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My moment of revelation – indeed, the starting point for writing this book – was while trying to make sense of Archimedes' Stomachion. This treatise, surviving on a single parchment leaf containing the introduction, a preliminary proof, and one stump of a proof – all mutilated and difficult to read – has gained little scholarship since its first publication by Heiberg in 1915. I would have never paid it much attention myself – it did not appear to be a “serious” work – but it is after all a page out of the Archimedes Palimpsest, and just looking at the parchment one could not resist the temptation to work on it. The page looked to be in such a bad shape, surely Heiberg did not manage to read it satisfactorily!
My reading did not add many words to those read by Heiberg. But I was probably the first person in many years to have read, slowly and attentively, the introduction to the Stomachion. I quote a tentative translation:
As the so-called Stomachion has a variegated theoria of the transposition of the figures from which it is set up, I deemed it necessary: first, to set out in my investigation of the magnitude of the whole figure each of the <figures> to which it is divided, by which <number> it is measured; and further also, which are <the> angles, taken by combinations and added together; <all of the above> said for the sake of finding out the fitting-together of the arising figures, whether the resulting sides in the figures are on a line or whether they are slightly short of that <but so as to be> unnoticed by sight. […]
The overall structure of the argument is simple. First, we have covered, in the first three chapters of this book, a substantial body of evidence pointing to a certain style of Hellenistic mathematics. Its three major constituents are: (1) mosaic composition, (2) narrative surprise, (3) generic experimentation (a more specialized phenomenon is that of the carnival of calculation). Second, we have briefly noted, in chapter 4, how such stylistic features may also be typical of the major literary works of the same period (with the carnival of calculation paralleled by the carnival of erudition). The minimal claim of the book, then – the one backed up by evidence – is of a certain homology of style between the exact sciences and poetry in the Hellenistic world. In the conclusion to the preceding chapter I have already pointed beyond, to much more tentative claims. It is tempting to postulate a historical force underlying the homology. More than this: if indeed we suggest that a certain historical process led to a Hellenistic interest in generic experimentation, then it becomes very tempting to suggest that the rise of the exact sciences as a major cultural phenomenon should be seen as part and parcel of this practice of experiment in genre, where a hitherto minor genre suddenly gains in prominence.
All of this, however, is highly tentative, largely because our evidence can support such historical interpretations only with difficulty. In this section I acknowledge and address the limitations imposed by our evidence.
The claim of the following chapter is twofold, looking at how poetic practices are (i) complementary to those of the exact sciences, and (ii) parallel to them. Section 4.1 makes the case for (i) complementarity. It shows how Greek poets turned to scientific concepts and contents, weaving science into their poetry just as the scientists were weaving poetry into their science. Sections 4.2–4.3 make the case for (ii) parallelism. Section 4.2 takes a central example of the practices of mythography in Hellenistic poetry as a starting-point for an analysis of the familiar role of “erudition” in this poetry – now considered in light of the scientific practices discussed in this book. Section 4.3 broadens the discussion to look at the poetic parallels to the scientific practices seen throughout this book, as a whole: the narrative surprise and the mosaic text. Of course, the complementarity and parallelism are tightly connected. Section 4.4 offers a brief summary, with some tentative conclusions.
The Hellenistic world was, for generations, the least intensively studied of all ancient periods, its culture alien and uninviting for classicists inspired by Greek glory or by Roman grandeur. With changes in contemporary taste, as well as with the overall explosion of academic writing, considerable and sophisticated studies of Hellenistic civilization have appeared over the last couple of decades. Even this scholarship, however – as is not surprising – concentrates on Hellenistic literature to the exclusion of science.
Euclid's Elements stand out, among Hellenistic mathematical works, in their pedagogic intent. Yet their very end – book xiii – already suggests the ludic, and at the very end is a theorem, attached as a kind of appendix, that would have been worthy of Archimedes. The theorem is often considered to have been discovered early (though its form may be due to Euclid himself, or even to some later reader of him). However this may be, it may serve as an example of an important compositional phenomenon: the mosaic proof. Here then is the proof that there are exactly five regular solids (adapted from Heath's translation):
(1) For a solid angle cannot be constructed with two triangles (or, in general, <two> planes). [This is based on a definition in book xi and in principle represents a fundamental three-dimensional intuition.] (2) With three triangles the angle of the pyramid is constructed, with four the angle of the octahedron, and with five the angle of the icosahedron [this moves into the mode of exhaustive survey]; (3) but a solid angle cannot be formed by six equilateral and equiangular triangles placed together at one point, (4) for, the angle of the equilateral triangle being two-thirds of a right angle, (5) the six will be equal to four right angles: (6) which is impossible, (7) for any solid angle is contained by angles less than four right angles. [Step 7 is a result proved at Elementsxi.21. […]
This, my third study on Greek mathematics, serves to complete a project. My first study, The Shaping of Deduction in Greek Mathematics (1999) analyzed Greek mathematical writing in its most general form, applicable from the fifth century bc down to the sixth century ad and, in truth, going beyond into Arabic and Latin mathematics, as far as the scientific revolution itself. This form – in a nutshell, the combination of the lettered diagram with a formulaic language – is the constant of Greek mathematics, especially (though not only) in geometry. Against this constant, the historical variations could then be played. The historical variety is formed primarily of the contrast of the Hellenistic period (when Greek mathematics reached its most remarkable achievements) and Late Antiquity (when Greek mathematics came to be re-shaped into the form in which it influenced all of later science). My second study, The Transformation of Mathematics in the Early Mediterranean (2004), was largely concerned with the nature of this re-shaping of Greek mathematics in Late Antiquity and the Middle Ages.
