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Eratosthenes
An etching of a man's head and neck in profile, looking to the right. The man has a beard and is balding.
Portrait of Eratosthenes
Born 276 BC
Cyrene
Died 194 BC
Alexandria
Ethnicity Greek
Occupation Scholar, librarian, poet and inventor

Eratosthenes of Cyrene (Ancient Greek: Ἐρατοσθένης, IPA: [eratostʰénɛːs]; English /ɛrəˈtɒsθənz/; c. 276 BC[1] – c. 195 BC[2]) was a Greek mathematician, geographer, poet, astronomer, and music theorist.

He was the first person to use the word "geography" in Greek and he invented the discipline of geography as we understand it.[3] He invented a system of latitude and longitude.

He was the first person to calculate the circumference of the earth by using a measuring system using stades, or the length of stadiums during that time period (with remarkable accuracy). He was the first to calculate the tilt of the Earth's axis (also with remarkable accuracy). He may also have accurately calculated the distance from the earth to the sun and invented the leap day.[4] He also created the first map of the world incorporating parallels and meridians within his cartographic depictions based on the available geographical knowledge of the era. In addition, Eratosthenes was the founder of scientific chronology; he endeavoured to fix the dates of the chief literary and political events from the conquest of Troy.

According to an entry[5] in the Suda (a 10th-century reference), his contemporaries nicknamed him beta, from the second letter of the Greek alphabet, because he supposedly proved himself to be the second best in the world in almost every field.[6]

Contents

Life[edit]

Eratosthenes' map of the world (194 B.C.)
19th-century reconstruction of Eratosthenes' map of the known world, c. 194 BC

Eratosthenes was born in Cyrene (in modern-day Libya). He was the third chief librarian of the Great Library of Alexandria, the center of science and learning in the ancient world, and died in Alexandria, then the capital of Ptolemaic Egypt.

Eratosthenes studied in Alexandria, and claimed to have also studied for some years in Athens. In 236 BC, he was appointed by Ptolemy III Euergetes as librarian of the Alexandrian library, succeeding the second librarian, Apollonius of Rhodes.[7] He made several important contributions to mathematics and science, and was a good friend to Archimedes. Around 255 BC, he invented the armillary sphere. In On the Circular Motions of the Celestial Bodies, Cleomedes credited him with having calculated the Earth's circumference around 240 BC, using knowledge of the angle of elevation of the sun at noon on the summer solstice in Alexandria and on Elephantine Island near Syene (now Aswan, Egypt).

Eratosthenes believed there was good and bad in every nation and criticized Aristotle for arguing that humanity was divided into Greeks and barbarians, and that the Greeks should keep themselves racially pure.[8] By 195 BC, Eratosthenes became blind. He died in 194 BC at the age of 82.

Eratosthenes' measurement of the Earth's circumference[edit]

Illustration showing a portion of the globe showing a part of the African continent. The sun beams shown as 2 rays hitting earth at Syene and Alexandria. Angle of sun beam and the gnomons (vertical sticks) is shown at Alexandria which allowed Eratosthenes' estimates of radius and circumference of Earth.

