Eratosthenes
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Mathematical Discourse in Philosophical Authors: Examples from Theon of Smyrna and Cleomedes on Mathematical Astronomy
Mathematical discourse in philosophical authors: Examples from Theon of Smyrna and Cleomedes on mathematical astronomy Nathan Sidoli Introduction Ancient philosophers and other intellectuals often mention the work of mathematicians, al- though the latter rarely return the favor.1 The most obvious reason for this stems from the im- personal nature of mathematical discourse, which tends to eschew any discussion of personal, or lived, experience. There seems to be more at stake than this, however, because when math- ematicians do mention names they almost always belong to the small group of people who are known to us as mathematicians, or who are known to us through their mathematical works.2 In order to be accepted as a member of the group of mathematicians, one must not only have mastered various technical concepts and methods, but must also have learned how to express oneself in a stylized form of Greek prose that has often struck the uninitiated as peculiar.3 Be- cause of the specialized nature of this type of intellectual activity, in order to gain real mastery it was probably necessary to have studied it from youth, or to have had the time to apply oneself uninterruptedly.4 Hence, the private nature of ancient education meant that there were many educated individuals who had not mastered, or perhaps even been much exposed to, aspects of ancient mathematical thought and practice that we would regard as rather elementary (Cribiore 2001; Sidoli 2015). Starting from at least the late Hellenistic period, and especially during the Imperial and Late- Ancient periods, some authors sought to address this situation in a variety of different ways— such as discussing technical topics in more elementary modes, rewriting mathematical argu- ments so as to be intelligible to a broader audience, or incorporating mathematical material di- rectly into philosophical curricula. -
Implementing Eratosthenes' Discovery in the Classroom: Educational
Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention Nicolas Decamp, C. de Hosson To cite this version: Nicolas Decamp, C. de Hosson. Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention. Science and Education, Springer Verlag, 2012, 21 (6), pp.911-920. 10.1007/s11191-010-9286-3. hal-01663445 HAL Id: hal-01663445 https://hal.archives-ouvertes.fr/hal-01663445 Submitted on 18 Dec 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Sci & Educ DOI 10.1007/s11191-010-9286-3 Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention Nicolas De´camp • Ce´cile de Hosson Ó Springer Science+Business Media B.V. 2010 Abstract This paper presents a critical analysis of the accepted educational use of the method performed by Eratosthenes to measure the circumference of Earth which is often considered as a relevant means of dealing with issues related to the nature of science and its history. This method relies on a number of assumptions among which the parallelism of sun rays. The assumption of sun rays parallelism (if it is accurate) does not appear spontaneous for students who consider sun rays to be divergent. -
Astronomy and Hipparchus
CHAPTER 9 Progress in the Sciences: Astronomy and Hipparchus Klaus Geus Introduction Geography in modern times is a term which covers several sub-disciplines like ecology, human geography, economic history, volcanology etc., which all con- cern themselves with “space” or “environment”. In ancient times, the definition of geography was much more limited. Geography aimed at the production of a map of the oikoumene, a geographer was basically a cartographer. The famous scientist Ptolemy defined geography in the first sentence of his Geographical handbook (Geog. 1.1.1) as “imitation through drafting of the entire known part of the earth, including the things which are, generally speaking, connected with it”. In contrast to chorography, geography uses purely “lines and label in order to show the positions of places and general configurations” (Geog. 1.1.5). Therefore, according to Ptolemy, a geographer needs a μέθοδος μαθεματική, abil- ity and competence in mathematical sciences, most prominently astronomy, in order to fulfil his task of drafting a map of the oikoumene. Given this close connection between geography and astronomy, it is not by default that nearly all ancient “geographers” (in the limited sense of the term) stood out also as astronomers and mathematicians: Among them Anaximander, Eudoxus, Eratosthenes, Hipparchus, Poseidonius and Ptolemy are the most illustrious. Apart from certain topics like latitudes, meridians, polar circles etc., ancient geography also took over from astronomy some methods like the determina- tion of the size of the earth or of celestial and terrestrial distances.1 The men- tioned geographers Anaximander, Eudoxus, Hipparchus, Poseidonius and Ptolemy even constructed instruments for measuring, observing and calculat- ing like the gnomon, sundials, skaphe, astrolabe or the meteoroscope.2 1 E.g., Ptolemy (Geog. -
