HISTORY OF GREEK SCIENCE -1

Greek atmospheric devices: 1st century AD
                                    

Hero, a mathematician in Alexandria in about AD 75, enjoys inventing mechanical gadgets, which he describes in his work Pneumatica. Whether he has the technology to make them we do not know, but his scientific principles are correct.

One such gadget is a primitive version of a steam turbine. Hero says steam should be directed into a hollow globe with outlets through nozzles on opposite sides of the circumference. The nozzles are directed round the rim of the globe. As the steam rushes out, like sparks from a catherine wheel, the globe spins.

Hero makes another significant use of atmospheric pressure in a magic altar, putting to work the expansion and contraction of air. A fire heats the air in a container, causing it to expand and force water up a tube into a bucket. The increased weight of the bucket opens the doors of an altar. When the fire is extinguished, the air contracts, the water in the bucket is sucked out and the doors close.

Any temple managing to work this trick is certain to attract more pilgrims, and more money, than its rivals.

The influential errors of Ptolemy: 2nd century AD


Ptolemy, working in Alexandria in the 2nd century AD, is one of the great synthesizers of history. In several important fields (cosmology, astronomy, geography) he brings together in encyclopedic form an account of the received wisdom of his time.

His influence derives from the accident that his predecessors' works are lost while his have survived. Their achievements are known only through him, and when he disagrees with them it is usually he who is wrong. Just as in astronomy he wrongly adjusts the degree of precession of Hipparchus, so in geography he rejects Eratosthenes, whose calculation of the circumference of the earth is very close, and prefers instead another estimate which is 30% too small.

Ptolemy's astronomical work is divided into thirteen books. The first proves that the earth is the immovable centre of the universe; the last five describe the movement of the sun, moon and five planets, each attached to its own crystal sphere. By adding adjustments to reflect the erratic behaviour seen in the sky, Ptolemy achieves a system capable of satisfying scientific enquiry in the unscientific centuries of the Middle Ages.

His book becomes known as Ho megiste astronomas (Greek for 'the greatest astronomer'), or Megiste for short. The Arabs call it Al Megiste (the Megiste). Reaching northern Europe through the Arab civilization in Spain, it acquires its eventual title - as Ptolemy's Almagest.

In geography Ptolemy seems to offer what Hipparchus had proposed - the location of the world's natural and man-made features on a grid of 360° of latitude and longitude. He lists and places some 8000 towns, islands, rivers and mountains. But he is no more capable of providing accurate data, astronomically based, than Hipparchus was. The relative positions of his named features are calculated by collating travellers' accounts of the number of days taken on their journeys.

The results are wildly inaccurate. But the great prestige of Ptolemy means that with the revival of classical learning, in the Renaissance, his errors become enshrined in the earliest printed maps.

The influential errors of Galen: 2nd century AD


The newly appointed chief physician to the gladiators in Pergamum, in AD 158, is a native of the city. He is a Greek doctor by the name of Galen. The appointment gives him the opportunity to study wounds of all kinds. His knowledge of muscles enables him to warn his patients of the likely outcome of certain operations - a wise precaution recommended in Galen's Advice to doctors.

But it is Galen's dissection of apes and pigs which give him the detailed information for his medical tracts on the organs of the body. Nearly 100 of these tracts survive. They become the basis of Galen's great reputation in medieval medicine, unchallenged until the anatomical work of Vesalius.

Through his experiments Galen is able to overturn many long-held beliefs, such as the theory (first proposed by the Hippocratic school in about 400 BC, and maintained even by the physicians of Alexandria) that the arteries contain air - carrying it to all parts of the body from the heart and the lungs. This belief is based originally on the arteries of dead animals, which appear to be empty.

Galen is able to demonstrate that living arteries contain blood. His error, which will become the established medical orthodoxy for centuries, is to assume that the blood goes back and forth from the heart in an ebb-and-flow motion. This theory holds sway in medical circles until the time ofHarvey. 

