Bicentenary of Four Platinum Group Metals
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Mister Mary Somerville: Husband and Secretary
Open Research Online The Open University’s repository of research publications and other research outputs Mister Mary Somerville: Husband and Secretary Journal Item How to cite: Stenhouse, Brigitte (2020). Mister Mary Somerville: Husband and Secretary. The Mathematical Intelligencer (Early Access). For guidance on citations see FAQs. c 2020 The Author https://creativecommons.org/licenses/by/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1007/s00283-020-09998-6 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Mister Mary Somerville: Husband and Secretary BRIGITTE STENHOUSE ary Somerville’s life as a mathematician and mathematician). Although no scientific learned society had a savant in nineteenth-century Great Britain was formal statute barring women during Somerville’s lifetime, MM heavily influenced by her gender; as a woman, there was nonetheless a great reluctance even toallow women her access to the ideas and resources developed and into the buildings, never mind to endow them with the rights circulated in universities and scientific societies was highly of members. Except for the visit of the prolific author Margaret restricted. However, her engagement with learned institu- Cavendish in 1667, the Royal Society of London did not invite tions was by no means nonexistent, and although she was women into their hallowed halls until 1876, with the com- 90 before being elected a full member of any society mencement of their second conversazione [15, 163], which (Societa` Geografica Italiana, 1870), Somerville (Figure 1) women were permitted to attend.1 As late as 1886, on the nevertheless benefited from the resources and social nomination of Isis Pogson as a fellow, the Council of the Royal networks cultivated by such institutions from as early as Astronomical Society chose to interpret their constitution as 1812. -
Philosophical Transactions, »
INDEX TO THE PHILOSOPHICAL TRANSACTIONS, » S e r ie s A, FOR THE YEAR 1898 (VOL. 191). A. Absorption, Change of, produced by Fluorescence (B urke), 87. Aneroid Barometers, Experiments on.—Elastic After-effect; Secular Change; Influence of Temperature (Chree), 441. B. Bolometer, Surface, Construction of (Petavel), 501. Brilliancy, Intrinsic, Law of Variation of, with Temperature (Petavel), 501. Burke (John). On the Change of Absorption produced by Fluorescence, 87. C. Chree (C.). Experiments on Aneroid Barometers at Kew Observatory, and their Discussion, 441. Correlation and Variation, Influence of Random Selection on (Pearson and Filon), 229. Crystals, Thermal Expansion Coefficients, by an Interference Method (Tutton), 313. D. Differential Equations of the Second Order, &c., Memoir on the Integration of; Characteristic Invariant of (Forsyth), 1. 526 INDEX. E. Electric Filters, Testing Efficiency of; Dielectrifying Power of (Kelvin, Maclean, and Galt), 187. Electricity, Diffusion of, from Carbonic Acid Gas to Air; Communication of, from Electrified Steam to Air (Kelvin, Maclean, and Galt), 187. Electrification of Air by Water Jet, Electrified Needle Points, Electrified Flame, &c., at Different Air-pressures; at Different Electrifying Potentials; Loss of Electrification (Kelvin, Maclean, and Galt), 187. Electrolytic Cells, Construction and Calibration of (Veley and Manley), 365. Emissivity of Platinum in Air and other Gases (Petavel), 501. Equations, Laplace's and other, Some New Solutions of, in Mathematical Physics (Forsyth), 1. Evolution, Mathematical Contributions to Theory o f; Influence of Random Selection on the Differentiation of Local Races (Pearson and Filon), 229. F. Filon (L. N. G.) and Pearson (Karl). Mathematical Contributions to the Theory of Evolution.—IV. On the Probable Errors of Frequency Constants and on the Influence of Random Selection on Variation and Correlation, 229. -
Archibald Geikie (1835–1924): a Pioneer Scottish Geologist, Teacher, and Writer
