They show light hair, usually reddish brown, and blue eyes, as do larger statues from the time of the Persian Wars in the early fifth century BC. Lunar eclipse viewed from Merritt Island, Florida, U.S., November 8, 2003.Eratosthenes' method of measuring Earth's circumference.By knowing the length of an arc (Ptolemy's equant modelIn Ptolemy's geocentric model of the universe, the Sun, the Moon, and each planet orbit a stationary Earth. This resulted in disorienting illustrations.To escape the complicated nature of this extensive number of circles, Ptolomy added a series of new concepts. Given that opportunities for observations of a lunar eclipse do not come along that often, there was also evidence of the roundness of the earth in the experiences of sailors.When a ship appears on the horizon it's the top of the ship that is visible first. While the earth was a place of transition and flux, the heavens were unchanging. Earth was the heaviest, water less so, and air and fire the lightest. Ptolemy was also interested in deploying his model of the heavens to describe its physical reality. Think of the night's sky. So the planets moved on circles that moved on circular orbits. More-detailed astronomical knowledge is found in Hesiod’s Works and Days, from perhaps a generation later than Homer. Looking at the night sky the ancient Greeks found two primary kinds of celestial objects; the fixed stars and the wandering stars.

Babylonian and Egyptian astronomers developed systems that became the basis for Greek astronomy, while societies in the Americas, China and India developed their own.Ancient Greek astronomers' work is richly documented in the collections of the Library of Congress largely because of the way the Greek tradition of inquiry was continued by the work of Islamic astronomers and then into early modern European astronomy. He is considered by many to be the greatest observational astronomer of ancient Greece. It is difficult for us to fully understand what this meant as today we think about matter in very different terms. If the Earth were flat, it would be expected that you would be able to see the entire ship as soon as it became visible.Lunar eclipses also allowed for another key understanding about our home here on Earth. Then Night alone produced Doom, Fate, Death, Sleep, Dreams, Nemesis, and others that come to man out of darkness. Benefiting from hundreds of years of observation from the time of Hipparchus and Eudoxus, as well as a set of astronomical data collected by the Babylonians, Ptolemy developed a system for predicting the motion of the stars that was published in his primary astronomical work, By the time of Ptolemy Greek astronomers had proposed adding circles on the circular orbits of the wandering stars (the planets, the moon and the sun) to explain their motion.

For an ancient scientist, he was unusually generous in crediting his predecessors, particularly Hipparchus, for discoveries. There is some dispute on the accuracy of his calculations as we don't know exactly how long the units of measure were. Ptolomy also needed to introduce equants, a tool that enabled the planets to move at different speeds as they moved around these circles. The heavens are a separate realm governed by their own rules.In contrast to the terrestrial, the celestial region of the heavens had a fundamentally different nature. The Greeks were applying mathematics to theorize about the nature of their world. In any case, Ptolemy’s publications fundamentally changed the way astronomy was done in the Ptolemy also wrote a speculative cosmological work, the As the shadow moves across the moon it is clearly round. The large circle is the sun, the medium circle is the Earth and the smallest circle is the moon.

The centre of the deferent is midway between the equant and Earth.


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