The celestial spheres, or celestial orbs, were the fundamental entities of the cosmological
models developed by Plato
, and others. In these celestial models, the apparent motions
of the fixed stars
are accounted for by treating them as embedded in rotating spheres made of an aetherial, transparent fifth element (quintessence
), like jewels set in orbs. Since it was believed that the fixed stars did not change their positions relative to one another, it was argued that they must be on the surface of a single starry sphere.
In modern thought, the orbits of the planets
are viewed as the paths of those planets through mostly empty space. Ancient and medieval thinkers, however, considered the celestial orbs to be thick spheres of rarefied matter nested one within the other, each one in complete contact with the sphere above it and the sphere below.
[Lindberg, ''Beginnings of Western Science'', p. 251.]
When scholars applied Ptolemy's epicycles
, they presumed that each planetary sphere was exactly thick enough to accommodate them.
By combining this nested sphere model with astronomical observations, scholars calculated what became generally accepted values at the time for the distances to the Sun: about , to the other planets, and to the edge of the universe: about . The nested sphere model's distances to the Sun and planets differ significantly from modern measurements of the distances, and the size of the universe
is now known to be inconceivably large and continuously expanding
Albert Van Helden has suggested that from about 1250 until the 17th century, virtually all educated Europeans were familiar with the Ptolemaic model of "nesting spheres and the cosmic dimensions derived from it". Even following the adoption of Copernicus's heliocentric model
of the universe, new versions of the celestial sphere model were introduced, with the planetary spheres following this sequence from the central Sun: Mercury, Venus, Earth-Moon, Mars, Jupiter and Saturn.
Mainstream belief in the theory of celestial spheres did not survive the Scientific Revolution
. In the early 1600s, Kepler
continued to discuss celestial spheres, although he did not consider that the planets were carried by the spheres but held that they moved in elliptical paths described by Kepler's laws of planetary motion
. In the late 1600s, Greek and medieval theories concerning the motion of terrestrial and celestial objects were replaced by Newton's law of universal gravitation
and Newtonian mechanics
, which explain how Kepler's laws arise from the gravitational attraction between bodies.
Early ideas of spheres and circles
In Greek antiquity
the ideas of celestial spheres and rings first appeared in the cosmology of Anaximander
in the early 6th century BC. In his cosmology both the Sun and Moon are circular open vents in tubular rings of fire enclosed in tubes of condensed air; these rings constitute the rims of rotating chariot-like wheels pivoting on the Earth at their centre. The fixed stars are also open vents in such wheel rims, but there are so many such wheels for the stars that their contiguous rims all together form a continuous spherical shell encompassing the Earth. All these wheel rims had originally been formed out of an original sphere of fire
wholly encompassing the Earth, which had disintegrated into many individual rings. Hence, in Anaximanders's cosmogony, in the beginning was the sphere, out of which celestial rings were formed, from some of which the stellar sphere was in turn composed. As viewed from the Earth, the ring of the Sun was highest, that of the Moon was lower, and the sphere of the stars was lowest.
Following Anaximander, his pupil Anaximenes
(c. 585–528/4) held that the stars, Sun, Moon, and planets are all made of fire. But whilst the stars are fastened on a revolving crystal sphere like nails or studs, the Sun, Moon, and planets, and also the Earth, all just ride on air like leaves because of their breadth. And whilst the fixed stars are carried around in a complete circle by the stellar sphere, the Sun, Moon and planets do not revolve under the Earth between setting and rising again like the stars do, but rather on setting they go laterally around the Earth like a cap turning halfway around the head until they rise again. And unlike Anaximander, he relegated the fixed stars to the region most distant from the Earth. The most enduring feature of Anaximenes' cosmos was its conception of the stars being fixed on a crystal sphere as in a rigid frame, which became a fundamental principle of cosmology down to Copernicus and Kepler.
After Anaximenes, Pythagoras
all held that the universe was spherical. And much later in the fourth century BC Plato's ''Timaeus
'' proposed that the body of the cosmos was made in the most perfect and uniform shape, that of a sphere containing the fixed stars. But it posited that the planets were spherical bodies set in rotating bands or rings rather than wheel rims as in Anaximander's cosmology.
Emergence of the planetary spheres
Instead of bands, Plato's student Eudoxus developed a planetary model
using concentric spheres
for all the planets, with three spheres each for his models of the Moon and the Sun and four each for the models of the other five planets, thus making 26 spheres in all.
