Two New Sciences

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Discourses and Mathematical Demonstrations Relating to Two New Sciences
Galileo Galilei, Discorsi e Dimostrazioni Matematiche Intorno a Due Nuove Scienze, 1638 (1400x1400).png
Author Galileo Galilei
LanguageItalian, Latin
Published1638

The Discourses and Mathematical Demonstrations Relating to Two New Sciences (Italian : Discorsi e dimostrazioni matematiche intorno a due nuove scienzepronounced [diˈskorsieddimostratˈtsjoːnimateˈmaːtikeinˈtornoadˈduːeˈnwɔːveʃˈʃɛntse] ) published in 1638 was Galileo Galilei's final book and a scientific testament covering much of his work in physics over the preceding thirty years. It was written partly in Italian and partly in Latin.

Contents

After his Dialogue Concerning the Two Chief World Systems , the Roman Inquisition had banned the publication of any of Galileo's works, including any he might write in the future. [1] After the failure of his initial attempts to publish Two New Sciences in France, Germany, and Poland, it was published by Lodewijk Elzevir who was working in Leiden, South Holland, where the writ of the Inquisition was of less consequence (see House of Elzevir). [2] Fra Fulgenzio Micanzio, the official theologian of the Republic of Venice, had initially offered to help Galileo publish the new work there, but he pointed out that publishing the Two New Sciences in Venice might cause Galileo unnecessary trouble; thus, the book was eventually published in Holland. Galileo did not seem to suffer any harm from the Inquisition for publishing this book since in January 1639, the book reached Rome's bookstores, and all available copies (about fifty) were quickly sold. [3]

Discourses was written in a style similar to Dialogues, in which three men (Simplicio, Sagredo, and Salviati) discuss and debate the various questions Galileo is seeking to answer. There is a notable change in the men, however; Simplicio, in particular, is no longer quite as simple-minded, stubborn and Aristotelian as his name implies. His arguments are representative of Galileo's own early beliefs, as Sagredo represents his middle period, and Salviati proposes Galileo's newest models.

Introduction

The book is divided into four days, each addressing different areas of physics. Galileo dedicates Two New Sciences to Lord Count of Noailles. [4]

Figure 1 out of Galileo's Two New Sciences in the First Day section Fig1DM.png
Figure 1 out of Galileo's Two New Sciences in the First Day section

In the First Day, Galileo addressed topics that were discussed in Aristotle's Physics and also the Aristotelian school Mechanics. It also provides an introduction to the discussion of both of the new sciences. The likeness between the topics discussed, specific questions that are hypothesized, and the style and sources throughout give Galileo the backbone to his First Day. The First Day introduces the speakers in the dialogue: Salviati, Sagredo, and Simplicio, the same as in the Dialogue. These three people are all Galileo just at different stages of his life, Simplicio the youngest and Salviati, Galileo's closest counterpart. The Second Day addresses the question of the strength of materials.

The Third and Fourth days address the science of motion. The Third day discusses uniform and naturally accelerated motion, the issue of terminal velocity having been addressed in the First day. The Fourth day discusses projectile motion.

In Two Sciences uniform motion is defined as a motion that, over any equal periods of time, covers equal distance. With the use of the quantifier ″any″, uniformity is introduced and expressed more explicitly than in previous definitions. [5]

Galileo had started an additional day on the force of percussion, but was not able to complete it to his own satisfaction. This section was referenced frequently in the first four days of discussion. It finally appeared only in the 1718 edition of Galilei's works. [6] and it is often quoted as "Sixth Day" following the numbering in the 1898 edition. [7] During this additional day Simplicio was replaced by Aproino, a former scholar and assistant of Galileo in Padua.

Summary

Page numbers at the start of each paragraph are from the 1898 version, [7] presently adopted as standard, and are found in the Crew and Drake translations.

Day one: Resistance of bodies to separation

[50] Preliminary discussions. Sagredo (taken to be the younger Galileo) cannot understand why with machines one cannot argue from the small to the large: "I do not see that the properties of circles, triangles and...solid figures should change with their size". Salviati (speaking for Galileo) says the common opinion is wrong. Scale matters: a horse falling from a height of 3 or 4 cubits will break its bones whereas a cat falling from twice the height won't, nor will a grasshopper falling from a tower.

