Geography, ethnology and geology
Posidonius’s fame beyond specialized philosophical circles had begun, at the latest, in the eighties with the publication of the work "about the ocean and the adjacent areas". This work was not only an overall representation of geographical questions according to current scientific knowledge, but it served to popularize his theories about the internal connections of the world, to show how all the forces had an effect on each other and how the interconnectedness applied also to human life, to the political just as to the personal spheres. In this work, Posidonius detailed his theory of the effect on a people’s character by the climate, which included his representation of the "geography of the races". This theory was not solely scientific, but also had political implications -- his Roman readers were informed that the climatic central position of Italy was an essential condition of the Roman destiny to dominate the world. As a Stoic he did not, however, make a fundamental distinction between the civilized Romans as masters of the world and the less civilized peoples.
Posidonius measured the
Earth's circumference by reference to the position of the star
Canopus. As explained by Cleomedes, Posidonius observed Canopus on but never above the horizon at Rhodes, while at
Alexandria he saw it ascend as far as 7 1/2 degrees above the horizon (the arc between the latitude of the two locales is actually 5 degrees 14 minutes). Since he thought Rhodes was 5,000 stadia due north of Alexandria, and the difference in the star's elevation indicated the distance between the two locales was 1/48th of the circle, he multiplied 5,000 by 48 to arrive at a figure of 240,000 stadia for the circumference of the earth. While translating stadia into modern units of distance is problematic, as an ancient stadium could measure anywhere from about 157 to around 211 meters, it is generally thought that the stadium used by Posidonius was almost exactly 1/10 of a modern statute mile, near the middle of the ancient range. Thus Posidonius' measure of 240,000 stadia translates to 24,000 miles, not much short of the actual circumference of 24,901 miles.
Posidonius was informed in his approach to finding the earth's circumference by
Eratosthenes, who a century earlier used the elevation of the sun at different latitudes to arrive at a figure of 250,000 stadia (which he rounded to 252,000 so that it would be divisible by 60). As with Posidonius, Eratosthenes' stadium is thought to have equated to 1/10th of a mile, so that his measure translates to 25,000 (or 25,200) miles. Both men's figures for the earth's circumference were uncannily accurate, aided in part in each case by mutually compensating errors in measurement. However, Posidonius later revised his original calculation by correcting the distance between Rhodes and Alexandria to 3,750 stadia, resulting in a circumference of 180,000 stadia, or 18,000 miles.
Ptolemy discussed and favored this revised figure of Posidonius over Eratosthenes in his
Geographia, and during the
Middle Ages scholars divided into two camps regarding the circumference of the earth, identified with Eratosthenes' calculation on the one hand and Posidonius' 180,000-stadium measure on the other.
Like
Pytheas, Posidonius believed the
tide is caused by the
Moon. Posidonius was, however, wrong about the cause. Thinking that the Moon was a mixture of air and fire, he attributed the cause of the tides to the heat of the Moon, hot enough to cause the water to swell but not hot enough to evaporate it.
He recorded observations on both earthquakes and volcanoes, including accounts of the eruptions of the volcanoes in the
Aeolian Islands, north of
Sicily.