The Project Gutenberg Ebook #35588: <TITLE>
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Charles Darwin: a Companion
CHARLES DARWIN: A COMPANION Charles Darwin aged 59. Reproduction of a photograph by Julia Margaret Cameron, original 13 x 10 inches, taken at Dumbola Lodge, Freshwater, Isle of Wight in July 1869. The original print is signed and authenticated by Mrs Cameron and also signed by Darwin. It bears Colnaghi's blind embossed registration. [page 3] CHARLES DARWIN A Companion by R. B. FREEMAN Department of Zoology University College London DAWSON [page 4] First published in 1978 © R. B. Freeman 1978 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording or otherwise without the permission of the publisher: Wm Dawson & Sons Ltd, Cannon House Folkestone, Kent, England Archon Books, The Shoe String Press, Inc 995 Sherman Avenue, Hamden, Connecticut 06514 USA British Library Cataloguing in Publication Data Freeman, Richard Broke. Charles Darwin. 1. Darwin, Charles – Dictionaries, indexes, etc. 575′. 0092′4 QH31. D2 ISBN 0–7129–0901–X Archon ISBN 0–208–01739–9 LC 78–40928 Filmset in 11/12 pt Bembo Printed and bound in Great Britain by W & J Mackay Limited, Chatham [page 5] CONTENTS List of Illustrations 6 Introduction 7 Acknowledgements 10 Abbreviations 11 Text 17–309 [page 6] LIST OF ILLUSTRATIONS Charles Darwin aged 59 Frontispiece From a photograph by Julia Margaret Cameron Skeleton Pedigree of Charles Robert Darwin 66 Pedigree to show Charles Robert Darwin's Relationship to his Wife Emma 67 Wedgwood Pedigree of Robert Darwin's Children and Grandchildren 68 Arms and Crest of Robert Waring Darwin 69 Research Notes on Insectivorous Plants 1860 90 Charles Darwin's Full Signature 91 [page 7] INTRODUCTION THIS Companion is about Charles Darwin the man: it is not about evolution by natural selection, nor is it about any other of his theoretical or experimental work. -
Philosophical Rhetoric in Early Quantum Mechanics, 1925-1927
b1043_Chapter-2.4.qxd 1/27/2011 7:30 PM Page 319 b1043 Quantum Mechanics and Weimar Culture FA 319 Philosophical Rhetoric in Early Quantum Mechanics 1925–27: High Principles, Cultural Values and Professional Anxieties Alexei Kojevnikov* ‘I look on most general reasoning in science as [an] opportunistic (success- or unsuccessful) relationship between conceptions more or less defined by other conception[s] and helping us to overlook [danicism for “survey”] things.’ Niels Bohr (1919)1 This paper considers the role played by philosophical conceptions in the process of the development of quantum mechanics, 1925–1927, and analyses stances taken by key participants on four main issues of the controversy (Anschaulichkeit, quantum discontinuity, the wave-particle dilemma and causality). Social and cultural values and anxieties at the time of general crisis, as identified by Paul Forman, strongly affected the language of the debate. At the same time, individual philosophical positions presented as strongly-held principles were in fact flexible and sometimes reversible to almost their opposites. One can understand the dynamics of rhetorical shifts and changing strategies, if one considers interpretational debates as a way * Department of History, University of British Columbia, 1873 East Mall, Vancouver, British Columbia, Canada V6T 1Z1; [email protected]. The following abbreviations are used: AHQP, Archive for History of Quantum Physics, NBA, Copenhagen; AP, Annalen der Physik; HSPS, Historical Studies in the Physical Sciences; NBA, Niels Bohr Archive, Niels Bohr Institute, Copenhagen; NW, Die Naturwissenschaften; PWB, Wolfgang Pauli, Wissenschaftlicher Briefwechsel mit Bohr, Einstein, Heisenberg a.o., Band I: 1919–1929, ed. A. Hermann, K.V. -
Charles Galton Darwin's 1922 Quantum Theory of Optical Dispersion