[56] The first example is a hemp rope which is constructed from small fibres which bind together in the same way as a rope round a windlass to produce something much stronger. Then the vacuum that prevents two highly polished plates from separating even though they slide easily gives rise to an experiment to test whether water can be expanded or whether a vacuum is caused. In fact, Sagredo had observed that a suction pump could not lift more than 18 cubits of water and Salviati observes that the weight of this is the amount of resistance to a void. The discussion turns to the strength of a copper wire and whether there are minute void spaces inside the metal or whether there is some other explanation for its strength.

[68] This leads into a discussion of infinites and the continuum and thence to the observation that the number of squares equal the number of roots. He comes eventually to the view that "if any number can be said to be infinite, it must be unity" and demonstrates a construction in which an infinite circle is approached and another to divide a line.

[85] The difference between a fine dust and a liquid leads to a discussion of light and how the concentrated power of the sun can melt metals. He deduces that light has motion and describes an (unsuccessful) attempt to measure its speed.

[106] Aristotle believed that bodies fell at a speed proportional to weight but Salviati doubts that Aristotle ever tested this. He also did not believe that motion in a void was possible, but since air is much less dense than water Salviati asserts that in a medium devoid of resistance (a vacuum) all bodies—a lock of wool or a bit of lead—would fall at the same speed. Large and small bodies fall at the same speed through air or water providing they are of the same density. Since ebony weighs a thousand times as much as air (which he had measured), it will fall only a very little more slowly than lead which weighs ten times as much. But shape also matters—even a piece of gold leaf (the densest of all substances [asserts Salviati]) floats through the air and a bladder filled with air falls much more slowly than lead.

[128] Measuring the speed of a fall is difficult because of the small time intervals involved and his first way round this used pendulums of the same length but with lead or cork weights. The period of oscillation was the same, even when the cork was swung more widely to compensate for the fact that it soon stopped.

[139] This leads to a discussion of the vibration of strings and he suggests that not only the length of the string is important for pitch but also the tension and the weight of the string.

Day two: Cause of cohesion

[151] Salviati proves that a balance can not only be used with equal arms but with unequal arms with weights inversely proportional to the distances from the fulcrum. Following this he shows that the moment of a weight suspended by a beam supported at one end is proportional to the square of the length. The resistance to fracture of beams of various sizes and thicknesses is demonstrated, supported at one or both ends.

[169] He shows that animal bones have to be proportionately larger for larger animals and the length of a cylinder that will break under its own weight. He proves that the best place to break a stick placed upon the knee is the middle and shows how far along a beam that a larger weight can be placed without breaking it.

[178] He proves that the optimum shape for a beam supported at one end and bearing a load at the other is parabolic. He also shows that hollow cylinders are stronger than solid ones of the same weight.

Day three: Naturally accelerated motion

[191] He first defines uniform (steady) motion and shows the relationship between speed, time and distance. He then defines uniformly accelerated motion where the speed increases by the same amount in increments of time. Falling bodies start very slowly and he sets out to show that their velocity increases in simple proportionality to time, not to distance which he shows is impossible.

[208] He shows that the distance travelled in naturally accelerated motion is proportional to the square of the time. He describes an experiment in which a steel ball was rolled down a groove in a piece of wooden moulding 12 cubits long (about 5.5m) with one end raised by one or two cubits. This was repeated, measuring times by accurately weighing the amount of water that came out of a thin pipe in a jet from the bottom of a large jug of water. By this means he was able to verify the uniformly accelerated motion. He then shows that whatever the inclination of the plane, the square of the time taken to fall a given vertical height is proportional to the inclined distance.

[221] He next considers descent along the chords of a circle, showing that the time is the same as that falling from the vertex, and various other combinations of planes. He gives an erroneous solution to the brachistochrone problem, claiming to prove that the arc of the circle is the fastest descent. 16 problems with solutions are given.

