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Papers on History of Science
Carlos Mederos Martín
Fundación Canaria Orotava de Historia de la Ciencia

 

CONTENTS

 

Introduction

Some ways of understanding the didactic use of instruments:

The problem

The instrument

The asociated theorical knowledge

Theorem of leg

The solution to the problem

A didactic resource:

Parallactic ruler

The astrolabe

C. Huygens's clock

 

 

 

 

 

THE ROLE OF INSTRUMENTS IN THE TEACHING OF HISTORY OF SCIENCE

 

 

 

Introduction

In 1630 Galileo published his "Dialogue of the two maximum systems of Ptolemaic and Copernican world". In the third day, he says, referring to the Heliocentric Theory:

"I can not stop admiring the eminence of ingenuity of those who have received and accepted it as true... I can not find an end to my admiration, as I see how Aristarchus and Copernicus have been able to reason such violence against the senses, so that, against these, it has taken over their beliefs"

In effect, Aristarchus of Samos was an astronomer of the school of Alexandria who in the third century BC decided to measure the distance between the Earth and the Sun. For this he took advantage of the fact that, in the lunar quarters, the Sun, the Earth and the Moon are on the vertexes of a right angled triangle with the right angle at the Moon, in such a way that the segment Earth-Moon is the smaller leg, and the segment Earth-Sun is the hypotenuse. Aristarchus measured in this position the angle Earth-Sun-Moon (with vertex on the Earth), getting a value of 87º (this angle is really 89º 59’). Then he observed a right angled triangle with one of its acute angles measuring 87º, similar to the previous one, proving that the hypotenuse is twenty times longer than the smaller leg, and, therefore, as similar triangles have proportional sides, Aristarchus concluded that the distance Earth-Sun is twenty times longer than the distance Earth-Moon (really it is 370 times longer). He also observed, that the apparent sizes of the Sun and the Moon are approximately the same, with which, if the Sun is much further away than the Moon, it should be much bigger, and even bigger than the Earth (he had got the relation between the sizes of the Earth and the Moon by the means of other astronomical considerations; possibly observing the shadow of the Earth over the Moon during an eclipse). In these conditions, Aristarchus thought that it was not reasonable to suppose that such a big Sun revolves around a smaller Earth. This is how the first heliocentric model of the universe emerges.

In the above we can distinguish, on one hand, a change in the cosmological concept of the universe; on the other hand, geometrical figures are resorted to, the similarity, the proportions,...; but, what is there in between?... In between there is the measurement of an angle, only just one angle, that together with geometry allowed Cosmology to be changed: and, evidently, this angle was measured with a determined instrument.

Therefore, one of the possible ways of travelling through the History of Science is to do it through the study of the scientific instruments. In effect, we can consider Science as an "organism" whose working order leaves, through time, a trail made up by two main "products": written texts and the instruments. These are products quite appropriate for their "manipulation" and whose study can be tackled from different points of view, which gives them a high didactic applicability. The following diagram, that in a way, could be considered trivial intends to make a summary of the working order of the scientific "system":

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 In short, this diagram can be interpreted as the working order of an organism, Science, that through History leaves a trail of "exquisite waste", by means of which we can follow its "vital route".

In what follows we will concentrate on one of those products and its possible didactic applications: the instruments.

In first place we want to point out that we are talking about instruments in a "wide sense", this is, that we consider instrument any device capable of generating any kind of knowledge. So, a particle accelerator is an instrument, but a simple post stuck into the ground (a gnomon) or a numeric table, for example, are also instruments. Anyway, taking into consideration our didactic intentions, an aspect we consider important is the simplicity; or even better, the relation between simplicity and quantity of knowledge produced.

In second place we can see that instruments can be considered as a refinement of our senses, which acquire through them, bigger capacity for penetrating nature, increasing our power of observation, making induction processes easier, the establishment of speculations, of hypothesis, etc. And mainly, the achievement of measurements of magnitudes that can be represented in an abstract mathematical space in which axiomatic-deductive methods proper of mathematics can be applied, which allows us, in many cases to check, refute, or change statements established previously. In this way the instrument becomes the key that locks (or opens?) that eternal circle of happenings and mishaps, of doing and undoing (like Penelope), that we call Science.