Eur. Phys. J. H https://doi.org/10.1140/epjh/e2020-80058-7 THE EUROPEAN PHYSICAL JOURNAL H Charles Galton Darwin's 1922 quantum theory of optical dispersion Benjamin Johnson1,2, a 1 Max Planck Institute for the History of Science Boltzmannstraße 22, 14195 Berlin, Germany 2 Fritz-Haber-Institut der Max-Planck-Gesellschaft Faradayweg 4, 14195 Berlin, Germany Received 13 October 2017 / Received in final form 4 February 2020 Published online 29 May 2020 c The Author(s) 2020. This article is published with open access at Springerlink.com Abstract. The quantum theory of dispersion was an important concep- tual advancement which led out of the crisis of the old quantum theory in the early 1920s and aided in the formulation of matrix mechanics in 1925. The theory of Charles Galton Darwin, often cited only for its reliance on the statistical conservation of energy, was a wave-based attempt to explain dispersion phenomena at a time between the the- ories of Ladenburg and Kramers. It contributed to future successes in quantum theory, such as the virtual oscillator, while revealing through its own shortcomings the limitations of the wave theory of light in the interaction of light and matter. After its publication, Darwin's theory was widely discussed amongst his colleagues as the competing inter- pretation to Compton's in X-ray scattering experiments. It also had a pronounced influence on John C. Slater, whose ideas formed the basis of the BKS theory. 1 Introduction Charles Galton Darwin mainly appears in the literature on the development of quantum mechanics in connection with his early and explicit opinions on the non- conservation (or statistical conservation) of energy and his correspondence with Niels Bohr. -
Essays on Francis Galton, George Darwin and the Normal Curve of Evolutionary Biology, Mathematical Association, 2018, 127 Pp, £9.00, ISBN 978-1-911616-03-0
This work by Dorothy Leddy is licensed under a Creative Commons Attribution- ShareAlike 4.0 International License. To view a copy of this license, visit http://creativecommons.org/licenses/by-sa/4.0/ or send a letter to Creative Commons, PO Box 1866, Mountain View, CA 94042, USA. This is the author’s original submitted version of the review. The finally accepted version of record appeared in the British Journal for the History of Mathematics, 2019, 34:3, 195-197, https://doi.org/10.1080/26375451.2019.1617585 Chris Pritchard, A Common Family Weakness for Statistics: Essays on Francis Galton, George Darwin and the Normal Curve of Evolutionary Biology, Mathematical Association, 2018, 127 pp, £9.00, ISBN 978-1-911616-03-0 George Darwin, born halfway through the nineteenth century into a family to whom the principle of evolution was key, at a time when the use of statistics to study such a concept was in its infancy, found a kindred spirit in Francis Galton, 23 years his senior, who was keen to harness statistics to aid the investigation of evolutionary matters. George Darwin was the fifth child of Charles Darwin, the first proponent of evolution. He initially trained as a barrister and was finally an astronomer, becoming Plumian Professor of Astronomy and Experimental Philosophy at Cambridge University and President of the Royal Astronomical Society. In between he was a mathematician and scientist, graduating as Second Wrangler in the Mathematics Tripos in 1868 from Trinity College Cambridge. Francis Galton was George Darwin’s second cousin. He began his studies in medicine, turning after two years to mathematics at Trinity College Cambridge. -
Moon-Earth-Sun: the Oldest Three-Body Problem
Moon-Earth-Sun: The oldest three-body problem Martin C. Gutzwiller IBM Research Center, Yorktown Heights, New York 10598 The daily motion of the Moon through the sky has many unusual features that a careful observer can discover without the help of instruments. The three different frequencies for the three degrees of freedom have been known very accurately for 3000 years, and the geometric explanation of the Greek astronomers was basically correct. Whereas Kepler’s laws are sufficient for describing the motion of the planets around the Sun, even the most obvious facts about the lunar motion cannot be understood without the gravitational attraction of both the Earth and the Sun. Newton discussed this problem at great length, and with mixed success; it was the only testing ground for his Universal Gravitation. This background for today’s many-body theory is discussed in some detail because all the guiding principles for our understanding can be traced to the earliest developments of astronomy. They