Day four: The motion of projectiles

Last figure of the Fourth Day of Galileo's Two New Sciences BilanciaGalilei2.png
Last figure of the Fourth Day of Galileo's Two New Sciences

[268] The motion of projectiles consists of a combination of uniform horizontal motion and a naturally accelerated vertical motion which produces a parabolic curve. Two motions at right angles can be calculated using the sum of the squares. He shows in detail how to construct the parabolas in various situations and gives tables for altitude and range depending on the projected angle.

[274] Air resistance shows itself in two ways: by affecting less dense bodies more and by offering greater resistance to faster bodies. A lead ball will fall slightly faster than an oak ball, but the difference with a stone ball is negligible. However the speed does not go on increasing indefinitely but reaches a maximum. Though at small speeds the effect of air resistance is small, it is greater when considering, say, a ball fired from a cannon.

[292] The effect of a projectile hitting a target is reduced if the target is free to move. The velocity of a moving body can overcome that of a larger body if its speed is proportionately greater than the resistance.

[310] A cord or chain stretched out is never level but also approximates to a parabola. (But see also catenary.)

Additional day: The force of percussion

[323] What is the weight of water falling from a bucket hanging on a balance arm onto another bucket suspended to the same arm?

[325] Piling of wooden poles for foundations; hammers and the force of percussion.

[336] Speed of fall along inclined planes; again on the principle of inertia.

Methodology

Many contemporary scientists, such as Gassendi, dispute Galileo's methodology for conceptualizing his law of falling bodies. Two of the main arguments are that his epistemology followed the example of Platonist thought or hypothetico-deductivist. It has now been considered to be ex suppositione, or knowing the how and why effects from past events in order to determine the requirements for the production of similar effects in the future. Galilean methodology mirrored that of Aristotelian and Archimedean epistemology. Following a letter from Cardinal Bellarmine in 1615 Galileo distinguished his arguments and Copernicus' as natural suppositions as opposed to the "fictive" that are "introduced only for the sake of astronomical computations," such as Ptolemy's hypothesis on eccentrics and equants. [8]

Galileo's earlier writing considered Juvenilia, or youthful writings, are considered his first attempts at creating lecture notes for his course "hypothesis of the celestial motions" while teaching in at the University of Padua. These notes mirrored those of his contemporaries at the Collegio as well as contained an "Aristotelian context with decided Thomistic (St. Thomas Aquinas) overtones." [9] These earlier papers are believed to have encouraged him to apply demonstrative proof in order to give validity to his discoveries on motion.

Discovery of folio 116v gives evidence of experiments that had previously not been reported and therefore demonstrated Galileo's actual calculations for the Law of Falling Bodies.

His methods of experimentation have been proved by the recording and recreation done by scientists such as James MacLachlan, Stillman Drake, R.H. Taylor and others in order to prove he did not merely imagine his ideas as historian Alexandre Koyré argued, but sought to prove them mathematically.

Galileo believed that knowledge could be acquired through reason, and reinforced through observation and experimentation. Thus, it can be argued that Galileo was a rationalist, and also that he was an empiricist.

The two new sciences

The two sciences mentioned in the title are the strength of materials and the motion of objects (the forebears of modern material engineering and kinematics). [10] In the title of the book "mechanics" and "motion" are separate, since at Galileo's time "mechanics" meant only statics and strength of materials. [11]

The science of materials

The discussion begins with a demonstration of the reasons that a large structure proportioned in exactly the same way as a smaller one must necessarily be weaker known as the square–cube law. Later in the discussion this principle is applied to the thickness required of the bones of a large animal, possibly the first quantitative result in biology, anticipating J. B. S. Haldane's work On Being the Right Size, and other essays, edited by John Maynard Smith.

The motion of objects

Galileo expresses clearly for the first time the constant acceleration of a falling body which he was able to measure accurately by slowing it down using an inclined plane.

