How to use this course
John Philoponus lived in sixth-century Alexandria, at the end of the Greek philosophical schools of antiquity. He was trained as a commentator on Aristotle and wrote some of the most careful commentaries we have. He also wrote the most thorough attack on Aristotle’s physics before the seventeenth century. Many of his objections reappear in Ibn Sina, in the Paris impetus theorists such as Jean Buridan, and in the young Galileo, who cited him by name.
- Basic Newtonian mechanics: velocity, acceleration, drag and terminal speed.
- Simple differential equations and integrals.
- For Lesson 08, the idea of a one-to-one correspondence between sets; Cantor’s cardinals are introduced as needed.
- For Lesson 10, elementary spherical geometry and trigonometry.
- The Aristotle course, especially its lessons on motion and the void and on the infinite, is useful background.
Each technical lesson opens with a paragraph for the general reader, then states Philoponus’s positions as closely as the texts allow and compares them with modern physics or mathematics. Philoponus wrote in Greek prose. Formulas are our models of his claims, and we say so. His life is poorly documented: we have the dates his own works reveal, the replies of his opponents, and later Syriac, Arabic and Byzantine reports. Where a date or detail is contested, we give the range.
Timeline
| c. 490 | Born, probably in Alexandria, into a Christian family (some older accounts suggest Caesarea). |
| c. 510–517 | Studies with the Neoplatonist Ammonius, son of Hermias. Publishes commentaries based on Ammonius’s lectures: On Generation and Corruption, On the Soul, Categories, Prior and Posterior Analytics. |
| 517 | Commentary on Aristotle’s Physics; a date in the text corresponds to 517. Contains the theory of impressed force and the falling-bodies argument. |
| c. 520–540 | On the Use and Construction of the Astrolabe, the oldest surviving Greek treatise on the instrument. |
| 529 | On the Eternity of the World against Proclus. |
| c. 530–534 | Against Aristotle on the Eternity of the World, now known from fragments, mainly through Simplicius. |
| c. 530–535 | Commentary on the Meteorology (incomplete); On the Contingency of the World (lost; an Arabic summary survives). |
| late 530s | Simplicius, a fellow pupil of Ammonius, attacks him in his commentaries on On the Heavens and the Physics. |
| c. 546–560 | On the Creation of the World (De opificio mundi), dedicated to Sergius, patriarch of Antioch; dates proposed range from 546–549 to 557–560. |
| c. 552–553 | The Arbiter, a miaphysite treatise on the nature of Christ, written shortly before the Second Council of Constantinople. |
| 567 | On the Trinity (lost; Syriac fragments), the source of the charge of tritheism. |
| c. 570 | Dies, probably in Alexandria. |
| 680–681 | Condemned posthumously as a tritheist by the Third Council of Constantinople. |
| 9th–10th c. | Known in Arabic as Yahya al-Nahwi. Al-Kindi draws on his arguments for a beginning of the world; al-Farabi writes a refutation of him. |
Alexandria and the school of Ammonius
Alexandria around 500 was a Christian city of the Eastern Roman Empire, governed from Constantinople, with a powerful patriarch and a long tradition of Greek learning. It still had public teachers of philosophy, medicine and grammar. The leading philosopher was Ammonius, son of Hermias, who had studied in Athens under the Neoplatonist Proclus and then taught in Alexandria for decades. Ammonius was a pagan in a Christian city. According to the later philosopher Damascius, he reached some accommodation with the Christian authorities that allowed him to keep teaching.
Name and origins
Philoponus called himself John the Grammarian (Iōannēs ho Grammatikos). “Grammarian” was a professional title: a teacher of language and literature, a rank below the chair of philosophy. The surname Philoponus means “lover of work”. It may have been a nickname for his industry or a reference to the philoponoi, lay Christian associations in Alexandria that were active in church life. Arabic writers knew him as Yahya al-Nahwi, John the Grammarian. Nothing reliable is known of his family. Most scholars think he was born around 490 and was a Christian from birth, though some earlier accounts placed his origins in Caesarea and some argued for a later conversion.
The curriculum
In Ammonius’s school, students read Aristotle’s logic first, then his natural philosophy, as preparation for Plato and for Neoplatonic metaphysics. Teaching took the form of lectures on a text, often taken down by students and edited for publication. Several of Philoponus’s early commentaries carry the heading “from the seminars of Ammonius, with some observations of his own”. They show a pupil who knew Aristotle extremely well and had begun to disagree with him.
