Galileo on Corpuscularianism (1623)

Total Page:16

File Type:pdf, Size:1020Kb

Galileo on Corpuscularianism (1623) Galileo on Corpuscularianism (1623) In the early 1600’s, a certain view of matter swept across the academic world, to be adopted by nearly every major scientific or philosophical figure for at least the next 100 years. That view was corpuscularianism, a resurgance of ‘atomism’ held by ancient Greek philosophers such as Epicurus and Lucretius, the view that the physical world is composed of tiny particles, atoms, or corpuscles, and that nearly everything one observes can be explained in terms of these. Galileo (of physics and astronomy fame) explains and defends this view in The Assayer. 1. On Tickling: Up until Galileo’s time, it was thought that all observed properties of material objects actually resided in those objects. Not only does an apple have solidity and roundness, but also redness, sweetness, and so on. Lemons have sourness in them. Fires have heat in them. And so on. Galileo challenged this claim: “I strongly suspect that the commonly held conception of the matter is very far from the truth, inasmuch as heat is generally believed to be a true accident, affection, or quality which actually resides in the material which we feel to be heated.” [Historical note: Why did they think this? Throughout the medieval period, it was assumed that an object could only IMPART a property if it already HAD that property. For instance, a fire imparts heat to a kettle only because the fire itself HAS heat. Similarly, a tomato only imparts redness into your mind because it too HAS redness. It was thought that the “form” of redness emanated from the object and “stamped” itself onto your mind like a seal on hot wax. Other scientific explanations were even spookier. For instance, a sedative was said to work in virtue of its “soporific power” – the power of putting one to sleep.] Galileo considers an experiment: Imagine running your hand over someone who is ticklish. They experience the titillating sensation of tickling. But, nowhere in your hand is there anything like tickling! All that the hand contributes is movement and contact: “And it seems to me that he would be gravely in error who would assert that the hand, in addition to movement and contact, intrinsically possesses another and different faculty which we might call the ‘tickling faculty,’ as though tickling were a resident property of the hand per se.” Similarly, if one is tickled by a feather, we do not think that somehow the tickling is IN THE FEATHER, or that the feather somehow possesses a real power called “the tickling faculty”. Rather, all the feather seems to contribute are certain sizes, shapes, textures, and motions of its parts, while the SENSATION of being tickled is merely within US. 1 2. The “Real Properties” of Bodies: From here, Galileo speculates that things like color, taste, odor, etc. are ALL like this; that is, like tickling, do not exist in the objects themselves – but rather “have really no existence save in us”. He writes, “Now this titillation is completely ours and not the feather’s, so that if the living, sensing body were removed, nothing would remain of the titillation but an empty name. And I believe that many other qualities, such as taste, odor, color, and so on, often predicated of natural bodies, have a similar and no greater existence than this.” It is at least CONCEIVABLE that objects do not really have these properties. For, while we cannot coherently imagine a material thing without size, shape, or degree of motion, we CAN imagine one without color, odor, or sound. (Give it a try: Imagine an apple that is silent, not sweet, gives off no odor, and has no color. It’s possible, right?) Thus, material objects are at least LOGICALLY separable from these properties. Galileo writes, “Now, whenever I conceive of any material or corporeal substance, I am necessarily constrained to conceive of that substance as bounded and as possessing this or that shape, as large or small in relationship to some other body, as in this or that place during this or that time, as in motion or at rest, as in contact or not in contact with some other body, as being one, many, or few—and by no stretch of imagination can I conceive of any corporeal body apart from these conditions. But I do not at all feel myself compelled to conceive of bodies as necessarily conjoined with such further conditions as being red or white, bitter or sweet, having sound or being mute, or possessing a pleasant or unpleasant fragrance. On the contrary, were they not escorted by our physical senses, perhaps neither reason nor understanding would ever, by themselves, arrive at such notions. I think, therefore, that these tastes, odors, colors, etc., so far as their objective existence is concerned, are nothing but mere names for something which resides exclusively in our sensitive body, so that if the perceiving creatures were removed, all of these qualities would be annihilated and abolished from existence.” It seems that objects MUST have the following: Size Shape Location in space and time Motion or rest Number (or quantity) Galileo calls these the “primary and real properties”. Things like color, taste, and odor, he calls the “sensible qualities.”(Note: Later, we will discuss this distinction in detail, as made by John Locke. He calls the former “primary qualities” and the latter “secondary qualities.”) 