In Two New Sciences, Galileo (Salviati speaks for him) used a wood molding, "12 cubits long, half a cubit wide and three finger-breadths thick" as a ramp with a straight, smooth, polished groove to study rolling balls ("a hard, smooth and very round bronze ball"). He lined the groove with "parchment, also smooth and polished as possible". He inclined the ramp at various angles, effectively slowing down the acceleration enough so that he could measure the elapsed time. He would let the ball roll a known distance down the ramp, and use a water clock to measure the time taken to move the known distance. This clock was

a large vessel of water placed in an elevated position; to the bottom of this vessel was soldered a pipe of small diameter giving a thin jet of water, which we collected in a small glass during the time of each descent, whether for the whole length of the channel or for a part of its length. The water collected was weighed, and after each descent on a very accurate balance, the differences and ratios of these weights gave him the differences and ratios of the times. This was done with such accuracy that although the operation was repeated many, many times, there was no appreciable discrepancy in the results. [12]

The law of falling bodies

While Aristotle had observed that heavier objects fall more quickly than lighter ones, in Two New Sciences Galileo postulated that this was due not to inherently stronger forces acting on the heavier objects, but to the countervailing forces of air resistance and friction. To compensate, he conducted experiments using a shallowly inclined ramp, smoothed so as to eliminate as much friction as possible, on which he rolled down balls of different weights. In this manner, he was able to provide empirical evidence that matter accelerates vertically downward at a constant rate, regardless of mass, due to the effects of gravity. [13]

The unreported experiment found in folio 116V tested the constant rate of acceleration in falling bodies due to gravity. [14] This experiment consisted of dropping a ball from specified heights onto a deflector in order to transfer its motion from vertical to horizontal. The data from the inclined plane experiments were used to calculate the expected horizontal motion. However, discrepancies were found in the results of the experiment: the observed horizontal distances disagreed with the calculated distances expected for a constant rate of acceleration. Galileo attributed the discrepancies to air resistance in the unreported experiment, and friction in the inclined plane experiment. These discrepancies forced Galileo to assert that the postulate held only under "ideal conditions," i.e., in the absence of friction and/or air resistance.

Bodies in motion

Aristotelian physics argued that the Earth must not move as humans are unable to perceive the effects of this motion. [15] A popular justification of this is the experiment of an archer shooting an arrow straight up into the air. If the Earth were moving, Aristotle argued, the arrow should fall in a different location than the launch point. Galileo refuted this argument in Dialogues Concerning the Two Chief World Systems. He provided the example of sailors aboard a boat at sea. The boat is obviously in motion, but the sailors are unable to perceive this motion. If a sailor were to drop a weighted object from the mast, this object would fall at the base of the mast rather than behind it (due to the ship's forward motion). This was the result of simultaneously the horizontal and vertical motion of the ship, sailors, and ball. [16]

Relativity of motions

Picture in Galileo's Discorsi (1638) illustrating relativity of motions Galileo-1638-173.jpg
Picture in Galileo's Discorsi (1638) illustrating relativity of motions

One of Galileo's experiments regarding falling bodies was that describing the relativity of motions, explaining that, under the right circumstances, "one motion may be superimposed upon another without effect upon either...". In Two New Sciences, Galileo made his case for this argument and it would become the basis of Newton's first law, the law of inertia.

He poses the question of what happens to a ball dropped from the mast of a sailing ship or an arrow fired into the air on the deck. According to Aristotle's physics, the ball dropped should land at the stern of the ship as it falls straight down from the point of origin. Likewise the arrow when fired straight up should not land in the same spot if the ship is in motion. Galileo offers that there are two independent motions at play. One is the accelerating vertical motion caused by gravity while the other is the uniform horizontal motion caused by the moving ship which continues to influence the trajectory of the ball through the principle of inertia. The combination of these two motions results in a parabolic curve. The observer cannot identify this parabolic curve because the ball and observer share the horizontal movement imparted to them by the ship, meaning only the perpendicular, vertical motion is perceivable. Surprisingly, nobody had tested this theory with the simple experiments needed to gain a conclusive result until Pierre Gassendi published the results of said experiments in his letters entitled De Motu Impresso a Motore Translato (1642). [17]

Infinity

The book also contains a discussion of infinity. Galileo considers the example of numbers and their squares. He starts by noting that:

It cannot be denied that there are as many [squares] as there are numbers because every number is a [square] root of some square: 1 ↔ 1, 2 ↔ 4, 3 ↔ 9, 4 ↔ 16, and so on.

