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| − | '''Eratosthenes''' ([[Greek language|Greek]] {{polytonic|Ἐρατοσθένης}}; [[276 B.C.E.]] - [[194 B.C.E.]]) was a [[Greeks|Greek]] [[mathematician]], [[geographer]] and [[astronomer]]. His contemporaries nicknamed him | + | '''Eratosthenes''' ([[Greek language|Greek]] {{polytonic|Ἐρατοσθένης}}; [[276 B.C.E.]] - [[194 B.C.E.]]) was a [[Greeks|Greek]] [[mathematics|mathematician]], [[geography|geographer]] and [[astronomy|astronomer]]. His contemporaries nicknamed him "beta" (Greek for "number two") because he supposedly proved himself to be the second in the ancient Mediterranean world in many fields. He was the first to use the word “geography” ("writing about the earth" in Greek) as the title of a treatise about the world. ''Geography'' also introduced the climatic concepts of torrid, temperate, and frigid zones. |
| + | |||
| + | Eratosthenes was noted for devising a system of latitude and longitude for the maps he created, and was the first person known to have calculated the circumference of the [[Earth]], using [[trigonometry]] and knowledge of the angle of elevation of the [[Sun]] at noon in Alexandria and Syene (now Aswan, Egypt). He calculated the earth’s circumference as 39,690 kilometers, an error of less than 1% (the actual distance is 40,008 kilometers). His calculation was accepted by scholars through the [[Middle Ages]]. | ||
==Life== | ==Life== | ||
| − | Eratosthenes was born in | + | Eratosthenes was born around 276 B.C.E. in Cyrene (in modern-day [[Libya]]), but lived and worked in [[Alexandria]], capital of [[Egypt|Ptolemaic Egypt]]. Eratosthenes studied at Alexandria and for some years in [[Athens]]. In 236 b.c.e. he was appointed by [[Ptolemy III of Egypt|Ptolemy III Euergetes I]] as librarian of the [[Library of Alexandria|Alexandrian library]], succeeding the first librarian, Zenodotos, in that post. While serving as head librarian, Eratosthenes wrote a comprehensive treatise about the world, called ''Geography''. This was the first use of the word “geography,” which literally means "writing about the earth" in Greek. ''Geography'' also introduced the climatic concepts of torrid, temperate, and frigid zones. |
| − | Eratosthenes studied at Alexandria and for some years in [[Athens]]. In | + | |
| + | Eratosthenes made several important contributions to [[mathematics]] and [[science]], and was a good friend to [[Archimedes]]. Around 255 b.c.e. he invented the armillary sphere, which was widely used until the invention of the orrery in the eighteenth century. In 194 b.c.e. he became blind, and a year later he supposedly starved himself to death. He never married and was reputedly known for his haughty character. | ||
| + | |||
| + | ==Thought and Works== | ||
| + | ===Measurement of the Earth=== | ||
| + | Eratosthenes is credited by Cleomedes in ''On the Circular Motions of the Celestial Bodies'' with having calculated the Earth's circumference around 240 B.C.E., using [[trigonometry]] and knowledge of the angle of elevation of the [[Sun]] at noon in Alexandria and Syene (now Aswan, Egypt). | ||
| − | + | [[Image:Iran.jpg|right|thumb|300px|Eratosthenes world map]] | |
| − | + | Eratosthenes heard of a deep well at Syene (near the Tropic of Cancer and modern Aswan) where sunlight only struck the bottom of the well on the summer solstice, and determined that he could discover the circumference of the earth. (Greek scholars knew that the earth was a a sphere). | |
| − | |||
| − | |||
| − | + | He knew that on the summer [[solstice]] at local noon in the town of Syene on the Tropic of Cancer, the sun would appear at the [[zenith]], directly overhead. He then measured the angle of the shadow in Alexandria on the solstice and found it to be 7°12' south. Assuming that the sun’s rays were parallel, Eratosthenes knew from geometry that that the measured angle equaled the measurement of the angle formed at the earth’s center by two lines passing through Alexandria and Syene. Assuming that Alexandria was due [[north]] of Syene he concluded that the distance from Alexandria to Syene must be 7.2/360 of the total circumference of the Earth. The distance between the cities was known from camel caravans to be about 5000 ''stadia'', approximately 800 km. Eratosthenes established 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 no longer known (the common Attic ''stadion'' was about 185 m), but it is generally believed that the circumference calculated by Eratosthenes corresponds to 39,690 kilometers. The estimate is over 99% of the actual distance of 40,008 km. | |
