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A learned artisan debates the system of the world: Le Clerc versus Mallemant de Messange

Published online by Cambridge University Press:  11 October 2017

ODED RABINOVITCH*
Affiliation:
Department of History, Tel Aviv University, Israel. Email: [email protected].

Abstract

Sébastien Le Clerc (1637–1714) was the most renowned engraver of Louis XIV's France. For the history of scientific publishing, however, Le Clerc represents a telling paradox. Even though he followed a traditional route based on classic artisanal training, he also published extensively on scientific topics such as cosmology and mathematics. While contemporary scholarship usually stresses the importance of artisanal writing as a direct expression of artisanal experience and know-how, Le Clerc's publications, and specifically the work on cosmology in his Système du monde (1706–1708), go far beyond this. By reconstructing the debate between Le Clerc and the professor Mallemant de Messange on the authorship of this ‘system of the world’, this article argues that Le Clerc's involvement in publishing ventures shaped his identity both as an artisan and as a scientific author. Whereas the Scientific Revolution supposedly heralded a change from the world of ‘more or less’ to the ‘world of precision’, this article shows how an artisan could be more ‘precise’ than the learned scholar whose claims he disputed, and points to the importance of the literary field as a useful lens for observing the careers of early modern scientific practitioners.

Type
Research Article
Copyright
Copyright © British Society for the History of Science 2017 

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References

1 de Messange, Claude Mallemant, Discours de Monsieur de Messange sur trois articles du Journal de Trévoux …, Paris, 1705, 1213 Google Scholar, 15–18.

2 Hall, R., ‘The scholar and the craftsman in the scientific revolution’, in Clagett, M. (ed.), Critical Problems in the History of Science, Madison: University of Wisconsin Press, 1962, pp. 323 Google Scholar, 21.

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4 See Ash, Eric H., ‘Introduction: expertise and the early modern state’, Osiris, second series (2010) 25, pp. 124 Google Scholar; as well as Klein, Ursula, ‘Artisanal–scientific experts in eighteenth-century France and Germany’, Annals of Science (2012) 69, pp. 303306 Google Scholar – the articles both introduce the arguments and further references; Bertucci, Paola and Courcelle, Olivier, ‘Artisanal knowledge, expertise, and patronage in early eighteenth-century Paris: the Société des arts (1728–36)’, Eighteenth-Century Studies (2015) 48, pp. 159179 Google Scholar.

5 Following the hypotheses in Rabinovitch, Oded, ‘Chameleons between science and literature: observation, writing, and the early Parisian academy of sciences in the literary field’, History of Science (2013) 51, pp. 3362 Google Scholar.

6 In fact, Pamela Long has recently argued that there is a great need for works on artisanal reading and writing practices: Long, ‘Trading Zones’, op. cit. (3), p. 846.

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8 Other categories of objects, such as instruments, can lead to different conclusions: Bennett, J.A., ‘The mechanics’ philosophy and the mechanical philosophy’, History of Science (1986) 24, pp. 128 Google Scholar; Jean-François Gauvin, ‘Habits of knowledge: artisans, savants, and mechanical devices in seventeenth-century French natural philosophy’, PhD dissertation, Harvard University, 2008. Other forms of writing could also be important in this world: the painter Charles Le Brun came from a family of writing teachers who also designed letters. Gady, Bénédicte, L'ascension de Charles Le Brun: Liens sociaux et production artistique, Paris: Edition de la Maison des sciences de l'homme, 2010, pp. 1623 Google Scholar.

9 While they are strongly associated with Descartes's cosmology, vortices became a common mechanism for explaining the motions of the heavens after the overthrow of the Aristotelian divide between the sub-lunar and supra-lunar world in the early seventeenth century. Le Clerc and Mallemant should not therefore be immediately seen as ‘Cartesians’ (and see below for Mallemant's debates with self-proclaimed Cartesians). See Aiton, E.J., The Vortex Theory of Planetary Motions, London: Macdonald, 1972 Google Scholar.

