Almagest

The Almagest /ˈælmədʒɛst/ is a 2nd-century mathematical and astronomical treatise on the apparent motions of the stars and planetary paths, written by Claudius Ptolemy (c. AD 100 – c. 170) in Koine Greek.^[1] One of the most influential scientific texts in history, it canonized a geocentric model of the Universe that was accepted for more than 1,200 years from its origin in Hellenistic Alexandria, in the medieval Byzantine and Islamic worlds, and in Western Europe through the Middle Ages and early Renaissance until Copernicus. It is also a key source of information about ancient Greek astronomy.

An edition in Latin of the Almagestum in 1515

Ptolemy set up a public inscription at Canopus, Egypt, in 147 or 148. N. T. Hamilton found that the version of Ptolemy's models set out in the Canopic Inscription was earlier than the version in the Almagest. Hence the Almagest could not have been completed before about 150, a quarter-century after Ptolemy began observing.^[2][3]

Names

The name comes from Arabic اَلْمَجِسْطِيّ al-majisṭī, with اَل al meaning "the", and magesti being a corruption of Greek μεγίστη megístē 'greatest'.^{[citation needed]}

The work was originally titled "Μαθηματικὴ Σύνταξις" (Mathēmatikē Syntaxis) in Koine Greek, and also called Syntaxis Mathematica in Latin. The treatise was later titled Hē Megalē Syntaxis (Ἡ Μεγάλη Σύνταξις, "The Great Treatise"; Latin: Magna Syntaxis), and the superlative form of this (Ancient Greek: μεγίστη, megiste, "greatest") lies behind the Arabic name al-majisṭī (المجسطي), from which the English name Almagest derives. The Arabic name is important due to the popularity of a Latin translation known as Almagestum made in the 12th century from an Arabic translation, which would endure until original Greek copies resurfaced in the 15th century.^{[citation needed]}

Contents

The Syntaxis Mathematica books

 

Table of contents to a 1528 copy of Almagest, translated to Latin from Greek by George of Trebizond

The Syntaxis Mathematica consists of thirteen sections, called books. As with many medieval manuscripts that were handcopied or, particularly, printed in the early years of printing, there were considerable differences between various editions of the same text, as the process of transcription was highly personal. An example illustrating how the Syntaxis was organized is given below; it is a Latin edition printed in 1515 at Venice by Petrus Lichtenstein.^[4]

• Book I contains an outline of Aristotle's cosmology: on the spherical form of the heavens, with the spherical Earth lying motionless as the center, with the fixed stars and the various planets revolving around the Earth. Then follows an explanation of chords with table of chords; observations of the obliquity of the ecliptic (the apparent path of the Sun through the stars); and an introduction to spherical trigonometry.
• Book II covers problems associated with the daily motion attributed to the heavens, namely risings and settings of celestial objects, the length of daylight, the determination of latitude, the points at which the Sun is vertical, the shadows of the gnomon at the equinoxes and solstices, and other observations that change with the observer's position. There is also a study of the angles made by the ecliptic with the vertical, with tables.
• Book III covers the length of the year, and the motion of the Sun. Ptolemy explains Hipparchus' discovery of the precession of the equinoxes and begins explaining the theory of epicycles.
• Books IV and V cover the motion of the Moon, lunar parallax, the motion of the lunar apogee, and the sizes and distances of the Sun and Moon relative to the Earth.
• Book VI covers solar and lunar eclipses.
• Books VII and VIII cover the motions of the fixed stars, including precession of the equinoxes. They also contain a star catalogue of 1022 stars, described by their positions in the constellations, together with ecliptic longitude and latitude.^{[note 1]}
• Book IX addresses general issues associated with creating models for the five naked eye planets, and the motion of Mercury.
• Book X covers the motions of Venus and Mars.
• Book XI covers the motions of Jupiter and Saturn.
• Book XII covers stations and retrograde motion, which occurs when planets appear to pause, then briefly reverse their motion against the background of the zodiac. Ptolemy understood these terms to apply to Mercury and Venus as well as the outer planets.
• Book XIII covers motion in latitude, that is, the deviation of planets from the ecliptic.

