The Birth of American Astrophysics: the Development of a Science in Its Cultural Context Orville Roderick Butler Iowa State University

Total Page:16

File Type:pdf, Size:1020Kb

The Birth of American Astrophysics: the Development of a Science in Its Cultural Context Orville Roderick Butler Iowa State University Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1993 The birth of American astrophysics: the development of a science in its cultural context Orville Roderick Butler Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Astrophysics and Astronomy Commons, History of Science, Technology, and Medicine Commons, and the United States History Commons Recommended Citation Butler, Orville Roderick, "The birth of American astrophysics: the development of a science in its cultural context " (1993). Retrospective Theses and Dissertations. 10407. https://lib.dr.iastate.edu/rtd/10407 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand corner and continuing from left to right in equal sections with small overlaps. Each original is also photographed in one exposure and is included in reduced form at the back of the book. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6" x 9" black and v/hite photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. Contact UMI directly to order. University Microfilms International A Bell & Howell Information Company 300 North! Zeeb Road. Ann Arbor, fvll 48106-1346 USA 313/761-4700 800/521-0600 Order Number 9821124 The birth of American astrophysics: The development of a science in its cultural context Butler, Orville Roderick, Ph.D. Iowa State University, 1993 Copyright ©1993 by Butler, Orville Roderick. All rights reserved. 300 N. ZeebRd. Ann Arbor, Ml 48106 The birth of American astrophysics; The development of a science in its cultural context by Orville Roderick Butler A Dissertation Submitted to the Graduate Faculty in Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY Department: History Major: History of Technology & Science Members of the Committee: Signature was redacted for privacy. or ^wo^k Signature was redacted for privacy. For thte Major D^artment Signature was redacted for privacy. Signature was redacted for privacy. For the Graduate College Iowa State University Ames, Iowa 1993 Copyright © Orville Roderick Butler, 1993. All rights reserved. ii DEDICATION To Hsieyun Serena Butler-Yang, who has encouraged her father in ways that she will never know, and to Xiaohua Yang, whose support and organizational skills have made finishing this dissertation so much easier. iii TABLE OF CONTENTS DEDICATION INTRODUCTION CHAPTER 1. THE NEBULAR HYPOTHESIS IN AMERICAN THOUGHT CONFLICT AND UNITY, 1830-1860. CHAPTER 2. FROM COSMIC METEOROLOGY TO SOLAR PHYSICS: POPULAR THEORIES OF METEOROLOGY AND THE SETTLING OF THE WESTERN PLAIN. CHAPTER 3. UP TO GOD AND DOWN TO NATURE: CONFLICTING COSMOLOGICAL METHODOLOGIES. CHAPTER 4. POPULAR METEOROLOGY AND THE RISE OF ASTROPHYSICS; WEATHER PROGNOSTICATORS, THE U.S. ARMY SIGNAL SERVICE AND THE DEMAND FOR LONG RANGE WEATHER PREDICTION. CHAPTER 5. FROM HENRY DRAPER TO HARVARD'S DRAPER MEMORIAL PROGRAM: THE NEBULAR HYPOTHESIS IN THE DEVELOPMENT OF ASTROPHYSICS AT HARVARD COLLEGE OBSERVATORY. CHAPTER 6. FROM THE WEATHER BUREAU TO THE SMITHSONIAN; SAMUEL PIERPONT LANGLEY AND THE DEVELOPMENT OF THE SMITHSONIAN ASTROPHYSICAL OBSERVATORY. CHAPTER 7. THE ESTABLISHMENT OF ASTROPHYSICS: JAMES EDWARD KEELER'S SPEECH AT THE DEDICATION OF THE YERKES ASTROPHYSICAL OBSERVATORY. BIBLIOGRAPHY ACKNOWLEDGEMENTS 1 INTRODUCTION Most historians have found the birth of astrophysics in the application of the spectroscope to the study of the sun and stars. They have generally traced its roots to Bunsen and Kirchhoff's 1859 paper which suggested the useful­ ness of the spectroscope for astronomical research and have found the development of astrophysics as a profession in the employment of the spectroscope, and other appliances in the laboratories of nineteenth century physicists, for research into the chemical and physical makeup of heavenly bodies. A history which concentrates on the role of instrumentation in the development of astrophysics is, at best, incomplete. As important as instrumentation was, and is, in astrophysical research, separating astrophysics from the intellectual questions and the cultural issues which gave rise to those questions removes from the historical record answers to some questions about the nature of the science and why it came to be a specialized professional field. Contrary to the views of the positivists, and others who see science as providing objective truth, scientific ideas do not develop in a cultural vacuum any more than political, religious or social ideas. To the extent that the motivation and even ideas for research in a field result from the impact of broader social and cultural issues, science takes place in a cultural context. The questions raised by scientists, the answers they give and the way they answer 2 those questions are often part of a response to issues raised by the broader culture. The role of these questions and answers in the birth of American astrophysics helps to illuminate one aspect