2 3. Corpuscularianism: From this unmysterious explanation of the tickling sensation, it is a short journey to similar explanations for all other sensations. Galileo concluded that, just as the shape of the parts of the feather, the speed with which it is drawn across the skin, etc., seemed to be what produced the tickling sensation, so too the shapes, sizes, speeds, and so forth, of the particles being emitted by material objects must be what produce the different sensations of colors, sounds, flavors, etc. in us: “Thus our tastes are caused, pleasant or harsh in accordance with variations in the contact of diversely shaped particles, and depending upon whether they are few or many, and whether they have high or low velocity.” Heat: For instance, he speculates that HEAT is also like this. He thought that perhaps the difference between a pleasant warmth and a painful burning may be the difference between the particles of a fire or heat source moving more slowly or more quickly. (Note: Francis Bacon actually proposed this 3 years earlier, in 1620.) Light: He even speculates that light itself is merely the smallest particle—arrived at by breaking up matter into smaller and smaller bits until you reach the very smallest, indivisible thing: “once we arrive at the point of ultimate and maximum dissolution into truly indivisible atoms, light itself may be created, with an instantaneous motion … capable, I say, of filling vast spaces.” Conclusion: This conclusion may seem trivial and obvious, but this was a revolutionary way of thinking in the 16th and 17th centuries, and it marked a huge leap forward for science and philosophy alike. Yet, as we shall see, it inadvertantly led to several skeptical worries. Galileo foreshadows the coming age: “But I should not like, … while removing one doubt, to give birth to a hundred more, as I fear might in part be the case even in this timid venture from shore.” 3 .
Recommended publications
  • Galileo Galilei Introduction Galileo Galilei (1564–1642) Was One of The
    Galileo Galilei Introduction Galileo Galilei (1564–1642) was one of the most significant figures of the Scientific Revolution. Galileo was involved in nearly all fields of natural philosophy, including astronomy, mathematics, and what we now term “physics.” He is rightly considered one of the founders of modern physics and astronomy, and one of the main originators of the modern scientific method. Galileo’s study of motion became the foundation for Newton’s laws of motion and the principles of inertia and gravity. His astronomical studies were instrumental in supporting the heliocentric model of the solar system first propounded by Copernicus. He should also be credited with making experimentation the basis of scientific study, and with the use of mathematics as the fundamental means for expressing and validating the findings of experimental investigation. Galileo’s application of mathematics to experimental results has become one of the most important aspects of modern science. Galileo made important improvements to the telescope, which enabled him to make great advances in astronomical observation. His observations emboldened him to become the most important advocate of Copernicanism—the astronomical system created by Nicolaus Copernicus (1473–1543)—and his support ultimately ushered in the Copernican revolution in astronomy. Copernicus had devised a heliocentric model in which he posited that the Earth revolved around the sun (in perfect circles). Contrary to the Ptolemaic system and Christian cosmology, Copernicus positioned the sun as a fixed center around which Mercury, Venus, Earth, Mars, Jupiter, and Saturn orbited. Furthermore, Copernicus posited the diurnal rotation of the Earth on its own axis in addition to its annual revolutions around the sun.
    [Show full text]
  • Galileo's Assayer
    University of Nevada, Reno Galileo's Assayer: Sense and Reason in the Epistemic Balance A thesis submitted in partial fulfillment of the requirements for the degree of Master of Arts in History. by James A Smith Dr. Bruce Moran/Thesis Advisor May 2018 c by James A Smith 2018 All Rights Reserved THE GRADUATE SCHOOL We recommend that the thesis prepared under our supervision by JAMES A. SMITH entitled Galileo's Assayer: Sense and Reason in the Epistemic Balance be accepted in partial fulfillment of the requirements for the degree of MASTER OF ARTS Bruce Moran, Ph.D., Advisor Edward Schoolman, Ph.D., Committee Member Carlos Mariscal, Ph.D., Committee Member Stanislav Jabuka, Ph.D., Graduate School Representative David W. Zeh, Ph.D., Dean, Graduate School May, 2018 i Abstract Galileo's The Assayer, published in 1623, represents a turning point in Galileo's philo- sophical work. A highly polemical \scientific manifesto," The Assayer was written after his astronomical discoveries of the moons of Jupiter and sunspots on a rotating sun, but before his mature Copernican work on the chief world systems (Ptolemaic versus Copernican). The Assayer included major claims regarding the place of math- ematics in natural philosophy and how the objects of the world and their properties can be known. It's in The Assayer that Galileo wades into the discussion about the ultimate constituents of matter and light, namely, unobservable particles and atoms. Galileo stressed the equal roles that the senses and reason served in the discovery of knowledge, in contradistinction to Aristotelian authoritarian dogma that he found to hinder the processes of discovery and knowledge acquisition.