Ptolemy's cosmos

The cosmology of the Syntaxis includes five main points, each of which is the subject of a chapter in Book I. What follows is a close paraphrase of Ptolemy's own words from Toomer's translation.^[7]

• The celestial realm is spherical, and moves as a sphere.
• The Earth is a sphere.
• The Earth is at the center of the cosmos.
• The Earth, in relation to the distance of the fixed stars, has no appreciable size and must be treated as a mathematical point.^[8]
• The Earth does not move.

The star catalogue

 

Example of a Greek manuscript of the Almagest, showing a table layout for the stars of Ursa Minor. The functions of the columns, colours and rows are labelled in this depiction.

The layout of the catalogue has always been tabular.^[9] Ptolemy writes explicitly that the coordinates are given as (ecliptical) "longitudes" and "latitudes", which are given in columns, so this has probably always been the case. It is significant that Ptolemy chooses the ecliptical coordinate system because of his knowledge of precession, which distinguishes him from all his predecessors. Hipparchus' celestial globe had an ecliptic drawn in, but the coordinates were equatorial.^[10] Since Hipparchus' star catalogue has not survived in its original form, but was absorbed into the Almagest star catalogue (and heavily revised in the 265 years in between),^[11][10] the Almagest star catalogue is the oldest one in which complete tables of coordinates and magnitudes have come down to us.

As mentioned, Ptolemy includes a star catalog containing 1022 stars. He says that he "observed as many stars as it was possible to perceive, even to the sixth magnitude". The ecliptic longitudes are given in terms of a zodiac constellation and a number of degrees and fractions of a degree. The zodiac constellations each represent exactly 30°, starting with Aries representing longitude 0° to 30°. The degrees are added to the lower limit of the 30-degree range to obtain the longitude. Unlike the situation with the zodiac of modern-day astrology, most of the stars of a given zodiac constellation in the catalog fall in the 30-degree range designated by the same name. The ecliptic longitudes are about 26° lower than those of AD 2000 (the J2000 epoch).^[12] Ptolemy says that the ecliptic longitudes are for the beginning of the reign of Antoninus Pius (138 AD) and that he found that the longitudes had increased by 2° 40′ since the time of Hipparchus which was 265 years earlier (Alm. VII, 2). But calculations show that his ecliptic longitudes correspond more closely to around the middle of the first century CE (+48 to +58).^[7][13][10]

Since Tycho Brahe found this offset, astronomers and historians investigated this problem and suggested several causes:

• that all coordinates were calculated from Hipparchus' observations, whereby the precession constant, which was known too inaccurately at the time, led to a summation error (Delambre 1817);^[13][14]
• that the data had in fact been observed a century earlier by Menelaus of Alexandria (Björnbo 1901);^[13]
• that the difference is a sum of individual errors of various kinds, including calibration with outdated solar data;^[15][13]
• that Ptolemy's instrument was wrongly calibrated and had a systematic offset.^[16]

 

Errors in Ptolemy’s star catalogue: In blue are the stars in the Almagest’s list; in orange, the points of modern measurements transformed to the second century, taking proper motion into account; the orange and blue band is the ecliptic; and the blue curve is the equator. Figure inspired by Hoffmann 2017.^[10]

Subtracting the systematic error leaves other errors that cannot be explained by precession. Of these errors, about 18 to 20 are also found in Hipparchus' star catalogue (which can only be reconstructed incompletely).^[16][10] From this it can be concluded that a subset of star coordinates in the Almagest can indeed be traced back to Hipparchus,^[13] but not that the complete star catalogue was simply "copied". Rather, Hipparchus' major errors are no longer present in the Almagest^[10] and, on the other hand, Hipparchus' star catalogue had some stars that are entirely absent from the Almagest.^[10] It can be concluded that Hipparchus' star catalogue, while forming the basis, has been reobserved and revised.^[10][11]