ROCK STARS Archibald Geikie (1835–1924): A Pioneer Scottish Geologist, Teacher, and Writer Rasoul Sorkhabi, University of Utah, Salt Lake City, Utah 84108, USA; [email protected] years later, but there he learned how to write reports. Meanwhile, he read every geology book he could find, including John Playfair’s Illustrations of the Huttonian Theory, Henry de la Beche’s Geological Manual, Charles Lyell’s Principles of Geology, and Hugh Miller’s The Old Red Sandstone. BECOMING A GEOLOGIST In the summer of 1851, while the Great Exhibition in London was attracting so many people, Geikie decided instead to visit the Island of Arran in the Clyde estuary and study its geology, aided by a brief report by Andrew Ramsay of the British Geological Survey. Geikie came back with a report titled “Three weeks in Arran by a young geologist,” published that year in the Edinburgh News. This report impressed Hugh Miller so much that the renowned geologist invited its young author to discuss geology over a cup of tea. Miller became Geikie’s first mentor. In this period, Geikie became acquainted with local scientists and pri- vately studied chemistry, mineralogy, and geology under Scottish naturalists, such as George Wilson, Robert Chambers, John Fleming, James Forbes, and Andrew Ramsay—to whom he con- fessed his desire to join the Geological Survey. In 1853, Geikie visited the islands of Skye and Pabba off the coast Figure 1. Archibald Geikie as a young geolo- of Scotland and reported his observations of rich geology, including gist in Edinburgh. (Photo courtesy of the British Geological Survey, probably taken in finds of Liassic fossils. -
The Partnership of Smithson Tennant and William Hyde Wollaston
“A History of Platinum and its Allied Metals”, by Donald McDonald and Leslie B. Hunt 9 The Partnership of Smithson Tennant and William Hyde Wollaston “A quantity of platina was purchased by me a few years since with the design of rendering it malleable for the different purposes to which it is adapted. That object has now been attained. ” WILLIAM HYDE W O L L A S T O N Up to the end of the eighteenth century the attempts to produce malleable platinum had advanced mainly in the hands of practical men aiming at its pre paration and fabrication rather than at the solution of scientific problems. These were now to be attacked with a marked degree of success by two remarkable but very different men who first became friends during their student days at Cam bridge and who formed a working partnership in 1800 designed not only for scientific purposes but also for financial reasons. They were of the same genera tion and much the same background as the professional scientists of London whose work was described in Chapter 8, and to whom they were well known, but with the exception of Humphry Davy they were of greater stature and made a greater advance in the development of platinum metallurgy than their predecessors. Their combined achievements over a relatively short span of years included the successful production for the first time of malleable platinum on a truly com mercial scale as well as the discovery of no less than four new elements contained in native platinum, a factor that was of material help in the purification and treatment of platinum itself. -
RBRC-32 BNL-6835.4 PARITY ODD BUBBLES in HOT QCD D. KHARZEEV in This ~A~Er We Give a Pedawwicalintroduction~0 Recent Work Of
RBRC-32 BNL-6835.4 PARITY ODD BUBBLES IN HOT QCD D. KHARZEEV RIKEN BNL Research Center, Br$ookhauenNational Laboratory, . Upton, New York 11973-5000, USA R.D. PISARSKI Department of Physics, Brookhaven National Laboratoy, Upton, New York 11973-5000, USA M.H.G. TYTGAT Seruice de Physique Th&orique, (7P 225, Uniuersitc4Libre de Bruzelles, B[ud. du !t%iomphe, 1050 Bruxelles, Belgium We consider the topological susceptibility for an SU(N) gauge theory in the limit of a large number of colors, N + m. At nonzero temperature, the behavior of the topological susceptibility depends upon the order of the reconfining phrrse transition. The meet interesting possibility is if the reconfining transition, at T = Td, is of second order. Then we argue that Witten’s relation implies that the topological suscepti~lfity vanishes in a calculable fdion at Td. Ae noted by Witten, this implies that for sufficiently light quark messes, metaetable etates which act like regions of nonzero O — parity odd bubbles — can arise at temperatures just below Td. Experimentally, parity odd bubbles have dramatic signature% the rI’ meson, and especially the q meson, become light, and are copiously produced. Further, in parity odd bubbles, processes which are normally forbidden, such as q + rr”ro, are allowed. The most direct way to detect parity violation is by measuring a parity odd global seymmetry for charged pions, which we define. 