TITLE: Posidonius' World Map
DATE: 150-130 B.C.
AUTHOR: Posidonius (Petrus Bertius)
DESCRIPTION: This slide shows a 1630 reconstruction by Petrus Bertius
(Pieter Bert) of the world view of the Greek philosopher Posidonius who
proposed that the earth was sling-shaped, broad in the middle, with tapered
ends and an estimated circumference that was three-quarters of its true
size, resulting in an oikumene [inhabited world] that stretched half
way around a globe. The Bertius reconstruction, published in his Ancient
Geography (Paris, 1630), represents a literal interpretation of Posidonius'
"sling", complete with looped handles.
The better-known contemporary of Theodosius, Posidonius(ca. 135-51/50 B.C.),is
generally associated with his measurement of the circumference of the earth.
By some scholars, who view the history of mapping as mainly concerned with
the diagnosis of increasing accuracy, this measurement has been "deemed
disastrous in the history of geography." Depending on the value of
the stade that is adopted, it may be true that Posidonius, seeking to improve
on Eratosthenes, underestimated the size of the earth, and this measurement,
copied by Ptolemy, was thereafter transmitted to Renaissance Europe.
But Posidonius clearly did more than measure the earth: such was his reputation
as an educator that Strabo described him as "one of the most learned
philosophers in our time." He was born in Apamea in Syria; after traveling
widely in the western Mediterranean countries and visiting Rome on several
occasions, he established himself in Rhodes, where he opened a school. This
was patronized by distinguished visitors, including Pompey, the Roman general
and statesman, and Cicero, from whom some of our knowledge of Posidonius
derives. It was also at Rhodes that he constructed a planetarium in the
style of Archimedes, intended for teaching students the laws of the cosmos.
Cicero describes "the orrery recently constructed by our friend Posidonius,
which at each revolution reproduces the same motions of the sun, the moon
and the five planets that take place in the heavens every twenty-four hours."
Besides demonstrating his mechanical skill in this way, Posidonius was engaged
in reassessing some of the theories about the earth current in his day.
Indeed, in this respect his writing was to serve as an important conceptual
link between cartography in the ancient and medieval worlds. In his treatise
The Ocean (now lost but known to us through Strabo), for example,
he discussed the problem of terrestrial zones, which is relevant to an understanding
of the zonal mappaemundi of the Middle Ages.
In this text, inspired by the work of Pytheas, Posidonius began by criticizing
the usual division of the earth into five zones - one uninhabited (torrid)
zone, two inhabitable (temperate) zones, and two uninhabited (frigid) zones
- for he considered the limits between them to be uncertain and inaccurate.
According to Strabo's Geography (Slide #115)
Posidonius criticized Parmenides' division of the earth into five zones
because he represented the torrid zone as almost double its real breadth,
and he criticized Aristotle for calling the region between the tropics "torrid"
and the regions between the tropics and the arctic circles "temperate."
Posidonius disagreed with both Parmenides and Aristotle and asked "how
one could determine the limits of the temperate zones, which are nonvariable,
by means of the 'arctic circles,' which are neither visible among all men
nor the same everywhere." Instead of employing the traditional terms
for the zones, based on temperature or habitability, he proposed terms based
on clearly defined astronomical criteria. He divided the terrestrial globe
by means of the tropics and the polar circles and named the zones as in
the table below.
POSIDONIUS' TERRESTRIAL ZONES
ZONE AREA MEANING
Amphiskian Between the tropics Where the shadow of the
(one zone) gnomon is directed alternately
to the north and to the south.
Heteroskian Between each tropic Where the shadow of the
(two zones) and each polar circle
gnomon is directed either
to the north or to the south,
depending on the hemisphere.
Note: The Greek skia means shadow.
At the same time, Posidonius appreciated that if he altered the criteria
for the division, so as to take temperature distribution more fully into
account, the earth could be divided into seven zones. These he identified
as the two frigid zones around the poles, the two temperate zones in their
usual places, two narrow, extremely arid zones along the terrestrial tropics
having the sun directly over head for about half a month each year, and
finally the equatorial zone, more temperate and better watered than the
two tropical ones. At one point Posidonius also proposed dividing the inhabited
world not into continents, as was usual in his day, but by means of circles
parallel to the equator, indicating variations in fauna, flora, and climate.
However, Strabo commented unfavorably on this innovative idea. It was, he
said, "a mere matter of argument, with no useful end in view."
Equally revisionist was Posidonius' challenge to Eratosthenes' measurement
of the circumference of the earth. Our knowledge of his methods, as with
the earlier reasoning of Eratosthenes, is derived from Cleomedes, and it
becomes clear that it was based on assumptions that were sometimes false.
These assumptions included the belief that Rhodes and Alexandria lay on
the same meridian and that the distance between the two places was 5,000
stades. Then Posidonius (according to Cleomedes), noting that Canopus
was seen just on the horizon at Rhodes but rose as far as a quarter of a
zodiacal sign (7.5°) above the horizon at Alexandria, concluded that
the center angle intercepting the Rhodes-Alexandria arc of meridian was
one-forty-eighth of the total circle or 4.5° (the arc is actually 5°14')
. Thus, he argued, the total length of the meridian was forty-eight times
the distance between Rhodes and Alexandria, and, assuming this latter to
be 5,000 stades, this gave a figure of 240,000 stades for
the circumference of the earth.
This, however, is only a partial history of the confusion attached to the
measurement. As a teacher interested in promoting discussion, Posidonius
seems to have criticized his own assumptions, in particular the estimate
of 5,000 stades for the distance from Rhodes to Alexandria. Evidently,
at some point in his calculations he employed an alternative value of 3,750
stades, derived from a careful estimate Eratosthenes made "by
means of shadow-catching sundials." When applied to the 1:48 ration,
this gave a correspondingly smaller length for the circumference of the
earth of 180,000 stades.
What is important for the history of cartography is that it was this measurement
- whether directly or through an intermediary -that was later adopted by
both Marinus of Tyre and Ptolemy. Its main effect was greatly to exaggerate
the portion of the globe occupied by the inhabited world, so that the length
from the Straits of Gibraltar to India, along the parallel of Rhodes, came
to be considered half of the entire parallel around the earth. And such
was the authority of Ptolemy that this misconception was carried forward
by geographers, cosmographers, and cartographers into the sixteenth century.
Historians of discovery have noted that it long colored the perception of
that age as to the size of the unknown portion of the world. Most famously
in Columbus' belief in the proximity of the Indies when sailing westward.
LOCATION: (this map only exists as a reconstruction)
*Bricker, C., Landmarks in Mapmaking,. p. 15.
Brown, L., The Story of Maps, pp. 30-32.
Harley, J.B., The History of Cartography, Volume One, pp. 168-170.