it seems to have reached its goal, the old task is ever set anew with a wider range and with a deeper meaning.

      Italy

      Our aim is to exhibit the last act of this great historical drama, to relate the ancient history of the central peninsula projecting from the northern continent into the Mediterranean. It is formed by the mountain-system of the Apennines branching off in a southern direction from the western Alps. The Apennines take in the first instance a south-eastern course between the broader gulf of the Mediterranean on the west, and the narrow one on the east; and in the close vicinity of the latter they attain their greatest elevation, which, however, scarce reaches the line of perpetual snow, in the Abruzzi. From the Abruzzi the chain continues in a southern direction, at first undivided and of considerable height; after a depression which forms a hill-country, it splits into a somewhat flattened succession of heights towards the south-east and a more rugged chain towards the south, and in both directions terminates in the formation of narrow peninsulas.

      The flat country on the north, extending between the Alps and the Apennines as far down as the Abruzzi, does not belong geographically, nor until a very late period even historically,