Well now, how can we materialise these considerations in the frame of teaching the History of Science in secondary education? To answer this question we resort again to Galileo’s words. In the first day of the book "Considerations and mathematical demonstrations of two new sciences", published in 1638, Salviati (spokesman for the Academic) says to Sagredo and Simplicio:

SALVIATI: I think that the frequent activity in your famous arsenal, Venetian Gentleman, offers a great field for philosophising to the intellects that speculate, specially, in that part called mechanics, where continually all kinds of instruments and machinery are built by a great number of artisans, some of which have to be very knowledgeable and with a very acute talent due to both the observations made by their predecessors as by what they discover themselves without interruptions.

The meaning of this text can be interpreted as the recognition, by Galileo, that the scientific activity that emerges in the Renaissance is related with the abandoning of the elitist Greek prejudices against practical arts, as well as the increasing interest for mechanical problems related with artisan production, which makes scientific theories appear from the empirical discoveries accumulated by the tradition of the artisan workshops. In the same way, if we want our secondary pupils to acquire knowledge of the History of Science in a significant way, we also should abandon our "elitist Greek prejudices" (and we could add academical) and try to emulate the artisans, building even in a simple version, some instrument from which we could obtain empirical knowledge.

Thus, we propose to try to build the scientific knowledge of the pupils running over that trail of instruments left by science through history, stopping specially at some selected points; that is to say stopping at some instruments whose relation between simplicity and quantity of knowledge produced, mentioned before, is satisfactory and, also, distributed along the historical period to be studied. Each of these selected instruments will be the epistemological connection between a determined practical question, inserted in a determined era and with all the political, economical, religious, cosmological conditionings, etc, that are inherent to it on one hand and, on the other some kind of theoretic knowledge such as Geometry, Mechanics, Chemistry, etc. In this way the instrument becomes the nucleus around which the didactic activity concentrates, which can be tackled from different disciplines, that is to say, in a interdisciplinary way and aimed at a diversity of pupils because we use different activities adaptable to diverse intellectual capacities: use, construction, design, explanation of working order, theoretical fundaments etc. The above can be summarised in the following diagram:

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Here we have some examples of the didactical use of instruments with the intention of clarifying what was exposed before.

2. SOME WAYS OF UNDERSTANDING THE DIDACTIC USE OF INSTRUMENTS:

In the didactic application instruments can be considered from many points of view. Below we have some examples of different ways of understanding their use in the classroom that we consider especially interesting.

An instrument can be considered as: A generator of new knowledge of nature's behaviour with which we can solve problems.

Let's suppose we are studying the Science of the XVII century. One of the most significant themes of this era is the study of bodies in motion. In effect, during the XVI and XVII centuries the Aristotelian conceptions about motion are questioned and new ideas on the subject emerge, as for example the crystallisation of the Law of Inertia; which lead to new approaches, that together with the irruption of Mathematics as the language of Nature, sets the foundations of Modern Science. We can find all this, amongst others, in the work of Galileo, who in the third day of his book, mentioned before "Mathematical considerations and demonstrations of two new sciences", establishes definition s of constant motion and constantly accelerated motion that correspond to the essence of these two kinds of motion. This correspondence, says Galileo, "... we think we have accomplished it at last, after long reflections specially if we take into account that the properties that we have successively demonstrated, (from our definition) seem to correspond and coincide exactly with what natural experiments put in front of our senses. In short the study of naturally accelerated motion has led us, as if we were taken by the hand, to the observation of customs and rules that are followed by nature in all its remaining works, that for their performance the most immediate, simple and easiest means are usually used..."

So, in this context we will situate the following example, with the aim of illustrating the use of SCIENTIFIC INSTRUMENTS in the construction of knowledge and the solving of problems, from the point of view of the History of Science.

THE PROBLEM

If from the points P1, P2 and P3 we drop a body to the point A, following inclined planes, which of the three routes will be covered in less time?