Eratosthenes calculated the circumference of the Earth without leaving Egypt. Eratosthenes knew that, on the summer solstice, at local noon in the Ancient Egyptian city of Swenet (known in Greek as Syene, and in the modern day as Aswan) on the Tropic of Cancer, the sun would appear at the zenith, directly overhead (he had been told that the shadow of someone looking down a deep well would block the reflection of the Sun at noon). Using a gnomon, he measured the sun's angle of elevation at noon on the solstice in his hometown of Alexandria, and found it to be 1/50th of a circle (7°12') south of the zenith. He could have used a compass to measure the angle of the shadow cast.[9] Assuming that the Earth was spherical (360°), and that Alexandria was due north of Syene, he concluded that the meridian arc distance from Alexandria to Syene must therefore be 1/50 = 7°12'/360°, and was therefore 1/50 of the total circumference of the Earth. His knowledge of the size of Egypt after many generations of surveying trips for the Pharaonic bookkeepers gave a distance between the cities of 5,000 stadia (about 500 geographical miles or 927.7 km). This distance was corroborated by inquiring about the time that it takes to travel from Syene to Alexandria by camel. He rounded the result to a final value of 700 stadia per degree, which implies a circumference of 252,000 stadia. The exact size of the stadion he used is frequently debated. The common Attic stadion was about 185 m,[10] which would imply a circumference of 46,620 km, which is off the actual circumference by 16.3%. However, if we assume that Eratosthenes used the "Egyptian stadion"[11] of about 157.5 m, his measurement turns out to be 39,690 km, an error of 1.6%.[12] Nevertheless, it is impossible Eratosthenes got an accurate measurement of the circumference of the earth, given errors in the assumptions he made. He must have had a considerable margin of error and therefore couldn't have used the egyptian stadion.[13]

Other astronomical distances[edit]

Eusebius of Caesarea in his Preparatio Evangelica includes a brief chapter of three sentences on celestial distances (Book XV, Chapter 53). He states simply that Eratosthenes found the distance to the sun to be "σταδίων μυριάδας τετρακοσίας καὶ ὀκτωκισμυρίας" (literally "of stadia myriads 400 and 80,000") and the distance to the moon to be 780,000 stadia. The expression for the distance to the sun has been translated either as 4,080,000 stadia (1903 translation by E. H. Gifford), or as 804,000,000 stadia (edition of Edouard des Places, dated 1974–1991). The meaning depends on whether Eusebius meant 400 myriad plus 80,000 or "400 and 80,000" myriad. With a stadium of 185 meters, 804,000,000 stadia is 149,000,000 kilometers, approximately the distance from the earth to the sun.

Prime numbers[edit]

Eratosthenes also proposed a simple algorithm for finding prime numbers. This algorithm is known in mathematics as the Sieve of Eratosthenes.

In mathematics, the sieve of Eratosthenes (Greek: κόσκινον Ἐρατοσθένους), one of a number of prime number sieves, is a simple, ancient algorithm for finding all prime numbers up to any given limit. It does so by iteratively marking as composite (i.e. not prime) the multiples of each prime, starting with the multiples of 2. The multiples of a given prime are generated starting from that prime, as a sequence of numbers with the same difference, equal to that prime, between consecutive numbers. This is the sieve's key distinction from using trial division to sequentially test each candidate number for divisibility by each prime.

Works[edit]

Things named after Eratosthenes[edit]

grayscale image of a crater on the moon

See also[edit]

Notes[edit]