10 Journal de Trévoux, April 1704, article lviii, pp. 644–647.

11 Journal de Trévoux, April 1705, article lxv, pp. 663–665. Le Clerc dated Galileo's publication to 7 January 1610; this was the date of Galileo's first letter recounting his telescopic discoveries. Drake, Stillman, ‘Galileo's first telescopic observations’, Journal for the History of Astronomy (1976) 7, pp. 153168 Google Scholar. Sidereus nuncius was published in March 1610.

12 Journal de Trévoux, July 1705, article cxvi, pp. 1253–1256.

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15 Modern scholars have pointed out that even in Copernicus's system, the Sun does not occupy the exact centre of the world. This nuance was lost, however, on Le Clerc and Mallemant, as well as on seventeenth-century compilers of systems on which they relied. Compare Kuhn, Thomas S., The Copernican Revolution: Planetary Astronomy in the Development of Western Thought, Cambridge, MA: Harvard University Press, 1957, pp. 170171 Google Scholar; or Westman, Robert S., ‘Proof, poetics and patronage: Copernicus's preface to De revolutionibus ’, in Lindberg, David C. and Westman, Robert S. (eds.), Reappraisals of the Scientific Revolution, Cambridge: Cambridge University Press, 1990, pp. 167205 Google Scholar, 170; with Gadrois, Claude, Le systeme du monde selon les trois hypotheses, Paris: Guillaume Desprez, 1675, p. 86Google Scholar. Even a sophisticated astronomer like Riccioli began his descriptions of the Copernican system by claiming that the Sun is in its centre. Riccioli, Giovanni Battista, Almagestum Novum …, Bologna: Benacci, 1651, p. 102Google Scholar: ‘Copernicus itaq. in centro Universi Solem ponit immobilem’.

16 For this somewhat forced explanation see Le Clerc, op. cit. (13), pp. 120–129, and 62–65 for a putative refutation of Copernicus.

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19 Le Clerc, op. cit. (13), preface, pp. 1–5, 20–21.

20 Le Clerc, op. cit. (13), p. 3.

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22 Le Clerc, op. cit. (13), pp. 183–188, quote at 187–188. Candles were used by artists to illustrate the use of perspective as a light source internal to the image, and Le Clerc discussed elsewhere the passage of light through globules and its impact on the perception of colour. Bosse, Abraham, Moyen universel de pratiquer la perspective sur les tableaux …, Paris : A. Bosse, 1653 Google Scholar, Figure 15 (between pp. 54 and 55); Bosse, Traité des pratiques géometrales et perspectives enseignées dans l'Académie royale de la peinture et sculpture, Paris: A. Bosse, 1665 Google Scholar, Figure 39 (between pp. 88 and 89); Le Clerc, Sébastien, Système de la vision fondée sur de nouveaux principes, Paris: F. Delaulne, 1712, pp. 7983 Google Scholar.

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24 Schaffer, Simon, ‘A science whose business is bursting: soap bubbles as commodities in classical physics’, in Daston, Lorraine (ed.), Things That Talk: Object Lessons from Art and Science, New York: Zone Books, 2004, pp. 147192 Google Scholar, 158.

25 Quoted in Birch, Thomas, History of the Royal Society of London, 4 vols., London: A. Millar, 1756–1757, vol. 3, p. 29Google Scholar.

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28 Le Clerc, op. cit. (13), unpaginated appendix, based on Mallemant, op. cit. (18), pp. 216–223.

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33 Turnbull, H.W. et al. (eds.), The Correspondence of Isaac Newton, 7 vols., Cambridge: Published for the Royal Society at the University Press, 1959–1977, vol. 2, pp. 297298 Google Scholar, 301.

34 I follow the terms both authors used, even though they are not completely technically accurate, relating as they are to a geocentric situation.