The grammarian as commentator, c. 510–517
Between about 510 and 517 Philoponus published commentaries on Aristotle’s On Generation and Corruption, On the Soul, the Categories, and the Prior and Posterior Analytics, along with a work on Greek words with several meanings. The commentaries follow the Neoplatonic convention of harmonizing Aristotle with Plato and explaining difficulties away.
The Physics commentary
The commentary on the Physics is different. In it Philoponus refers to a date that corresponds to 517, so it was finished in or soon after that year. It may have been revised later. In long digressions he rejects several of Aristotle’s central doctrines: the definition of place as the boundary of the containing body, the impossibility of void, the account of projectile motion, and the law that speed is proportional to weight and inversely proportional to the density of the medium. Lessons 04 to 06 reconstruct these arguments. They are the main reason historians of physics know his name.
Philoponus did not reject Aristotle wholesale. He kept the four elements, natural places, the distinction between natural and forced motion, and Aristotle’s logic. His method was internal criticism: he used Aristotle’s own principles, and common experience, to show where the system failed.
DiscussionPhiloponus’s early commentaries are partly records of his teacher’s lectures. How should a historian decide which ideas in such a text belong to the teacher and which to the editor? What features of the Physics commentary suggest the critical digressions are Philoponus’s own?
529: the turn against Proclus
The Neoplatonists held that the world has no beginning. Plato’s Timaeus seems to describe a creation in time, but they read the story as an allegory of eternal dependence on a cause. Proclus had collected eighteen arguments for the eternity of the world. In 529 Philoponus published On the Eternity of the World against Proclus, a long work that answers each argument in turn.
The same year is the traditional date of Emperor Justinian’s measures against pagan teaching, which ended the Neoplatonic school in Athens. Historians debate how far the coincidence was deliberate. Some see the book as a Christian scholar’s bid to show that philosophy could serve the faith; others stress that its arguments are philosophical throughout and that Philoponus quotes Plato and Aristotle against Proclus far more than Scripture.
Against Aristotle
In the early 530s he followed it with Against Aristotle on the Eternity of the World, in at least eight books. It attacked Aristotle’s fifth element, the aether, and the eternity of motion and time. The work is lost, but the Athenian philosopher Simplicius, who had also studied with Ammonius, quoted it extensively in order to refute it, so we know much of its content from its enemy. Simplicius treated Philoponus with contempt and mocked him as an outsider to philosophy. A further work, On the Contingency of the World, survives only in an Arabic summary. Lessons 07 and 08 present the arguments.
From the 530s Philoponus seems to have turned mainly to theology, though he still wrote on natural philosophy and probably on the astrolabe.
DiscussionMuch of what we know about Philoponus’s Against Aristotle comes from Simplicius, who wrote to refute it. What are the risks of reconstructing a lost work from its opponent’s quotations? Name a modern example of the same problem.
Impressed force
For the general reader. What keeps a thrown stone moving after it leaves the hand? Aristotle said the air. Philoponus showed that the air cannot do the job and proposed instead that the thrower gives the stone an incorporeal motive power, which carries it on until the power is used up. This is the first clear statement of the idea later called impetus.
- State Aristotle’s two air theories and Philoponus’s objections.
- State the theory of impressed force and its main features.
- Model a self-exhausting impressed force and compare it with Newtonian motion.
The air theories
Aristotle held that a forced motion needs a mover in contact. For a projectile he offered the air: either displaced air flows round and pushes from behind (antiperistasis, which he reported but did not accept), or the thrower moves the air along with the stone and gives it a power of moving that passes from layer to layer (Physics VIII.10).
- On the replacement theory, the air in front is pushed forward by the stone. Nothing explains why it should then turn back, flow round, and push the stone from behind, rather than simply move aside.
- If the hand moves the air and the air the stone, why must the hand touch the stone at all? Set a stone on a stand and drive air at it with bellows, as violently as you like: it barely moves. A stone flung by hand flies far.
Some incorporeal motive power (energeia asōmatos kinētikē) is imparted by the thrower to the projectile. The air contributes little or nothing to the motion, and in fact resists it. If a projectile were moved through a void, it would move even better, since nothing would hinder it.