  1. ^ The Suda states that he was born in the 126th Olympiad, (276–272 BC). Strabo (Geography, i.2.2), though, states that he was a "pupil" (γνωριμος) of Zeno of Citium (who died 262 BC), which would imply an earlier year-of-birth (c. 285 BC) since he is unlikely to have studied under him at the young age of 14. However, γνωριμος can also mean "acquaintance", and the year of Zeno's death is by no means definite. Cf. Eratosthenes entry in the Dictionary of Scientific Biography (1971)
  2. ^ The Suda states he died at the age of 80, Censorinus (De die natali, 15) at the age of 81, and Pseudo-Lucian (Makrobioi, 27) at the age of 82.
  3. ^ Erastothenes (2010). Eratosthenes' "Geography". Fragments collected and translated, with commentary and additional material by Duane W. Roller. Princeton University Press. ISBN 978-0-691-14267-8. 
  4. ^ Alfred, Randy (June 19, 2008). "June 19, 240 B.C.: The Earth Is Round, and It's This Big". Wired. 
  5. ^ Entry ε 2898
  6. ^ See also Asimov, Isaac. Asimov's Biographical Encyclopedia of Science and Technology, new revised edition. 1975. Entry #42, "Eratosthenes", Page 29. Pan Books Ltd, London. ISBN 0-330-24323-3. It was also asserted by Carl Sagan, 31 minutes into his Cosmos episode The Shores of the Cosmic Ocean
  7. ^ Oxford Reference (subscription required)
  8. ^ * p439 Vol. 1 William Woodthorpe Tarn Alexander the Great. Vol. I, Narrative; Vol. II, Sources and Studies0. Cambridge: Cambridge University Press, 1948. (New ed., 2002 (paperback, ISBN 0-521-53137-3)).
  9. ^ How did Eratosthenes measure the circumference of the earth?
  10. ^ Engels, Donald (Autumn 1984). "The Length of Eratosthenes' Stade". American Journal of Philology 106 (3): 298–311. doi:10.2307/295030. JSTOR 295030. 
  11. ^ Isaac Moreno Gallo (3–6 November 2004). "Roman Surveying" (PDF). translated by Brian R. Bishop. Archived from the original on 2007-02-05 
  12. ^ There is a huge volume of Eratosthenes-got-it-right literature based on attacking the applicability of the standard 185 m stadium to his experiment. Among advocates: F. Hultsch, Griechische und Römische Metrologie, Berlin, 1882; E. Lehmann-Haupt, Stadion entry in Paulys Real-Encyclopädie, Stuttgart, 1929; I. Fischer, Q. Jl. R. astr. Soc. 16.2:152–167, 1975; Gulbekian (1987); Dutka (1993). The means employed include worrying various ratios of the stadium to the unstably defined "schoenus", or using a truncated passage from Pliny. (Gulbekian just computes the stadium from Eratosthenes' experiment instead of the reverse.) Nicastro (2008), however, uses statistical analysis of Eratosthenes' linear distances (as reported by Strabo) to establish a 95% probability that Eratosthenes used a stade between 153.5 and 162.4 meters, with the 185 m "Attic" stade well outside the 3-sigma confidence interval. A disproportionality of literature exists because some professional scholars of ancient science have regarded such speculation as special pleading and so have not bothered to write extensively on the issue. Skeptical works include E. Bunbury's classic History of Ancient Geography, 1883; D. Dicks, Geographical Fragments of Hipparchus, University of London, 1960; O. Neugebauer, History of Ancient Mathematical Astronomy, Springer, 1975; J. Berggren and A. Jones, Ptolemy's Geography, Princeton, 2000. Some difficulties with the several arguments for Eratosthenes' exact correctness are discussed by Rawlins in 1982b page 218 and in his Contributions and Distillate. See also, at [1], "The Shores of the Cosmic Ocean", chapter 1 of Cosmos: A Personal Voyage, a TV series by Carl Sagan, Ann Druyan and Steven Sotter (1978–1979), where a description of Eratosthenes' experiment is presented.
  13. ^ How did Eratosthenes measure the circumference of the earth?
  14. ^ Mentioned by Hero of Alexandria in his Dioptra. See p. 272, vol. 2, Selections Illustrating the History of Greek Mathematics, tr. Ivor Thomas, London: William Heinemann Ltd.; Cambridge, MA: Harvard University Press, 1957.

Further reading[edit]