| − | Eratosthenes' | + | Although Eratosthenes' method was well founded, the accuracy of his calculation was inherently limited. The accuracy of Eratosthenes' measurement would have been reduced by the fact that Syene is not precisely on the Tropic of Cancer, is not directly south of Alexandria, and that the Sun appears as a disk located at a finite distance from the Earth instead of as a point source of light at an infinite distance. There are other possible sources of experimental error; in antiquity, angles could only be measured to within about a quarter of a degree, and overland distance measurements were even less reliable. The accuracy of the result of Eratosthenes' calculation is surprising. |
| − | ==Other | + | Eratosthenes' experiment was highly regarded at the time, and his estimate of the Earth’s size was accepted for hundreds of years afterwards. About 150 years later, the Greek geographer [[Posidonius]] thought Eratosthenes' circumference was too large, and used a similar method to calculated the circumference as 18,000 miles, 7,000 miles too short. During the [[Middle Ages]], most scholars accepted Eratosthenes' circumference, though [[Christopher Columbus]] used Posidonius' shorter measurement to convince his supporters that he could quickly reach Asia by sailing west from [[Europe]]. |
| + | ==Other Contributions== | ||
Eratosthenes' other contributions include: | Eratosthenes' other contributions include: | ||
| − | * The | + | * The Sieve of Eratosthenes as a way of finding [[prime number]]s. The numbers from 1 to 400 are written in a table, with the numbers 1-20 across the top row. Starting with the first prime number, 2, all multiples of 2 are crossed off. The first number following 2 that is not crossed off will be the next prime number, 3. All multiples of 3 are crossed off, and so on. When all multiples in the top row have been crossed off, the table contains only prime numbers. |
| − | * Possibly, the measurement of the Sun | + | * Possibly, the measurement of the distance from the Sun to the Earth, now called the astronomical unit and of the distance to the [[Moon]] (see below). |
| − | * The measurement of the | + | * The measurement of the inclination of the ecliptic at 23.5 degrees, with an angle error of 7'. |
| − | * | + | * A star catalogue containing 675 stars, which was not preserved. |
| − | * A map of the [[Nile]] | + | * A map of the route of the River [[Nile]] as far as [[Khartoum]]. |
* A map of the entire known world, from the [[British Isles]] to [[Ceylon]], and from the [[Caspian Sea]] to [[Ethiopia]]. Only [[Hipparchus (astronomer)|Hipparchus]], [[Strabo]], and [[Ptolemy]] were able to make more accurate maps in the classical and post-classical world. | * A map of the entire known world, from the [[British Isles]] to [[Ceylon]], and from the [[Caspian Sea]] to [[Ethiopia]]. Only [[Hipparchus (astronomer)|Hipparchus]], [[Strabo]], and [[Ptolemy]] were able to make more accurate maps in the classical and post-classical world. | ||
| − | * A number of works on | + | * A number of works on theater and [[ethics]] |
* A calendar with leap years, in which he attempted to work out the precise dates and relations of various events in politics and literature from his day back to the [[Trojan War]]. | * A calendar with leap years, in which he attempted to work out the precise dates and relations of various events in politics and literature from his day back to the [[Trojan War]]. | ||
==The mysterious astronomical distances== | ==The mysterious astronomical distances== | ||