    [Show full text]
  • Galilei-1632 Dialogue Concerning the Two Chief World Systems
    Galileo di Vincenzo Bonaulti de Galilei ([ɡaliˈlɛːo ɡaliˈlɛi]; 15 February 1564 – 8 January 1642) was an Italian astronomer, physicist and engineer, sometimes described as a polymath, from Pisa. Galileo has been called the "father of observational astronomy", the "father of modern physics", the "father of the scientific method", and the "father of modern science". Galileo studied speed and velocity, gravity and free fall, the principle of relativity, inertia, projectile motion and also worked in applied science and technology, describing the properties of pendulums and "hydrostatic balances", inventing the thermoscope and various military compasses, and using the telescope for scientific observations of celestial objects. His contributions to observational astronomy include the telescopic confirmation of the phases of Venus, the observation of the four largest satellites of Jupiter, the observation of Saturn's rings, and the analysis of sunspots. Galileo's championing of heliocentrism and Copernicanism was controversial during his lifetime, when most subscribed to geocentric models such as the Tychonic system. He met with opposition from astronomers, who doubted heliocentrism because of the absence of an observed stellar parallax. The matter was investigated by the Roman Inquisition in 1615, which concluded that heliocentrism was "foolish and absurd in philosophy, and formally heretical since it explicitly contradicts in many places the sense of Holy Scripture". Galileo later defended his views in Dialogue Concerning the Two Chief World Systems (1632), which appeared to attack Pope Urban VIII and thus alienated him and the Jesuits, who had both supported Galileo up until this point. He was tried by the Inquisition, found "vehemently suspect of heresy", and forced to recant.
    [Show full text]
  • A Phenomenology of Galileo's Experiments with Pendulums
    BJHS, Page 1 of 35. f British Society for the History of Science 2009 doi:10.1017/S0007087409990033 A phenomenology of Galileo’s experiments with pendulums PAOLO PALMIERI* Abstract. The paper reports new findings about Galileo’s experiments with pendulums and discusses their significance in the context of Galileo’s writings. The methodology is based on a phenomenological approach to Galileo’s experiments, supported by computer modelling and close analysis of extant textual evidence. This methodology has allowed the author to shed light on some puzzles that Galileo’s experiments have created for scholars. The pendulum was crucial throughout Galileo’s career. Its properties, with which he was fascinated from very early in his career, especially concern time. A 1602 letter is the earliest surviving document in which Galileo discusses the hypothesis of pendulum isochronism.1 In this letter Galileo claims that all pendulums are isochronous, and that he has long been trying to demonstrate isochronism mechanically, but that so far he has been unable to succeed. From 1602 onwards Galileo referred to pendulum isochronism as an admirable property but failed to demonstrate it. The pendulum is the most open-ended of Galileo’s artefacts. After working on my reconstructed pendulums for some time, I became convinced that the pendulum had the potential to allow Galileo to break new ground. But I also realized that its elusive nature sometimes threatened to undermine the progress Galileo was making on other fronts. It is this ambivalent nature that, I thought, might prove invaluable in trying to understand crucial aspects of Galileo’s innovative methodology.
    [Show full text]
  • Ch. 3: the Solar System
    1 Ch. 3: The Solar System Brief outline: Ideas of Copernicus >> Galileo >> Kepler >> Isaac Newton This chapter discusses how the scientific contributions by Copernicus, Galileo and Kepler led to Newton's discovery of the Universal Gravitation. • It must be understood that the ancient Greek ‘philosophers-scientists’ had various opinions about the ‘center of the universe’ and the relation between Earth and the Sun. Some thought that the Sun is at the center. Others that it is Earth. • Aristotle (384-322 BC) chose to follow the opinion that it is Earth. It appears that he also believed that heavier bodies fall faster than light ones, and many other things. • Much later in 312 AD Constantine was made emperor of Rome and protector of Christianity. Christianity evolved rapidly after the council of Nicaea (AD 325), when intellectuals/philosophers within the Catholic church made efforts to establish doctrine that would make the ideas found in the bible more complete, and eventually added concepts of both Plato and then Aristotle. • Once this was done it became DOGMA of the church, and to attack this view was to attack the foundation of the church. And so this incorrect view lasted for over 1,000 years, until Copernicus. <Nicolaus Copernicus> (1473-1543) Ideas The earth is NOT the center of the universe, although it is the center of the moon’s orbit and of its own gravity. The sun is the center of the planetary system and the sphere of stars. Earth is just one of the planets. Since the moon rotates around the Earth, the heavenly bodies do not share the same center.