of the role of a culture in the development and eventual profes- sionalization of a science. Research into the application of the laws of mechanics, and particularly the application of Newton's theory of gravitation, to the development of an understanding of the makeup and evolution of heavenly bodies, as well as the study of solar heat and its influence on the earth, took place within the context of broader cultural interest, input and demands upon the criteria which the ans­ wers would meet.l The nebular hypothesis was widely discussed in American literature as well as scientific papers beginning in the early 1840s. In the nineteenth century the nebular hypothesis included components which "explained" the collapse from nebulous material into stars, the nature of the sun and possible explanations of the sun's heat source. It Iprom the perspective of many modern astronomers and astrophysicists, the field of astrophysics, as it was defined at the end of the nineteenth century, was closer to the "new astronomy" then the specialized research of today. The modern self-described "astronomer" is as likely to use the astrophysical principles and study the problems reserved to the astrophysicist in the 1890s. The astrophysicist of today is more likely to specialize in the study of special­ ized fields of physics—high energy physics or plasma physics for example—in which stars play as much the role of a laboratory as they do the object of modern astrophysical study itself. 3 influenced American thought, providing a challenge to tradi­ tional theological explanations of creation and ultimately of the origin of humankind. It provided an issue around which scrutiny into the nature, role and realm of valid scientific inquiry, as well as into the interrelationship between scientific and theological truths, took place. Utilized by Herbert Spencer and his American dis­ ciples the nebular hypothesis became a crucial starting point for their development hypothesis and notions of progress which enamored the American public in the second half of the nineteenth century. The application of the nebular hypothesis, by Lord Kelvin and others, to calculations of the age of the solar system and the earth, created turmoil within the geological community when the results provided an inadequate time frame for then current theories of geological and biological evolution. The extra import given the nebular hypothesis by those seeking to reconcile science and religion or by those seeking to provide their philosophy with scientific credibility leavened the debate over its validity and encour­ aged American astronomers, along with their European counter­ parts, to search for a mechanism by which it might be vali­ dated or disconfirmed for all time. The attempts by American astronomers to affirm or falsify the nebular hypothesis can be seen as one cultural component of the development of astrophysics in America. 4 In many respects the study of the causes and nature of the sun's heat provided a more intimate connection between American culture and the rise of astrophysics in the United States. With the westward movement of the American popula­ tion onto the plains, land speculators, farmers and advocates of westward expansion eagerly sought after
Recommended publications
  • Resonance in the Solar System
    Resonance In the Solar System Steve Bache UNC Wilmington Dept. of Physics and Physical Oceanography Advisor : Dr. Russ Herman Spring 2012 Goal • numerically investigate the dynamics of the asteroid belt • relate old ideas to new methods • reproduce known results • the sky and heavenly bodies History The role of science: • make sense of the world • perceive order out of apparent randomness History The role of science: • make sense of the world • perceive order out of apparent randomness • the sky and heavenly bodies Anaximander (611-547 BC) • Greek philosopher, scientist • stars, moon, sun 1:2:3 Figure: Anaximander's Model Pythagoras (570-495 BC) • Mathematician, philosopher, started a religion • all heavenly bodies at whole number ratios • "Harmony of the spheres" Figure: Pythagorean Model Tycho Brahe (1546-1601) • Danish astronomer, alchemist • accurate astronomical observations, no telescope • importance of data collection • orbits are ellipses • equal area in equal time • T 2 / a3 Johannes Kepler (1571-1631) • Brahe's assistant • Used detailed data provided by Brahe • Observations led to Laws of Planetary Motion Johannes Kepler (1571-1631) • Brahe's assistant • Used detailed data provided by Brahe • Observations led to Laws of Planetary Motion • orbits are ellipses • equal area in equal time • T 2 / a3 Kepler's Model • Astrologer, Harmonices Mundi • Used empirical data to formulate laws Figure: Kepler's Model Isaac Newton (1642-1727) • religious, yet desired a physical mechanism to explain Kepler's laws • contributions to mathematics and science • Principia • almost entirety of an undergraduate physics degree • Law of Universal Gravitation ~ m1m2 F12 = −G 2 ^r12: jr12j • Commensurability The property of two orbiting objects, such as planets, satellites, or asteroids, whose orbital periods are in a rational proportion.
