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Introduction -- Stout's proto-new-realism -- Situating G.F. Stout -- Stout's doctrine of primary and secondary qualities -- Stout and the Brentano School -- Representative function of presentations -- Sensible space and real space -- Cook Wilson's geometrical counter-example -- Stout's central question -- Ideal constructions -- Ideal constructions in psychology and epistemology -- British new realism : the language of madness -- Stout's criticisms of Alexander -- Alexander's response -- The nature of sensations, images, and other presentations -- What is (...) the metaphysical problem? -- "How can the interpretation which is supplied by the mind be a constituent of the [physical] object?" -- Some general remarks -- British new realism : the language of common-sense -- T.P. Nunn and the new realism -- Nunn and things -- Nunn's postulate -- Russell and Stout on sensible objects -- Russell, sense-data and sensibilia -- The methods of construction -- Russell's constructions and Nunn's postulate -- Constructions, psychology, and the essence of philosophy -- The methods of logical construction -- A mathematical development -- The principle of abstraction. (shrink)

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What Russell regarded to be the ‘chief outcome’ of his 1914 Lowell Lectures at Harvard can only be fully appreciated, I argue, if one embeds the outcome back into the ‘classificatory problem’ that many at the time were heavily engaged in. The problem focused on the place and relationships between the newly formed or recently professionalized disciplines such as psychology, Erkenntnistheorie, physics, logic and philosophy. The prime metaphor used in discussions about the classificatory problem by British philosophers was a spatial (...) one, with such motifs as ‘standpoints’, ‘place’ and ‘perspectives’ in the space of knowledge. In fact, Russell’s construction of a perspectival space of six-dimensions was meant precisely to be a timely solution to the widely discussed classificatory problem. (shrink)

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This paper examines the interrelations between astronomical images of nebulae and their observation. In particular, using the case of the ‘Great Spiral’ , we follow this nebula beginning with its discovery and first sketch made by the third Earl of Rosse in 1845, to giving an account, using archival sources, of exactly how other images of the same object were produced over the years and stabilized within the record books of the Rosse project. It will be found that a particular (...) ‘procedure’ was employed using ‘working images’ that interacted with descriptions, other images and the telescopic object itself. This stabilized not only some set of standard images of the object, but also a very potent conception of spirality as well, i.e. as a ‘normal form’. Finally, two cases will be contrasted, one being George Bond's application of this spiral conception to the nebula in Orion, and the other Wilhelm Tempel's rejection of the spiral form in M51. (shrink)

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In lieu of an abstract, here is a brief excerpt of the content:February 19, 2011 (11:48 am) E:\CPBR\RUSSJOUR\TYPE3002\russell 30,2 040 red.wpd russell: the Journal of Bertrand Russell Studies n.s. 30 (winter 2010–11): 155–82 The Bertrand Russell Research Centre, McMaster U. issn 0036-01631; online 1913-8032 eviews AN INTRODUCTION TO THE PROBLEMSz Omar W. Nasim Science Studies / Swiss Federal Institute of Technology (eth) 8092 Zürich, Switzerland[email protected] David Mills Daniel and Megan Daniel. BrieXy: Russell’sz The Problems of Philosophy. London: scm P., (...) 2007. Pp. viii, 131. isbn 978-0-334-04118-4. £7.99. The following book is a part of the SCM BrieXyz series, which already includes such titles as Anselm’s Prosologion and Kierkegaard’s Fear and Trembling. The series objective is to “enable students and general readers to acquire knowledge and understanding of key texts in philosophy, philosophy of religion, theology and ethics” (p. vii). Each volume is a “short guide” to a particular philosopher ’s ideas through a close reading of a primary text by that philosopher. This review looks at the volume on Bertrand Russell’s The Problems of Philosophy, which is divided by the authors into a few parts, including a section on the “Context”, a “Detailed Summary of Bertrand Russell’s The Problem of Philosophy ”, an overview and a helpful glossary of terms. The “Context” provides a very brief statement about who Russell was, and spends most of its pages summarizing the arguments of Russell’s Problems. The last few pages of this section provide some helpful “Issues to Consider,” which are a list of pertinent questions one may ask of Russell’s Problems, and ends with some further reading. It ought to be noted that the “Context” is not about the history of Russell’s text, nor is it an attempt to relate the latter to Russell’s other works. This is unfortunate, considering Russell’s well-known philosophical development and the rich history surrounding Problems. The volume under review is indeed a problemoriented study of Problems which uncritically rehearses the same embedding of problems that Russell urges, especially in relation to the British empiricist tradition of the early modern period. The main section of the book is the “Detailed Summary” and is itself divided in the same way in which Russell’s Problems is divided; that is, into Wfteen subsections, with exactly the same headings and order. Using a reissued second edi- February 19, 2011 (11:48 am) E:\CPBR\RUSSJOUR\TYPE3002\russell 30,2 040 red.wpd 156 Reviews 1 It has the same pagination as oup’s 1967 edition in the uk.z—zEd. tion of Russell’s Problems by Oxford University Press (2001),1 Daniel and Daniel provide a very close, page-by-page exposition of each chapter of Russell’s Problems. The reading is in fact so close that not only is there nearly the same number of pages dedicated to each chapter as in the original, but just about every sentence teems with scare quotes. This goes for not only technical terms such as “universal”, “sense-data”, “relations”, etc., which remain snared by scare quotes throughout the entire section, but also all sorts of other terms such as “light”, “motion”, “just”, “forgotten”, etc. The rationale for this is given in the introduction and is supposed to “enable the reader to follow each development in the philosopher’s argument” (p. vii). Unlike the terms that are in bold type, which are given some explanation in the glossary, the reviewer Wnds the sheer number of scare quotes distracting and pedagogically confusing, because there is no distinction made between terms central to Russell’s argument and those used only in the construction of a sentence. But even the glossary entries are oddly compiled. While most correspond to the bold-type terms in the Summary, some are terms not found anywhere but in the introduction or the “Context” section. So Sartre, Wittgenstein, McMaster University, and Bertrand Russell Peace Foundation are nowhere to be found in Russell’s original, or in the summary provided by the authorsz—zthey are simply terms used in passing in the introduction or “Context” and without being introduced in bold type. Other... (shrink)

