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Theodosius'Spherics

From Wikipedia, the free encyclopedia
Ancient Greek spherical geometry treatise

TheSpherics (Greek:τὰ σφαιρικά,tà sphairiká) is a three-volumetreatise onspherical geometry written by theHellenistic mathematicianTheodosius of Bithynia in the 2nd or 1st century BC.

Book I and the first half of Book II establish basicgeometric constructions needed for spherical geometry using the tools ofEuclideansolid geometry, while the second half of Book II and Book III contain propositions relevant toastronomy as modeled by thecelestial sphere.

Primarily consisting of theorems which were known at least informally a couple centuries earlier, theSpherics was a foundational treatise for geometers and astronomers from its origin until the 19th century. It was continuously studied and copied in Greek manuscript for more than a millennium. It was translated intoArabic in the 9th century during theIslamic Golden Age, and thence translated intoLatinin 12th century Iberia, though the text and diagrams were somewhat corrupted. In the 16th century printed editions in Greek were published along with better translations into Latin.

History

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Several of the definitions and theorems in theSpherics were used without mention inEuclid'sPhenomena and two extant works byAutolycus concerning motions of the celestial sphere, all written about two centuries before Theodosius. It has been speculated that this tradition of Greek "spherics" – founded in the axiomatic system and using the methods of proof of solid geometry exemplified byEuclid'sElements but extended with additional definitions relevant to the sphere – may have originated in a now-unknown work byEudoxus, who probably established a two-sphere model of the cosmos (spherical Earth and celestial sphere) sometime between 370–340 BC.[1]

TheSpherics is a supplement to theElements, and takes its content for granted as a prerequisite. TheSpherics follows the general presentation style of theElements, with definitions followed by a list of theorems (propositions), each of which is first stated abstractly as prose, then restated withpoints lettered for the proof. It analysesspherical circles as flat circles lying in planes intersecting the sphere and provides geometric constructions for various configurations of spherical circles. Spherical distances and radii are treated as Euclidean distances in the surrounding 3-dimensional space. The relationship between planes is described in terms ofdihedral angle. As in theElements, there is no concept ofangle measure ortrigonometry per se.

This approach differs from other quantitative methods of Greek astronomy such as the analemma (orthographic projection),[2]stereographic projection, or trigonometry (a fledgling subject introduced by Theodosius' contemporaryHipparchus). It also differs from the approach taken inMenelaus'Spherics, a treatise of the same title written 3 centuries later, which treats the geometry of the sphereintrinsically, analyzing the inherent structure of the spherical surface and circles drawn on it rather than primarily treating it as a surface embedded in three-dimensional space.

Inlate antiquity, theSpherics was part of a collection of treatises now called theLittle Astronomy, an assortment of shorter works on geometry and astronomy building on Euclid'sElements. Other works in the collection includedAristarchus'On the Sizes and Distances, Autolycus'On Rising and Settings andOn the Moving Sphere, Euclid'sCatoptrics,Data,Optics, andPhenomena,Hypsicles'On Ascensions, Theodosius'On Geographic Places andOn Days and Nights, and Menelaus'Spherics. Often several of these were bound together in a single volume. During theIslamic Golden Age, the books in the collection were translated intoArabic, and with the addition of a few new works, were known as theMiddle Books, intended to fit between theElements andPtolemy'sAlmagest.[3]

Authoritative critical editions of the Greek text, compiled from several manuscripts, were made byHeiberg (1927) andCzinczenheim (2000).Sidoli & Thomas (2023) is an English translation by modern scholars.

Editions and translations

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1529 title page: EditorJohannes Vögelin [de] presents his work to the king

Notes

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  1. ^Berggren, John L. (1991)."The relation of Greek Spherics to early Greek astronomy". In Bowen, Alan C. (ed.).Science and Philosophy in Classical Greece. Garland. pp. 227–248.
    For more about the two-sphere model, see:
    Goldstein, Bernard R.; Bowen, Alan C. (1983). "A New View of Early Greek Astronomy".Isis.74 (3):330–340.JSTOR 232593.
  2. ^A description of the analemma method can be found in:
    Sidoli, Nathan (2005)."Heron'sDioptra 35 and analemma methods: An astronomical determination of the distance between two cities"(PDF).Centaurus.47 (3):236–258.doi:10.1111/j.1600-0498.2005.470304.x.
  3. ^Evans, James (1998).The History & Practice of Ancient Astronomy. Oxford University Press. "TheLittle Astronomy", pp. 89–91.ISBN 0-19-509539-1.
    Roughan, Christine (2023).The Little Astronomy and Middle Books between the 2nd and 13th Centuries CE: Transmissions of Astronomical Curricula (PhD thesis). New York University.

References

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