| − | [[Eusebius of Caesarea]] in his '' | + | [[Eusebius of Caesarea]] in his ''Preparation for the Gospel|Praeparatio Evangelica'' includes a brief chapter of three sentences on celestial distances ([http://www.tertullian.org/fathers/eusebius_pe_15_book15.htm Book XV], Chapter 53). He states simply that Eratosthenes found the distance to the sun to be "σταδίων μυριάδας τετρακοσίας και οκτωκισμυρίας" (literally "of stadia myriads 400 and 80000") 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 80000 or "400 and 80000" myriad. |
| − | This testimony of Eusebius is dismissed by the scholarly | + | This testimony of Eusebius is dismissed by the scholarly ''Dictionary of Scientific Biography''. The distance Eusebius quotes for the moon is much too low (about 144,000 km); Eratosthenes should have been able to be more accurate than this since he knew the size of the earth and [[Aristarchos of Samos]] had already found the ratio of the moon's distance to the size of the earth. But if what Eusebius wrote was pure fiction, then it is difficult to explain the fact that, using the Greek ''stadium'' of 185 metres, the figure of 804 million ''stadia'' that he quotes for the distance to the sun comes to 149 million kilometres. The difference between this and the modern accepted value is less than 1%. |
==Works== | ==Works== | ||
| − | * ''On the Measurement of the Earth'' (lost, summarized by | + | * ''On the Measurement of the Earth'' (lost, summarized by Cleomedes) |
* ''Geographica'' (lost, criticized by [[Strabo]]) | * ''Geographica'' (lost, criticized by [[Strabo]]) | ||
| − | * ''Arsinoe'' (a memoir of queen | + | * ''Arsinoe'' (a memoir of queen Arsinoe III of Egypt; lost; quoted by [[Athenaeus]] in the ''Deipnosophistae'') |
| − | * A fragmentary collection of [[Hellenistic]] myths about the [[constellation]]s, called '' | + | * A fragmentary collection of [[ancient Greece|Hellenistic]] myths about the [[constellation]]s, called ''Catasterismi'' (''Katasterismoi''), was attributed to Eratosthenes, perhaps to add to its credibility. |
==Named after Eratosthenes== | ==Named after Eratosthenes== | ||
| − | * | + | * Sieve of Eratosthenes |
| − | * | + | * Eratosthenes crater on the [[Moon]] |
| − | * | + | * Eratosthenian period in the [[lunar geologic timescale]] |
| − | * | + | * Eratosthenes Seamount in the eastern Mediterranean Sea |
==See also== | ==See also== | ||
* [[History of geodesy]] | * [[History of geodesy]] | ||
| − | == | + | ==References== |
| + | *Boyer, Carl B.; Merzbach, Uta C. A history of mathematics. New York : Wiley, 1991. ISBN: 0471543977 : 9780471543978 | ||
| + | *Ferguson, Kitty. Measuring the universe : our historic quest to chart the horizons of space and time.New York : Walker and Company, 1999. ISBN: 0802713513 9780802713513 | ||
| + | *Fraser, P M. Eratosthenes of Cyrene. London, Oxford University Press, 1971 ISBN: 0197256619 9780197256619 | ||
* Lasky, Kathryn. ''The Librarian Who Measured the Earth''. New York: Little, Brown and Company, 1994. ISBN 0-316-51526-4. An illustrated biography for children focusing on the measurement of the earth. Kevin Hawkes, illustrator. | * Lasky, Kathryn. ''The Librarian Who Measured the Earth''. New York: Little, Brown and Company, 1994. ISBN 0-316-51526-4. An illustrated biography for children focusing on the measurement of the earth. Kevin Hawkes, illustrator. | ||
| + | |||
| + | |||
* {{cite encyclopedia|author=J J O'Connor and E F Robertson|url= http://www-history.mcs.st-andrews.ac.uk/Biographies/Eratosthenes.html|encyclopedia=MacTutor|title=Eratosthenes of Cyrene|publisher=School of Mathematics and Statistics University of St Andrews Scotland|date=January 1999}} | * {{cite encyclopedia|author=J J O'Connor and E F Robertson|url= http://www-history.mcs.st-andrews.ac.uk/Biographies/Eratosthenes.html|encyclopedia=MacTutor|title=Eratosthenes of Cyrene|publisher=School of Mathematics and Statistics University of St Andrews Scotland|date=January 1999}} | ||