are the oldest results of scientific inquiry, and they were the first ones to be confirmed by the great physicist-mathematicians of the 18th century. By a variety of methods, Laplace was able to claim complete agreement of celestial mechanics with the astronomical observations. Lagrange initiated a new trend wherein the mathematical problems of mechanics could all be solved by the same uniform process; canonical transformations eventually won the field. They were used for the first time on a large scale by Delaunay to find the ultimate solution of the lunar problem by perturbing the solution of the two-body Earth-Moon problem. -
Calcul Des Probabilités
1913.] SHORTER NOTICES. 259 by series to the Legendre, Bessel, and hypergeometric equations will be useful to the student. The last of the important Zusâtze (see pages 637-663) is devoted to an exposition of the theory of systems of simul taneous differential equations of the first order. Having thus passed in quick review the contents of the book, it is now apparent that the translator has certainly accom plished his purpose of making it more useful to the student of pure mathematics. There remains the question whether there are not other additions which would have been desirable in accomplishing this purpose. There is at least one which, in the reviewer's opinion, should have been inserted. In connection with the theory of formal integration by series it would have been easy to insert a proof of the convergence in general of the series for the case of second order equations; and one can but regret that this was not done. Such a treat ment would have required only a half-dozen pages; and it would have added greatly to the value of this already valuable section. The translator's reason for omitting it is obvious; he was making no use of function-theoretic considerations, and such a proof would have required the introduction of these notions. But the great value to the student of having at hand this proof, for the relatively simple case of second order equations, seems to be more than a justification for departing in this case from the general plan of the book; it seems indeed to be a demand for it. -
Analytical Model for the Tidal Evolution of the Evection 10.1029/2019JE006266 Resonance and the Timing of Resonance Escape Key Points: William R
RESEARCH ARTICLE Analytical Model for the Tidal Evolution of the Evection 10.1029/2019JE006266 Resonance and the Timing of Resonance Escape Key Points: William R. Ward1, Robin M. Canup1 , and Raluca Rufu1 • Capture of the Moon into the evection resonance with the Sun 1Planetary Science Directorate, Southwest Research Institute, Boulder, CO, USA transfers angular momentum from the Earth‐Moon to Earth's heliocentric orbit • Using the Mignard tidal model, we Abstract A high‐angular momentum giant impact with the Earth can produce a Moon with a silicate find that escape from evection isotopic composition nearly identical to that of Earth's mantle, consistent with observations of terrestrial occurs early with minimal angular and lunar rocks. However, such an event requires subsequent angular momentum removal for consistency momentum loss from the Earth‐Moon with the current Earth‐Moon system. The early Moon may have been captured into the evection resonance, • Processes beyond formal evection occurring when the lunar perigee precession period equals 1 year. It has been proposed that after a high‐ resonance are needed to reconcile a angular momentum giant impact, evection removed the angular momentum excess from the Earth‐Moon high‐angular momentum giant impact with the current Earth‐Moon pair and transferred it to Earth's orbit about the Sun. However, prior N‐body integrations suggest this result Supporting Information: depends on the tidal model and chosen tidal parameters. Here, we examine the Moon's encounter with • Supporting Information S1 evection using a complementary analytic description and the Mignard tidal model. While the Moon is in resonance, the lunar longitude of perigee librates, and if tidal evolution excites the libration amplitude Correspondence to: sufficiently, escape from resonance occurs. -
Arxiv:1603.07071V1