Errors in the coordinates

The figure he used is based on Hipparchus' own estimate for precession, which was 1° in 100 years, instead of the correct 1° in 72 years. Dating attempts through proper motion of the stars also appear to date the actual observation to Hipparchus' time instead of Ptolemy.^[17]

Many of the longitudes and latitudes have been corrupted in the various manuscripts. Most of these errors can be explained by similarities in the symbols used for different numbers. For example, the Greek letters Α and Δ were used to mean 1 and 4 respectively, but because these look similar copyists sometimes wrote the wrong one. In Arabic manuscripts, there was confusion between for example 3 and 8 (ج and ح). (At least one translator also introduced errors. Gerard of Cremona, who translated an Arabic manuscript into Latin around 1175, put 300° for the latitude of several stars. He had apparently learned from Moors, who used the letter س (sin) for 300 (like the Hebrew ש (shin)), but the manuscript he was translating came from the East, where س was used for 60, like the Hebrew ס (samekh).)^[18]

Even without the errors introduced by copyists, and even accounting for the fact that the longitudes are more appropriate for 58 AD than for 137 AD, the latitudes and longitudes are not fully accurate, with errors as great as large fractions of a degree. Some errors may be due to atmospheric refraction causing stars that are low in the sky to appear higher than where they really are.^[19] A series of stars in Centaurus are off by a couple of degrees, including the star we call Alpha Centauri. These were probably measured by a different person or persons from the others, and in an inaccurate way.^[20]

Constellations in the star catalogue

The star catalogue contains 48 constellations, which have different surface areas and numbers of stars. In Book VIII, Chapter 3, Ptolemy writes that the constellations should be outlined on a globe, but it is unclear exactly how he means this: should surrounding polygons be drawn or should the figures be sketched or even line figures be drawn? This is not stated.

Although no line figures have survived from antiquity, the figures can be reconstructed on the basis of the descriptions in the star catalogue: The exact celestial coordinates of the figures' heads, feet, arms, wings and other body parts are recorded.^[10] It is therefore possible to draw the stick figures in the modern sense so that they fit the description in the Almagest.^{[note 2]}

These constellations form the basis for the modern constellations that were formally adopted by the International Astronomical Union in 1922, with official boundaries that were agreed in 1928.

Of the stars in the catalogue, 108 (just over 10%) were classified by Ptolemy as 'unformed', by which he meant lying outside the recognized constellation figures. These were later absorbed into their surrounding constellations or in some cases used to form new constellations.^[21]

Ptolemy's planetary model

 

16th-century representation of Ptolemy's geocentric model in Peter Apian's Cosmographia, 1524

Ptolemy assigned the following order to the planetary spheres, beginning with the innermost:

1. Moon
2. Mercury
3. Venus
4. Sun
5. Mars
6. Jupiter
7. Saturn
8. Sphere of fixed stars

Other classical writers suggested different sequences. Plato (c. 427 – c. 347 BC) placed the Sun second in order after the Moon. Martianus Capella (5th century AD) put Mercury and Venus in motion around the Sun. Ptolemy's authority was preferred by most medieval Islamic and late medieval European astronomers.

Ptolemy inherited from his Greek predecessors a geometrical toolbox and a partial set of models for predicting where the planets would appear in the sky. Apollonius of Perga (c. 262 – c. 190 BC) had introduced the deferent and epicycle and the eccentric deferent to astronomy. Hipparchus (2nd century BC) had crafted mathematical models of the motion of the Sun and Moon. Hipparchus had some knowledge of Mesopotamian astronomy, and he felt that Greek models should match those of the Babylonians in accuracy. He was unable to create accurate models for the remaining five planets.

 

Geometric construction used by Hipparchus in his determination of the distances to the Sun and Moon, which was later incorporated into Ptolemy's work

The Syntaxis adopted Hipparchus' solar model, which consisted of a simple eccentric deferent. For the Moon, Ptolemy began with Hipparchus' epicycle-on-deferent, then added a device that historians of astronomy refer to as a "crank mechanism":^[22] he succeeded in creating models for the other planets, where Hipparchus had failed, by introducing a third device called the equant.

