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<TEI.2><text lang="en"><body><div1 type="book" n="2" org="uniform" sample="complete"><div2 type="chapter" n="5" org="uniform" sample="complete"><p><milestone ed="P" n="8" unit="section" /></p>
<p>It is true that Pytheas of Marseilles affirms that the

farthest country north of the British islands is Thule; for

which place he says the summer tropic and the arctic circle

is all one. But he records no other particulars concerning

it; [he does not say] whether Thule is an island, or whether

it continues habitable up to the point where the summer

tropic becomes one with the arctic circle.<note anchored="yes" place="unspecified">The tropic being placed at 24° from the equator by Strabo, and most

probably by Pytheas also, the latitude of Thule, according to the observation of this traveller, would be fixed at 66°, which corresponds with the

north of Iceland.</note> For myself, I

fancy that the northern boundaries of the habitable earth are

greatly south of this. Modern writers tell us of nothing beyond Ierne, which lies just north of Britain, where the people live miserably and like savages on account of the severity

of the cold. It is here in my opinion the bounds of the habitable earth ought to be fixed.
</p><p>If on the one hand the parallels of Byzantium and Marseilles are the same, as Hipparchus asserts on the faith of

Pytheas, (for he<note anchored="yes" place="unspecified">Hipparchus.</note> says that at Byzantium the gnomon indicates the same amount of shadow as Pytheas gives for

Marseilles,) and at the same time the parallel of the Dnieper

is distant from Byzantium about 3800 stadia, it follows, if

we take into consideration the distance between Marseilles

and Britain, that the circle which passes over the Dnieper

traverses Britain as well.<note anchored="yes" place="unspecified">Hipparchus placed Marseilles and Byzantium at 30,142 stadia, or

43° 3′ 38″ of latitude, and estimated the parallel for the centre of Britain at 33,942 stadia, or 48° 29′ 19″. Whereas Strabo only allowed for this latter 32,700 stadia, or 46° 42′ 51″.</note> But the truth is that Pytheas,

who so frequently misleads people, deceives in this instance

too.
</p><p>It is generally admitted that a line drawn from the Pillars

of Hercules, and passing over the Strait [of Messina], Athens,

and Rhodes, would lie under the same parallel of latitude.<note anchored="yes" place="unspecified">Viz. the 36° of latitude. The actual latitudes are as follow:

<p>The Pillars of Hercules, or Strait of Gibraltar, 360.
</p><p>The Strait of Messina, 38° 12′.
</p><p>Athens, 38° 5′.
</p><p>The middle of the Isle of Rhodes, 36° 18′; and the city, 36° 28′ 30″.</p></note> It

is likewise admitted, that the line in passing from the Pillars to

the Strait of Sicily divides the Mediterranean through the



<pb n="174" />



midst.<note anchored="yes" place="unspecified">This mistake of Strabo caused the derangement in his chart of the

whole contour of this portion of the Mediterranean, and falsifies the position of the surrounding districts.</note> Navigators tell us that the greatest distance from

Keltica to Libya, starting from the bottom of the Galatic Bay, is

5000 stadia, and that this is likewise the greatest breadth of

the Mediterranean. Consequently from the said line to the

bottom of the bay is 2500 stadia; but to Marseilles the distance is rather less, in consequence of that city being more to

the south than the bottom of the bay.<note anchored="yes" place="unspecified">Strabo having allowed 25,400 stadia, or 36° 17′ 8″, for the latitude

of Rhodes and the Strait of Messina, determined the latitude of Marseilles

at 27,700 stadia, or 39° 34′ 17″; its real latitude being 43° 17′ 45″, as exactly stated by Pytheas.</note> But since from

Rhodes to Byzantium is about 4900<note anchored="yes" place="unspecified">Or about 70. The actual difference in latitude between Rhodes and

Byzantium is 4° 32′ 54″.</note> stadia, it follows that

Byzantium must be far north of Marseilles.<note anchored="yes" place="unspecified">On the contrary, Marseilles is 2° 16′ 21″ north of Byzantium.</note> The distance

from this latter city to Britain is about the same as from Byzantium to the Dnieper.<note anchored="yes" place="unspecified">3800 stadia, or 5° 25′ 43″.</note> How far it may be from Britain to the island of Ierne is not known. As to whether

beyond it there may still be habitable lands, it is not our business to inquire, as we stated before. It is sufficient for our

science to determine this in the same manner that we did the

southern boundaries. We there fixed the bounds of the habitable earth at 3000 stadia south of Meroe (not that these

were its exact limits, but because they were sufficiently near);

so in this instance they should be placed about the same number of stadia north of Britain, certainly not more than 4000.<note anchored="yes" place="unspecified">The following is a tabular form of the latitudes as stated by Strabo:



<table>
<row role="data"><cell cols="1" role="data" rows="1" /><cell cols="1" role="data" rows="1">Stadia.</cell><cell cols="1" role="data" rows="1">Latitude.</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the equator to Alexandria</cell><cell cols="1" role="data" rows="1">21,800</cell><cell cols="1" role="data" rows="1">31° 8′ 34″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From Alexandria to Rhodes, he computes in this instance 3600 stadia</cell><cell cols="1" role="data" rows="1">25,400</cell><cell cols="1" role="data" rows="1">36 17′ 8″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the parallel of Rhodes to Marseilles, about 2300 stadia</cell><cell cols="1" role="data" rows="1">27,700</cell><cell cols="1" role="data" rows="1">39° 34′ 17″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the parallel of Rhodes to the bottom of the Galatic Gulf, 2500 stadia</cell><cell cols="1" role="data" rows="1">27,900</cell><cell cols="1" role="data" rows="1">39° 51′ 25″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From Marseilles to the northern extremity of Gaul, or the southern extremity of Britain, 3800 stadia</cell><cell cols="1" role="data" rows="1">31,500</cell><cell cols="1" role="data" rows="1">45° 0′ 0″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From Marseilles to the middle of Britain, 5000 stadia</cell><cell cols="1" role="data" rows="1">32,700</cell><cell cols="1" role="data" rows="1">46° 42′ 51″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the northern extremity of Gaul to the parallel of the northern extremity of Britain, 2500 stadia</cell><cell cols="1" role="data" rows="1">34,000</cell><cell cols="1" role="data" rows="1">48° 34′ 17″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the northern extremity of Gaul to Ierne, 5000 stadia</cell><cell cols="1" role="data" rows="1">36,500</cell><cell cols="1" role="data" rows="1">52° 8′ 34″</cell></row>
<row role="data"><cell cols="1" role="data" rows="1">From the northern extremity of Britain to the limits of the habitable earth, 4000 stadia</cell><cell cols="1" role="data" rows="1">38,000</cell><cell cols="1" role="data" rows="1">54° 17′ 9″</cell></row>
</table></note>



<pb n="175" />



It would not serve any political purpose to be well acquainted with these distant places and the people who inhabit

them; especially if they are islands whose inhabitants can

neither injure us, nor yet benefit us by their commerce. The

Romans might easily have conquered Britain, but they did

not care to do so, as they perceived there was nothing to fear

from the inhabitants, (they not being powerful enough to attack us,) and that they would gain nothing by occupying the

land. Even now it appears that we gain more by the customs

they pay, than we could raise by tribute, after deducting the

wages of the soldiers necessary for guarding the island and

exacting the taxes. And the other islands adjacent to this

would be still more unproductive.

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