[Lloyd, "Heavenly aberrations," p. 173.] Callippus
modified this system, using five spheres for his models of the Sun, Moon, Mercury, Venus, and Mars and retaining four spheres for the models of Jupiter and Saturn, thus making 33 spheres in all.
Each planet is attached to the innermost of its own particular set of spheres. Although the models of Eudoxus and Callippus qualitatively describe the major features of the motion of the planets, they fail to account exactly for these motions and therefore cannot provide quantitative predictions. Although historians of Greek science have traditionally considered these models to be merely geometrical representations, recent studies have proposed that they were also intended to be physically real or have withheld judgment, noting the limited evidence to resolve the question.
In his ''Metaphysics
developed a physical cosmology of spheres, based on the mathematical models of Eudoxus. In Aristotle's fully developed celestial model, the spherical Earth is at the centre of the universe and the planets are moved by either 47 or 55 interconnected spheres that form a unified planetary system, whereas in the models of Eudoxus and Callippus each planet's individual set of spheres were not connected to those of the next planet. Aristotle says the exact number of spheres, and hence the number of movers, is to be determined by astronomical investigation, but he added additional spheres to those proposed by Eudoxus and Callippus, to counteract the motion of the outer spheres. Aristotle considers that these spheres are made of an unchanging fifth element, the aether
. Each of these concentric spheres is moved by its own god—an unchanging divine unmoved mover
, and who moves its sphere simply by virtue of being loved by it.
, eccentric deferent
point. Georg von Peuerbach
, ''Theoricae novae planetarum'', 1474.
In his ''Almagest
'', the astronomer Ptolemy
(fl. ca. 150 AD) developed geometrical predictive models of the motions of the stars and planets and extended them to a unified physical model of the cosmos
in his ''Planetary hypotheses''. By using eccentrics and epicycles
, his geometrical model achieved greater mathematical detail and predictive accuracy than had been exhibited by earlier concentric spherical models of the cosmos. In Ptolemy's physical model, each planet is contained in two or more spheres,
[Neugebauer, ''History of Ancient Mathematical Astronomy'', vol. 2, pp. 917–926.]
but in Book 2 of his ''Planetary Hypotheses'' Ptolemy depicted thick circular slices rather than spheres as in its Book 1. One sphere/slice is the deferent
, with a centre offset somewhat from the Earth; the other sphere/slice is an epicycle
embedded in the deferent, with the planet embedded in the epicyclical sphere/slice. Ptolemy's model of nesting spheres provided the general dimensions of the cosmos, the greatest distance of Saturn being 19,865 times the radius of the Earth and the distance of the fixed stars being at least 20,000 Earth radii.
The planetary spheres were arranged outwards from the spherical, stationary Earth at the centre of the universe in this order: the spheres of the Moon
, and Saturn
. In more detailed models the seven planetary spheres contained other secondary spheres within them. The planetary spheres were followed by the stellar sphere containing the fixed stars; other scholars added a ninth sphere to account for the precession of the equinoxes
, a tenth to account for the supposed trepidation of the equinoxes
, and even an eleventh to account for the changing obliquity of the ecliptic
. In antiquity the order of the lower planets was not universally agreed. Plato and his followers ordered them Moon, Sun, Mercury, Venus, and then followed the standard model for the upper spheres. Others disagreed about the relative place of the spheres of Mercury and Venus: Ptolemy placed both of them beneath the Sun with Venus above Mercury, but noted others placed them both above the Sun; some medieval thinkers, such as al-Bitruji
, placed the sphere of Venus above the Sun and that of Mercury below it.
A series of astronomers, beginning with the Muslim astronomer al-Farghānī
, used the Ptolemaic model of nesting spheres to compute distances to the stars and planetary spheres. Al-Farghānī's distance to the stars was 20,110 Earth radii which, on the assumption that the radius of the Earth was , came to . An introduction to Ptolemy's ''Almagest'', the ''Tashil al-Majisti'', believed to be written by Thābit ibn Qurra
, presented minor variations of Ptolemy's distances to the celestial spheres. In his ''Zij
presented independent calculations of the distances to the planets on the model of nesting spheres, which he thought was due to scholars writing after Ptolemy. His calculations yielded a distance of 19,000 Earth radii to the stars.