Ptolemy wrote the Syntaxis as a textbook of mathematical astronomy. It explained geometrical models of the planets based on combinations of circles, which could be used to predict the motions of celestial objects. In a later book, the Planetary Hypotheses, Ptolemy explained how to transform his geometrical models into three-dimensional spheres or partial spheres. In contrast to the mathematical Syntaxis, the Planetary Hypotheses is sometimes described as a book of cosmology.

Influence

 

Ptolemy's Almagest became an authoritative work for many centuries.

 

Picture of George of Trebizond's Latin translation of the Syntaxis Mathematica or Almagest

Ptolemy's comprehensive treatise of mathematical astronomy superseded most older texts of Greek astronomy. Some were more specialized and thus of less interest; others simply became outdated by the newer models. As a result, the older texts ceased to be copied and were gradually lost. Much of what we know about the work of astronomers like Hipparchus comes from references in the Syntaxis.

The first translations into Arabic were made in the 9th century, with two separate efforts, one sponsored by the caliph Al-Ma'mun, who received a copy as a condition of peace with the Byzantine emperor.^[23] Sahl ibn Bishr is thought to be the first Arabic translator.

No Latin translation was made before the 12th century. Henry Aristippus made the first Latin translation directly from a Greek copy, but it was not as influential as a later translation into Latin made in Spain by the Italian scholar Gerard of Cremona from the Arabic (finished in 1175).^[24][25] Gerard translated the Arabic text while working at the Toledo School of Translators, although he was unable to translate many technical terms such as the Arabic Abrachir for Hipparchus. In the 13th century a Spanish version was produced, which was later translated under the patronage of Alfonso X.

In the 15th century, a Greek version appeared in Western Europe. The German astronomer Johannes Müller (known as Regiomontanus, after his birthplace of Königsberg) made an abridged Latin version at the instigation of the Greek churchman Cardinal Bessarion. Around the same time, George of Trebizond made a full translation accompanied by a commentary that was as long as the original text. George's translation, done under the patronage of Pope Nicholas V, was intended to supplant the old translation. The new translation was a great improvement; the new commentary was not, and aroused criticism.^[26] The Pope declined the dedication of George's work,^[26] and Regiomontanus's translation had the upper hand for over 100 years.^{[citation needed]}

During the 16th century, Guillaume Postel, who had been on an embassy to the Ottoman Empire, brought back Arabic disputations of the Almagest, such as the works of al-Kharaqī, Muntahā al-idrāk fī taqāsīm al-aflāk ("The Ultimate Grasp of the Divisions of Spheres", 1138–39).^[27]

Commentaries on the Syntaxis were written by Theon of Alexandria (extant), Pappus of Alexandria (only fragments survive), and Ammonius Hermiae (lost).

Modern assessment

Under the scrutiny of modern scholarship, and the cross-checking of observations contained in the Almagest against figures produced through backwards extrapolation, various patterns of errors have emerged within the work.^[28][29] A prominent example is Ptolemy's use of measurements said to have been taken at noon, but which systematically produce readings that are off by half an hour, as if the observations were taken at 12:30pm.^[28] However, an explanation for this error was found in 1969.^[30][31][32]

The overall quality of Claudius Ptolemy's scholarship and place as "one of the most outstanding scientists of antiquity" has been challenged by several modern writers, most prominently by Robert R. Newton in the 1977 book The Crime of Claudius Ptolemy, which asserted that the scholar fabricated his observations to fit his theories. Newton accused Ptolemy of systematically inventing data or doctoring the data of earlier astronomers, and labelled him "the most successful fraud in the history of science".^[28] One striking error noted by Newton was an autumn equinox said to have been observed by Ptolemy and "measured with the greatest care" at 2pm on 25 September 132, when the equinox should have been observed at 9:54am the day prior.^[28] Herbert Lewis, who had reworked some of Ptolemy's calculations, agreed with Newton that "Ptolemy was an outrageous fraud", and that "all those results capable of statistical analysis point beyond question towards fraud and against accidental error".^[29]