(In modern language, there is a bijection between the elements of the set of positive integers N and the set of squares S, and S is a proper subset of density zero.) But he notes what appears to be a contradiction:

Yet at the outset we said there are many more numbers than squares, since the larger portion of them are not squares. Not only so, but the proportionate number of squares diminishes as we pass to larger numbers.

He resolves the contradiction by denying the possibility of comparing infinite numbers (and of comparing infinite and finite numbers):

We can only infer that the totality of all numbers is infinite, that the number of squares is infinite, and that the number of their roots is infinite; neither is the number of squares less than the totality of all numbers, nor the latter greater than the former; and finally the attributes "equal," greater," and "less," are not applicable to infinite, but only to finite, quantities.

This conclusion, that ascribing sizes to infinite sets should be ruled impossible, owing to the contradictory results obtained from these two ostensibly natural ways of attempting to do so, is a resolution to the problem that is consistent with, but less powerful than, the methods used in modern mathematics. The resolution to the problem may be generalized by considering Galileo's first definition of what it means for sets to have equal sizes, that is, the ability to put them in one-to-one correspondence. This turns out to yield a way of comparing the sizes of infinite sets that is free from contradictory results.

These issues of infinity arise from problems of rolling circles. If two concentric circles of different radii roll along lines, then if the larger does not slip it appears clear that the smaller must slip. But in what way? Galileo attempts to clarify the matter by considering hexagons and then extending to rolling 100 000-gons, or n-gons, where he shows that a finite number of finite slips occur on the inner shape. Eventually, he concludes "the line traversed by the larger circle consists then of an infinite number of points which completely fill it; while that which is traced by the smaller circle consists of an infinite number of points which leave empty spaces and only partly fill the line," which would not be considered satisfactory now.

Reactions by commentators

So great a contribution to physics was Two New Sciences that scholars have long maintained that the book anticipated Isaac Newton's laws of motion.

Galileo ... is the father of modern physics—indeed of modern science

Part of Two New Sciences was pure mathematics, as has been pointed out by the mathematician Alfréd Rényi, who said that it was the most significant book on mathematics in over 2000 years: Greek mathematics did not deal with motion, and so they never formulated mathematical laws of motion, even though Archimedes developed differentiation and integration. Two New Sciences opened the way to treating physics mathematically by treating motion mathematically for the first time. The Greek mathematician Zeno had designed his paradoxes to prove that motion could not be treated mathematically, and that any attempt to do so would lead to paradoxes. (He regarded this as an inevitable limitation of mathematics.) Aristotle reinforced this belief, saying that mathematic could only deal with abstract objects that were immutable. Galileo used the very methods of the Greeks to show that motion could indeed be treated mathematically. His idea was to separate out the paradoxes of the infinite from Zeno's paradoxes. He did this in several steps. First, he showed that the infinite sequence S of the squares 1, 4, 9, 16, ...contained as many elements as the sequence N of all positive integers (infinity); this is now referred to as Galileo's paradox. Then, using Greek style geometry, he showed a short line interval contained as many points as a longer interval. At some point he formulates the general principle that a smaller infinite set can have just as many points as a larger infinite set containing it. It was then clear that Zeno's paradoxes on motion resulted entirely from this paradoxical behavior of infinite quantities. Renyi said that, having removed this 2000-year-old stumbling block, Galileo went on to introduce his mathematical laws of motion, anticipating Newton. [20]

Gassendi's thoughts

Pierre Gassendi defended Galileo's opinions in his book, De Motu Impresso a Motore Translato. In Howard Jones' article, Gassendi's Defence of Galileo: The Politics of Discretion, Jones says Gassendi displayed an understanding of Galileo's arguments and a clear grasp of their implications for the physical objections to the earth's motion.