1 Introduction In this .-~a~er we give a Pedawwicalintroduction~0 recent work of ours? We I consider an SU(IV) gau”ge t~e~ry in the limit of a large number of colors, N + co, This is, of course, a familiar limit? We use the large N expansion I to investigate the behavior of the theory at nonzero temperature, especially for the topological susceptibility. -
William Hyde Wollaston Eric Clark
Downloaded from https://www.cambridge.org/core MicroscopyPioneers Pioneers in Optics: William Hyde Wollaston Eric Clark . IP address: From the website Molecular Expressions created by the late Michael Davidson and now maintained by Eric Clark, National Magnetic Field Laboratory, Florida State University, Tallahassee, FL 32306 170.106.202.226 [email protected] , on William Hyde Wollaston bladder stone that he named cystic oxide, later called cystine, the 03 Oct 2021 at 02:49:34 (1766–1828) first known amino acid. Twelve years later Wollaston provided The quantity and diversity the best contemporary physiological description of the ear. of William Hyde Wollaston’s Wollaston formed another alliance to perform chemis- research made him one of the try studies and experiments, this time with Smithson Tennant. most influential scientists of his Platinum had long evaded the efforts of chemists to concentrate , subject to the Cambridge Core terms of use, available at time. Although formally trained and purify the precious element, and the pair decided to join in as a physician, Wollaston studied the endeavor. When Tennant first tried to produce platinum, the and made advances in many sci- result was his discovery of the new elements iridium and osmium. entific fields, including chemistry, Wollaston’s later attempt led him to the discovery of palladium physics, botany, crystallography, and rhodium. He then invented the technique of powder metal- optics, astronomy, and mineral- lurgy and produced malleable platinum in 1805. The feat proved ogy. He is particularly noted for extremely profitable and provided him with financial indepen- being the first to observe dark lines dence for the rest of his life. -
James Hutton's Reputation Among Geologists in the Late Eighteenth and Nineteenth Centuries
The Geological Society of America Memoir 216 Revising the Revisions: James Hutton’s Reputation among Geologists in the Late Eighteenth and Nineteenth Centuries A. M. Celâl Şengör* İTÜ Avrasya Yerbilimleri Enstitüsü ve Maden Fakültesi, Jeoloji Bölümü, Ayazağa 34469 İstanbul, Turkey ABSTRACT A recent fad in the historiography of geology is to consider the Scottish polymath James Hutton’s Theory of the Earth the last of the “theories of the earth” genre of publications that had begun developing in the seventeenth century and to regard it as something behind the times already in the late eighteenth century and which was subsequently remembered only because some later geologists, particularly Hutton’s countryman Sir Archibald Geikie, found it convenient to represent it as a precursor of the prevailing opinions of the day. By contrast, the available documentation, pub- lished and unpublished, shows that Hutton’s theory was considered as something completely new by his contemporaries, very different from anything that preceded it, whether they agreed with him or not, and that it was widely discussed both in his own country and abroad—from St. Petersburg through Europe to New York. By the end of the third decade in the nineteenth century, many very respectable geologists began seeing in him “the father of modern geology” even before Sir Archibald was born (in 1835). Before long, even popular books on geology and general encyclopedias began spreading the same conviction. A review of the geological literature of the late eighteenth and the nineteenth centuries shows that Hutton was not only remembered, but his ideas were in fact considered part of the current science and discussed accord- ingly. -