    [Show full text]
  • Ocabulary of Definitions : P
    Service bibliothèque Catalogue historique de la bibliothèque de l’Observatoire de Nice Source : Monographie de l’Observatoire de Nice / Charles Garnier, 1892. Marc Heller © Observatoire de la Côte d’Azur Février 2012 Présentation << On trouve… à l’Ouest … la bibliothèque avec ses six mille deux cents volumes et ses trentes journaux ou recueils périodiques…. >> (Façade principale de la Bibliothèque / Phot. attribuée à Michaud A. – 188? - Marc Heller © Observatoire de la Côte d’Azur) C’est en ces termes qu’Henri Joseph Anastase Perrotin décrivait la bibliothèque de l’Observatoire de Nice en 1899 dans l’introduction du tome 1 des Annales de l’Observatoire de Nice 1. Un catalogue des revues et ouvrages 2 classé par ordre alphabétique d’auteurs et de lieux décrivait le fonds historique de la bibliothèque. 1 Introduction, Annales de l’Observatoire de Nice publiés sous les auspices du Bureau des longitudes par M. Perrotin. Paris,Gauthier-Villars,1899, Tome 1,p. XIV 2 Catalogue de la bibliothèque, Annales de l’Observatoire de Nice publiés sous les auspices du Bureau des longitudes par M. Perrotin. Paris,Gauthier-Villars,1899, Tome 1,p. 1 Le présent document est une version remaniée, complétée et enrichie de ce catalogue. (Bibliothèque, vue de l’intérieur par le photogr. Jean Giletta, 191?. - Marc Heller © Observatoire de la Côte d’Azur) Chaque référence est reproduite à l’identique. Elle est complétée par une notice bibliographique et éventuellement par un lien électronique sur la version numérisée. Les titres et documents non encore identifiés sont signalés en italique. Un index des auteurs et des titres de revues termine le document.
    [Show full text]
  • Severe Space Weather
    Severe Space Weather ThePerfect Solar Superstorm Solar storms in +,-. wreaked havoc on telegraph networks worldwide and produced auroras nearly to the equator. What would a recurrence do to our modern technological world? Daniel N. Baker & James L. Green SOHO / ESA / NASA / LASCO 28 February 2011 !"# $ %&'&!()*& SStormtorm llayoutayout FFeb.inddeb.indd 2288 111/30/101/30/10 88:09:37:09:37 AAMM DRAMATIC AURORAL DISPLAYS were seen over nearly the entire world on the night of August !"–!&, $"%&. In New York City, thousands watched “the heavens . arrayed in a drapery more gorgeous than they have been for years.” The aurora witnessed that Sunday night, The New York Times told its readers, “will be referred to hereafter among the events which occur but once or twice in a lifetime.” An even more spectacular aurora occurred on Septem- ber !, $"%&, and displays of remarkable brilliance, color, and duration continued around the world until Septem- ber #th. Auroras were seen nearly to the equator. Even after daybreak, when the auroras were no longer visible, disturbances in Earth’s magnetic fi eld were so powerful ROYAL ASTRONOMICAL SOCIETY / © PHOTO RESEARCHERS that magnetometer traces were driven off scale. Telegraph PRELUDE TO THE STORM British amateur astronomer Rich- networks around the globe experienced major disrup- ard Carrington sketched this enormous sunspot group on Sep- tions and outages, with some telegraphs being completely tember $, $()*. During his observations he witnessed two brilliant unusable for nearly " hours. In several regions, operators beads of light fl are up over the sunspots, and then disappear, in disconnected their systems from the batteries and sent a matter of ) minutes.
