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Fig. 2: Soria E Terra Sancta Nova Tabvla from<br />

La Geographia... by Giacomo Gastaldi, published<br />

by Giovanni Battista Pedrezano, Venice<br />

1548; 130 x 170 mm<br />

[24] [25]<br />

Classical scripts including Ptolemy’s books at the end of the 14th century<br />

when a delegation of Byzantine scholars visited Venice and Florence. For the<br />

Florentines this was a revelation. They were so impressed that several decided<br />

to learn Greek and translate them. Jacopo Angeli da Scarperia with the help of<br />

his teacher Manuel Chrysoloras, translated the Cosmographia into Latin during<br />

the years 1400–1407 making it available to the West for the first time in<br />

manuscript form.<br />

GeoGrAphicAl knowledGe At the time of ptolemy<br />

Ptolemy’s concept that the earth was a perfect sphere was based on the teachings<br />

of Pythagoras in the 6th century Bc and the proofs provided by Aristotle<br />

(384–322). He accepted the calculation of the earth’s circumference by Poseidonius<br />

of Apameia (130–52 Bc) of 18,000 miles (50 miles to an arc of 1 degree)<br />

rather than that of Eratosthenes of Cyrene of 25,200 miles (70 miles to an arc<br />

of 1 degree). This made the Earth circumference 18% smaller than the true<br />

size. His concept of the sun and planets in orderly orbits around the stationary<br />

earth at the centre of the universe with the stars fixed<br />

on an outer celestial sphere also rotating round the earth<br />

was the most popular at the time, while rejecting the heliocentric<br />

hypothesis of Aristarchus of Samos (310–230 Bc).<br />

The latitude of a locality was the angle of inclination<br />

from the equator and was between 00 and 900 depending<br />

on the distance from the equator. It could be determined<br />

from several measurements such as (a) the elevation of the<br />

north celestial pole above the horizon, (b) the ratio of a vertical<br />

stick (gnomon) to its shadow on the longest and shortest<br />

days of the year or (c) the ratio of the longest day of the<br />

year to the shortest, or even the length of the longest day.<br />

Thus, Ptolemy gives latitude as hours of sunlight.<br />

Longitude was measured eastward starting at the Fortunate (Canary)<br />

islands and Ptolemy drew his meridians at “intervals of a third of an equinoctial<br />

hour” i.e. at 50 intervals.<br />

“The Zodiacal circle”, the ecliptic, was recognised as the circle tilted at<br />

an angle of 240 traversed by the sun at a rate of just under a degree a day opposite<br />

to the rotation of the stars. The most northerly point of the ecliptic defined<br />

the Tropic of Cancer and the most southerly the Tropic of Capricorn.<br />

Tow further circles were recognised, the Arctic and Antarctic where the<br />

longest day of the year just reached 24 hours.<br />

Although the division of the circle to 3600 dates to Babylonian times<br />

and was used by the Greek astronomers and mathematicians,<br />

Ptolemy was the first to apply it in the use of terrestrial coordinates<br />

for specifying geographic positions.<br />

The habitable world of Ptolemy, the oikoumene, occupied<br />

one quarter of the earth, from just south of the equator to the<br />

64½ degrees north of the equator, and from the fortunate islands<br />

00 longitude to the end of the “Silk country” 1800 longitude.<br />

Thus, the width of Europe and Asia were exaggerated by 30%.<br />

Ptolemy believed that there was a southern land counterbalancing<br />

the land north of the equator so that the Indian Ocean was<br />

shown as a closed sea, but this land south of the equator was too<br />

hot to sustain human life. On the question whether the land on<br />

the other side of the earth was inhabited Ptolemy kept an open mind. The<br />

oikoumene was divided in three continents, Europe, Libye (Africa) and Asia.<br />

In the Geographia, Ptolemy states that to draw the world map on a globe<br />

is a method of ensuring correct representation of distances, but argues that<br />

globes are usually too small to show detail and he describes how to make<br />

projections on a flat surface. He gives detailed instructions how to make three<br />

different projections. His first projection is a conical one. In this projection<br />

east-west distances are portrayed in correct proportionality to north-south<br />

distances only along the parallel of Rhodes. His second projection is a pseudoconical<br />

one that preserves the ratio of the total latitudinal dimension to the<br />

total longitudinal dimension for all parallels. A third spherical projection is a<br />

modification of the second, but has not been used in any of the manuscript or<br />

printed Ptolemaic atlases. In addition to the world map, Ptolemaic atlases<br />

contain 26 regional maps with equidistant meridians and parallels: 10 for<br />

MAPPING CYPRUS EUROPEAN CARTOGRAPHERS AND CYPRUS<br />

Fig. 3: Asiae IIII Tab: From Tabvlae Goographicae<br />

Cl. Ptolomei... edited by Gerard<br />

Mercator, and printed by Godefrid von<br />

Kempen, Cologne, 1578; 345 x 465 mm

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