The Greek legacy


By the time Ptolemy and Galen are putting into lasting form the fruits of Greek science in two important fields, astronomy and medicine, Rome has long displaced Greece as the dominant power in the Mediterranean and Middle East.

The relative scientific record of these two ancient civilizations is one of the amazing contrasts of history. From Miletus in the 6th century BC to Alexandria in the 2nd century AD, the Greeks produce a glittering stream of scientific experiment and speculation. In Rome's equivalently long period of wealth and power, there is political and military genius in abundance but not a scientist to be seen.

After the official establishment of Christianity in the Byzantine empire, in the 4th century, the Greeks themselves become more interested in theological than scientific speculation. And with the fall of classical civilization toGerman tribes in the west and to Arabs in the east, it seems at first that the Greek scientific legacy may be lost in the widespread destruction of the 5th to 7th centuries.

But the Arab conquerors, establishing their own civilization in previously Byzantine lands, develop an interest in the old Greek texts. In Arabic translation, Greek manuscripts find their way through Spain to a western Europe ready, by about 1200, for a renewed interest in scientific theory (seeGreek texts and the Arabs).


When the texts begin to circulate among the learned in medieval monasteries, it is soon clear how broad a basis has been provided by the Greeks. In fields capable of proof by theorem, such as geometry and mathematics, answers are available in surviving texts of Euclid and Archimedes. In areas where accurate observation is required, Aristotle's work in natural history offers a model of the appropriate method. And in two subjects of absorbing interest, astronomy and medicine, Ptolemy and Galen will stimulateCopernicus and Vesalius to fruitful disagreement.

Medieval science, recovering the Greek texts, is not inclined to experiment. But the springboard is in place for a new attitude to science in the Renaissance.

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Hipparchus, a scientific astronomer: 2nd century BC
       

An observatory is erected by Hipparchus on the island of Rhodes. Here, in 129 BC, he completes the first scientific star catalogue. He lists about 850 stars, placing each in terms of its celestial latitude and longitude and recording its relative brightness on a scale of six.


He measures the altitude of a star by means of an astrolabe, a revolving calibrated disc which will be used for this purpose for nearly two millennia. It is invented either by Hipparchus himself or by his 3rd-century predecessor, Apollonius of Perga. Hipparchus also imagines another use for his astronomical instruments, to createmaps of the earth's surface. But this is a task even more demanding than his charting of the heavens.


Hipparchus is so accurate in his placing of the stars that he becomes the first scientist to observe an important phenomenon. Although almost fixed in relation to the sun, the stars move gradually over a long period. This means that at any repeated and identifiable moment in the sun's year, such as the equinox (when day and night are of equal length), the star positions will be seen to have shifted very slightly.


Hipparchus observes this effect in relation to the equinox, and calculates that there is a shift each year of about 45 seconds of arc. It is a phenomenon known now as precession, or the precession of the equinoxes.

Hipparchus has no way of explaining this phenomenon (which is due to a slow wobble of the earth's axis, completing one cycle every 26,000 years), but his accuracy is astonishing. Modern measurements give a figure close to 50 seconds of arc. His 45 seconds are only about 10% out.


The works of Hipparchus are lost. They are known only through the use made of them by Ptolemy, a much less scientific astronomer whose influence derives from the encyclopedic nature of his work. Ptolemy acknowledges the greatness of Hipparchus, and fails lamentably when he tries to improve on his predecessor. Attempting to make the figure for precession more accurate, he moves in the wrong direction - and comes up with 36 seconds of arc.



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The circumference of the earth: calculated c. 220 BC

Eratosthenes, the librarian of themuseum at Alexandria, has more on his mind than just looking after the scrolls. He is making a map of the stars (he will eventually catalogue nearly 700), and he is busy with his search for prime numbers; he does this by an infinitely laborious process now known as the Sieve of Eratosthenes.


But his most significant project is working out the circumference of the earth.