    [Show full text]
  • Ira Sprague Bowen Papers, 1940-1973
    http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington.
    [Show full text]
  • Smithsonian Miscellaneous Collections
    BULLETIN PHILOSOPHICAL SOCIETY WASHINGTON. VOL. IV. Containing the Minutes of the Society from the 185th Meeting, October 9, 1880, to the 2020! Meeting, June 11, 1881. PUBLISHED BY THE CO-OPERATION OF THE SMITHSONIAN INSTITUTION. WASHINGTON JUDD & DETWEILER, PRINTERS, WASHINGTON, D. C. CONTENTS. PAGE. Constitution of the Philosophical Society of Washington 5 Standing Rules of the Society 7 Standing Rules of the General Committee 11 Rules for the Publication of the Bulletin 13 List of Members of the Society 15 Minutes of the 185th Meeting, October 9th, 1880. —Cleveland Abbe on the Aurora Borealis , 21 Minutes of the 186th Meeting, October 25th, 1880. —Resolutions on the decease of Prof. Benj. Peirce, with remarks thereon by Messrs. Alvord, Elliott, Hilgard, Abbe, Goodfellow, and Newcomb. Lester F. Ward on the Animal Population of the Globe 23 Minutes of the 187th Meeting, November 6th, 1880. —Election of Officers of the Society. Tenth Annual Meeting 29 Minutes of the 188th Meeting, November 20th, 1880. —John Jay Knox on the Distribution of Loans in the Bank of France, the National Banks of the United States, and the Imperial of Bank Germany. J. J. Riddell's Woodward on Binocular Microscope. J. S. Billings on the Work carried on under the direction of the National Board of Health, 30 Minutes of the 189th Meeting, December 4th, 1880. —Annual Address of the retiring President, Simon Newcomb, on the Relation of Scientific Method to Social Progress. J. E. Hilgard on a Model of the Basin of the Gulf of Mexico 39 Minutes of the 190th Meeting, December iSth, 1880.
    [Show full text]
  • Wiki Template-1Eb7p59
    Wikipedia Reader https://en.wikipedia.org/wiki/Aurora Selected by Julie Madsen - Entry 10 1 Aurora From Wikipedia, the free encyclopedia An aurora, sometimes referred to as a polar lights or north- ern lights, is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions.[1] Au- roras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (ther- mosphere/exosphere), where their energy is lost. The resulting ion- ization and excitation of atmospheric constituents emits light of varying color and complexity. The form of the aurora, occur- ring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating parti- cles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton Images of auroras from around the world, auroras are usually observed at including those with rarer red and blue lower latitudes.[2] lights Wikipedia Reader 2 May 1 2017 Contents 1 Occurrence of terrestrial auroras 1.1 Images 1.2 Visual forms and colors 1.3 Other auroral radiation 1.4 Aurora noise 2 Causes of auroras 2.1 Auroral particles 2.2 Auroras and the atmosphere 2.3 Auroras and the ionosphere 3 Interaction of the solar wind with Earth 3.1 Magnetosphere 4 Auroral particle acceleration 5 Auroral events of historical significance 6 Historical theories, superstition and mythology 7 Non-terrestrial auroras 8 See also 9 Notes 10 References 11 Further reading 12 External links Occurrence of terrestrial auroras Most auroras occur in a band known as the auroral zone,[3] which is typically 3° to 6° wide in latitude and between 10° and 20° from the geomagnetic poles at all local times (or longitudes), most clearly seen at night against a dark sky.