* {{cite book|author=E P Wolfer|title=Eratosthenes von Kyrene als Mathematiker und Philosoph|publisher=Groningen-Djakarta|date=1954}} | * {{cite book|author=E P Wolfer|title=Eratosthenes von Kyrene als Mathematiker und Philosoph|publisher=Groningen-Djakarta|date=1954}} | ||
| Line 81: | Line 92: | ||
* [http://www.christopherhenden.com/previously/primenumbers/ Eratosthenes' sieve explored and visualised in Flash] | * [http://www.christopherhenden.com/previously/primenumbers/ Eratosthenes' sieve explored and visualised in Flash] | ||
* [http://www.quitebasic.com/prj/math/eratosthenes/ Eratosthenes' sieve in classic BASIC all-web based interactive programming environment] | * [http://www.quitebasic.com/prj/math/eratosthenes/ Eratosthenes' sieve in classic BASIC all-web based interactive programming environment] | ||
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{{Persondata | {{Persondata | ||
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|ALTERNATIVE NAMES=Beta | |ALTERNATIVE NAMES=Beta | ||
|SHORT DESCRIPTION=Greek mathematician, astronomer, and geographer. | |SHORT DESCRIPTION=Greek mathematician, astronomer, and geographer. | ||
| − | |DATE OF BIRTH= | + | |DATE OF BIRTH=276 b.c.e. |
| − | |PLACE OF BIRTH= | + | |PLACE OF BIRTH= Cyrene (in modern-day [[Libya]]) |
| − | |DATE OF DEATH= | + | |DATE OF DEATH= 194 b.c.e. |
| − | |PLACE OF DEATH=[[ | + | |PLACE OF DEATH=[[Egypt|Ptolemaic]] [[Alexandria]] |
}} | }} | ||
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Revision as of 23:46, 24 February 2007
Eratosthenes (Greek Ἐρατοσθένης; 276 B.C.E. - 194 B.C.E.) was a Greek mathematician, geographer and astronomer. His contemporaries nicknamed him "beta" (Greek for "number two") because he supposedly proved himself to be the second in the ancient Mediterranean world in many fields. He was the first to use the word “geography” ("writing about the earth" in Greek) as the title of a treatise about the world. Geography also introduced the climatic concepts of torrid, temperate, and frigid zones.
Eratosthenes was noted for devising a system of latitude and longitude for the maps he created, and was the first person known to have calculated the circumference of the Earth, using trigonometry and knowledge of the angle of elevation of the Sun at noon in Alexandria and Syene (now Aswan, Egypt). He calculated the earth’s circumference as 39,690 kilometers, an error of less than 1% (the actual distance is 40,008 kilometers). His calculation was accepted by scholars through the Middle Ages.
Life
Eratosthenes was born around 276 B.C.E. in Cyrene (in modern-day Libya), but lived and worked in Alexandria, capital of Ptolemaic Egypt. Eratosthenes studied at Alexandria and for some years in Athens. In 236 B.C.E. he was appointed by Ptolemy III Euergetes I as librarian of the Alexandrian library, succeeding the first librarian, Zenodotos, in that post. While serving as head librarian, Eratosthenes wrote a comprehensive treatise about the world, called Geography. This was the first use of the word “geography,” which literally means "writing about the earth" in Greek. Geography also introduced the climatic concepts of torrid, temperate, and frigid zones.
Eratosthenes made several important contributions to mathematics and science, and was a good friend to Archimedes. Around 255 B.C.E. he invented the armillary sphere, which was widely used until the invention of the orrery in the eighteenth century. In 194 B.C.E. he became blind, and a year later he supposedly starved himself to death. He never married and was reputedly known for his haughty character.
Thought and Works
Measurement of the Earth
Eratosthenes is credited by Cleomedes in On the Circular Motions of the Celestial Bodies with having calculated the Earth's circumference around 240 B.C.E., using trigonometry and knowledge of the angle of elevation of the Sun at noon in Alexandria and Syene (now Aswan, Egypt).
Eratosthenes heard of a deep well at Syene (near the Tropic of Cancer and modern Aswan) where sunlight only struck the bottom of the well on the summer solstice, and determined that he could discover the circumference of the earth. (Greek scholars knew that the earth was a a sphere).