    [Show full text]
  • The Galileo Affair in Context: an Investigation of Influences on the Church During Galileo’S 1633 Trial
    Xavier University Exhibit Honors Bachelor of Arts Undergraduate 2020-5 The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial Evan W. Lamping Xavier University, Cincinnati, OH Follow this and additional works at: https://www.exhibit.xavier.edu/hab Part of the Ancient History, Greek and Roman through Late Antiquity Commons, Ancient Philosophy Commons, Classical Archaeology and Art History Commons, Classical Literature and Philology Commons, and the Other Classics Commons Recommended Citation Lamping, Evan W., "The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial" (2020). Honors Bachelor of Arts. 45. https://www.exhibit.xavier.edu/hab/45 This Capstone/Thesis is brought to you for free and open access by the Undergraduate at Exhibit. It has been accepted for inclusion in Honors Bachelor of Arts by an authorized administrator of Exhibit. For more information, please contact [email protected]. Evan Lamping Dr. Byrne CPHAB Thesis The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial 1 I. Introduction When most people learn about the Galileo controversy of 1633, their knowledge of the affair is most commonly comprised of the facts of his condemnation on counts of heresy and possibly some other details about how and why his inquisition was conducted. These details are often simply concerned with the Church’s indefensible view of the earth as the center of the universe, combined with some scripture passages describing the sun as standing still or the earth being fixed in place and unmovable.
    [Show full text]
  • THE TRIAL of GALILEO-REVISITED Dr
    THE TRIAL OF GALILEO-REVISITED Dr. George DeRise Professor Emeritus, Mathematics Thomas Nelson Community College FALL 2018 Mon 1:30 PM- 3:30 PM, 6 sessions 10/22/2018 - 12/3/2018 (Class skip date 11/19) Sadler Center, Commonwealth Auditorium Christopher Wren Association BOOKS: THE TRIAL OF GALILEO, 1612-1633: Thomas F. Mayer. (Required) THE CASE FOR GALILEO- A CLOSED QUESTION? Fantoli, Annibale. GALILEO; THE RISE AND FALL OF A TROUBLESOME GENIUS. Shea, William; Artigas, Mariano. BASIC ONLINE SOURCES: Just Google: “Galileo” and “Galileo Affair” (WIKI) “Galileo Project” and “Trial of Galileo-Famous Trials” YOUTUBE MOVIES: Just Google: “GALILEO'S BATTLE FOR THE HEAVENS – NOVA – YOUTUBE” “GREAT BOOKS, GALILEO’S DIALOGUE – YOUTUBE” HANDOUTS: GLOSSARY CAST OF CHARACTERS BLUE DOCUMENTS GALILEO GALILEI: b. 1564 in Pisa, Italy Astronomer, Physicist, Mathematician Professor of Mathematics, Universities of Pisa and Padua. In 1610 he observed the heavens with the newly invented telescope- mountains and craters of the moon, moons of Jupiter, many stars never seen before; later the phases of Venus; sunspots. These observations supported his belief that the Copernican (Heliocentric) system was correct, i.e. that the Sun was the center of the Universe; the planets including earth revolved around it. This was in direct contrast to the Ptolemaic-Aristotelian (Geocentric) System which was 1500 years old at the time. Galileo’s Copernican view was also in conflict with the Christian interpretation of Holy Scripture. Because of the Counter Reformation Catholic theologians took a literal interpretation of the Bible. Galileo was investigated by the Inquisition in 1615 and warned not to defend the Copernican view.