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In order to solve this problem, we need a method to measure or compare the time that a body takes in sliding down each of the inclined planes. This, in the era that we have situated ourselves, represents a complicated technical problem, taking into consideration that the construction of precise clocks is not very advanced.

THE INSTRUMENT

Let's consider a circumference situated on a vertical plane, where various inclined planes have been built (in this case two), forming strings that meet at the lowest point of a vertical diameter. These have different inclinations, and on them we can release simultaneously two equal objects; for example, two crystal balls (to avoid, as far as possible, friction). In the following figure we can see a diagram of the instrument:

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With this instrument we can prove "empirically" that the falling time along all the strings considered, is the same. This means, that the instrument PRODUCES new knowledge: "the falling times along the strings that meet at the lowest point of a vertical diameter are all the same", or said in a different way, the mentioned strings are TAUTOCRONAS (from the Greek: equal time).

THE ASOCIATED THEORICAL KNOWLEDGE

But, as we have pointed out on the diagram, each instrument has some theoretical fundaments associated of a mechanical, geometrical or arithmetical nature, etc; accumulated through history, until the era in which we are situated. In the case of our instrument we can PROVE the property obtained empirically using the II and III theorems on naturally accelerated motion included in the third day of "Considerations and mathematical demonstrations of two new sciences" and the "Theorem of Leg" that we can find enunciated and demonstrated in the "Elements" of Euclid:

THEOREM II: If an object in motion falls, starting from rest with a constantly accelerated motion, the spaces covered by it in whatever time, are between each other like the quadrate of the times.

THEOREM III: If one and the same object in motion moves, starting from rest, upon an inclined plane and along a vertical one both having the same height, the times of motion between each other will be like the length of the plane and the vertical.

THEOREM OF LEG:

The leg is the proportional media between the hypotenuse and its projection upon it. Using the results above, we can do the following demonstration:

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To conclude, we will use the knowledge acquired through the instrument to solve the problem that we had set out:

THE SOLUTION TO THE PROBLEM

If we take into consideration the theoretical results acquired by means of the instrument, we can observe that the times that the moving object in sliding from the points Q, P2, R towards A, are the same. So the time from P2 to A is the shortest, because in the other inclined planes the moving object has to cover a supplementary space (the space outside the circumference), so the times will be longer. The following drawing shows the situation:

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2. A didactic resource:

It is to say, an object around which different activities can be organised aimed at diverse types of pupils. Around an instrument activities can be designed that range from handcraft (using tools for its construction) to the most abstract formalisation proper of geometry that explains its working order, passing through empirical activities (use of the instrument to make observations and to obtain information). This way we can try to solve one of the biggest problems product of the new educational legislation, that assures the access of education to all the society, independent of their social, economical, cultural conditions, etc, that means, on the one hand, an advance in social justice, but, on the other hand, results in teachers finding themselves in the classroom with some pupils who want to pursue universities studies, together with others that do not know what to do with their future, and others that do not even want to be in the classroom; However, something must be offered to each of them. So, we can start by proposing to those who do not want to be in the classroom, the construction of an instrument like the one in the following drawing (called

PARALLACTIC RULER):

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The instrument consists in a ruler AB length 1 with a longitudinal slot in which the extreme of the segment Pk, ½ long, slides, which is articulated at P with a segment AP of the same length as PK, and that can turn around point A. This way, to each angle with a vertex at A corresponds a segment of length AK, which can be used to indirectly measure the said angle.

Once built, it is very possible that we could convince one of the pupils unsure of his / her future, to try to use this instrument to measure angles, after those who are interested in achieving a certain level of knowledge have investigated the geometrical relation needed to be able to associate to each angle, a length on the ruler. In this way, the building up of knowledge, covers a process that goes from the use of hands (handcraft) up to certain levels of abstraction, passing through the acquisition of data about what surrounds us, using instruments (empirical knowledge).

3. A storeroom of knowledge, or what is the same, a book where the History of Science is written. To study Science means to study its history, its genesis; for this we must read these books, and so we must understand the language in which they are written : GEOMETRY.