[Van Helden, ''Measuring the Universe'', pp. 31–2.]
Around the turn of the millennium, the Arabic astronomer
and polymath Ibn al-Haytham (Alhacen)
presented a development of Ptolemy's geocentric model
s in terms of nested spheres. Despite the similarity of this concept to that of Ptolemy's ''Planetary Hypotheses'', al-Haytham's presentation differs in sufficient detail that it has been argued that it reflects an independent development of the concept. In chapters 15–16 of his ''Book of Optics
'', Ibn al-Haytham also said that the celestial spheres do not consist of solid
Near the end of the twelfth century, the Spanish Muslim
astronomer al-Bitrūjī (Alpetragius)
sought to explain the complex motions of the planets without Ptolemy's epicycles and eccentrics, using an Aristotelian framework of purely concentric spheres that moved with differing speeds from east to west. This model was much less accurate as a predictive astronomical model, but it was discussed by later European astronomers and philosophers.
In the thirteenth century the astronomer al-'Urḍi
proposed a radical change to Ptolemy's system of nesting spheres. In his ''Kitāb al-Hayáh'', he recalculated the distance of the planets using parameters which he redetermined. Taking the distance of the Sun as 1,266 Earth radii, he was forced to place the sphere of Venus above the sphere of the Sun; as a further refinement, he added the planet's diameters to the thickness of their spheres. As a consequence, his version of the nesting spheres model had the sphere of the stars at a distance of 140,177 Earth radii.
About the same time, scholars in European universities
began to address the implications of the rediscovered philosophy of Aristotle and astronomy of Ptolemy. Both astronomical scholars and popular writers considered the implications of the nested sphere model for the dimensions of the universe. Campanus of Novara
's introductory astronomical text, the ''Theorica planetarum'', used the model of nesting spheres to compute the distances of the various planets from the Earth, which he gave as 22,612 Earth radii or 73,387,747 miles. In his ''Opus Majus
'', Roger Bacon
cited Al-Farghānī's distance to the stars of 20,110 Earth radii, or 65,357,700 miles, from which he computed the circumference of the universe to be 410,818,517 miles. Clear evidence that this model was thought to represent physical reality is the accounts found in Bacon's ''Opus Majus'' of the time needed to walk to the Moon and in the popular Middle English
''South English Legendary
'', that it would take 8,000 years to reach the highest starry heaven. General understanding of the dimensions of the universe derived from the nested sphere model reached wider audiences through the presentations in Hebrew by Moses Maimonides
, in French by Gossuin of Metz, and in Italian by Dante Alighieri
Philosophical and theological discussions
Philosophers were less concerned with such mathematical calculations than with the nature of the celestial spheres, their relation to revealed accounts of created nature, and the causes of their motion.
Adi Setia describes the debate among Islamic scholars in the twelfth century, based on the commentary of Fakhr al-Din al-Razi
about whether the celestial spheres are real, concrete physical bodies or "merely the abstract circles in the heavens traced out… by the various stars and planets." Setia points out that most of the learned, and the astronomers, said they were solid spheres "on which the stars turn… and this view is closer to the apparent sense of the Qur'anic verses regarding the celestial orbits." However, al-Razi mentions that some, such as the Islamic scholar Dahhak, considered them to be abstract. Al-Razi himself, was undecided, he said: "In truth, there is no way to ascertain the characteristics of the heavens except by authority f divine revelation or prophetic traditions
" Setia concludes: "Thus it seems that for al-Razi (and for others before and after him), astronomical models, whatever their utility or lack thereof for ordering the heavens, are not founded on sound rational proofs, and so no intellectual commitment can be made to them insofar as description and explanation of celestial realities are concerned."
Christian and Muslim philosophers modified Ptolemy's system to include an unmoved outermost region, the empyrean
heaven, which came to be identified as the dwelling place of God
and all the elect. Medieval Christians identified the sphere of stars with the Biblical firmament
and sometimes posited an invisible layer of water above the firmament, to accord with Genesis
. An outer sphere, inhabited by angels
, appeared in some accounts.
, a historian of science, has provided evidence that medieval scholastic philosophers generally considered the celestial spheres to be solid in the sense of three-dimensional or continuous, but most did not consider them solid in the sense of hard. The consensus was that the celestial spheres were made of some kind of continuous fluid.