    [Show full text]
  • ARE DRONES a FORCE for GOOD? How Drones Are Being Used to Benefit Society
    BRIEF FOOD AND DRINK CULTURE GEAR SPORTS STYLE WOMEN HOME > BANNER- HOME > MAGAZINE ARE DRONES A FORCE FOR GOOD? How drones are being used to benefit society By Matthew Priest Words: Max Mueller NEWSLETTER SUBSCRIPTION Get the lowdown on the week ahead to your inbox, together with reviews, exclusive competitions and the occasional funny list. Enter Your Email SUBSCRIBE MOST POPULAR THIS WEEK Read Shared Galleries HOW TO BULK UP LIKE A RUGBY PLAYER Drones usually feature in the news due to their controversial use as weapons of war or, more prosaically, for their use as fun but largely impractical toys. But what if the technology could be used to help the environment or save lives? This month, the UAE is again promoting the humanitarian use of drones with a $1 million competition that features the best designs from around the world. Here is a bird’s eye view of the technology and its pitfalls, in the Middle East and beyond. *** WHAT I’VE LEARNT: FLAVIO BRIATORE Fukushima Daiichi nuclear power station, April 10, 2015. Four years after the March 2011 meltdown, a stream of images is being recorded inside reactor No 1, one of three that was badly damaged after the plant was hit by a devastating tsunami. As the remote-controlled robot crawls through debris, the on-board searchlight struggles to penetrate a thick dust cloud. It also has to navigate charred concrete girders coated in solidified molten metal that now resemble warped stalactites. CESARO: 8 THINGS WE’VE At the bottom of the video screen is a digital display of the radiation exposure.
    [Show full text]
  • Homotopy Perturbation Method with Laplace Transform (LT-HPM) Is Given in “Homotopy Perturbation Method” Section
    Tripathi and Mishra SpringerPlus (2016) 5:1859 DOI 10.1186/s40064-016-3487-4 RESEARCH Open Access Homotopy perturbation method with Laplace Transform (LT‑HPM) for solving Lane–Emden type differential equations (LETDEs) Rajnee Tripathi and Hradyesh Kumar Mishra* *Correspondence: [email protected] Abstract Department In this communication, we describe the Homotopy Perturbation Method with Laplace of Mathematics, Jaypee University of Engineering Transform (LT-HPM), which is used to solve the Lane–Emden type differential equa- and Technology, Guna, MP tions. It’s very difficult to solve numerically the Lane–Emden types of the differential 473226, India equation. Here we implemented this method for two linear homogeneous, two linear nonhomogeneous, and four nonlinear homogeneous Lane–Emden type differential equations and use their appropriate comparisons with exact solutions. In the current study, some examples are better than other existing methods with their nearer results in the form of power series. The Laplace transform used to accelerate the convergence of power series and the results are shown in the tables and graphs which have good agreement with the other existing method in the literature. The results show that LT- HPM is very effective and easy to implement. Keywords: Homotopy Perturbation Method (HPM), Laplace Transform (LT), Singular Initial value problems (IVPs), Lane–Emden type equations Background Two astrophysicists, Jonathan Homer Lane and Robert had explained the Lane–Emden type differential equations. In this study, they had designed these types of differential equations, which is a dimensionless structure of Poisson’s equation for the gravitational potential of a self-gravitating, spherically symmetric, polytropic fluid and the thermal behavior of a spherical bunch of gas according to the laws of thermodynamics (Lane 1870; Richardson 1921).
    [Show full text]
  • JRASC-2007-04-Hr.Pdf
    Publications and Products of April / avril 2007 Volume/volume 101 Number/numéro 2 [723] The Royal Astronomical Society of Canada Observer’s Calendar — 2007 The award-winning RASC Observer's Calendar is your annual guide Created by the Royal Astronomical Society of Canada and richly illustrated by photographs from leading amateur astronomers, the calendar pages are packed with detailed information including major lunar and planetary conjunctions, The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada meteor showers, eclipses, lunar phases, and daily Moonrise and Moonset times. Canadian and U.S. holidays are highlighted. Perfect for home, office, or observatory. Individual Order Prices: $16.95 Cdn/ $13.95 US RASC members receive a $3.00 discount Shipping and handling not included. The Beginner’s Observing Guide Extensively revised and now in its fifth edition, The Beginner’s Observing Guide is for a variety of observers, from the beginner with no experience to the intermediate who would appreciate the clear, helpful guidance here available on an expanded variety of topics: constellations, bright stars, the motions of the heavens, lunar features, the aurora, and the zodiacal light. New sections include: lunar and planetary data through 2010, variable-star observing, telescope information, beginning astrophotography, a non-technical glossary of astronomical terms, and directions for building a properly scaled model of the solar system. Written by astronomy author and educator, Leo Enright; 200 pages, 6 colour star maps, 16 photographs, otabinding. Price: $19.95 plus shipping & handling. Skyways: Astronomy Handbook for Teachers Teaching Astronomy? Skyways Makes it Easy! Written by a Canadian for Canadian teachers and astronomy educators, Skyways is Canadian curriculum-specific; pre-tested by Canadian teachers; hands-on; interactive; geared for upper elementary, middle school, and junior-high grades; fun and easy to use; cost-effective.