Koyré's thoughts

The law of falling bodies was published by Galileo in 1638. But in the 20th century some authorities challenged the reality of Galileo's experiments. In particular, the French historian of science Alexandre Koyré bases his doubt on the fact that the experiments reported in Two New Sciences to determine the law of acceleration of falling bodies, required accurate measurements of time which appeared to be impossible with the technology of 1600. According to Koyré, the law was created deductively, and the experiments were merely illustrative thought experiments. In fact, Galileo's water clock (described above) provided sufficiently accurate measurements of time to confirm his conjectures.

Later research, however, has validated the experiments. The experiments on falling bodies (actually rolling balls) were replicated using the methods described by Galileo, [21] and the precision of the results was consistent with Galileo's report. Later research into Galileo's unpublished working papers from 1604 clearly showed the reality of the experiments and even indicated the particular results that led to the time-squared law. [22]

See also

Notes

  1. ( Drake 1978 , p. 367) See Galileo affair for further details.
  2. "The foundation of mechanics". The Independent . Jul 6, 1914. Retrieved July 28, 2012.
  3. Finocchiaro, Maurice A., ed. (2014). The Trial of Galileo: Essential Documents. Hackett Publishing Company. p. 30. ISBN   978-1-62466-132-7.
  4. Plotnitsky, Arkady; Reed, David (1 January 2001). "Discourse, Mathematics, Demonstration, and Science in Galileo's Discourses Concerning Two New Sciences". Configurations. 9 (1): 37–64. doi:10.1353/con.2001.0007. S2CID   145756372.
  5. Plotnitsky, Arkady; Reed, David (1 January 2001). "Discourse, Mathematics, Demonstration, and Science in Galileo's Discourses Concerning Two New Sciences". Configurations 9 (1): 37–64.
  6. Opere di Galileo Galilei. Tartini e Franchi, Florence. 1718.
  7. 1 2 Antonio Favaro, ed. (1898). Le Opere di Galileo Galilei, vol. VIII. Edizione Nazionale, Florence.
  8. Wallace, Jones (1976). "Galileo and Reasoning ex Suppositione: The Methodology of the two New Sciences". Psa 1974. Boston Studies in the Philosophy of Science. Vol. 1974. University of Chicago Press, Springer, Philosophy of Science Association. pp. 79–104. doi:10.1007/978-94-010-1449-6_4. ISBN   978-90-277-0648-5. JSTOR   495799.
  9. Wallace, Jones (1976). "Galileo and Reasoning ex Suppositione: The Methodology of the two New Sciences". Psa 1974. Boston Studies in the Philosophy of Science. Vol. 1974. University of Chicago Press, Springer, Philosophy of Science Association. pp. 79–104. doi:10.1007/978-94-010-1449-6_4. ISBN   978-90-277-0648-5. JSTOR   495799.
  10. Tucker McElroy, A to Z of Mathematicians, Facts on File (Infobase Publishing), p. 109.
  11. Simon Gindikin, Tales of Physicists and Mathematicians, Springer Science & Business Media, p. 43.
  12. Galileo 1638 Discorsi e dimostrazioni matematiche, intorno à due nuove scienze213, Leida, Appresso gli Elsevirii (Leiden: Louis Elsevier), or Mathematical discourses and demonstrations, relating to Two New Sciences, English translation by Henry Crew and Alfonso de Salvio 1914. Section 213 is reprinted on pages 534-535 of On the Shoulders of Giants: The Great Works of Physics and Astronomy (works by Copernicus, Kepler, Galileo, Newton, and Einstein). Stephen Hawking, ed. 2002 ISBN   0-7624-1348-4
  13. Wallace, William. "Galileo and Reasoning Ex Suppositione: The Methodology of the Two New Sciences." (92).
  14. Wallace, William. "Galileo and Reasoning Ex Suppositione: The Methodology of the Two New Sciences." (96).
  15. Howard Jones. "Gassendi's Defence of Galileo: The Politics of Discretion." (224)
  16. Galileo Galilei (1953). Dialogue Concerning the Two Chief World Systems, p.144-145. Translator: Stillman Drake. Berkeley, CA: University of California Press. ISBN 0-520-00449-3.
  17. Howard, Jones (1988). Gassendi's defense of Galileo: The Politics of Discretion. Binghamton, N.Y.: Medieval and Renaissance Texts and Studies. pp. 221–232.
  18. Stephen Hawking, ed. p. 397, On the Shoulders of Giants.
  19. Stephen Hawking, ed. p. 398, On the Shoulders of Giants.
  20. Alfred Renyi, Dialogs on Mathematics, Holden-Day, San Francisco, 1967.
  21. Settle, Thomas B. (1961). "An experiment in the history of science". Science. 133 (3445): 19–23. Bibcode:1961Sci...133...19S. doi:10.1126/science.133.3445.19. PMID   17759858.
  22. Drake, Stillman (1973). "Galileo's Discovery of the Law of Free Fall". Scientific American . 228 (5). v. 228, #5, pp. 84-92. Bibcode:1973SciAm.228e..84D. doi:10.1038/scientificamerican0573-84.