This study, finally, is concerned with the nature of Greek mathematics in the Hellenistic period itself. Throughout, my main concern is with the form of writing: taken in a more general, abstract sense, in the first study, and in a more culturally sensitive sense, in the following two.
The three studies were not planned together, but the differences between them have to do not so much with changed opinions as with changed subject matter.
This paper focuses on the response of the Royal Society to the increasing contact with parts of the globe beyond Europe. Such contact was in accord with the programme of Baconian natural history that the early Royal Society espoused, but it also raised basic questions about the extent and nature of the pursuit of natural history. In particular, the paper is concerned with the attention paid to one particular branch of natural history, the study of other peoples and their customs. Such scrutiny of other peoples in distant lands raised basic questions about what methods natural history should employ and the extent to which it could serve as a foundation for more general and theoretical claims. By taking a wide sweep from the beginnings of the Royal Society until the end of the eighteenth century it is hoped light will be shed on the changing understanding of natural history over this period.
Robert Knox's An Historical Relation of the Island of Ceylon was produced, published and enlarged through the collaboration of the author with scholars including Robert Hooke and financial support from members of the East India Company. The Relation should be seen in the context of a number of texts collected, translated or commissioned by the East India Company in cooperation with the Royal Society during the late seventeenth century that informed and shaped both European expansion and natural philosophy. As well as circulating between European intellectual centres, often reorientated in the process of translation, these texts served as practical guides across settlements and trading posts abroad. Comparing written accounts with experience led to annotations and borrowings that served as the basis for further writings. Company records and Knox's own unpublished works reveal how the Relation was used as the basis for bio-prospecting for naturally occurring drugs and food sources and in efforts at agricultural transplantation spanning the Indian and Atlantic Oceans. Through the reports of seamen like Knox, such experiments contributed to contemporary theories concerning the effects of latitude on plant life.
The development of photographic reproduction in the late nineteenth century permitted images in a range of visual media to be published in the press. Focusing on the popular scientific monthly Knowledge, this paper explores the evidentiary status of reproductions of astronomical photographs. After succeeding its founder Richard Anthony Proctor in 1889, the new editor of Knowledge, Arthur Cowper Ranyard, introduced high-quality collotype reproductions into each number of the magazine. One of Ranyard's main interests was the structure of the Milky Way, evidence for which was only available through astronomical photographs. As Ranyard reproduced photographs in support of his arguments, he blurred the boundaries between the published collotype, the source negative and the astronomical phenomena themselves. Since each of these carried different evidentiary value, the confusion as to what, exactly, was under discussion did not go unremarked. While eminent astronomers disputed both Ranyard's arguments and the way in which they were presented, Knowledge disseminated both striking astronomical images and also a broader debate over how they should be interpreted.
In the 1940s the Marxist mathematician and historian of science Samuel Lilley (1914–87) made a substantial contribution to British history of science both intellectually and institutionally. His role, however, has largely gone unnoticed. Lilley is otherwise portrayed either as exemplifying the immaturity of Marxism, most famously by Rupert Hall in ‘Merton revisited’ (1963), or as a tragic figure marginalized during the Cold War because of his communist commitment. But both themes of exclusion and victimization keep Lilley's legacy hidden. By revisiting Lilley and his long-standing commitment to developing our discipline, this essay challenges the notion of radical discontinuity with respect to Lilley's legacy and argues for a more sustained contribution by Marxist historiography of science. This, in turn, requires a more appreciative understanding of the moderate Marxist model developed by Lilley in his popular, political and professional publications on the history of the social relations of science.
