192 PHYSICAL GEOGRAPHY. [CHAP earth, which, as we have seen, had already been determined by Eratosthenes. In this conclusion of his predecessor Posidonius was indisposed to acquiesce, and he endeavoured to solve the problem by means of observations of the position of the star Canopus at Alexandria and at Rhodes; but, owing to the inaccuracy both of these measurements and of the computation of the distance between the two places, he greatly underestimated the circuit of the globe, reducing it from 250,000 stadia, as computed by Eratosthenes, to 180,000J. Unfortunately, in con- sequence of the great weight that was attached to his authority, this estimate was adopted by his successors, and was even ac- cepted by Ptolemy. The history of the discovery by the Greeks of the movement of the tides is peculiarly interesting, because the knowledge of this phenomenon was only gradually obtainable by them, since the Mediterranean is, except in a slight degree, and in certain limited areas, such as the head of the Adriatic, a tideless sea. Herodotus notices the ebb and flow of the water in the Maliac gulf8, and also in the Red Sea3; and he uses the same terms in which these are described, when speaking of the extraordinary reflux and flux of the waves, which caused the destruction of a portion of the Persian force under the command of Artabazus which was besieging Potidaea4. The shifting currents of the Euripus, which served as a starting-point for speculations on this subject, are noticed by all three of the Greek tragedians; Aeschylus describing them as the "tides of Aulis surging to and fro8," and Sophocles as the "groaning strait6," while Euripides speaks of the " eddies of the whirling Euripus7." Aristotle, as we have seen, observed its movements, and he remarks generally on the tendency of the sea to sway to and fro, when a 1 Strabo, 2. 2. 2. a Herod., 7.198; $e is T> Mi/XiSa ?rapa K6\irov 6a\dT0, ?rop0jK6?. 7 Eurip., Iph* Taur.i 6, 7; djLt# Sbais, a* 0<£/*' Efywr atipcus i\ta-ffw Kvavtav aXa trr^fi