## Eratosthenes of Cyrene (c.276–c.195 BC)Among his many other accomplishments, he accurately measured the tilt of Earth's axis and the distance to the Sun and Moon, and devised a method for finding all the prime numbers up to a given number (the sieve of Eratosthenes). ## Eratosthenes' lifeEratosthenes spent his youth studying under famous masters in different Greek centers of learning and especially in Athens. He became well-known when still young and as a result he was asked to manage the library at Alexandria. This library was the most famous and the largest in the ancient world. He was also at this time appointed to be tutor to the Pharaohs, at the Egyptian court. He wrote about philosophy, drama, poetry, mathematics, and geography, but unfortunately very few of these writings have survived.Eratosthenes drew the first complete geographic map of the inhabited world and as he was convinced of the spherical shape of the Earth he suggested that it was possible to reach India by sailing westward from Spain. He also thought that there were other inhabited lands opposite his own and in this way guessed at the existence of the American continent 1,700 years before it was actually discovered. Even Christopher Columbus did not realize the existence of a new continent when he first set foot upon it. At the age of 80 Eratosthenes was blind and weary of life. He therefore committed suicide by voluntary starvation. ## How Eratosthenes measured the circumference of the Earth
Alexandria and Siene are two cities in Egypt. Siene is near the present-day town of Aswan and is on the equator. Both Alexandria and Siene are on the same meridian. They are about 500 miles apart. Refer to the diagram above. 1. Siene, June 21, mid-day. The Sun is perpendicular to the ground (shown by the fact that it is reflected in the water of wells) so its rays are directed towards the center of the Earth. 2. Alexandria is not on the equator, so the Sun's rays are not vertical to the Earth. 3. Knowing the height of an obelisk and by measuring the length of its shadows, one can calculate the inclination of the Sun's rays, something of the order of 7° 12'. 4. Now the ratio of 7° 12' to one revolution of the Sun (i.e. 360 °) is going to be proportional to the distance between Alexandria and Siene and the distance (circumference) around the Earth. 7° 12' is a fiftieth of 360; therefore the circumference of the Earth is 50 × 500 (the distance between Siene and Alexandria); this equals 25,000. The actual circumference of the Earth is very close to this figure and depends which way round it is measured. Some authorities differ as to how correct Eratosthenes' actual calculations were. Their estimation lies between 2 and 20%, depending on the value of the old measurement known as the stadium. ## Related categories• ASTRONOMERS AND ASTROPHYSICISTS• MATHEMATICIANS • GREEK ASTRONOMY | |||||||||

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