He knew that on the summer solstice at local noon in the town of Syene on the Tropic of Cancer, the sun would appear at the zenith, directly overhead. He then measured the angle of the shadow in Alexandria on the solstice and found it to be 7°12' south. Assuming that the sun’s rays were parallel, Eratosthenes knew from geometry that that the measured angle equaled the measurement of the angle formed at the earth’s center by two lines passing through Alexandria and Syene. Assuming that Alexandria was due north of Syene he concluded that the distance from Alexandria to Syene must be 7.2/360 of the total circumference of the Earth. The distance between the cities was known from camel caravans to be about 5000 stadia, approximately 800 km. Eratosthenes established 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 no longer known (the common Attic stadion was about 185 m), but it is generally believed that the circumference calculated by Eratosthenes corresponds to 39,690 kilometers. The estimate is over 99% of the actual distance of 40,008 km.
Although Eratosthenes' method was well founded, the accuracy of his calculation was inherently limited. The accuracy of Eratosthenes' measurement would have been reduced by the fact that Syene is not precisely on the Tropic of Cancer, is not directly south of Alexandria, and that the Sun appears as a disk located at a finite distance from the Earth instead of as a point source of light at an infinite distance. There are other possible sources of experimental error; in antiquity, angles could only be measured to within about a quarter of a degree, and overland distance measurements were even less reliable. The accuracy of the result of Eratosthenes' calculation is surprising.
Eratosthenes' experiment was highly regarded at the time, and his estimate of the Earth’s size was accepted for hundreds of years afterwards. About 150 years later, the Greek geographer Posidonius thought Eratosthenes' circumference was too large, and used a similar method to calculated the circumference as 18,000 miles, 7,000 miles too short. During the Middle Ages, most scholars accepted Eratosthenes' circumference, though Christopher Columbus used Posidonius' shorter measurement to convince his supporters that he could quickly reach Asia by sailing west from Europe.
Other Contributions
Eratosthenes' other contributions include:
- The Sieve of Eratosthenes as a way of finding prime numbers. The numbers from 1 to 400 are written in a table, with the numbers 1-20 across the top row. Starting with the first prime number, 2, all multiples of 2 are crossed off. The first number following 2 that is not crossed off will be the next prime number, 3. All multiples of 3 are crossed off, and so on. When all multiples in the top row have been crossed off, the table contains only prime numbers.
- Possibly, the measurement of the distance from the Sun to the Earth, now called the astronomical unit and of the distance to the Moon (see below).
- The measurement of the inclination of the ecliptic at 23.5 degrees, with an angle error of 7'.
- A star catalogue containing 675 stars, which was not preserved.
- A map of the route of the River Nile as far as Khartoum.
- A map of the entire known world, from the British Isles to Ceylon, and from the Caspian Sea to Ethiopia. Only Hipparchus, Strabo, and Ptolemy were able to make more accurate maps in the classical and post-classical world.
- A number of works on theater and ethics
- A calendar with leap years, in which he attempted to work out the precise dates and relations of various events in politics and literature from his day back to the Trojan War.
The mysterious astronomical distances
Eusebius of Caesarea in his Preparation for the Gospel|Praeparatio 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 και οκτωκισμυρίας" (literally "of stadia myriads 400 and 80000") 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 80000 or "400 and 80000" myriad.
This testimony of Eusebius is dismissed by the scholarly Dictionary of Scientific Biography. The distance Eusebius quotes for the moon is much too low (about 144,000 km); Eratosthenes should have been able to be more accurate than this since he knew the size of the earth and Aristarchos of Samos had already found the ratio of the moon's distance to the size of the earth. But if what Eusebius wrote was pure fiction, then it is difficult to explain the fact that, using the Greek stadium of 185 metres, the figure of 804 million stadia that he quotes for the distance to the sun comes to 149 million kilometres. The difference between this and the modern accepted value is less than 1%.
Works
- On the Measurement of the Earth (lost, summarized by Cleomedes)
- Geographica (lost, criticized by Strabo)
- Arsinoe (a memoir of queen Arsinoe III of Egypt; lost; quoted by Athenaeus in the Deipnosophistae)
- A fragmentary collection of Hellenistic myths about the constellations, called Catasterismi (Katasterismoi), was attributed to Eratosthenes, perhaps to add to its credibility.