    [Show full text]
  • GALILEO and the PHASES of VENUS Abstract
    GALILEO AND THE PHASES OF VENUS Charles-Henri Eyraud Institut National de Recherche Pédagogique (France) Abstract In this article we use Galileo’s letters and drawings to understand his observations of the phases of Venus in 1610-1611. Our article is presented as an exercise for students to understand the conclusions of the great astronomer. PERIODS OF VENUS • Synodical period and phases The synodic period is the time that it takes for the object to reappear at the same point in the sky, relative to the Sun, as observed from Earth; i.e. returns to the same elongation and planetary phase. This is the time that elapses between two successive conjunctions with the Sun. An inferior conjunction occurs when Venus and the Earth lie in a line on the same side of the Sun. When Venus is on the opposite side of the Sun, it is a superior conjunction. The synodic period of Venus is 584 days. The superior conjunction occured on 11th May 1610. Calculate the date of the quadrature, of the inferior conjunction and of the next superior conjunction, supposing the motions of the Earth and Venus are circular and uniform (Figure 2). In fact the next superior conjunction occured on 11th December 1611 and inferior conjunction on 26th February 1611. • Sidereal period The sidereal period is the time that it takes the object to make one full orbit around the Sun, relative to the stars. The sidereal period of the Earth is 365.25 days. Calculate the sidereal period of Venus. PHASES OF VENUS IN GEO AND HELIOCENTRIC MODELS • Phases 1) Determine the phases of Venus in geocentric models, where the Earth is at the center of the universe and planets orbit around (Mercury and Venus “above” or “below” the Sun).
    [Show full text]
  • Challenging the Paradigm: the Legacy of Galileo Symposium
    Challenging the Paradigm: The Legacy of Galileo Symposium November 19, 2009 California Institute of Technology Pasadena, California Proceedings of the 2009 Symposium and Public Lecture Challenging the Paradigm: The Legacy of Galileo NOVEMBER 19, 2009 CAHILL BUILDING - HAMEETMAN AUDITORIUM CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENA, CALIFORNIA, USA © 2011 W. M. KECK INSTITUTE FOR SPACE STUDIES, ISBN-13: 978-1-60049-005-07 CALIFORNIA INSTITUTE OF TECHNOLOGY ISBN-10: 1-60049-005-0 Sponsored by The W.M. Keck Institute for Space Studies Supported by The Italian Consulate – Los Angeles The Italian Cultural Institute – Los Angeles Italian Scientists and Scholars in North America Foundation The Planetary Society Organizing Committee Dr. Cinzia Zuffada – Jet Propulsion Laboratory (Chair) Professor Mike Brown – California Institute of Technology (Co-Chair) Professor Giorgio Einaudi – Università di Pisa Dr. Rosaly Lopes – Jet Propulsion Laboratory Professor Jonathan Lunine - University of Arizona Dr. Marco Velli – Jet Propulsion Laboratory Table of Contents Introduction……………………………………………………………………………….. 1 Galileo's New Paradigm: The Ultimate Inconvenient Truth…………………………... 3 Professor Alberto Righini University of Florence, Italy Galileo and His Times…………………………………………………………………….. 11 Professor George V. Coyne, S.J. Vatican Observatory The Galileo Mission: Exploring the Jovian System…………………………………….. 19 Dr. Torrence V. Johnson Jet Propulsion Laboratory, California Institute of Technology What We Don't Know About Europa……………………………………………………. 33 Dr. Robert T. Pappalardo Jet Propulsion Laboratory, California Institute of Technology The Saturn System as Seen from the Cassini Mission…………………………………. 55 Dr. Angioletta Coradini IFSI – Istituto di Fisica dello Spazio Interplanetario dell’INAF - Roma Solar Activity: From Galileo's Sunspots to the Heliosphere………………………….. 67 Professor Eugene N. Parker University of Chicago From Galileo to Hubble and Beyond - The Contributions and Future of the Telescope: The Galactic Perspective…………………………………………………….