Philoponus held that this power is temporary: it is expended in producing the motion and fades of itself, even without resistance. He extended the idea to light (Lesson 09), and in On the Creation of the World he suggested that God gave the heavenly bodies a motive power at their creation, an idea that Buridan would later develop with a permanent impetus.
A model
Let \(p\) be the impressed power, and suppose the horizontal speed is proportional to it, \(v=cp\). Philoponus’s power exhausts itself; air resistance also weakens it. A simple model is
\[ \frac{dp}{dt}=-\lambda-kp, \qquad p(0)=p_0, \]with \(\lambda>0\) the rate of self-exhaustion and \(k\ge0\) the resistance. In a void (\(k=0\)), \(p(t)=p_0-\lambda t\) and the motion stops at \(t^*=p_0/\lambda\). This is why Philoponus could accept motion in a void without accepting endless motion. Ibn Sina, who made the imparted inclination self-preserving, had to deny the void (see the Ibn Sina course, Lesson 05); Buridan, who also made it permanent, accepted endless motion where nothing resists.
Exercise 4.1In a void (\(k=0\)), find the distance travelled by a projectile with \(v(0)=v_0\) and self-exhausting power, as a function of \(v_0\) and the stopping time \(t^*\). How does the distance scale with \(v_0\) if \(\lambda\) is the same for all throws?
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Exercise 4.2Solve \(dp/dt=-\lambda-kp\) with \(k>0\). Show the motion stops at \(t^*=\frac1k\ln\!\big(1+\frac{kp_0}{\lambda}\big)\), and check the limit \(k\to0\).
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Exercise 4.3Philoponus’s bellows argument: estimate the force of a strong wind of 20 m/s on a stone of radius 3 cm (\(C_d\approx0.47\), \(\rho_{\text{air}}=1.2\) kg/m³). Compare with the force a hand exerts in throwing a 0.3 kg stone to 20 m/s over 0.15 s.
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Falling bodies and motion in a void
For the general reader. Aristotle said a body ten times heavier falls ten times faster, and that motion through empty space would take no time at all, which he thought absurd. Philoponus replied with a test anyone can make: drop two weights, one much heavier, from the same height, and the difference in their times is very small. He also offered a new rule for motion in a medium, in which the medium adds time to a motion that would take a definite time even in a void.
- State Aristotle’s law of fall and Philoponus’s experimental objection.
- State Philoponus’s additive rule for time in a medium.
- Compare both rules with Newtonian motion under drag.
Aristotle’s rule
In Physics IV.8 Aristotle argues that the speed of a falling body is proportional to its weight and inversely proportional to the density of the medium. In modern notation \(v\propto W/\rho\), so the time to fall a height \(h\) is \(t\propto h\rho/W\). As \(\rho\to0\) the time tends to zero, and Aristotle concluded that motion in a void is impossible.
If you drop from the same height two weights, one many times heavier than the other, the ratio of the times of fall does not follow the ratio of the weights. The difference in time is very small, so that if the weights do not differ greatly, one of them being, say, double the other, there will be no difference in time, or an imperceptible one.
He presents this as a matter of evidence, “by observation”, and against Aristotle’s rule it is decisive. Whether he performed a careful trial or reported common experience cannot be determined.
The additive rule
A body moving through a void would take a definite, finite time, determined by its own weight, the heavier body moving faster. A medium adds to this a further time, proportional to the density of the medium. Thus the total time is the time in the void plus the time added by the resistance of the medium.
As a formula for a fall through height \(h\),
\[ t = t_{\text{void}} + t_{\text{medium}} = \frac{h}{aW} + b\rho h, \]with \(a,b\) constants. The void time is finite, so Aristotle’s argument from infinite speed fails. A related rule, in which the speed is the motive power minus the resistance, was held in twelfth-century Spain by Ibn Bajja (Avempace) and reported by Ibn Rushd; through Averroes it reached Thomas Aquinas and the Latin debate.
The Newtonian picture
In a true vacuum all bodies fall with the same acceleration \(g\), and \(t=\sqrt{2h/g}\) for every weight. In air, drag makes heavy compact bodies fall slightly faster than light ones. The Aristotle course shows that Aristotle’s rule describes the terminal speed in a viscous medium. Philoponus’s “very small difference” is what one actually sees from a tower.