Although some have described the charges laid by Newton as "erudite and imposing", others have disagreed with the findings.^[28] Bernard R. Goldstein wrote, "Unfortunately, Newton’s arguments in support of these charges are marred by all manner of distortions, misunderstandings, and excesses of rhetoric due to an intensely polemical style."^[30] Owen Gingerich, while agreeing that the Almagest contains "some remarkably fishy numbers",^[28] including in the matter of the 30-hour displaced equinox, which he noted aligned perfectly with predictions made by Hipparchus 278 years earlier,^[33] rejected the qualification of fraud.^[28][34] John Phillips Britton, Visiting Fellow at Yale University, wrote of R.R. Newton, "I think that his main conclusion with respect to Ptolemy’s stature and achievements as an astronomer is simply wrong, and that the Almagest should be seen as a great, if not indeed the first, scientific treatise." He continued, "Newton’s work does focus critical attention on the many difficulties and inconsistencies apparent in the fine structure of the Almagest. In particular, his conclusion that the Almagest is not a historical account of how Ptolemy actually derived his models and parameters is essentially the same as mine, although our reasons for this conclusion and our inferences from it differ radically."^[32]

Modern editions

The Almagest under the Latin title Syntaxis mathematica, was edited by J. L. Heiberg in Claudii Ptolemaei opera quae exstant omnia, vols. 1.1 and 1.2 (1898, 1903).

 

1528 copy of a Latin translation of "Almagestum", translated from Greek by George of Trebizond

Three translations of the Almagest into English have been published. The first, by R. Catesby Taliaferro of St. John's College in Annapolis, Maryland, was included in volume 16 of the Great Books of the Western World in 1952. The second, by G. J. Toomer, Ptolemy's Almagest in 1984, with a second edition in 1998.^[35] The third was a partial translation by Bruce M. Perry in The Almagest: Introduction to the Mathematics of the Heavens in 2014.^[36]

A direct French translation from the Greek text was published in two volumes in 1813 and 1816 by Nicholas Halma, including detailed historical comments in a 69-page preface. It has been described as "suffer[ing] from excessive literalness, particularly where the text is difficult" by Toomer, and as "very faulty" by Serge Jodra.^[37] The scanned books are available in full at the Gallica French National library.^[38][39]

Gallery

•  
  Ptolemy's catalogue of stars; a revision of the Almagest by Christian Heinrich Friedrich Peters and Edward Ball Knobel, 1915
•  
  Epytoma Ioannis de Monte Regio in Almagestum Ptolomei, Latin, 1496
•  
  Almagestum, Latin, 1515

See also

• Abū al-Wafā' Būzjānī (who also wrote an Almagest)
• Book of Fixed Stars
• Star cartography
• Euclid's Elements

References

Notes

1. The catalogue actually contained 1,028 entries, but three of these were deliberate duplicates, because Ptolemy regarded certain stars as being shared between adjacent constellations. Three other entries were non-stellar, i.e. the Double Cluster in Perseus, M44 (Praesepe) in Cancer, and the globular cluster Omega Centauri.^[5] Ptolemy states that the longitudes (which increase due to precession) are for the beginning of the reign of Antoninus Pius (138 AD), whereas the latitudes do not change with time (but see the star catalog). The constellations north of the zodiac and the northern zodiac constellations (Aries through Virgo) are in the table at the end of Book VII, while the rest are in the table at the beginning of Book VIII. The brightest stars were marked first magnitude (m = 1), while the faintest visible to the naked eye were sixth magnitude (m = 6). Each numerical magnitude was considered twice the brightness of the following one, which is a logarithmic scale. (The ratio was subjective as no photodetectors existed.) This system is believed to have originated with Hipparchus. The stellar positions too are of Hipparchan origin, despite Ptolemy's claim to the contrary. Ptolemy identified 48 constellations: The 12 of the zodiac, 21 to the north of the zodiac, and 15 to the south.^[6]
2. These modern stick figures as a reconstruction of the historical constellations of the Almagest are available in the free planetarium software Stellarium since 2019.^{[citation needed]}