Eratosthenes hears that in noon at midsummer the sun shines straight down a well at Aswan, in the south of Egypt. He finds that on the same day of the year in Alexandria it casts a shadow 7.2 degrees from the vertical. If he can calculate the distance between Aswan and Alexandria, he will know the circumference of the earth (360 degrees instead of 7.2 degrees, or 50 times greater).


He discovers that camels take 50 days to make the journey from Aswan, and he measures an average day's walk by this fairly predictable beast of burden. It gives him a figure of about 46,000 km for the circumference of the earth. This is, amazingly, only 15% out (40,000 km is closer to the truth).

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The earth and the sun: a heresy of the 3rd century BC


A lone voice on the Greek island of Samos. In about 270 BC Aristarchus is busy trying to work out the size of the sun and the moon and their distance from the earth. His only surviving work is on this topic, and his calculations are inevitably wide of the mark.


But references in other authors make it clear that his studies have brought him to a startling conclusion. 

Aristarchus believes that the earth is in orbit round the sun (quite contrary to what is plain for anyone to see). There is an attempt, which comes to nothing, to have the man prosecuted for impiety. His idea joins the many other dotty notions which enliven the history of human thought, untilCopernicusmentions him, in an early draft of his great book, as someone who had the right idea first.


On reflection Copernicus drops the name of Aristarchus from later versions of the text.


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Greek science in Alexandria: from the 3rd century BC


Classical Greece has produced a brilliant tradition of theorists, the dreamers of science. Attracted by the intellectual appeal of good theories, they are disinclined to engage in the manual labour of the laboratory where those theories might be tested.


This limitation is removed when the centre of the Greek world transfers, in the 3rd century BC, to Alexandria. In this bustling commercial centre, linked with long Egyptian traditions of skilled work in precious metals, people are interested in making practical use of Greek scientific theory. IfAristotlesays that the difference in material substances is a matter of balance, then that balance might be changed. Copper might become gold.


Among the practical scientists of Alexandria are men who can be seen as the first alchemists and the first experimental chemists. Their trade, as workers in precious metals, involves melting gold and silver, mixing alloys, changing the colour of metals by mysterious process.


These are the activities of chemistry. The everyday items of a chemical laboratory - stills, furnaces, flasks - are all in use in Alexandria.


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Euclid and Archimedes: 3rd century BC

                  

Euclid teaches in Alexandria during the reign of Ptolemy. No details of his life are known, but his brilliance as a teacher is demonstrated in theElements, his thirteen books of geometrical theorems. Many of the theorems derive from Euclid's predecessors (in particularEudoxus), but Euclid presents them with a clarity which ensures the success of his work. It becomes Europe's standard textbook in geometry, retaining that position until the 19th century.


Archimedes is a student at Alexandria, possibly within the lifetime of Euclid. He returns to his native Syracuse, in Sicily, where he far exceeds the teacher in the originality of his geometrical researches.

    The fame ofArchimedes history and legend derives largely from his practical inventions and discoveries, but he himself regards these as trivial compared to his work in pure geometry. He is most proud of his calculations of surface area and of volume in spheres and cylinders. He leaves the wish that his tomb be marked by a device of a sphere within a cylinder. 

A selection of titles from his surviving treatises suggests well his range of interests: On the Sphere and the Cylinder; On Conoids and Spheroids; On Spirals; The Quadrature of the Parabola; or, closer to one of his practical discoveries,On Floating Bodies.


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The Hippocratic Oath and the four humours: 4th c. BC


Hippocrates practises and teaches medicine in about 400 BC on the Greek island of Kos. He will later be regarded as the father of medicine - partly because he is unlike his more theoretical contemporaries in paying close attention to the symptoms of disease, but also because a century or more after his death a group of medical works is gathered together under his name.


This Hippocratic Collection, and in particular theHippocratic oath which is part of it, has remained the broad basis of medical principle up to our own day.