A good example to illustrate this could be:

THE ASTROLABE

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It is very possible that astronomy appeared when someone combined the observation of the heavens with memory. If we observe the heavens on a clear night we can see an infinity of stars. If we observe it a while later we see that the position of the stars has changed, this is, we prove that there is motion in the heaven. Repeating the observation and memorising the previous positions of the different stars, the idea of trajectory appears; geometry of the cosmos appears, that later would become simply Geometry.

But something that moves spontaneously is not perfect, because if it moves, it is not occupying its place in an orderly cosmos. Does this mean that the cosmos is not perfect? To answer this question, let us observe, let us memorise, that is, let us do geometry.

In this way a trajectory appears that will forever determine the geometry of the cosmos: the circumference (the wheel?). In any other geometrical figure, if we make it rotate a certain angle, its points will abandon the initial figure; however, if we make a circumference rotate around its centre, its points will always remain within it, that is to say, it is inmutable, or in other words, it is closed in respect to the movement of rotation around its centre. In consequence, the only natural motion possible in an orderly and inmutable cosmos, is that which follows a circular trajectory, which made the circle and its extension to a tridimentional space, the sphere, arise as the basic geometrical figures for the construction of explicative models of the cosmos.

This is how the theories in the antiquity appear, ranging from Euxodus of Cnido ( IV Century BC), creator of the first model known that used concentric spheres to explain the motion of stars, to Ptolomy( II Century AD), who managed to project the celestial sphere upon a circle, which allowed him to build an instrument whose circular geometry reproduces "the working order" of the cosmos: the astrolabe, the noctolabe, etc.

These theories developed in the Hellenic world, together with the contributions of eastern cultures, as well as the techniques of construction of instruments, were assimilated and improved by the Arabs, and spread to western Europe during the Middle Ages.

Lastly, we can observe that the different "signs" which appear over the circles that constitute an astrolabe, are the traces left by the contributions made to astronomy over the centuries, so to understand its meaning (understand its working order), means to understand the history of astronomy, or what is the same, understand the genesis of the astronomical knowledge. And it is obvious that these signs are written in a geometrical language on circular books called astrolabe, noctolabe,...

4. The connection between a practical or theoretical problem set in the society at a determined era under economical, political, cultural religious conditions, etc; and a scientific, mathematical theory, more or less abstract. The study of this aspect of the instruments allows us to make interdisciplinary approaches, which involve matters related to all branches of knowledge.

C.HUYGEN'S CLOCK

One of the main problems that navigation encountered during the modern ages, was the exact determination of the position of ships at sea. In the XVI century the problem of the determination of latitude had been solved by the observation of the apparent height of the stars in the different points of the globe, this was not the case of longitude. The importance of this problem was such, due to its economical, political, and geographical implications, that for three centuries it turned into a permanent object of investigation and it was a real challenge for the science of that era.

From the XVI century the European monarchies were interested in the solution to this problem and international contests were held, with important prizes for a definite resolution; as well, official boards were created in order to discuss the available methods.

The first attempts at a solution came from Astronomy. In effect, the observation of astronomical happenings done simultaneously in different places allowed the position to be established easily. In this way the methods based upon the observation of sun and moon eclipses appeared, the one of Saturn's satellites, and especially, the method of the lunar distances.

The scarce results of these methods, together with the difficulty of calculus for the elaboration of tables, drew the attention towards the use of clocks that allowed the comparison of the time at the dock of departure with the time on the boat, deducing in this way, the difference of longitude.

One of the attempts to find a solution is due to Christian Huygens, who in the book "HORULOGIUM OSCILLATORUM", published in 1673, describes, among other things, the construction of a pendulum based on the properties of the cycloid curve that would work on a ship, independently of the movement of this due to the waves. It turns out to be a proposition of great "geometrical beauty" due to the surprising properties of the mentioned curve.

The theoretical knowledge associated to these instruments are mainly its mechanical properties, the BRACHISTOCRONY and the TAUTOCHRONY, and their geometrical properties; that can be found in the mentioned work of Huygens: "Horulogium Oscillatorum". These properties can be proved empirically with the instruments mentioned in the previous section, PROVED using the Euclidean geometry and the results of Galileo's study of motion of falling bodies.

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