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<span class="mw-page-title-main">Galileo's Leaning Tower of Pisa experiment</span> Celebrated demonstration of gravity

Between 1589 and 1592, the Italian scientist Galileo Galilei is said to have dropped "unequal weights of the same material" from the Leaning Tower of Pisa to demonstrate that their time of descent was independent of their mass, according to a biography by Galileo's pupil Vincenzo Viviani, composed in 1654 and published in 1717. The basic premise had already been demonstrated by Italian experimenters a few decades earlier.

Aristotelian physics is the form of natural philosophy described in the works of the Greek philosopher Aristotle. In his work Physics, Aristotle intended to establish general principles of change that govern all natural bodies, both living and inanimate, celestial and terrestrial – including all motion, quantitative change, qualitative change, and substantial change. To Aristotle, 'physics' was a broad field including subjects which would now be called the philosophy of mind, sensory experience, memory, anatomy and biology. It constitutes the foundation of the thought underlying many of his works.

<span class="mw-page-title-main">Theory of impetus</span>

The theory of impetus is an auxiliary or secondary theory of Aristotelian dynamics, put forth initially to explain projectile motion against gravity. It was introduced by John Philoponus in the 6th century, and elaborated by Nur ad-Din al-Bitruji at the end of the 12th century. The theory was modified by Avicenna in the 11th century and Abu'l-Barakāt al-Baghdādī in the 12th century, before it was later established in Western scientific thought by Jean Buridan in the 14th century. It is the intellectual precursor to the concepts of inertia, momentum and acceleration in classical mechanics.

<span class="mw-page-title-main">Galileo Galilei</span> Florentine physicist and astronomer (1564–1642)

Galileo di Vincenzo Bonaiuti de' Galilei, commonly referred to as Galileo Galilei or mononymously as Galileo, was an Italian (Florentine) astronomer, physicist and engineer, sometimes described as a polymath. He was born in the city of Pisa, then part of the Duchy of Florence and present-day Italy. Galileo has been called the father of observational astronomy, modern-era classical physics, the scientific method, and modern science.

Quaestiones quaedam philosophicae is the name given to a set of notes that Isaac Newton kept for himself during his earlier years in Cambridge. They concern questions in the natural philosophy of the day that interested him. Apart from the light it throws on the formation of his own agenda for research, the major interest in these notes is the documentation of the unaided development of the scientific method in the mind of Newton, whereby every question is put to experimental test.

De motu antiquiora, or simply De Motu, is Galileo Galilei's early written work on motion. It was written largely between 1589 and 1592, but was not published in full until 1890. De Motu is known for expressing Galileo's ideas on motion during his Pisan period prior to transferring to Padua.

Jacques-Alexandre Le Tenneur (1604—1659) was a French mathematician who defended Galileo Galilei’s ideas. He corresponded with fellow mathematicians such as Pierre Gassendi, Pierre Hérigone and Marin Mersenne. It is unclear when or where he died but he probably lived from 1610 to 1660.

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