A slightly later Greek text, called On the Nature of Manand attributed to an author by the name of Polybus, introduces a medical theory which will be orthodox in Europe for some 2000 years. It states that human beings are composed of four substances or 'humours', just as inanimate matter is made up of four elements. India has asimilar theorybased on three.


The humours are blood, phlegm, black bile (melancholia) and yellow bile (chole). Too much of any one will give a person certain recognizable characteristics. He or she will be sanguine, phlegmatic, melancholy or choleric.

Aristotle's variable atoms: 4th century BC


Aristotle, practical as ever in his determination to get things worked out in detail, proposes a new theory to explain how the four elements ofEmpedoclesand the atoms of Democritusproduce the wide range of substances apprehended by our senses.


He suggests that there are two pairs of alternatives - hot and cold, moist and dry - which provide the exact nature of matter. In broad terms the four possible combinations are the four elements: earth (cold and dry), air (hot and moist), fire (hot and dry), water (cold and moist). But it is the infinitely variable balance between these qualities which creates the different atoms of stone or wood, bone or flesh.

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The birth of biology: 5th - 4th century BC

The Greek philosophers, voracious in their curiosity, look with interest at the range of living creatures, from the humblest plant to man himself. A Greek name is coined by a German naturalist in the early 19th century for this study of all physical aspects of natural life - biology, frombios (life) andlogos (word or discourse). It is a subject with clear subdivisions, such as botany, zoology or anatomy. But all are concerned with living organisms.


The first man to make a significant contribution in biology is Alcmaeon, living inCrotona in the 5th century. Crotona is famous at the time for its Pythagorean scholars, but Alcmaeon seems not to have been of their school. 

Alcmaeon is the first scientist known to have practised dissection in his researches. His aim is not anatomical, for his interest lies in trying to find the whereabouts of human intelligence. But in the course of his researches he makes the first scientific discoveries in the field of anatomy.


The subsequent Greek theory, subscribed to even byAristotle, is that the heart is the seat of intelligence. Alcmaeon reasons that since a blow to the head can affect the mind, in concussion, this must be where reason lies. In dissecting corpses to pursue this idea, he observes passages linking the brain with the eyes (the optic nerves) and the back of the mouth with the ears (Eustachian tubes). 

Aristotle may be wrong about the brain being in the heart, but in general he gives a far more complete and well observed account of biology than any other Greek philosopher.


He inaugurates scientific zoology in his reliance on careful observation. He is particularly acute in his study of marine life, having much to say on the habits of fishes, the development of the octopus family, and the nature of whales, dolphins and porpoises. He is also a pioneer in attempting a system ofclassification. Observing an unbroken chain of gradual developments, as the life of plants shades into that of animals, he acknowledges the complexity of the subject and seems almost to glimpse the pattern of evolution.


Aristotle's notes on botany are lost, but many of his observations no doubt survive in the earliest known botanical text - nine booksOn the History of Plantswritten by Aristotle's favourite pupil,Theophrastus.


Writing in about 300 BC, Theophrastus attempts to classify plants, as well as describing their structure, habits and uses. His remarks are based on observations carried out in Greece, but he also includes information brought back from the newHellenisticempire in the Middle East, Persia and India, resulting from the conquests of Alexander the Great.

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Democritus and the atom: c.420 BC


In the late 5th century BC Democritus sets out an interesting theory of elemental physics. Notions of a similar kind have been hinted at by other Greek thinkers, but never so fully elaborated.


He states that all matter is composed of eternal, indivisible, indestructible and infinitely small substances which cling together in different combinations to form the objects perceptible to us. The Greek word for indivisible is atomos. This theory gives birth to the atom.

Democritus describes an extraordinary beginning to the universe. He explains that originally all atoms were whirling about in a chaotic manner, until collisions brought them together to form ever larger units - including eventually the world and all that is in it.


His theory will find few followers over the centuries. But his imagination provides an astonishing first glimpse of the Big Bang.