Later in the century, the mutakallim
Adud al-Din al-Iji (1281–1355) rejected the principle of uniform and circular motion, following the Ash'ari
doctrine of atomism
, which maintained that all physical effects were caused directly by God's will rather than by natural causes.
He maintained that the celestial spheres were "imaginary things" and "more tenuous than a spider's web".
[pp. 55–57 of ]
His views were challenged by al-Jurjani
(1339–1413), who maintained that even if the celestial spheres "do not have an external reality, yet they are things that are correctly imagined and correspond to what xists
Medieval astronomers and philosophers developed diverse theories about the causes of the celestial spheres' motions. They attempted to explain the spheres' motions in terms of the materials of which they were thought to be made, external movers such as celestial intelligences, and internal movers such as motive souls or impressed forces. Most of these models were qualitative, although a few incorporated quantitative analyses that related speed, motive force and resistance. By the end of the Middle Ages, the common opinion in Europe was that celestial bodies were moved by external intelligences, identified with the angel
s of revelation
. The outermost moving sphere
, which moved with the daily motion affecting all subordinate spheres, was moved by an unmoved mover
, the Prime Mover
, who was identified with God. Each of the lower spheres was moved by a subordinate spiritual mover (a replacement for Aristotle's multiple divine movers), called an intelligence.
Early in the sixteenth century Nicolaus Copernicus
drastically reformed the model of astronomy by displacing the Earth from its central place in favour of the Sun, yet he called his great work ''De revolutionibus orbium coelestium
'' (''On the Revolutions of the Celestial Spheres''). Although Copernicus does not treat the physical nature of the spheres in detail, his few allusions make it clear that, like many of his predecessors, he accepted non-solid celestial spheres. Copernicus rejected the ninth and tenth spheres, placed the orb of the Moon around the Earth, and moved the Sun from its orb to the center of the universe
. The planetary orbs circled the center of the universe in the following order: Mercury, Venus, the great orb containing the Earth and the orb of the Moon, then the orbs of Mars, Jupiter, and Saturn. Finally he retained the eighth sphere of the star
s, which he held to be stationary.
The English almanac maker, Thomas Digges
, delineated the spheres of the new cosmological system in his ''Perfit Description of the Caelestiall Orbes …'' (1576). Here he arranged the "orbes" in the new Copernican order, expanding one sphere to carry "the globe of mortalitye", the Earth, the four classical elements
, and the Moon, and expanding the sphere of stars infinitely to encompass all the stars and also to serve as "the court of the Great God, the habitacle of the elect, and of the coelestiall angelles."
In the sixteenth century, a number of philosophers, theologians, and astronomers—among them Francesco Patrizi
, Andrea Cisalpino, Peter Ramus
, Robert Bellarmine
, Giordano Bruno
, Jerónimo Muñoz, Michael Neander
, Jean Pena, and Christoph Rothmann
—abandoned the concept of celestial spheres. Rothmann argued from observations of the comet
of 1585 that the lack of observed parallax
indicated that the comet was beyond Saturn, while the absence of observed refraction indicated the celestial region was of the same material as air, hence there were no planetary spheres.
's investigations of a series of comets from 1577 to 1585, aided by Rothmann's discussion of the comet of 1585 and Michael Maestlin
's tabulated distances of the comet of 1577, which passed through the planetary orbs, led Tycho to conclude that "the structure of the heavens was very fluid and simple." Tycho opposed his view to that of "very many modern philosophers" who divided the heavens into "various orbs made of hard and impervious matter." Edward Grant found relatively few believers in hard celestial spheres before Copernicus and concluded that the idea first became common sometime between the publication of Copernicus's ''De revolutionibus'' in 1542 and Tycho Brahe's publication of his cometary research in 1588.
In his early ''Mysterium Cosmographicum'', Johannes Kepler
considered the distances of the planets and the consequent gaps required between the planetary spheres implied by the Copernican system, which had been noted by his former teacher, Michael Maestlin. Kepler's Platonic cosmology filled the large gaps with the five Platonic polyhedra
, which accounted for the spheres' measured astronomical distance. In Kepler's mature celestial physics, the spheres were regarded as the purely geometric spatial regions containing each planetary orbit rather than as the rotating physical orbs of the earlier Aristotelian celestial physics. The eccentricity of each planet's orbit thereby defined the radii
of the inner and outer limits of its celestial sphere and thus its thickness. In Kepler's celestial mechanics
, the cause of planetary motion became the rotating Sun, itself rotated by its own motive soul. However, an immobile stellar sphere was a lasting remnant of physical celestial spheres in Kepler's cosmology.