Named after Eratosthenes
- Sieve of Eratosthenes
- Eratosthenes crater on the Moon
- Eratosthenian period in the lunar geologic timescale
- Eratosthenes Seamount in the eastern Mediterranean Sea
See also
- History of geodesy
ReferencesISBN links support NWE through referral fees
- Boyer, Carl B.; Merzbach, Uta C. A history of mathematics. New York : Wiley, 1991. ISBN: 0471543977 : 9780471543978
- Ferguson, Kitty. Measuring the universe : our historic quest to chart the horizons of space and time.New York : Walker and Company, 1999. ISBN: 0802713513 9780802713513
- Fraser, P M. Eratosthenes of Cyrene. London, Oxford University Press, 1971 ISBN: 0197256619 9780197256619
- Lasky, Kathryn. The Librarian Who Measured the Earth. New York: Little, Brown and Company, 1994. ISBN 0-316-51526-4. An illustrated biography for children focusing on the measurement of the earth. Kevin Hawkes, illustrator.
- J J O'Connor and E F Robertson. (January 1999). "Eratosthenes of Cyrene". MacTutor. School of Mathematics and Statistics University of St Andrews Scotland.
- E P Wolfer (1954). Eratosthenes von Kyrene als Mathematiker und Philosoph. Groningen-Djakarta.
- A V Dorofeeva (1988). Eratosthenes (ca. 276-194 B.C.E.). Mat. v Shkole (4): i.
- J Dutka (1993). Eratosthenes' measurement of the Earth reconsidered. Arch. Hist. Exact Sci. 46 (1): 55 – 66.
- B A El'natanov (1983). A brief outline of the history of the development of the sieve of Eratosthenes. Istor.-Mat. Issled. 27: 238 – 259.
- D H Fowler (1983). Eratosthenes' ratio for the obliquity of the ecliptic. Isis 74 (274): 556 – 562.
- B R Goldstein (1984). Eratosthenes on the "measurement" of the earth. Historia Math. 11 (4): 411 – 416.
- E Gulbekian (1987). The origin and value of the stadion unit used by Eratosthenes in the third century B.C.E. Arch. Hist. Exact Sci. 37 (4): 359 – 363.
- G Knaack (1907). Eratosthenes. Pauly-Wissowa VI: 358 – 388.
- F Manna (1986). The Pentathlos of ancient science, Eratosthenes, first and only one of the "primes". Atti Accad. Pontaniana (N.S.) 35: 37 – 44.
- A Muwaf and A N Philippou (1981). An Arabic version of Eratosthenes writing on mean proportionals. J. Hist. Arabic Sci. 5 (1 – 2): 174 – 147.
- D Rawlins (1982). Eratosthenes' geodest unraveled : was there a high-accuracy Hellenistic astronomy. Isis 73: 259 – 265.
- D Rawlins (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.
- C M Taisbak (1984). Eleven eighty-thirds. Ptolemy's reference to Eratosthenes in Almagest I.12. Centaurus 27 (2): 165 – 167.
External links
- Bernhardy, Gottfried: "Eratosthenica" Berlin 1822 Reprinted Osnabruck 1968 (German text)
- John J. O'Connor and Edmund F. Robertson. Eratosthenes at the MacTutor archive
- Eratosthenes' sieve in Javascript
- Eratosthenes' sieve as a simple algorithm
- About Eratosthenes' methods, including a Java applet
- How to measure the earth with Eratosthenes' method
- How the Greeks estimated the distances to the moon and sun
- Eratosthenes on PBS.org
- Inter-collegiate project for measuring the earth with Eratosthenes' method
- Measuring the earth with Eratosthenes' method
- List of ancient Greek mathematecians and contemporaries of Eratosthenes
- New Advent Encyclopedia article on the Library of Alexandria
- Eratosthenes' sieve explored and visualised in Flash
- Eratosthenes' sieve in classic BASIC all-web based interactive programming environment
| Persondata | |
|---|---|
| NAME | Erastosthenes |
| ALTERNATIVE NAMES | Beta |
| SHORT DESCRIPTION | Greek mathematician, astronomer, and geographer. |
| DATE OF BIRTH | 276 B.C.E. |
| PLACE OF BIRTH | Cyrene (in modern-day Libya) |
| DATE OF DEATH | 194 B.C.E. |
| PLACE OF DEATH | Ptolemaic Alexandria |
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