Philosophical Transactions (A)
INDEX TO THE PHILOSOPHICAL TRANSACTIONS (A) FOR THE YEAR 1889. A. A bney (W. de W.). Total Eclipse of the San observed at Caroline Island, on 6th May, 1883, 119. A bney (W. de W.) and T horpe (T. E.). On the Determination of the Photometric Intensity of the Coronal Light during the Solar Eclipse of August 28-29, 1886, 363. Alcohol, a study of the thermal properties of propyl, 137 (see R amsay and Y oung). Archer (R. H.). Observations made by Newcomb’s Method on the Visibility of Extension of the Coronal Streamers at Hog Island, Grenada, Eclipse of August 28-29, 1886, 382. Atomic weight of gold, revision of the, 395 (see Mallet). B. B oys (C. V.). The Radio-Micrometer, 159. B ryan (G. H.). The Waves on a Rotating Liquid Spheroid of Finite Ellipticity, 187. C. Conroy (Sir J.). Some Observations on the Amount of Light Reflected and Transmitted by Certain 'Kinds of Glass, 245. Corona, on the photographs of the, obtained at Prickly Point and Carriacou Island, total solar eclipse, August 29, 1886, 347 (see W esley). Coronal light, on the determination of the, during the solar eclipse of August 28-29, 1886, 363 (see Abney and Thorpe). Coronal streamers, observations made by Newcomb’s Method on the Visibility of, Eclipse of August 28-29, 1886, 382 (see A rcher). Cosmogony, on the mechanical conditions of a swarm of meteorites, and on theories of, 1 (see Darwin). Currents induced in a spherical conductor by variation of an external magnetic potential, 513 (see Lamb). 520 INDEX. -
May 2016 Alan J. Rocke EDUCATION BA, 1969, Chemistry, Beloit College
-1- May 2016 Alan J. Rocke EDUCATION B.A., 1969, Chemistry, Beloit College, Beloit, Wisconsin M.A., 1973, History of Science, University of Wisconsin-Madison Thesis: “Isaac Newton’s Theory of Matter” University of Munich, West Germany, 1974-75 Ph.D., 1975, History of Science, University of Wisconsin-Madison Dissertation: “Origins of the Structural Theory in Organic Chemistry” ACADEMIC EMPLOYMENT University of Wisconsin-Madison 1969-74 Teaching Assistant, Depts. of Chemistry and History of Science 1975-78 Lecturer, Depts. of Chemistry and Integrated Liberal Studies Case Western Reserve University 1978-84 Assistant Professor of History of Science and Technology, Department of Interdisciplinary Studies 1984-93 Associate Professor of History of Technology and Science 1993-2016 Professor of History 1995-2016 Henry Eldridge Bourne Professor of History 2012- Distinguished University Professor AWARDS AND HONORS Jack Youden Prize (American Society for Quality Control, Chemical Division), 1982 Carl F. Wittke Award for Excellence in Undergraduate Teaching, 1988 Outstanding Paper Award (American Chemical Society, History Division), 1992 Dexter Award for Outstanding Lifetime Contributions to the History of Chemistry (American Chemical Society), 2000 Fellow of the American Association for the Advancement of Science, 2000 Liebig-Wöhler Freundschafts-Preis, Lewicki Foundation, Göttingen, 2002 Membre correspondant, Académie Internationale d’Histoire des Sciences, 2007 Fellow of the American Chemical Society, 2012 Distinguished University Professor, 2012 -
the Papers Philosophical Transactions
ABSTRACTS / OF THE PAPERS PRINTED IN THE PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY OF LONDON, From 1800 to1830 inclusive. VOL. I. 1800 to 1814. PRINTED, BY ORDER OF THE PRESIDENT AND COUNCIL, From the Journal Book of the Society. LONDON: PRINTED BY RICHARD TAYLOR, RED LION COURT, FLEET STREET. CONTENTS. VOL. I 1800. The Croonian Lecture. On the Structure and Uses of the Meinbrana Tympani of the Ear. By Everard Home, Esq. F.R.S. ................page 1 On the Method of determining, from the real Probabilities of Life, the Values of Contingent Reversions in which three Lives are involved in the Survivorship. By William Morgan, Esq. F.R.S.................... 4 Abstract of a Register of the Barometer, Thermometer, and Rain, at Lyndon, in Rutland, for the year 1798. By Thomas Barker, Esq.... 5 n the Power of penetrating into Space by Telescopes; with a com parative Determination of the Extent of that Power in natural Vision, and in Telescopes of various Sizes and Constructions ; illustrated by select Observations. By William Herschel, LL.D. F.R.S......... 5 A second Appendix to the improved Solution of a Problem in physical Astronomy, inserted in the Philosophical Transactions for the Year 1798, containing some further Remarks, and improved Formulae for computing the Coefficients A and B ; by which the arithmetical Work is considerably shortened and facilitated. By the Rev. John Hellins, B.D. F.R.S. .......................................... .................................. 