Literary and visual expressions
gaze upon the highest Heaven; from Gustave Doré
's illustrations to the ''Divine Comedy
, Paradiso'' Canto 28, lines 16–39
's ''Dream of Scipio
,'' the elder Scipio Africanus
describes an ascent through the celestial spheres, compared to which the Earth and the Roman Empire dwindle into insignificance. A commentary on the ''Dream of Scipio'' by the Roman writer Macrobius
, which included a discussion of the various schools of thought on the order of the spheres, did much to spread the idea of the celestial spheres through the Early Middle Ages
Nicole Oresme, ''Le livre du Ciel et du Monde,'' Paris, BnF, Manuscrits, Fr. 565, f. 69, (1377)
Some late medieval figures noted that the celestial spheres' physical order was inverse to their order on the spiritual plane, where God was at the center and the Earth at the periphery. Near the beginning of the fourteenth century Dante
, in the ''Paradiso
'' of his ''Divine Comedy
'', described God as a light at the center of the cosmos. Here the poet ascends beyond physical existence to the Empyrean
Heaven, where he comes face to face with God himself and is granted understanding of both divine and human nature. Later in the century, the illuminator of Nicole Oresme
's ''Le livre du Ciel et du Monde'', a translation of and commentary on Aristotle's ''De caelo''
produced for Oresme's patron, King Charles V
, employed the same motif. He drew the spheres in the conventional order, with the Moon closest to the Earth and the stars highest, but the spheres were concave upwards, centered on God, rather than concave downwards, centered on the Earth. Below this figure Oresme quotes the Psalms
that "The heavens declare the Glory of God and the firmament showeth his handiwork."
The late-16th-century Portuguese epic ''The Lusiads
'' vividly portrays the celestial spheres as a "great machine of the universe" constructed by God. The explorer Vasco da Gama is shown the celestial spheres in the form of a mechanical model. Contrary to Cicero's representation, da Gama's tour of the spheres begins with the Empyrean, then descends inward toward Earth, culminating in a survey of the domains and divisions of earthly kingdoms, thus magnifying the importance of human deeds in the divine plan.
* Aristotle ''Metaphysics'', in 'The Basic Works of Aristotle' Richard McKeon (Ed) The Modern Library, 2001
* Clagett, Marshall ''Science of Mechanics in the Middle Ages'' University of Wisconsin Press 1959
* Cohen, I.B. & Whitman, A. ''Principia'' University of California Press 1999
* Cohen & Smith (eds) ''The Cambridge Companion to Newton'' CUP 2002
* Copernicus, Nicolaus ''On the Revolutions of the Heavenly Spheres'', in ''Great Books of the Western World : 16 Ptolemy Copernicus Kepler'' Encyclopædia Britannica Inc 1952
* Duhem, Pierre. "History of Physics." The Catholic Encyclopedia. Vol. 12. New York: Robert Appleton Company, 1911. 18 Jun. 2008 .
* Duhem, Pierre. ''Le Système du Monde: Histoire des doctrines cosmologiques de Platon à Copernic,'' 10 vols., Paris: Hermann, 1959.
* Duhem, Pierre. ''Medieval Cosmology: Theories of Infinity, Place, Time, Void, and the Plurality of Worlds'', excerpts from ''Le Système du Monde'', translated and edited by Roger Ariew, Chicago: University of Chicago Press, 1987
* Eastwood, Bruce, "Astronomy in Christian Latin Europe c. 500 – c. 1150," ''Journal for the History of Astronomy,'' 28(1997): 235–258.
* Eastwood, Bruce, ''Ordering the Heavens: Roman Astronomy and Cosmology in the Carolingian Renaissance,'' Leiden: Brill, 2007. .
* Eastwood, Bruce and Gerd Graßhoff, ''Planetary Diagrams for Roman Astronomy in Medieval Europe, ca. 800–1500,'' ''Transactions of the American Philosophical Society,'' vol. 94, pt. 3, Philadelphia, 2004.