Citations

1. Tomarchio 2022, p. xv.
2. Hamilton & Swerdlow 1987, p. ^{[pages needed]}.
3. Kunitzsch 2008, pp. 140–141.
4. Lichtenstein 1515, p. ^{[pages needed]}.
5. Ridpath 2023, "Ptolemy’s Almagest".
6. Ridpath 2023, Ptolemy’s 48 constellations.
7. Toomer 1984, p. ^{[pages needed]}.
8. Ptolemy 1952, Book I, Chapter 5, p.9.
9. Lichtenstein 1515, p. 79.
10. Hoffmann 2017, p. ^{[pages needed]}.
11. Hoffmann 2018, p. ^{[pages needed]}.
12. For instance, the stars nu Orionis and 62 Orionis which are now around ecliptic longitude 91° are attributed longitudes in the Almagest of 66° and 64°20' respectively.
13. Graßhoff 2011, p. ^{[pages needed]}.
14. Peters & Knobel 1915, p. 15.
15. Dreyer 1917, p. 528.
16. Vogt 1925, pp. 17–54.
17. Dambis & Efremov 2000, pp. 115–134.
18. Peters & Knobel 1915, pp. 9–14.
19. Peters & Knobel 1915, p. 14.
20. Peters & Knobel 1915, p. 112.
21. Ridpath 2023, "How Ptolemy’s spare stars became new constellations".
22. Hoskin 1999, p. 44.
23. Angelo 2006, p. 78.
24. Toomer 1984, p. 3.
25. Kunitzsch 1986, p. 89.
26. Shank 2020, pp. 305–307.
27. Saliba 2011, pp. 217–221.
28. Wade 1977.
29. Lewis 1979.
30. Goldstein 1978.
31. Britton 1969.
32. Britton 1992.
33. Gingerich 1980.
34. Gingerich 1981.
35. Toomer 1984.
36. Ptolemy 2014.
37. Jodra 2013.
38. Halma 1813.
39. Halma 1816.