Exercise 5.1Two iron balls of 1 kg and 10 kg are dropped from 20 m. Under Aristotle’s rule, how far has the light ball fallen when the heavy one lands? Using Newtonian mechanics with drag neglected, what is the actual separation? (Drag adds only a few centimetres.)
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Exercise 5.2In Philoponus’s additive rule, take weights \(W\) and \(2W\). Show that the ratio of fall times is \(\dfrac{t_1}{t_2}=\dfrac{1+r}{\tfrac12+r}\) where \(r=t_{\text{medium}}/t_{\text{void}}(W)\). For what values of \(r\) is the difference imperceptible, as he claimed? What does this reveal about the rule?
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Exercise 5.3Newtonian fall with linear drag: \(m\dot v=mg-bv\). Show that for \(t\ll m/b\) the time to fall \(h\) is nearly independent of \(m\), and for \(t\gg m/b\) it is approximately \(h b/(mg)+m/b\). Which regime matches Aristotle, and which Philoponus?
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Place as extension
For the general reader. Where is a thing? Aristotle said: inside the surface of whatever surrounds it. Philoponus said: in a three-dimensional region of space, the same size as the thing, which would still be there if the thing were removed. Such a region is never actually empty, but it is a coherent idea, and it is what we mean by place. This is close to the modern idea of space as a container.
- State Aristotle’s and Philoponus’s definitions of place.
- Reconstruct Philoponus’s objections to Aristotle.
- Understand his view that void is never actual but explains real phenomena.
Aristotle (Physics IV.4): the place of a body is the innermost motionless boundary of the body that contains it.
Philoponus (In Physica, the Corollary on Place): the place of a body is a certain extension, measurable in three dimensions, distinct from the bodies that occupy it, and in its own definition incorporeal: dimensions alone, void of any body.
Objections to the surface definition
- The outermost sphere. On Aristotle’s definition, the outermost heaven is not contained by anything, so it has no place, yet it moves in a circle. Motion without place is incoherent.
- Size. A place should be equal to what it contains. A surface is two-dimensional and a body three-dimensional, so a surface cannot be equal to a body.
- Natural places. Bodies move toward their natural places. A mere surface has no power to attract; an extension with an order of up and down can explain why each element has its region.
Void never actual
Philoponus distinguished conceptual possibility from physical fact. Place as extension can be conceived empty, but in nature it is always filled. He cited the clepsydra, a vessel with small holes in the bottom that holds water in while its top is stopped, and the way liquid rises in a tube when air is sucked out. These show a natural force that prevents a void from forming. This “force of the void” is real, he argued, only because a void is a meaningful idea; one cannot resist what makes no sense.
The explanation was replaced in 1643, when Evangelista Torricelli showed that the weight of the atmosphere supports a column of mercury, and later experiments produced a vacuum above it.
Exercise 6.1A clepsydra is filled with water and its top hole is stopped. Using atmospheric pressure \(1.013\times10^5\) Pa, find the greatest height of water that the air below can hold up. Why does Philoponus’s “force of the void” not set a limit of this kind?
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Exercise 6.2A boat is moored in a flowing river. On Aristotle’s definition, does the boat change place while it stays moored? On Philoponus’s? Explain how Aristotle tried to save his definition.
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Against the aether
For the general reader. Aristotle split the cosmos in two. Below the Moon, things are made of earth, water, air and fire, and they change and decay. Above the Moon, everything is made of a fifth element, aether, which moves only in circles and never changes. Philoponus argued that there is no fifth element: the stars and the Sun are made of the same kinds of stuff as things on Earth, mostly fire. Then the heavens are subject to the same physics, and like everything composite, they could perish.
- Reconstruct Aristotle’s argument for the aether.
- State Philoponus’s objections, especially those from colour and from the motion of fire.
- Check his claims against stellar physics.
Aristotle’s argument
In On the Heavens I.2 Aristotle argues: every simple body has one simple natural motion. Straight motion up or down belongs to the four elements. Circular motion is also simple, so it must be natural to some simple body, which is neither heavy nor light, and which, having no contrary, cannot be generated or destroyed.
Philoponus’s objections (from Against Aristotle, via Simplicius)
- Circular motion of fire. Aristotle himself says, in the Meteorology, that the fire and upper air beneath the Moon rotate along with the heavens. So circular motion is not peculiar to a fifth body.