* Field, J. V., ''Kepler's geometrical cosmology''. Chicago: Chicago University Press, 1988
* Golino, Carlo (ed.), ''Galileo Reappraised'', University of California Press 1966
* Grant, Edward, "Celestial Orbs in the Latin Middle Ages," ''Isis,'' 78(1987): 153–73; reprinted in Michael H. Shank, ed., ''The Scientific Enterprise in Antiquity and the Middle Ages,'' Chicago: Univ. of Chicago Pr., 2000.
* Grant, Edward, ''Planets, Stars, and Orbs: The Medieval Cosmos, 1200–1687,'' Cambridge: Cambridge Univ. Pr., 1994.
*Grant, Edward, ''The Foundations of Modern Science in the Middle Ages'', Cambridge: Cambridge Univ. Pr., 1996.
*Gingerich, Owen ''The Eye of Heaven'', American Institute of Physics 1993
* Heath, Thomas, ''Aristarchus of Samos'' Oxford University Press/Sandpiper Books Ltd. 1913/97
* Jarrell, R.A., ''The contemporaries of Tycho Brahe'' in Taton & Wilson (eds)1989
* Koyré, Alexandre, ''Galileo Studies'' (translator Mepham) Harvester Press 1977
* Kepler, Johannes, ''Epitome of Copernican Astronomy'' (Bks 4 & 5), published in ''Great Books of the Western World : 16 Ptolemy Copernicus Kepler'', Encyclopædia Britannica Inc. 1952
* Lewis, C. S., ''The Discarded Image: An Introduction to Medieval and Renaissance Literature'', Cambridge: Cambridge University Press 1964
* Lindberg, David C. (ed.), ''Science in the Middle Ages'' Chicago: Univ. of Chicago Pr., 1978.
* Lloyd, G. E. R., ''Aristotle: The Growth and Structure of his Thought,'' pp. 133–153, Cambridge: Cambridge Univ. Pr., 1968. .
* Lloyd, G. E. R., "Heavenly aberrations: Aristotle the amateur astronomer," pp. 160–183 in his ''Aristotelian Explorations,'' Cambridge: Cambridge Univ. Pr., 1996. .
* Mach, Ernst, ''The Science of Mechanics'' Open Court 1960.
* Maier, Annaliese, ''At the Threshold of Exact Science: Selected Writings of Annaliese Maier on Late Medieval Natural Philosophy'', edited by Steven Sargent, Philadelphia: University of Pennsylvania Press, 1982.
* McCluskey, Stephen C., ''Astronomies and Cultures in Early Medieval Europe,'' Cambridge: Cambridge Univ. Pr., 1998.
* Neugebauer, Otto, ''A History of Ancient Mathematical Astronomy,'' 3 vols., New York: Springer, 1975.
* Popper, Karl, ''The World of Parmenides'' Routledge 1996
* Rosen, Edward, ''Three Copernican Treatises'' Dover 1939/59.
* Sambursky, S., ''The Physical World of Late Antiquity'' Routledge & Kegan Paul, 1962
* Schofield, C., ''The Tychonic and Semi-Tychonic World Systems'' in Taton & Wilson (eds) 1989
* Sorabji, Richard, ''Matter, Space and Motion'' London: Duckworth, 1988
* Sorabji, Richard, (ed.) ''Philoponus and the Rejection of Aristotelian Science'' London & Ithaca NY 1987
* Sorabji, Richard, ''The Philosophy of the Commentators, 200–600 AD: Volume 2 Physics'' Duckworth 2004
* R. Taton & C. Wilson (eds.), ''The General History of Astronomy: Volume 2 Planetary astronomy from the Renaissance to the rise of astrophysics Part A Tycho Brahe to Newton'' Cambridge: Cambridge Univ. Pr., 1989
* Thoren, Victor E., "The Comet of 1577 and Tycho Brahe's System of the World," ''Archives Internationales d'Histoire des Sciences,'' 29 (1979): 53–67.
* Thoren, Victor E., ''Tycho Brahe'' in Taton & Wilson 1989
Working model and complete explanation of the Eudoxus's Spheres
*Henry Mendell, Vignettes of Ancient Mathematics:
M. Blundevile his exercises, p 282
– Depiction of celestial spheres in a 1613 book
Category:Ancient Greek astronomy
Category:Early scientific cosmologies