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ArgumentKeeping records has always been an essential part of science. Aside from natural history and the laboratory sciences, no other observational science reflects this activity of record-keeping better than astronomy. Central to this activity, historically speaking, are tools so mundane and common that they are easily overlooked; namely, the notebook and the pencil. One obvious function of these tools is clearly a mnemonic one. However, there are other relevant functions of paperwork that often go unnoticed. Among these, I argue, is (...) the strategic use made of different procedures of record keeping to prolong observational time with a target object. Highlighting this function will help us to appreciate the supporting role played by the notebook and the pencil to extend the observational time spent with a target object. With objects as delicate, faint, and mysterious as the nebulae, the procedures used to record their observations helped nineteenth-century observers overcome the temporal handicaps and limitations of large and clumsy telescopes, mounted in the altazimuth manner. To demonstrate the importance of paper and pencil, I will closely examine the observing books, the drawings found therein, and the telescopes of three nineteenth-century observers of the nebulae: Sir John F. W. Herschel, Lord Rosse, and William Lassell. (shrink)

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Today we are all familiar with the iconic pictures of the nebulae produced by the Hubble Space Telescope’s digital cameras. But there was a time, before the successful application of photography to the heavens, in which scientists had to rely on handmade drawings of these mysterious phenomena. Observing by Hand sheds entirely new light on the ways in which the production and reception of handdrawn images of the nebulae in the nineteenth century contributed to astronomical observation. Omar W. Nasim investigates (...) hundreds of unpublished observing books and paper records from six nineteenth-century observers of the nebulae: Sir John Herschel; William Parsons, the third Earl of Rosse; William Lassell; Ebenezer Porter Mason; Ernst Wilhelm Leberecht Tempel; and George Phillips Bond. Nasim focuses on the ways in which these observers created and employed their drawings in data-driven procedures, from their choices of artistic materials and techniques to their practices and scientific observation. He examines the ways in which the act of drawing complemented the acts of seeing and knowing, as well as the ways that making pictures was connected to the production of scientific knowledge. An impeccably researched, carefully crafted, and beautifully illustrated piece of historical work, Observing by Hand will delight historians of science, art, and the book, as well as astronomers and philosophers. (shrink)

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For this year’s Virtual Issue, our guest editor, Omar W. Nasim, has collected together papers from the Aristotelian Society archives that represent a substantial part of a dispute that contributed to the emergence of analytic philosophy in Britain at the turn of the 20th Century. The dispute was primarily concerned with the problem of the external world – the nature of the sensible objects of perception, and how they relate to physical things and the perceiving subject. The participants in this (...) controversy contested the nature of the appearance-reality distinction, whether it is it is possible for a thing to instantiate contrary sensible qualities at the same place and time, the distinction between presentation and representation, the nature of knowledge by acquaintance, and the nature of sense-data – e.g., whether sense-data are psychical or physical, whether they persist unperceived, and how they give rise to knowledge of the external world. G. E. Moore and Bertrand Russell were significant contributors to these debates, but so too were several philosophers whose names are now less well known: G. F. Stout, G. Dawes Hicks, Abraham Wolf, T. Percy Nunn, and S. Alexander. This Virtual Issue collects together, for the first time, the important contributions made to these debates by all of these figures. In doing so it provides a fascinating insight into the ways in which Russell’s earliest attempts to construct the external world from sense-data were influenced by the ideas and arguments of his immediate contemporaries. Omar W. Nasim’s specially commissioned introduction to the Virtual Issue sets out the historical context of these disputes about the external world, and details the prominent role played by the Aristotelian Society in making them possible. (shrink)

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This paper argues for continuity in purpose and specific results between some hand drawn nebulae, especially those ‘descriptive maps’ by John F. W. Herschel and E. P. Mason in the late 1830s, and the first photographs made of the nebulae in the 1880s. Using H. H. Turners’ explication in 1904 of the three great advantages of astrophotography, the paper concludes that to some extent Herschel’s and Mason’s hand-drawings of the nebulae were meant to achieve the same kinds of results. This (...) is surprising not only because such drawings were conceived and achieved over forty-years earlier, but also because the procedures used in the production of these pictorially and metrically rich images were those directly inspired by cartography, geodesy, and land-surveying. Such drawings provided the standard for what was depicted, expected and aimed at by way of successful representations of the nebulae; standards that seemed to have been used to judge the success of nebular photographs. Being conditions of expectation and possibility for later photography, these drawings were themselves made possible by such techniques of representation and measurement as isolines and triangulation, so fundamental to Imperial and ‘Humboltian science.’Keywords: Ebenezer Porter Mason; Cartography; Draughtsmanship; Observation; Scientific Representation; Philosophy of Scientific Practice. (shrink)

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