- Colours of the stars. The stars differ in colour and brightness. Differences of colour arise from differences in composition, as fires differ in colour with their fuel. So the stars are composite and are not made of one simple body.
- Heat of the Sun. The Sun heats and burns. Aristotle explained this by friction of the air, but the simplest explanation is that the Sun is fire.
- Composite implies perishable. What is composite can be dissolved. If the heavens are composite, nothing in their nature guarantees that they last forever; their permanence depends on God.
Philoponus also held that all bodies share three-dimensional extension as their common nature, prior to the qualities that distinguish the elements, a view sometimes compared with Descartes’s matter as extension.
A modern check
Philoponus was right that the Sun and stars are hot and are made of ordinary elements, and right that the colour of a star reveals its physical state. Spectroscopy in the nineteenth century confirmed that stars contain hydrogen, sodium, iron and other terrestrial elements. The colour of a star mainly indicates its surface temperature, through the thermal spectrum, rather than its fuel.
A black body at temperature \(T\) emits most strongly at wavelength \(\lambda_{\max}=b/T\), with \(b\approx2.898\times10^{-3}\) m·K.
Exercise 7.1Betelgeuse has a surface temperature of about 3500 K and Rigel about 12 000 K. Find their peak wavelengths and explain their colours. What does this say about Philoponus’s argument from the colours of the stars?
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Exercise 7.2Aristotle’s heavens never change. In 1572 Tycho Brahe saw a new star and found no daily parallax. The Moon’s daily parallax is about \(1^\circ\), and Tycho could detect a few arcminutes. Show that the new star was at least ten or so times farther than the Moon. Which of Philoponus’s claims does this support?
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The world had a beginning: arguments from the infinite
For the general reader. Could the world always have existed? Aristotle said yes: there was no first motion and no first moment. Philoponus turned Aristotle’s own principle against him. Aristotle had said an infinite can never be completed or crossed. If the world had no beginning, an infinite number of days would already have passed, which is an infinite that has been completed. So, Philoponus argued, the world must have a beginning.
- State Philoponus’s arguments from traversal, addition and multiplication of the infinite.
- Evaluate them with Cantor’s theory of cardinal numbers.
- Understand his argument from finite power.
Aristotle’s premise
Aristotle held that the infinite exists only potentially: a magnitude can be divided without end, but no infinite collection is ever present or completed (Physics III.6). He also held that the world, time and motion have no beginning. Philoponus argued that these two theses are inconsistent.
- Traversal. An infinite cannot be traversed. If the world had no beginning, the series of past generations or days is infinite, and it has been traversed to reach today. So today could never have arrived.
- Addition. Nothing can be greater than the infinite. But each new day adds to the number of past days. If that number were already infinite, it would become greater than infinite.
- Multiplication. Saturn revolves once in about thirty years, the Sun once a year, and the sphere of fixed stars once a day. If the past were infinite, Saturn’s revolutions would be infinite, the Sun’s about thirty times as many, and the fixed stars’ about ten thousand times as many: infinities many times greater than infinity.
Cantor’s verdict
After Georg Cantor, two sets have the same size (cardinality) when there is a one-to-one correspondence between them. The natural numbers \(\mathbb N\) and the even numbers have the same cardinality \(\aleph_0\), through \(n\mapsto2n\).
\(\aleph_0+1=\aleph_0\) and \(k\cdot\aleph_0=\aleph_0\) for every positive integer \(k\), and indeed \(\aleph_0\cdot\aleph_0=\aleph_0\).
So arguments 2 and 3 fail in Cantorian arithmetic: adding a day, or multiplying by thirty, does not make an infinite set larger. Philoponus was assuming the Euclidean axiom that the whole is greater than the part, which fails for infinite sets. Argument 1 is different. It concerns the completion of an infinite sequence of successive events that ends now, a series with no first term. Modern philosophers still dispute it. Mathematically, the negative integers \(\dots,-3,-2,-1\) form a consistent infinite sequence that ends, with no first term, which suggests that the traversal argument needs more than mathematics to succeed.
The argument from finite power
Aristotle proved that a finite body cannot contain an infinite power (Physics VIII.10). The world is a finite body. Philoponus argued that it therefore cannot have in itself the power to exist for an infinite time; if it lasts, its continued existence must come from outside, from God. He here read “power” as a capacity to be, rather than a force to move. Simplicius objected that this changes the meaning of Aristotle’s term.