Dynamical Evidence for a Late Formation of Saturn’s Moons Matija Cuk´ Carl Sagan Center, SETI Institute, 189 North Bernardo Avenue, Mountain View, CA 94043 [email protected] Luke Dones Southwest Research Institute, Boulder, CO 80302 and David Nesvorn´y Southwest Research Institute, Boulder, CO 80302 Received ; accepted Revised and submitted to The Astrophysical Journal arXiv:1603.07071v1 [astro-ph.EP] 23 Mar 2016 –2– ABSTRACT We explore the past evolution of Saturn’s moons using direct numerical in- tegrations. We find that the past Tethys-Dione 3:2 orbital resonance predicted in standard models likely did not occur, implying that the system is less evolved than previously thought. On the other hand, the orbital inclinations of Tethys, Dione and Rhea suggest that the system did cross the Dione-Rhea 5:3 resonance, which is closely followed by a Tethys-Dione secular resonance. A clear implica- tion is that either the moons are significantly younger than the planet, or that their tidal evolution must be extremely slow (Q > 80, 000). As an extremely slow-evolving system is incompatible with intense tidal heating of Enceladus, we conclude that the moons interior to Titan are not primordial, and we present a plausible scenario for the system’s recent formation. We propose that the mid-sized moons re-accreted from a disk about 100 Myr ago, during which time Titan acquired its significant orbital eccentricity. We speculate that this disk has formed through orbital instability and massive collisions involving the previous generation of Saturn’s mid-sized moons. We identify the solar evection resonance perturbing a pair of mid-sized moons as the most likely trigger of such an insta- bility. -
The Prodigious Life and Untimely Death of “Harry” Moseley
The prodigious life and untimely death of “Harry” Moseley Bretislav Friedrich Fritz Haber Institute of the Max Planck Society, Faradayweg 4-6, D-14195 Berlin “My Harry was killed in the Dardanelles” is the entry from 10 August 1915 in the diary of the mother of Henry (“Harry”) Gwin Jeffreys Moseley. He was shot on that day in the head during the failed Anglo-French invasion of the Ottoman Empire from the sea. The previous year, when he volunteered to join Lord Kitchener’s New Army, he was nominated for two Nobel Prizes, one for chemistry and one for physics, for his work on X-ray spectroscopy and atomic structure. Moseley’s tragic death at age 27 was widely reported not just in the Allied countries, but also in Germany. Its futility fired up Ernest Rutherford, Moseley’s mentor, to write an indignant letter to Nature: “It is a national tragedy that our military organization at the start of the war was so inelastic as to be unable, with a few exceptions, to utilise the scientific services of our men, except as combatants in the firing line. Our regret for the untimely death of Moseley is all the more poignant.” Three years before, as Rutherford’s affiliate at the University of Manchester, Moseley recognized that “a platinum target [upon electron impact] gives out a sharp line [X-ray] spectrum … which [a] crystal separates out [into monochromatic lines] as if it were a diffraction grating … There is here a whole new branch of spectroscopy which is sure to tell one much about the nature of an atom.” This letter of Moseley, addressed, as so many of his other letters, to his mother, marks the beginning of X-ray spectroscopy. -
Balfour V. Huxley on Evolutionary Naturalism: a 21St Century Perspective
S & CB (2003), 15, 41–63 0954–4194 JOHN GREENE Balfour v. Huxley on Evolutionary Naturalism: A 21st century Perspective This essay begins by setting forth the conflicting prophecies, in 1895, of Arthur James Balfour and Thomas Henry Huxley concerning the probable course of Western culture in the twentieth century if Huxley’s ‘scientific naturalism’ were to prevail over Balfour’s theistic conception of the relations between science and religion. The essay then examines some leading developments in the physical, biological, and social sciences and in philosophy and theology since 1900 to determine which of these prophecies, if either, proved to be truly prophetic. The author concludes that Balfour was the better prophet. Keywords: