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admin | Category: Business Phone Numbers | 11.08.2015
In the second place Schnabel’s statement that Agrippa reduced the itinerary figure of 745 miles to a straight line of 411 cannot be accepted. Thirdly, it may fairly be objected that the very method by which Schnabel obtains the figure of 411 miles is faulty. Tierney passes over Schnabel’s reasons for thinking that Agrippa established lines of meridian in Spain and in the eastern Mediterranean, all of which Tierney finds quite unconvincing. These were no doubt freedmen, of whom there were large numbers in Rome, including many skilled artisans. It is through such features that continents, nations, favorable sites of cities, and other refinements have been conceived, features of which a regional [chorographic] map is full; one also finds a quantity of islands scattered over the seas and along the coasts. The classical scholar Alfred Klotz, however, in his articles on the map has shown that a number of correspondences between the two works as against Pliny point rather to a common source from which both works are derived. It is difficult to see how Schnabel imagined that this line could be reduced to a straight line of 411 miles.

Without the stiffening of astronomical observation the Roman road systems were like a number of fingers probing blindly in the dark.
The variation in the figures is aggravated by the fact that our later authorities do not entirely understand the Roman method of expressing large numbers as used by Agrippa and Pliny.
When Agrippa’s Orbis Terrarum was originally created and put up for display on the wall of a portico, extensive commentary was likely consolidated within the center circular zone (2), but extending Jerusalem and Asia Minor into the map’s center displaced much of the central text and necessitated the text's redistribution about the mappamundi’s new design, relocating comments within the region to which each pertained, which is why we find the mappae mundi littered with commentary. When one considers the variants within the MSS groups it follows that one may have a dozen or more variants for a single number. Using Ptolemy’s reduction factor at 43° N latitude which is forty-three sixtieths we find that with Ptolemy’s degree of 500 stadia the difference in longitude between the two places in question is 3,135 and five-twelfths stadia and the difference in latitude is 958 and one-third stadia. He thinks the 411 miles represents the itinerary measurement from the Varus to Rimini through Dertona, and that the Arsia has got attached to it by a slight confusion in Pliny's mind in thinking of the boundaries between the mare superum and the mare inferum, with which, in fact, he equates the Varus-Arsia measurement.
Schnabel now treats the spherical triangle involved as a plane right-angled triangle, and using the theorem of Pythagoras, he finds that the hypotenuse, that is, the distance between the Varus and the Arsia is 3,291 stadia or 411 Roman miles.

Where this process is complete we have ready-made provinces, where it is still in progress we find the raw materials of provinces-to-be, which are still parts of large and scarcely known areas, and finally, where Roman armies have never set foot we find enormous, amorphous masses lumped together as geographical units. This argument, however, is unsound for a number of reasons, of which the most obvious in this context is that whereas the Dnieper is given by our sources as the west boundary of Sarmatia, it is never given as the east boundary of Dacia.
From the coincidence of the figures Schnabel strongly argues that Ptolemy must have taken over the figure of 411 miles from Agrippa. Agrippa, he thinks, took the itinerary figure for the distance from the Varus to the Arsia, which is given as 745 miles by Pliny (III, 132) and reduced it to a straight line of 411 miles by astronomical and mathematical measurement. Pages, canada, , walking fingers homepage or use Finding contact information on people or our contact information .

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