Sources

Books

• Angelo, Joseph A. Jr. (2006). Encyclopedia of Space and Astronomy (1st ed.). New York: Facts on File. ISBN 978-0-8160-5330-8 – via books.google.com.
• Britton, John Phillips (1992). Models and Precision: The Quality of Ptolemy's Observations and Parameters (PDF).
• Graßhoff, Gerd (2011) [1990]. The History of Ptolemy's Star Catalogue. Studies in the History of Mathematics and Physical Sciences. Vol. 14 (Reprint of the original 1st 1990 ed.). Berlin/Heidelberg/New York: Springer. doi:10.1007/978-1-4612-4468-4. ISBN 978-1-4612-8788-9.^{[pages needed]}
• Halma, Nicolas (1813). Composition mathématique de Claude Ptolémée (PDF) (in French). Vol. 1. Paris: J. Hermann – via Bibliothèque nationale de France.
• — (1816). Composition mathématique de Claude Ptolémée (PDF) (in French). Vol. 2. Paris: H. Grand – via Bibliothèque nationale de France.
• Hamilton, N. T.; Swerdlow, N. M. (1987). "The Canobic Inscription: Ptolemy's Earliest Work". In Berggren, J. L.; Goldstein, B. R. (eds.). From Ancient Omens to Statistical Mechanics. Copenhagen, Denmark: Copenhagen University Library. ISBN 978-8-7770-9002-8.^{[pages needed]}
• Hoffmann, Susanne M. (2017). Hipparchs Himmelsglobus (in German). Berlin/Heidelberg/New York: Springer. Bibcode:2017hihi.book.....H. doi:10.1007/978-3-658-18683-8. ISBN 978-3-658-18682-1.^{[pages needed]}
• Hoskin, Michael (1999). "2. Astronomy in Antiquity". In Hoskin, Michael (ed.). The Cambridge Concise History of Astronomy (1st ed.). Cambridge, England: Cambridge University Press. ISBN 978-0-521-57291-0.
• Kunitzsch, Paul (2008) [1997]. "Almagest: Its Reception and Transmission in the Islamic World". In Selin, Helaine (ed.). Encyclopaedia of the History of Science, Technology, and Medicine in Non-Western Cultures (2nd ed.). Berlin/Heidelberg/New York: Springer. doi:10.1007/978-1-4020-4425-0. ISBN 978-1-4020-4559-2. from the original on 10 June 2018. Retrieved 8 April 2021. Around AD 150, Ptolemy wrote his great handbook of astronomy called Mathematike Syntaxis...
• Lichtenstein, Petrus (1515). Claudius Ptolemaeus Almagestum (in Latin). Venice. OCLC 644484399. Retrieved 31 May 2014 – via Astronomy Library of the Vienna University.
• Peters, Christian Heinrich Friedrich; Knobel, Edward Ball (1915). Ptolemy's Catalogue of the Stars – A Revision of the Almagest. Vol. 86. Carnegie Institution of Washington.
• Ptolemy, Claudius (1952). "The Almagest". In Hutchins, Robert Maynard; Adler, Mortimer J. (eds.). Ptolemy, Copernicus, Kepler. Chicago: Encyclopaedia Brittanica, Inc.
• — (2014). Donahue, William H. (ed.). The Almagest: Introduction to the Mathematics of the Heavens. Translated by Perry, Bruce M. Santa Fe, NM: Green Lion Press. ISBN 978-1-88800-943-9.
• Saliba, George (2011) [2007]. Buchwald, Jed Z. (ed.). Islamic Science and the Making of European Renaissance (2nd ed.). Cambridge, Mass.: MIT Press. ISBN 978-0-262-51615-0.
• Shank, Michael H. (2020). "Regiomontanus versus George of Trebizond on Planetary Order, Distances, and Orbs (Almagest 9.1)". In Juste, David; van Dalen, Benno; Hasse, Dag Nikolaus; Burnett, Charles (eds.). Ptolemy's Science of the Stars in the Middle Ages. Ptolemaeus Arabus et Latinus. Turnhout: Brepols. pp. 305–307. doi:10.1484/M.PALS-EB.5.120189. ISBN 978-2-503-58639-7.
• Tomarchio, John (2022). A Sourcebook for Ancient Greek: Grammar, Poetry, and Prose. Washington, D.C.: CUA Press. ISBN 978-1-949822-20-5.
• Toomer, G. J. (1984). Ptolemy's Almagest. London: Duckworth Books. ISBN 978-0-387-91220-2.

Journals and magazines

• Britton, John Phillips (Dec 1969). "Ptolemy's Determination of the Obliquity of the Ecliptic". Centaurus. doi:10.1111/j.1600-0498.1969.tb00132.x. Reprinted as Chapter 1 of ^[1].
• Dambis, A. K.; Efremov, Yu. N. (2000). "Dating Ptolemy's Star Catalogue through Proper Motions: The Hipparchan Epoch". Journal for the History of Astronomy. 31 (2): 115–134. Bibcode:2000JHA....31..115D. doi:10.1177/002182860003100202.
• Dreyer, J. L. E. (1917). "On the Origin of Ptolemy's Catalogue of Stars". Monthly Notices of the Royal Astronomical Society. 77 (7): 528. doi:10.1093/mnras/77.7.528. OCLC 10340650.
• Gingerich, Owen (1980). "Was Ptolemy a Fraud?". Quarterly Journal of the Royal Astronomical Society. 21: 253. Bibcode:1980QJRAS..21..253G.
• Gingerich, Owen (1981). "Ptolemy Revisited - Reply to R.R. Newton". Quarterly Journal of the Royal Astronomical Society.
• Goldstein, Bernard R. (24 February 1978). "Casting Doubt on Ptolemy: The Crime of Claudius Ptolemy. Robert R. Newton". Science. 199 (4331): 872–873. doi:10.1126/science.199.4331.872.a. PMID 17757580.
• Hoffmann, Susanne M. (2018). "The Genesis of Hipparchus' Celestial Globe". Mediterranean Archaeology and Archaeometry. 18 (4): 281–287. doi:10.5281/ZENODO.1477980.
• Kunitzsch, Paul (1986). "The Star Catalogue Commonly Appended to the Alfonsine Tables". Journal for the History of Astronomy. Thousand Oaks, California. 17 (49): 89. Bibcode:1986JHA....17...89K. doi:10.1177/002182868601700202. Gerard of Cremona's Latin translation made in Toledo about 1175 from the Arabic, ...
• Lewis, H. A. G. (1979). "Review of The Crime of Claudius Ptolemy, by R. R. Newton". Imago Mundi. 31: 105–107. doi:10.1080/03085697908592494. JSTOR 1150735.
• Vogt, H. (1925). "Versuch einer Wiederherstellung von Hipparchs Fixsternverzeichnis". Astronomische Nachrichten (in German). 224 (2–3): 17–54. Bibcode:1925AN....224...17V. doi:10.1002/asna.19252240202.
• Wade, Nicholas (1977). "Scandal in the Heavens: Renowned Astronomer Accused of Fraud". Science. 198 (4318): 707–709. Bibcode:1977Sci...198..707W. doi:10.1126/science.198.4318.707.