evolution, naturalism, positivism, emergence, metaphor, science, philosophy, theology. In 1895, Arthur James Balfour, a philosophically trained Scottish politician- statesman then serving as Chancellor of the Exchequer, published a book enti- tled Foundations of Belief, Being Notes Introductory to the Study of Theology containing a searching criticism of the evolutionary naturalism which Thomas Henry Huxley had labeled ‘scientific naturalism’. The naturalism underlying positivism, agnosticism, and empiricism, Balfour argued, rested on two grounds: (1) it reduced human experience to sense perception with the result that the only knowledge available to human beings was knowledge of phe- nomena, the things that appear to our senses, and the laws connecting them; and (2) it viewed human nature in all its aspects as -
1. INTRODUCTION Imations, We Thought It Worthwhile to Verify the Evolution the Origin of the Moon Is Still Unclear
THE ASTRONOMICAL JOURNAL, 115:1653È1663, 1998 April ( 1998. The American Astronomical Society. All rights reserved. Printed in the U.S.A. RESONANCES IN THE EARLY EVOLUTION OF THE EARTH-MOON SYSTEM JIHAD TOUMA McDonald Observatory, University of Texas, Austin, TX 78712; touma=harlan.as.utexas.edu AND JACK WISDOM Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139; wisdom=mit.edu Received 1997 November 25; revised 1997 December 26 ABSTRACT Most scenarios for the formation of the Moon place the Moon near Earth in low-eccentricity orbit in the equatorial plane of Earth. We examine the dynamical evolution of the Earth-Moon system from such initial conÐgurations. We Ðnd that during the early evolution of the system, strong orbital resonances are encountered. Passage through these resonances can excite large lunar orbital eccentricity and modify the inclination of the Moon to the equator. Scenarios that resolve the mutual inclination problem are presented. A period of large lunar eccentricity would result in substantial tidal heating in the early Moon, providing a heat source for the lunar magma ocean. The resonance may also play a role in the formation of the Moon. Key words: celestial mechanics, stellar dynamics È Earth È Moon regression of the MoonÏs node. With so many approx- 1. INTRODUCTION imations, we thought it worthwhile to verify the evolution The origin of the Moon is still unclear. The classic sce- of the system with numerical simulation. Our hope was that narios for the formation of the Moon include coaccretion, through direct numerical simulation we would uncover Ðssion, and capture. -
A Modern Almagest an Updated Version of Ptolemy’S Model of the Solar System
A Modern Almagest An Updated Version of Ptolemy’s Model of the Solar System Richard Fitzpatrick Professor of Physics The University of Texas at Austin Contents 1 Introduction 5 1.1 Euclid’sElementsandPtolemy’sAlmagest . ......... 5 1.2 Ptolemy’sModeloftheSolarSystem . ..... 5 1.3 Copernicus’sModeloftheSolarSystem . ....... 10 1.4 Kepler’sModeloftheSolarSystem . ..... 11 1.5 PurposeofTreatise .................................. .. 12 2 Spherical Astronomy 15 2.1 CelestialSphere................................... ... 15 2.2 CelestialMotions ................................. .... 15 2.3 CelestialCoordinates .............................. ..... 15 2.4 EclipticCircle .................................... ... 17 2.5 EclipticCoordinates............................... ..... 18 2.6 SignsoftheZodiac ................................. ... 19 2.7 Ecliptic Declinations and Right Ascenesions. ........... 20 2.8 LocalHorizonandMeridian ............................ ... 20 2.9 HorizontalCoordinates.............................. .... 23 2.10 MeridianTransits .................................. ... 24 2.11 Principal Terrestrial Latitude Circles . ......... 25 2.12 EquinoxesandSolstices. ....... 25 2.13 TerrestrialClimes .................................. ... 26 2.14 EclipticAscensions .............................. ...... 27 2.15 AzimuthofEclipticAscensionPoint . .......... 29 2.16 EclipticAltitudeandOrientation. .......... 30 3 Dates 63 3.1 Introduction...................................... .. 63 3.2 Determination of Julian Day Numbers . .... 63 4 Geometric