  • Aujac, G. (2001). Eratosthène de Cyrène, le pionier de la geographie. Paris: Édition du CTHS. 224p.
  • Bulmer-Thomas, Ivor (1939-1940). Selections Illustlating the History of Greek Mathematics. Cambridge, MA: Harvard University Press. 
  • Cameron McPhail (2011). Reconstructing Eratosthenes' Map of the World: a Study in Source Analysis. A Thesis Submitted for the Degree of Master of Arts at the University of Otago. Dunedin, New Zealand.
  • Diller, A. (1934). “Geographical Latitudes in Eratosthenes, Hipparchus and Posidonius”. Klio 27(3): 258–269.
  • Dorofeeva, A. V. (1988). "Eratosthenes (ca. 276–194 B.C.)". Mat. V Shkole (in Russian) (4): i. 
  • Dutka, J. (1993). "Eratosthenes' measurement of the Earth reconsidered". Arch. Hist. Exact Sci. 46 (1): 55–66. doi:10.1007/BF00387726. 
  • El'natanov, B. A. (1983). "A brief outline of the history of the development of the sieve of Eratosthenes". Istor.-Mat. Issled. (in Russian) 27: 238–259. 
  • Fischer, I. (1975). "Another look at Eratosthenes' and Posidonius' determinations of the Earth’s circumference". Quarterly Journal of the Royal Astronomical Society 16: 152—167.
  • Fowler, D. H.; Rawlins, Dennis (1983). "Eratosthenes' ratio for the obliquity of the ecliptic". Isis 74 (274): 556–562. doi:10.1086/353361. 
  • Fraser, P. M. (1970). "Eratosthenes of Cyrene". Proceedings of the British Academy 56: 175–207. 
  • Fraser, P. M. (1972). Ptolemaic Alexandria. Oxford: Clarendon Press. 
  • Geus K. (2002). Eratosthenes von Kyrene. Studien zur hellenistischen Kultur- und Wissenschaftgeschichte. München: Verlag C.H. Beck. (Münchener Beiträge zur Papyrusforschung und antiken Rechtsgeschichte. Bd. 92) X, 412 S.
  • Goldstein, B. R. (1984). "Eratosthenes on the "measurement" of the earth". Historia Math. 11 (4): 411–416. doi:10.1016/0315-0860(84)90025-9. 
  • Gulbekian, E. (1987). "The origin and value of the stadion unit used by Eratosthenes in the third century B.C". Arch. Hist. Exact Sci. 37 (4): 359–363. doi:10.1007/BF00417008. 
  • Honigmann, E. (1929). Die sieben Klimata und die πολεις επισημοι. Eine Untersuchung zur Geschichte der Geographie und Astrologie in Altertum und Mittelalter. Heidelberg: Carl Winter’s Universitätsbuchhandlung. 247 S.
  • Knaack, G. (1907). "Eratosthenes". Pauly–Wissowa VI: 358–388. 
  • Manna, F. (1986). "The Pentathlos of ancient science, Eratosthenes, first and only one of the "primes"". Atti Accad. Pontaniana (N.S.) (in Italian) 35: 37–44. 
  • Muwaf, A.; Philippou, A. N. (1981). "An Arabic version of Eratosthenes writing on mean proportionals". J. Hist. Arabic Sci. 5 (1–2): 174–147. 
  • Nicastro, Nicholas (2008). Circumference: Eratosthenes and the ancient quest to measure the globe. New York: St. Martin's Press. ISBN 0-312-37247-7. 
  • O'Connor, John J.; Robertson, Edmund F., "Eratosthenes", MacTutor History of Mathematics archive, University of St Andrews .
  • Marcotte, D. (1998). “La climatologie d’Ératosthène à Poséidonios: genèse d’une science humaine”. G. Argoud, J.Y. Guillaumin (eds.). Sciences exactes et sciences appliquées à Alexandrie (IIIe siècle av J.C. – Ier ap J.C.). Saint Etienne: Publications de l'Université de Saint Etienne: 263–277.
  • Pfeiffer, Rudolf (1968). History of Classical Scholarship From the Beginnings to the End of the Hellenistic Age. Oxford: Clarendon Press. 
  • Rawlins, D. (1982). "Eratosthenes' geodesy unraveled : was there a high-accuracy Hellenistic astronomy". Isis 73 (2): 259–265. doi:10.1086/352973. 
  • Rawlins, D. (1982). "The Eratosthenes – Strabo Nile map. Is it the earliest surviving instance of spherical cartography? Did it supply the 5000 stades arc for Eratosthenes' experiment?". Arch. Hist. Exact Sci. 26 (3): 211–219. 
  • Rawlins, D. (2008). "Eratothenes's large earth and tiny universe" (PDF). DIO 14: 3–12. 
  • Roller, Duane W. (2010). Eratosthenes' Geography: Fragments collected and translated, with commentary and additional material. Princeton: Princeton University Press. ISBN 978-0-691-14267-8. 
  • Shcheglov, D.A. (2004/2006). “Ptolemy’s System of Seven Climata and Eratosthenes’ Geography”. Geographia Antiqua 13: 21–37.
  • Shcheglov, D.A. (2006). “Eratosthenes’ Parallel of Rhodes and the History of the System of Climata”. Klio 88: 351–359.
  • Strabo (1917). The Geography of Strabo. Horace Leonard Jones, trans. New York: Putnam. 
  • Taisbak, C. M. (1984). "Eleven eighty-thirds. Ptolemy's reference to Eratosthenes in Almagest I.12". Centaurus 27 (2): 165–167. Bibcode:1984Cent...27..165T. doi:10.1111/j.1600-0498.1984.tb00766.x. 
  • Thalamas, A. (1921). La géographe d’Ératosthène. Versailles.
  • Wolfer, E. P. (1954). Eratosthenes von Kyrene als Mathematiker und Philosoph. Groningen-Djakarta. 