7 Account of a Peculiarity in the Distribution of the Arteries sent to the ‘ Limbs of slow-moving Animals; together with some other similar Facts. In a Letter from Mr. -
Charles Lyell and Gideon Mantell, 1821 - 1852: Their Quest for Elite Status in English Geology
CHARLES LYELL AND GIDEON MANTELL, 1821 - 1852: THEIR QUEST FOR ELITE STATUS IN ENGLISH GEOLOGY. Alan John Wennerbom A thesis submitted in fulfilment of the requirements for the degree of Doctor of Philosophy Unit for the History University of Sydney and Philosophy of Science May 1999 SYNOPSIS An analysis of the correspondence between Charles Lyell and Gideon Mantell from 1821 to 1852, in conjunction with other manuscript material, highlights the contrasting backgrounds and geological careers of the two men. It is also characterised by two underlying themes: the nature and timing of their geological work; and the influence of various social factors on their career plans and desire to achieve high social and scientific status. In turn, these points raise several wider issues and inter-related questions concerning the following aspects of English geology in the first half of the nineteenth century. · When, why and how did an elite group of geologists emerge in England during this period? Who were its members and what were their characteristics in common? · What was the nature and scope of the geological work carried out by the identified elite? In what way did it differ from Mantell’s? · What social and other barriers did Mantell encounter in his search for scientific and social status? What were the critical factors? In this thesis these issues are examined on a decade-by-decade basis, in three main chapters, as a prelude to examining the central question of why Mantell, unlike Lyell, did not achieve the status of an elite geologist. First, an elite group of English geologists is identified through a series of prosopographic and ‘screening’ analyses of all members of council of the Geological Society of London (GSL). -
One Century of Cosmic Rays – a Particle Physicist\'S View
EPJ Web of Conferences 105, 00001 (2015) DOI: 10.1051/epjconf/201510500001 c Owned by the authors, published by EDP Sciences, 2015 One century of cosmic rays – A particle physicist’s view Christine Suttona CERN, 1211 Geneva 23, Switzerland Abstract. Experiments on cosmic rays and the elementary particles share a common history that dates back to the 19th century. Following the discovery of radioactivity in the 1890s, the paths of the two fields intertwined, especially during the decades after the discovery of cosmic rays. Experiments demonstrated that the primary cosmic rays are positively charged particles, while other studies of cosmic rays revealed various new sub-atomic particles, including the first antiparticle. Techniques developed in common led to the birth of neutrino astronomy in 1987 and the first observation of a cosmic γ -ray source by a ground-based cosmic-ray telescope in 1989. 1. Introduction remove the air led to the discovery of “cathode rays” emitted from the cathode at one end of the tube. In 1879, in “There are more things in heaven and earth than are the course of investigations in England, William Crookes dreamt of in your philosophy ...” (Hamlet, William discovered that the speed of the discharge along the length Shakespeare). of a vacuum tube decreased as he reduced the pressure. This indicated that ionization of the air was causing the The modern fields of cosmic-ray studies and experimental discharge. particle physics have much in common, as they both The last few years of the 19th century saw a burst investigate the high-energy interactions of subatomic of discoveries that not only cast light on the effect that particles.