Sprat situated his analysis of the Royal Society within an emerging Anglican Royalist narrative of the longue durée of post-Reformation England. A closer examination of Sprat's own religious views reveals that his principal interest in the History of the Royal Society, as in the closely related reply to Samuel de Sorbière, the Observations, was to appropriate the advantages and benefits of the Royal Society as support for a re-established, anti-Calvinist Church of England. Sprat connected the two through a reformulation of the powerful conventions of ‘Reformation’ and ‘Israel’, both of which still resonated strongly in the religious politics of the 1660s. Applying his voluntarist theology, Sprat changed especially the representation of the chosen nation from a tale of divine castigation and punishment to a rational and probabilistic covenant based on material success as the indicator of God's pleasure. Sprat proposed that the knowledge and application of nature, through the experimental labours of the Royal Society, could build an increasingly wealthy nation and so a permanent home for the reconfigured Israel. Attaching this to a renewed monarchical and Anglican state also meant security for the traditional forms of rule.
This paper examines the relationship between the Admiralty and the Royal Observatory, Greenwich, by studying the roles of the Hydrographer and the Astronomer Royal as they worked together on the problem of communicating accurate time to ships. The collaboration between the Astronomer Royal and the Hydrographer directed the development of time balls and other visual signals throughout their period of use in Britain and its colonies. This paper focuses on the time ball and clock developed by the Astronomer Royal William Christie and the Hydrographer William Wharton as a key example of significant and productive collaboration between the two institutions. The paper also highlights the importance of the telegraph system to visual time signals. The ability to drop a time ball at a distance from an observatory created significant opportunities to improve the time signal service to mariners and stimulated further innovation in this field.
In May 2003, from the Baikanur launchpad in the Central Asian deserts of Kazakhstan, British scientists fired a Russian Soyuz-Fregat rocket to launch a probe called the Mars Express, intended to determine whether recognizable chemical signs of life could be found in the thin atmosphere and dusty rocks of the red planet. In 1971, the Soviets had been the first to land a probe on Mars, and they were followed by the American Viking missions in 1976. In January 2004, the U.S. National Aeronautics and Space Administration (NASA) landed the mobile rovers Spirit and Opportunity on Mars. These represented huge and dangerous efforts. Of thirty previous missions to Mars, twenty had gone seriously wrong. In 2003, a British probe intended to explore the Martian surface, called – significantly – Beagle-2, failed to arrive on the surface. The European mission cost 300 million euros and the American mission ten times as much. Behind all these efforts lies the necessity of securing wide political and public support. Thus, the space missions are performed in “full view of the public.” As Alan Wells, director of space research at the University of Leicester, put it, “We are breaking new ground in the public presentation of space science.” His duty, in his words, is to be a professor of public relations as well as planetary science.
Among the modern life sciences, physiology trails only the evolutionary sciences in the attention it has received from historians. Lamarck, Darwin, and Mendel may be better known than the heroes of modern physiology, but names such as François Magendie (1783–1855), Johannes Müller (1801–1858), Claude Bernard (1813–1878), Hermann von Helmholtz (1821–1894), Ivan Pavlov (1849–1936), and Charles Sherrington (1857–1952) require little introduction for those who read more than occasionally in the history of science. Physiology may have attracted such attention because it has been widely viewed as the first of the modern biological disciplines to emerge from traditional approaches to the phenomena of life embodied in medicine and natural history. Furthermore, physiology allowed historians of science of the first generation after World War II to develop a series of narratives that reflected their broader concerns about the nature and significance of modern science and about how to write its history. If the historiography of the physical sciences in the 1950s and 1960s found its normative models in the “Scientific Revolution” of the sixteenth and seventeenth centuries, so, too, in those decades did historians of the life sciences locate their normative models in nineteenth-century physiology.
Buoyed by the combination of optimism of understanding the natural world from Isaac Newton’s version of the mechanical philosophy and the excitement of discovering natural artifacts of the natural world from naturalists such as Carl Linnaeus, Abraham Werner, and Georges Buffon, natural philosophers turned increasingly to studying nature in nature by the end of the eighteenth century and the beginning of the nineteenth century. Certainly the maturation of the cabinet tradition in the form of emerging national museums (Muséum d’Histoire Naturelle, British Museum) and national botanical gardens (Royal Botanical Gardens at Kew) at this same time underscores the importance of learning from the natural world. Furthermore, continued overseas expansion and exploration, especially in North America, the Indian subcontinent of Asia, and Australia, heightened European interests in this direction.
Many of these same eighteenth-century motivations continued into the nineteenth century and, moreover, may be described after the model of scientific transmission and development offered by George Basalla, which he developed by examining the early history of American science vis-à-vis science in England. It is certainly appropriate to borrow from and to expand on Basalla, for much of the eighteenth-century interest in the natural world was exhibited by Europeans who observed nature outside of Europe, primarily within their colonial holdings. They collected specimens on voyages of discovery and recruited local colonialists to collect specimens that could later be sent back to European museums and universities following the return of the imperial explorers to their mother country (see MacLeod, Chapter 3, this volume).