External links[edit]

Preceded by
Apollonius of Rhodes
Head of the Library of Alexandria Succeeded by
Aristophanes of Byzantium


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Offshore Oil and Gas Magazine

Offshore Oil and Gas Magazine
Fri, 07 Jun 2013 12:51:01 -0700

It has been a while since Eratosthenes measured the circumference of the Earth using geometry and optical analysis of the sun's reflection in a well bore. He remotely sensed the Earth to be about 39,690 km (24,662 mi) around. He could then calculate ...
 
WBXH
Mon, 10 Jun 2013 04:26:45 -0700

But don't tell that to Eratosthenes. He essentially invented geography and calculated the date to June 11, 1184 B.C. But take that with a grain of salt because the dates of Eratosthenes' birth and death aren't even known and he may have purposely ...
 
FOX19
Mon, 10 Jun 2013 04:27:49 -0700

But don't tell that to Eratosthenes. He essentially invented geography and calculated the date to June 11, 1184 B.C. But take that with a grain of salt because the dates of Eratosthenes' birth and death aren't even known and he may have purposely ...
 
LiveScience.com
Mon, 20 May 2013 15:24:50 -0700

In 200 B.C., Eratosthenes created an algorithm that calculated prime numbers, known as the Sieve of Eratosthenes. This algorithm is one of the earliest algorithms ever written. Eratosthenes put numbers in a grid, and then crossed out all multiples of ...

EducationGuardian.co.uk (blog)

EducationGuardian.co.uk (blog)
Thu, 30 May 2013 01:48:07 -0700

It was here that Archimedes invented the screw-shaped water pump; Eratosthenes measured the diameter of the Earth, and Euclid discovered the rules of geometry. The Renaissance witnessed the exponential growth in libraries with the invention of printing.
 
CANOE
Mon, 03 Jun 2013 06:43:15 -0700

It places Archimedes in the rich context of Mediterranean culture, exploring his contacts with Alexandria where he studies sciences and with geographer and astronomer Eratosthenes. During a period of peace that lasted half a century, Archimedes became ...

Scientific Computing

Scientific Computing
Tue, 21 May 2013 08:53:50 -0700

To use the Sieve of Eratosthenes to find, say, all the primes up to 100, start with the number two, and cross out any higher number on the list that is divisible by two. Next move on to three, and cross out all the numbers divisible by three. Four is ...

Haberciniz

Haberciniz
Wed, 12 Jun 2013 23:16:03 -0700

Adana'da öğrenciler, Eratosthenes'in Mısır'da dünyanın çevresini ölçmek için yaptığı deneyi 2 bin 300 yıl sonra tekrarladı. Adana'da öğrenciler, Eratosthenes'in Mısır'da dünyanın çevresini ölçmek için yaptığı deneyi 2 bin 300 yıl sonra tekrarladı ...
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