1.1 Eratosthenes Measures the Earth (Copyright: Bryan Dorner All Rights Reserved)
1.1 Eratosthenes Measures the Earth (Copyright: Bryan Dorner all rights reserved) How big is the Earth? The mathematician Eratosthenes (276-195 BCE) lived in the city of Alexandria in northern Egypt near the place where the Nile river empties into the Mediterranean. Eratosthenes was chief librarian at the Alexandria museum and one of the foremost scholars of the day - second only to Archimedes (who many consider one of the two or three best mathematicians ever to have lived). The city of Alexandria had been founded about one hundred years earlier by Alexander the Great whose conquests stretched from Egypt, through Syria, Babylonia, and Persia to northern India and central Asia. As the Greeks were also called Hellenes, the resulting empire was known as the Hellenistic empire and the following period in which Greek culture was dominant is called the Hellenistic age. The Hellenistic age saw a considerable exchange of culture between the conquering Greeks and the civilizations of the lands they controlled. It is from about this period that the predominantly geometric mathematics of the Greeks shows a computational aspect borrowed from the Babylonians. Some of the best mathematics we have inherited comes from just such a blend of contributions from diverse cultures. Eratosthenes is known for his simple but accurate measurement of the size of the earth. The imprint of Babylon (modern Iraq) as well as Greece can be seen in his method. He did not divide the arc of a circle into 360 parts as the Babylonians did, but into 60 equal parts. Still, the use of 60 reveals the influence of the Babylonian number system - the sexagesimal system - which was based on the number 60 in the same way ours is based on the number 10. -
9 · the Growth of an Empirical Cartography in Hellenistic Greece
9 · The Growth of an Empirical Cartography in Hellenistic Greece PREPARED BY THE EDITORS FROM MATERIALS SUPPLIED BY GERMAINE AUJAe There is no complete break between the development of That such a change should occur is due both to po cartography in classical and in Hellenistic Greece. In litical and military factors and to cultural developments contrast to many periods in the ancient and medieval within Greek society as a whole. With respect to the world, we are able to reconstruct throughout the Greek latter, we can see how Greek cartography started to be period-and indeed into the Roman-a continuum in influenced by a new infrastructure for learning that had cartographic thought and practice. Certainly the a profound effect on the growth of formalized know achievements of the third century B.C. in Alexandria had ledge in general. Of particular importance for the history been prepared for and made possible by the scientific of the map was the growth of Alexandria as a major progress of the fourth century. Eudoxus, as we have seen, center of learning, far surpassing in this respect the had already formulated the geocentric hypothesis in Macedonian court at Pella. It was at Alexandria that mathematical models; and he had also translated his Euclid's famous school of geometry flourished in the concepts into celestial globes that may be regarded as reign of Ptolemy II Philadelphus (285-246 B.C.). And it anticipating the sphairopoiia. 1 By the beginning of the was at Alexandria that this Ptolemy, son of Ptolemy I Hellenistic period there had been developed not only the Soter, a companion of Alexander, had founded the li various celestial globes, but also systems of concentric brary, soon to become famous throughout the Mediter spheres, together with maps of the inhabited world that ranean world. -
Geminus and the Isia
CORE Metadata, citation and similar papers at core.ac.uk Provided by DSpace at New York University GEMINUS AND THE ISIA ALEXANDER JONES T HE torical Greek interest, scientific including a lost writer treatise onGeminus the foundations wrote of several works of his- mathematics and an extant book on astronomy known as the Isagoge ("Introduction to the Phenomena"). The Isagoge is important to us as a witness to a stage of Greek astronomy that was both less advanced and less homogeneous in method than Ptolemy's. Approximate knowledge of when its author lived would be useful in several respects, for exam- ple in tracing the diffusion of elements originating in Babylonian lunar theory and in Hipparchus' work. Recent scholarship frequently cites Neugebauer's dating of Geminus to about A.D. 50, which has largely superseded the dating to the first half of the first century B.C. that used to be widely accepted.' Both dates derive, oddly enough, from analysis of the same passage in the Isagoge. The purpose of this note is to eluci- date the chronological issues, and to present documentary evidence that decisively establishes the earlier dating. The limits established by ancient citations are not very narrow. Isa- goge 4 mentions Hipparchus as an authority concerning constellations, and though Geminus does not say so, the lengths of the astronomical seasons listed in Isagoge I are the values that Hipparchus had used in deriving a model for the sun's motion. These passages cannot have been written before the 140s B.C. Moreover, Alexander of Aphrodisias (In Arist. -