35 [Claude Mallemant de Messange], Nouveau systheme du monde, s.l., s.d. (1679), pp. 17–18; Mallemant, op. cit. (18), pp. 216–217. Koyré, Alexandre, ‘The significance of the Newtonian synthesis’, in Koyré, Newtonian Studies, Chicago: The University of Chicago Press, 1965, pp. 324 Google Scholar, 4–5.

36 On the movement of the Sun see Le Clerc, op. cit. (13), pp. 25–27.

37 Le Clerc, op. cit. (13), pp. 94–95, 194–195.

38 Le Clerc, op. cit. (13), pp. 106–110. Le Clerc claimed the most qualified contemporary astronomers found that the greatest distance between the Earth and the Sun is 11,187 diameters of the Earth, and the shortest distance is 10,813.

39 [Mallemant], op. cit. (35), p. 12.

40 Kuhn, op. cit. (15), p. 270; Heilbron, op. cit. (14), pp. 162–163.

41 Le Clerc, op. cit. (13), pp. 54–57. The observed value for precession during the late seventeenth century was 50″, though the calculations for obtaining this value could be quite complex. Richard S. Westfall, ‘Newton and the fudge factor’, Science (23 February 1973) 179, pp. 751–758, esp. 756.

42 Le Clerc, op. cit. (13), p. 19. Le Clerc returns to this claim several times, e.g. at 141–148.

43 Philip Benedict, ‘The owl of Minerva at dusk: Philippe Le Noir de Crevain, a pastor–historian under Louis XIV’, in Benedict, The Faith and Fortunes of France's Huguenots, 1600–85, Aldershot: Ashgate, 2001, pp. 248–276, 257–258.

44 [Mallemant], op. cit. (35), pp. 42–43; Mallemant, op. cit. (18), pp. 251–252.

45 Mallemant, op. cit. (18), preface, n.p.

46 By making the fixed stars into planets revolving around their own vortices, the size of the universe could be reduced, thereby removing an objection to the Copernican system – thus argues [Alexandre Tinelis, Sieur de Castelet], Lettre de Monsieur de Castelet à Monsieur Mallement de Messange, sur les deux nouveaux Systhémes qu'ils ont inventez, s.l, s.d. (1679), pp. 3–5. At issue was the argument against the Copernican system based on the inability to measure the parallax of the fixed stars: Schofield, Christine Jones, Tychonic and Semi-Tychonic World Systems, New York: Arno Press, 1981, pp. 190201 Google Scholar; Helden, Albert Van, Measuring the Universe: Cosmic Dimension from Aristarchus to Halley, Chicago: The University of Chicago Press, 1985, pp. 4953 Google Scholar, 62–63, 73–76, 87–90, 116, 157–159.

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50 Le Clerc, op. cit. (13), pp. 80–81.

51 For Mallemant see Mallemant, op. cit. (18), p. 223 (parallax), 144–145, 221 (refraction).

52 Le Clerc, op. cit. (13), pp. 111–115. Le Clerc did not refer in this context to the greater thickness of the atmosphere when observing objects closer to the horizon.

53 Dew, ‘Vers la ligne’, op. cit. (48), pp. 62–63.

54 Le Clerc, op. cit. (13), pp. 183–188.

55 Discussion of the passage of a star in Aquarius, Le Clerc, op. cit. (13), pp. 78–79.

56 Heilbron, op. cit. (14), p. 98.

57 Le Clerc, op. cit. (13), pp. 34–39, quote at 36.

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72 Recueil d'observations …, op. cit. (48).

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89 [Castelet], op. cit. (46), pp. 1–3; [Mallemant], op. cit. (35), p. 4.

90 [Castelet], op. cit. (46), p. 3.

91 [Castelet], op. cit. (46), p. 3.

92 The Academy's registers drily note that on 22 January 1678 Cassini read his observations on Castelet's new system: Archives de l'Académie de sciences, procès-verbaux, t. 7 f. 135v.

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116 Castelet, op. cit. (99), preliminary discourse, n.p.

117 Jombert, op. cit. (64), vol. 1, p. lxxiii.

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