Afterlife of the arguments
Philoponus’s arguments passed into Arabic through translations and summaries. Al-Kindi used similar arguments from the infinite to prove that the world had a beginning, and the theologians of the kalam developed them. Al-Ghazali used them against the philosophers. In the Latin West, Bonaventure argued in the same way in the thirteenth century, while Thomas Aquinas held that reason alone can prove neither the eternity nor the beginning of the world.
Exercise 8.1Give an explicit bijection between the set of past days, indexed \(\{\dots,-2,-1,0\}\), and the set of past days with one more day added, \(\{\dots,-1,0,1\}\). Which of Philoponus’s arguments does this answer?
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Exercise 8.2Saturn completes 1 revolution for about every 29.5 solar years. Over an infinite past, set up a one-to-one correspondence between Saturn’s revolutions and the Sun’s. Then explain in what sense the Sun’s revolutions are “more numerous”, and why this notion of size differs from cardinality.
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Exercise 8.3Prove that the set of finite sequences of natural numbers is countable. Explain why this means that even the “product” of Saturn’s and the Sun’s revolutions, all pairs \((n,m)\), is no larger than either.
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Light as activity
For the general reader. Aristotle thought light was not a thing that moves but a state of the transparent medium, made actual by a source of fire. Philoponus reinterpreted this state as an activity, a kind of force sent out by a luminous body, which travels outward along straight lines and can even heat what it reaches. He used geometric rays going from the object to the eye, not from the eye outward.
- Understand Philoponus’s reinterpretation of Aristotle’s theory of light.
- State the law of reflection and its reversibility.
- Relate his idea of light as a kinetic activity to his theory of impressed force.
From state to activity
For Aristotle, light is the actuality of the transparent as transparent (On the Soul II.7). It is not a body and does not travel; the whole medium becomes lit at once. In his commentary on On the Soul and in the Physics commentary, Philoponus kept the claim that light is incorporeal but treated it as an activity (energeia) emitted by the luminous body, comparable to the incorporeal motive power impressed on a projectile. It spreads in straight lines, and he used it to explain why sunlight heats: the activity of the Sun warms the bodies it reaches.
He adopted the geometrical optics of rays, but reversed their direction: visual rays run from the object to the eye. In his discussion of reflection he noted that the geometry of a ray is the same whichever way it is traversed.
At a plane mirror, the reflected ray lies in the plane of the incident ray and the normal, and the angle of reflection equals the angle of incidence. The path is the shortest path from source to eye via the mirror (Heron of Alexandria), and it is reversible.
Exercise 9.1Prove Heron’s theorem: the path from point \(A\) to point \(B\), both above a plane mirror, that touches the mirror is shortest when the angles of incidence and reflection are equal.
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Exercise 9.2Philoponus, following Aristotle, did not assign a finite speed to light. Light takes about 8.3 minutes to reach us from the Sun. How far does the Sun move across the sky, as seen from Earth, in that time? Why would no one in antiquity have noticed the delay?
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The astrolabe
For the general reader. The astrolabe is a flat model of the sky: a brass disc on which the celestial sphere is drawn by a projection, with a rotating star map on top. It was used to tell the time, find the height of the Sun or a star, and solve problems of spherical astronomy without calculation. Philoponus wrote the oldest Greek treatise on its use and construction that has survived. The mathematics behind it, stereographic projection, has a remarkable property: it sends circles to circles.
- Define stereographic projection and prove that it maps circles on the sphere to circles or lines in the plane.
- Compute the radii of the circles on an astrolabe plate.
- Use the instrument to find time from a solar altitude.
Stereographic projection
Place the celestial sphere of radius \(R\) with its south pole \(S\). Project each point \(P\) of the sphere from \(S\) onto the plane of the equator: the image is where the line \(SP\) meets the plane. Points of the northern hemisphere land inside the equator circle; the south pole goes to infinity. Ptolemy described the projection in his Planisphaerium; the idea may go back to Hipparchus.
Stereographic projection maps every circle on the sphere not passing through \(S\) to a circle in the plane, and every circle through \(S\) to a straight line. It preserves angles (it is conformal).