    [Show full text]
  • New Light on the Galileo Affair (1)
    New light on the Galileo affair (1) Mariano Artigas Published in Metanexus, 30 April 2002 This is a written version of a lecture delivered at the Metanexus Institute (Philadelphia), on Monday 4 February 2002, and at Columbia University (New York), on Wednesday 6 February 2002, on a document related to the Galileo Affair, discovered by the author in 1999 in the archives of the Holy Office in Rome. (2) (3) More elaborate accounts of the discovery of document EE 291 and its meaning for the Galileo Affair have been published by Mariano Artigas, Rafael Martínez and William R. Shea: (4) (5) (6) (7) Mariano Artigas, Rafael Martínez and William R. Shea, “New light on the Galileo affair?”, in: The Church and Galileo, edited by Ernan McMullin (Notre Dame, In.: University of Notre Dame Press, 2005), pp. 213-233. Mariano Artigas, Rafael Martínez and William Shea, “New Light in the Galileo Affair”, in: John Brooke and Ekmeleddin Ihsanoglu, editores, Religious Values and the Rise of Science in Europe (Istanbul: Research Centre for Islamic History, Art and Culture, 2005), pp. 145-166. Mariano Artigas, Rafael Martínez y William R. Shea, “Nueva luz en el caso Galileo”, Anuario de Historia de la Iglesia, 12 (2003), pp. 159-179. “Un inedito sul caso Galilei. Presentazione”, Acta Philosophica, 10 (2001), pp. 197- 272: Mariano Artigas, “Un nuovo documento sul caso Galileo: EE 291”, pp. 199-214; Rafael Martínez, “Il manoscritto ACDF, Index, Protocolli, vol. EE, f. 291 r-v”, pp. 215- 242; Lucas F. Mateo-Seco, “Galileo e l’Eucaristia. La questione teologica dell’ACDF, Index, Protocolli, EE, f.
    [Show full text]
  • Galileo's Gout
    Gerald Weissmann, M.D. The author (AΩA, New York University, 1965) is Research ice-capped poles, one of those moons, Europa, seems the best Galileo’sGProfessora ofl Medicineile ando director’s of thegoutg Biotechnologyou t candidate yet as a habitat for extraterrestrial life.1 Earlier that Study Center at New York University School of Medicine. In year, Europe—the continent—filed its answer to the American 2002 he was elected to the Accademia Nazionale dei Lincei Global Positioning system; it shot a satellite into orbit and called as the sole American physician member. He is a previous it Galileo.2 Galileo’s own stock rose when physicists ranked two contributor to The Pharos. of Galileo’s experiments among “science’s 0 most beautiful experiments.”3 The year 2003 marked the four hundredth an- he first three years of our new millennium have niversary of the Accademia dei Lincei (established in Rome beenbeen bannerbanner yearsyears forfor GalileoGalileo (Galileo(Galileo Galilei,Galilei, 564–564– in 603), the world’s oldest scholarly society, of which, Galileo 642).642). IInn NNovemberovember 22002,002, oonene ooff NNASA’sASA’s llongest-ongest- was, dare we say, the star. To mark the occasion, a magisterial running missions came to an end when the Galileo spacecraft, volume by Columbia’s David Freedberg, The Eye of the Lynx launched in 989, made its final orbit of Jupiter, the planet showed how the new world view of Galileo and his Linceians whose four moons Galileo first described in 60. With its was an impetus for London’s Royal Society (660) and Colbert’s T Académie des Sciences (666).4 Finally, a definitive exhibition Above: Galileo presenting his telescope to the Doge, by Luigi on Albert Einstein at the American Museum of Natural History Sabatelli (1772–1850).
    [Show full text]
  • Excerpt from Learning from Six Philosophers
    Two chapters on Issues in Empiricism Jonathan Bennett Secondary Qualities Chapter 25 of Learning from Six Philosophers, (Oxford University Press, 2001), pp. 74–91. 187. Locke’s corpuscularianism is not one individual thing, neither is there any such Locke was attracted by the kind of physics he called ‘the thing existing as one material being, or one single corpuscularian hypothesis’1—the hypothesis that the physi- body that we know or can conceive. And therefore if cal world can be comprehensively explained in terms of how matter were the eternal first cogitative being, there corpuscles are assembled into larger structures and how would not be one eternal infinite cogitative being, but they move. One naturally thinks of the ‘corpuscles’ as atoms, an infinite number of eternal finite cogitative beings. unsplittable physical minima, but Locke does not confidently (Essay IV.x.10) do so. Let us consider his troubles with atoms. In this astonishing passage Locke implies that every material Like Descartes, Leibniz, and others at his time, Locke did thing is divisible into an infinite number of basic parts; he not believe in attractive forces.2 That left him, as he knew, calls them ‘beings’ but drops the adjective ‘material’ because unable to explain how bodies hang together so that there are if they were material they would be extended, so divisible, rocks and grains as well as air and water (II.xxiii.23–7). This so unbasic. He here goes a good distance with Leibniz, encouraged the view that there are no atoms because every but unlike him supposes that an extended thing can have portion of matter can be divided into still smaller bodies.
    [Show full text]