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The Pythagoreans and astronomy: 5th century BC
Followers of Pythagoras, in the 5th century, are the first to produce an astronomical theory in which a circular earth revolves on its own axis as well as moving in an orbit. The theory derives in part from the need to locate the great fire which they believe fuels the universe.


The Pythagoreans place this fire at the hidden centre of things, with the earth revolving round it more closely than any of the other bodies visible in the sky. The reason why we never see or are scorched by the fire is that we live on only half the sphere of the earth, and the earth revolves so that our half is always turned away from the flames.

Moving outwards from the earth in the sequence of heavenly bodies, they place the moon next, then the sun, the planets and finally the stars, which are unlike the others in being fixed on an outer sphere.

Heavenly spheres: from the 5th century BC


This theory introduces the concentric circles which become the false orthodoxy of the next 2000 years, as eventually enshrined by Ptolemy. It also starts a wild goose chase which will exercise many brilliant minds: what mechanical model can explain the erratic motion of the planets? Eudoxus of Cnidus, in the 4th century, is the first to propose a series of transparent spheres in the heavens, carrying the heavenly bodies at different speeds in linked groups with slightly varying centres.


To make such machinery conform to what can be observed in the sky, ever more complex arrangements are needed. Later in the 4th century Aristotle believes he has solved it. He requires no fewer than fifty-five transparent spheres.


The Pythagoreans are too far ahead of their time in proposing their one central grain of truth - the revolving globe of the earth. ButCopernicus, developing this idea, will acknowledge them as his earliest predecessors.


For most Greek astronomers there seems to be overwhelming evidence that the earth is stationary and the heavens move. This is true even of the greatest among them, Hipparchus. Like his predecessors, he believes that it must be possible to analyze the movement of the spheres. He finds the available data inadequate, so devotes himself not to cosmology but to the prime task of an astronomer - observation of individual stars.

The four elements: c.450 BC
The Greek philosopher Empedocles, a native of Sicily, introduces a theory which will be accepted in Europe until the 17th century. He states that all matter is made up, in differing proportions, of four elemental substances - earth, air, fire and water. Not until the arrival of a 'sceptical chemist' (the title of a book by Robert Boyle in 1661) is there a serious threat to this Greek theory of the elements.


Soon an equivalently simple notion is put forward to account for the make-up of living creatures, in the theory of the four humours.

Electricity and magnetism: 5th century BC


Two natural phenomena, central to the study of physics, are observed and speculated upon by Greek natural scientists - probably in the 5th century BC, though Aristotle gives credit for the first observation of each to the shadowy figure ofThales.


One such phenomenon is the strange property of amber. If rubbed with fur it will attract feathers or bits of straw. Modern science, in its terms for the forces involved, acknowledges this Greek experiment with amber (electron in Greek). The behaviour of the amber is caused by what we call electricity, resulting from the transfer of what are now known as electrons.

The other natural phenomenon, observed in lodestone rather than  amber, also derives its scientific name from Greek experiments. Lodestone is a naturally occurring mineral (formed of iron oxide), and it will surprisingly attract small pieces of iron. .

The Greeksfind this mineral in a region of Thessaly called Magnesia. They call itlithos magnetis, the 'stone of Magnesia'. Thus the magnet is identified and named, though like rubbed amber it will only be a source of interest and amusement for the next 1000 years and more - until a practical purpose is found for it in the form of the compass.



Democritus and the atom: c.420 BC

In the late 5th century BC Democritus sets out an interesting theory of elemental physics. Notions of a similar kind have been hinted at by other Greek thinkers, but never so fully elaborated.


He states that all matter is composed of eternal, indivisible, indestructible and infinitely small substances which cling together in different combinations to form the objects perceptible to us. The Greek word for indivisible isatomos. This theory gives birth to the atom. 

Democritus describes an extraordinary beginning to the universe. He explains that originally all atoms were whirling about in a chaotic manner, until collisions brought them together to form ever larger units - including eventually the world and all that is in it.