Proof sketch. Use coordinates with the sphere \(x^2+y^2+z^2=R^2\) and \(S=(0,0,-R)\). The projection is \((x,y,z)\mapsto(u,v)=\frac{R}{R+z}(x,y)\). Its inverse sends \((u,v)\) to a point on the sphere whose coordinates are rational functions of \(u,v\) with common denominator \(u^2+v^2+R^2\). A circle on the sphere is the intersection with a plane \(ax+by+cz=d\). Substituting the inverse map and clearing the denominator gives an equation of the form \(\alpha(u^2+v^2)+\beta u+\gamma v+\delta=0\), which is a circle, or a line when \(\alpha=0\), which happens exactly when the plane passes through \(S\).
Circles on the plate
For a point at declination \(\delta\) on the meridian, the image lies at distance \(r=R\tan\!\big(45^\circ-\tfrac{\delta}{2}\big)\) from the centre. The equator (\(\delta=0\)) maps to the circle of radius \(R\), the Tropic of Cancer (\(\delta=+\varepsilon\)) inside it, and the Tropic of Capricorn (\(\delta=-\varepsilon\)) outside, usually forming the rim of the plate.
Exercise 10.1Take the obliquity of the ecliptic \(\varepsilon=23.5^\circ\) and an equator circle of radius 6 cm. Find the radii of the two tropics on the plate, and show that their product equals \(R^2\).
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Exercise 10.2The ecliptic is a great circle tilted by \(\varepsilon\) to the equator. On the plate it is a circle through the images of the two solstices, which lie on opposite sides of the centre on one diameter. Find its radius and the distance of its centre from the centre of the plate.
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Exercise 10.3At Alexandria (latitude \(\phi=31.2^\circ\)) on an equinox (\(\delta=0\)), the Sun is observed at altitude \(30^\circ\) in the morning. Use \(\sin h=\sin\phi\sin\delta+\cos\phi\cos\delta\cos H\) to find the hour angle \(H\) and the local solar time. This is the calculation an astrolabe performs mechanically.
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Theology and condemnation
From the 530s Philoponus wrote mainly as a Christian theologian. On the Creation of the World, his only theological work to survive complete in Greek, is a commentary on the creation narrative in Genesis, dedicated to Sergius, patriarch of Antioch. It defends a creation that includes the heavens against the literalist cosmology of Cosmas Indicopleustes, who held that the universe is shaped like the Tabernacle. Philoponus combined the account in Genesis with Greek astronomy and physics, including a spherical Earth and heavens, and his view that the heavenly bodies received their motion from God.
Christology
In the controversies over the nature of Christ that divided the Eastern Church after the Council of Chalcedon (451), Philoponus took the miaphysite side, which held that Christ has one nature from two. His Arbiter, written about 552–553, defended this position with Aristotelian logic just before the Second Council of Constantinople. He argued that a nature exists in reality only as a particular, an Aristotelian principle that he applied to theology.
Tritheism
Applied to the Trinity, the same principle seemed to imply that the Father, Son and Spirit have three particular natures. In On the Trinity (567) and related works, Philoponus was understood by his opponents to teach three gods, and his followers were called tritheists. He died around 570. More than a century later, in 680–681, the Third Council of Constantinople condemned him posthumously as a tritheist. The condemnation helps explain why his Greek works were little copied in Byzantium and why several survive only in Syriac or Arabic.
DiscussionPhiloponus used the same principle, that only particulars exist in reality, to criticize Aristotle’s physics and to formulate a theology that was condemned. Does the history of his reputation suggest that ideas in natural philosophy and theology were judged separately or together in late antiquity and Byzantium?
Yahya the Grammarian and the road to Galileo
In late antiquity
Simplicius’s replies, written in the late 530s, ensured that Philoponus’s arguments against the eternity of the world survived even where his books did not. They also set the tone of later Greek judgments: a clever polemicist who did not understand Aristotle. Simplicius kept the Aristotelian physics that Philoponus attacked.
In the Islamic world
As Yahya al-Nahwi, Philoponus was read in Arabic from the ninth century. Al-Kindi’s proofs that the world has a beginning draw heavily on his arguments from the infinite. Al-Farabi wrote a treatise against him, defending Aristotle on the heavens. Ibn Sina knew the theory of impressed force and reworked it as violent inclination (mayl) that does not decay by itself. Abu’l-Barakat al-Baghdadi kept Philoponus’s self-exhausting version. Ibn Bajja held a rule of motion close to his, in which a finite speed in a void is reduced by the medium. Al-Ghazali and the kalam theologians used arguments like his for creation in time. Ibn Rushd defended Aristotle against them.