10 · Greek Cartography in the Early Roman World
10 · Greek Cartography in the Early Roman World PREPARED BY THE EDITORS FROM MATERIALS SUPPLIED BY GERMAINE AUJAe The Roman republic offers a good case for continuing to treat the Greek contribution to mapping as a separate CONTINUITY AND CHANGE IN THEORETICAL strand in the history ofclassical cartography. While there CARTOGRAPHY: POLYBIUS, CRATES, was a considerable blending-and interdependence-of AND HIPPARCHUS Greek and Roman concepts and skills, the fundamental distinction between the often theoretical nature of the Greek contribution and the increasingly practical uses The extent to which a new generation of scholars in the for maps devised by the Romans forms a familiar but second century B.C. was familiar with the texts, maps, satisfactory division for their respective cartographic in and globes of the Hellenistic period is a clear pointer to fluences. Certainly the political expansion of Rome, an uninterrupted continuity of cartographic knowledge. whose domination was rapidly extending over the Med Such knowledge, relating to both terrestrial and celestial iterranean, did not lead to an eclipse of Greek influence. mapping, had been transmitted through a succession of It is true that after the death of Ptolemy III Euergetes in well-defined master-pupil relationships, and the pres 221 B.C. a decline in the cultural supremacy of Alex ervation of texts and three-dimensional models had been andria set in. Intellectual life moved to more energetic aided by the growth of libraries. Yet this evidence should centers such as Pergamum, Rhodes, and above all Rome, not be interpreted to suggest that the Greek contribution but this promoted the diffusion and development of to cartography in the early Roman world was merely a Greek knowledge about maps rather than its extinction. -
Math 105 History of Mathematics
Math 105 History of Mathematics Second Test Prof. D. Joyce, November, 2010 You may refer to one sheet of notes on this test, and you may use a calculator if you like. Points for each problem are in square brackets. Start your answers to each problem on a separate page page of the bluebook. Please write or print clearly. Problem 1. Essay. [25] Select one of the two topics A or B. Please think about these topics and make an outline before you begin writing. You will be graded on how well you present your ideas as well as your ideas themselves. Each essay should be relatively short|one to three written pages. There should be no fluff in your essays. Make your essays well-structured and your points as clearly as you can. Topic A. One quality of the mathematics of ancient India and China, on the one hand, which differs from that of Greek and Islamic/Arabic mathematicians, on the other hand, is formalism. Here formalism means careful definitions and clear proofs. (Another aspect of for- malism which doesn't have much role here is symbolism, as in symbolic algebra which wasn't developed until later.) Explain what this difference is and describe the role of formalism in the development of mathematics in those cultures. Topic B. Trigonometry was part of the mathematical knowledge in several regions: Greece, India, China, and Islamic/Arabic. Briefly describe the trigonometry of each in a sentence or two. Describe how knowledge of trigonometry passed among these cultures. Problem 2. [21; 7 points each part] On the Chinese algorithm for solving polynomial equations. -
4. Alexandrian Mathematics After Euclid — I I I
4. Alexandrian mathematics after Euclid — I I I Due to the length of this unit , it has been split into three parts . This is the final part , and it deals with other Greek mathematicians and scientists from the period . The previously described works or Archimedes and Apollonius represent the deepest and most original discoveries in Greek geometry that have been passed down to us over the ages (there were probably others that did not survive) , and indeed they pushed the classical methods to their limits . More powerful tools would be needed to make further advances , and these were not developed until the 17 th century . Much of the subsequent activity in ancient Greek mathematics was more directed towards developing the trigonometry and spherical geometry needed for observational astronomy and studying questions of an arithmetic nature . At the beginning of this period there was also a resurgence of activity in astronomy and its related mathematics which continued the tradition of Babylonian mathematics in the Seleucid Empire ( c. 300 B.C.E. – 63 B.C.E) , and although there must have been some interaction , its precise extent is unclear . Eratosthenes of Cyrene Eratosthenes (276 – 197 B.C.E.) probably comes as close as anyone from this period to reaching the levels attained by Euclid , Archimedes and Apollonius . He is probably best known for applying geometric and trigonometric ideas to estimate the diameter of the earth to a fairly high degree of accuracy ; this work is summarized on pages 186 – 188 of Burton . Within mathematics itself , his main achievement was to give a systematic method for finding all primes which is known as the sieve of Eratosthenes. -