His theory will find few followers over the centuries. But his imagination provides an astonishing first glimpse of the Big Bang.

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The universe of the Greeks: from the 6th century BC


The Greek interest in scientific speculation is first seen in the city of Miletus, in Ionia. Here the philosopher Thales acquires fame by predicting a solar eclipse in 585 BC. None of his works survive, but his reputation among Greeks in the following centuries is that of a man who takes a reasonable or 'scientific' approach to the mysteries of the natural world. 


This reputation seems to be supported by the achievements of his pupil Anaximander. He is credited with being the first man to attempt a map of the world, and he offers a bold explanation of the origin of the universe. 

In Anaximander's theory the cosmos results from a struggle between the opposites of heat and cold. In the vast unlimited beginning of time the two begin to separate, resulting in a ball of fire surrounded by mist. The hot ball contracts and hardens, forming a solid sphere at the centre - the earth.


But the separation is not perfect. Some outer rings of fire trap layers of mist within them. The mist is our atmosphere. Through gaps in it we catch glimpses of the surrounding fire, in the form of sun, moon and stars.

If later accounts of Anaximander's ideas are correct (only a single sentence of his work remains), he even imagines a version of gravity. He says that the earth can remain unsupported at the centre of this system, by reason of its equal distance from the surrounding bodies.


Anaximander's concept of thebeginning of life is equally astonishing. He argues that humans cannot always have existed (our infants are too defenceless). The first living creatures, he believes, develop in water through the action of heat. They resemble sea urchins. Humans do not evolve from these urchins, but arrive later in a more welcoming environment.

The geographers of Miletus: 6th century BC


Nothing is known of the map of the world supposedly produced in Miletus by Anaximander in the mid-6th century BC. But by the end of the century, also in Miletus, another geographer writes a book of which sufficient details survive for his ideas to be reconstructed. He is Hecataeus.


Like most early mapmakers, Hecataeus puts the most important place at the centre of the world. For medieval Christian cartographers this isJerusalem. For Hecataeus it is the Aegean Sea, on the east coast of which stands Miletus.

 

The shape of the world according to Hecataeus has a geometrical simplicity. It is a flat circle, with a continuous ocean forming the rim. The circular land mass is divided into two parts by an almost unbroken stretch of water linked with the ocean on the west at the straits of Gibraltar, then running east the length of the Mediterranean, through the Black Sea and (after a short land bridge) into the Caspian Sea, which joins the ocean on the east.


The semicircle of land above this belt of water is Europe, while the semicircle below is Asia. The part west of the Nile has the subsidiary name of Libya, standing in for Africa.

Hecataeus is at the end of a pioneering century of Greek science in Miletus, which lies to the east of mainland Greece. At the same period a new centre of Greek scientific speculation is being developed far to the west, in the Pythagorean tradition of southern Italy.


Greek philosophy is strongly associated with Athens, because of Socrates, Plato and Aristotle. But scientific history testifies rather more to the colonial spread of Greek culture round the Mediterranean. Ionia and Samos, Italy and Sicily, Alexandria; these are the places where Greeks will establish the rational traditions of western science.

Pythagoras: 6th century BC


Ancient mathematics has reached the modern world largely through the work of Greeks in the classical period, building on the Babylonian tradition. A leading figure among the early Greek mathematicians is Pythagoras.


In about 529 BC Pythagoras moves from Greece to a Greek colony at Crotona, in the heel of Italy. There he establishes a philosophical sect based on the belief that numbers are the underlying and unchangeable truth of the universe. He and his followers soon make precisely the sort of discoveries to reinforce this numerical faith.

The Pythagoreans can show, for example, that musical notes vary in accordance with the length of a vibrating string; whatever length of string a lute player starts with, if it is doubled the note always falls by exactly an octave (still the basis of the scale in music today).


The followers of Pythagoras are also able to prove that whatever the shape of a triangle, its three angles always add up to the sum of two right angles (180 degrees).


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