In Latin Europe
Some of his commentaries were translated into Latin in the thirteenth century, and his arguments against eternity reached Bonaventure. In fourteenth-century Paris, Franciscus de Marchia proposed a self-spending impressed force and Jean Buridan a permanent impetus; both stand in the tradition Philoponus started, though they knew it mostly at second hand. Greek editions and Latin translations of his commentaries were printed in the sixteenth century. In his early treatise De motu (c. 1590), Galileo used a theory of self-decaying impressed force and named Philoponus among his authorities. Galileo’s later law of fall, with equal times for all weights in a void, went beyond Philoponus’s claim that the difference is very small.
Modern assessments
Pierre Duhem and later Shmuel Sambursky presented Philoponus as a forerunner of Galileo and of modern physics. Richard Sorabji, who organized the translation of the ancient commentators into English from the 1980s, and Christian Wildberg have emphasized both his originality and his place in the debates of his own century. His case is now a standard example of how criticism from within a tradition can prepare its replacement.
Final projectWrite a two-page comparison of Philoponus, Ibn Sina and Buridan on projectile motion. For each, state what keeps the projectile moving, whether that cause decays by itself, and what each concludes about motion in a void. Use the models of Lesson 04 and the Ibn Sina and Buridan courses, and finish with an assessment of the falling-bodies argument of Lesson 05 against Galileo’s law.
Connections
People linked to John Philoponus across this collection. A name without a link has no page here yet. See John Philoponus in the network of all 337 lives →
Teachers and advisors
- Ammonius, son of Hermias
Influenced by
Influenced
- Galileo Galilei
- Ibn Sina
- Jean Buridan
- Abu'l-Barakat al-Baghdadi
- al-Farabi
- al-Kindi
- Bonaventure
- Ibn Bajja (Avempace)
Rivals
- Simplicius
Also mentioned in this life
- Tycho Brahe
- Georg Cantor
- René Descartes
- Hipparchus
- Isaac Newton
- Plato
- Claudius Ptolemy
- Ole Rømer
- Evangelista Torricelli
Fields
- natural philosophy 12 lives
- mechanics 27 lives
- cosmology 7 lives
- astronomy 50 lives
- theology 8 lives
On CoursesHub
Sources and further reading
Biography and overview
- C. Wildberg, John Philoponus, Stanford Encyclopedia of Philosophy.
- S. Sambursky and C. Pearson, John Philoponus, Dictionary of Scientific Biography and New Dictionary of Scientific Biography.
- John Philoponus, Wikipedia.
- R. Sorabji (ed.), Philoponus and the Rejection of Aristotelian Science, Duckworth, 1987; 2nd ed., Institute of Classical Studies, 2010.
- K. Verrycken, The development of Philoponus’ thought and its chronology, in R. Sorabji (ed.), Aristotle Transformed, Duckworth, 1990.
Physics, cosmology and the astrolabe
- Philoponus, On Aristotle Physics, various translators, Ancient Commentators on Aristotle series, Duckworth / Bloomsbury.
- Philoponus, Corollaries on Place and Void, trans. D. Furley, with Simplicius, Against Philoponus on the Eternity of the World, trans. C. Wildberg, Duckworth, 1991.
- Philoponus, Against Aristotle on the Eternity of the World, trans. C. Wildberg, Duckworth, 1987.
- Philoponus, Against Proclus on the Eternity of the World, trans. M. Share and J. Wilberding, Ancient Commentators on Aristotle, 2004–2006.
- M. R. Cohen and I. E. Drabkin, A Source Book in Greek Science, Harvard University Press, 1948 (the falling-bodies passage).
- S. Sambursky, The Physical World of Late Antiquity, Routledge, 1962.
- R. Sorabji, Time, Creation and the Continuum, Duckworth, 1983.
- Theory of impetus, Wikipedia.
- H. A. Davidson, John Philoponus as a source of medieval Islamic and Jewish proofs of creation, Journal of the American Oriental Society 89 (1969).
- Philoponus, On the Use and Construction of the Astrolabe, ed. H. Hase (1839); English trans. in R. T. Gunther, The Astrolabes of the World, Oxford, 1932.