Eratosthenes (276-194 BCE)
Makers of Mathematics Eratosthenes (276-194 BCE) Eratosthenes was born in Cyrene (modern- day Libya). He was to become the third chief librarian of the Great Library of Alexandria, the centre of science and learning in the ancient world. It seems that he was not regarded by his contemporaries as a top rank mathematician. Perhaps, but even so most of us would like to have achievements like his to our name! Eratosthenes interests were very broad. He wrote about the philosophy of Plato, music and ethics. He also produced literary works about the theatre. We do not have all of his writings so that some of our knowledge comes from what others said about him or from quotations found in other authors. Eratosthenes is most famous today for two things (1) his 'sieve' for finding prime numbers, and (2) his calculation of the Earth's circumference. The sieve. Write down the numbers you want to 2 3 4 5 investigate in a table. Remove 1 since it is not a prime. 6 7 8 9 10 The first prime is 2. Remove all the multiples of 2 11 12 13 14 15 (shown in green). 16 17 18 19 20 The next number is 21 22 23 24 25 26 27 28 29 30 3. Remove all its Sunlight Shadow remaining multiples (shown in blue). The next number is 5. Remove all its remaining multiples (red). There are no more multiples to remove so the remaining numbers are the primes. Earth's surface Eratosthenes calculated the Earth's circumference to be 250,000 stadia. -
Ptolemy's Maltese Co-Ordinates
Ptolemy's Maltese Co-ordinates: A Re assessment - Frank Ventura On Inspiration - Michael Zammit The Philosophical Problem in Dostoevsky's Crime and Punishment - Paul Spiteri ~ Purgation in Plato and Dante - Charles Briffa Jfhe Heritage of Rome - Louis J. Scerri The Mediterranean Story-Telling Sailor: Odysseus and Sinbad - Peter Serracino Inglott General and Analytic Indexes Vols I - V Main Library Class Mark MIG No. of Volumes 111111111111111111111111111111111111111111111 *432916* 'Advanced The New I). copy, cents; numbers), Lm3.25,0, postage included. Back numbers, 55c. Other countries: please write for details. Volume V 1988 Number 6 CONTENTS Ptolemy's Maltese co-ordinates: A re-assessment Frank Ventura ......................... , ........................................................... 253 On Inspiration Michael Zammit ................................................................................... 270 The Philosophical Problem in Dostoevsky's Crime and Punishment Paul Spiteri ........................................................................................ 273 Purgation in Plato and Dante Charles Briffa ..................................................................................... 281 The Heritage of Rome Lous 1. Scerri ........................................................................... : ......... 285 The Mediterranean Story-Telling Sailor: Odysseus and Sinbad Peter Serracino Inglott .......................................................................... 289 Author and Analytical Title Indexes Vols -
The Two Earths of Eratosthenes Author(S): Christián Carlos Carman and James Evans Source: Isis, Vol
University of Puget Sound Sound Ideas All Faculty Scholarship Faculty Scholarship 3-2015 The woT Earths of Eratosthenes James Evans University of Puget Sound, [email protected] Christián Carlos Carman Buenos Aires, Argentina Follow this and additional works at: http://soundideas.pugetsound.edu/faculty_pubs Citation Christián C. Carman and James Evans, “The wT o Earths of Eratosthenes,” Isis 106 (2015), 1-16. This Article is brought to you for free and open access by the Faculty Scholarship at Sound Ideas. It has been accepted for inclusion in All Faculty Scholarship by an authorized administrator of Sound Ideas. For more information, please contact [email protected]. The Two Earths of Eratosthenes Author(s): Christián Carlos Carman and James Evans Source: Isis, Vol. 106, No. 1 (March 2015), pp. 1-16 Published by: The University of Chicago Press on behalf of The History of Science Society Stable URL: http://www.jstor.org/stable/10.1086/681034 . Accessed: 08/12/2015 15:41 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. The University of Chicago Press and The History of Science Society are collaborating with JSTOR to digitize, preserve and extend access to Isis.