Websites

• Jodra, Serge (2013). "L'Almageste". cosmovisions.com (in French) (Online ed.) – via Imago Mundi.
• Ridpath, Ian (2023). "Star Tales – Ptolemy's Almagest". ianridpath.com (Revised, online ed.).

Further reading

• Evans, James (1998). The History and Practice of Ancient Astronomy. Oxford University Press. ISBN 978-0-19-509539-5.
• Neugebauer, Otto (1948). "Mathematical Methods in Ancient Astronomy" (PDF). Bulletin of the American Mathematical Society. 54: 1013–104.
• Neugebauer, Otto (1975). A History of Ancient Mathematical Astronomy. Berlin: Springer. Part 1, Part 2, Part 3. ISBN 3-540-06995-X.
• Hanson, Norwood Russell (1960). "The Mathematical Power of Epicyclical Astronomy". Isis. 51 (2): 150–158.
• Ridpath, Ian (2018) [1998]. Star Tales (Rev. ed.). Cambridge: Lutterworth Press. ISBN 978-0-7188-9478-8.
• Pedersen, Olaf (1993) [1974]. Early Physics and Astronomy: A Historical Introduction (2nd ed.). Cambridge University Press. ISBN 978-0-521-40899-8.
• Pedersen, Olaf (2011) [1974]. A Survey of the Almagest (2nd ed.). Berlin: Springer. ISBN 978-1-4939-3922-0.
• Ptolemaeus, Claudius. Syntaxis mathematica (in Greek). OCLC 767751182. Retrieved 10 April 2023 – via MDZ/München, Bayerische Staatsbibliothek.
• Shank, Michael H. (2009). "Islamic Science and the Making of European Renaissance by George Saliba". Aestimatio (Book review). 6: 63–72.

External links

 

Wikimedia Commons has media related to Almagest.

• Syntaxis Mathematica (Almagest), original Greek, edited by Johan Ludvig Heiberg, 1898.
• Syntaxis mathematica in J.L. Heiberg's edition (1898–1903)
• Ptolemy's De Analemmate. PDF scans of Heiberg's Greek edition, now in the public domain (Koine Greek)
• Toomer's English translation Duckworth, 1984.
• Ptolemy. Almagest. Latin translation from the Arabic by Gerard of Cremona. Digitized version of manuscript made in Northern Italy c. 1200–1225 held by the State Library of Victoria.
• University of Vienna: Almagestum (1515) PDFs of different resolutions. Edition of Petrus Liechtenstein, Latin translation of Gerard of Cremona.
• Almagest Ephemeris Calculator by Robert Van Gent. Positions for any date, translation of dates in calendars used by Ptolemy. Extensive list of references and articles.
• Online luni-solar and planetary ephemeris calculator based on the Almagest
• in ASCII (in Latin)
• Animation of Ptolemy's model of the universe by Andre Rehak (YouTube)
• (in French) French translation, with some diagrams animated, interactive, or random
• (in Hebrew) Maimonides explaining why you need to learn Almagest first to understand science

1. Britton 1992.