    [Show full text]
  • The Asteroidal Belt and Kirkwood Gaps—I. a Statistical Study
    Pramfina, Vol. 8, No. 5, 1977, pp. 438-446i © Printed in India. The asteroidal belt and Kirkwood gaps--I. A statistical study R PRATAP Physical Research Laboratory, Ahmedabad 380009 MS received 2 February 1977 Abstract. In this paper we have made a spectral analysis study of matter distri- bution in the asteroidal belt. We have Fourier analysed this distribution and obtained the autocorrelation and power spectrum, and have identified the ratios from the resonance theory. We have shown that the Kirkwood gaps cannot be satisfactorily interpreted as due to mere resonance between the asteroid and Jupi(er orbital motions. We propose that they may be regarded as a consequence of density waves generated in the g~s disc in the ecliptic plane in the ncighbourhood of the Sun. We have also shown that the process is non-Marcovian and hence cannot be subjected to a hydrodynamical analysis. Keywords. D~nsity waves; Non-Marcovian; Kirkwood gaps. 1. Introduction It was observed by Daniel Kirkwood (1867) that the astetoidal belt had a ring struc- ture, and since then, resonance theory was invoked to explain the rings of minimal matter-gaps. The total mass distribution in these rings has been estimated to be about 0.1 M@. Recently Ovenden (1972) tried to estimate as to what would have b~n the mass in this region at the origin of the solar system. He invoked a "principle of least interaction action" and using this, he calaulated the semi- major axes of the various planets, trying to examine the physical contem of Titius-Bode's law.
    [Show full text]
  • History of Science and History of Technology (Class Q, R, S, T, and Applicable Z)
    LIBRARY OF CONGRESS COLLECTIONS POLICY STATEMENTS History of Science and History of Technology (Class Q, R, S, T, and applicable Z) Contents I. Scope II. Research strengths III. General collecting policy IV. Best editions and preferred formats V. Acquisitions sources: current and future VI. Collecting levels I. Scope This Collections Policy Statement covers all of the subclasses of Science and Technology and treats the history of these disciplines together. In a certain sense, most of the materials in Q, R, S, and T are part of the history of science and technology. The Library has extensive resources in the history of medicine and agriculture, but many years ago a decision was made that the Library should not intensively collect materials in clinical medicine and technical agriculture, as they are subject specialties of the National Library of Medicine and the National Agricultural Library, respectively. In addition, some of the numerous abstracting and indexing services, catalogs of other scientific and technical collections and libraries, specialized bibliographies, and finding aids for the history of science and technology are maintained in class Z. See the list of finding aids online: http://findingaids.loc.gov/. II. Research strengths 1. General The Library’s collections are robust in both the history of science and the history of technology. Both collections comprise two major elements: the seminal works of science and technology themselves, and historiographies on notable scientific and technological works. The former comprise the original classic works of science and technology as they were composed by the men and women who ushered in the era of modern science and invention.
    [Show full text]
  • Women Who Read the Stars Sue Nelson Delights in Dava Sobel’S Account of a Rare Band of Human Computers
    Some of the Harvard Observatory ‘computers’ in 1925. Annie Jump Cannon is seated fifth from left; Cecilia Payne is at the drafting table. HISTORY Women who read the stars Sue Nelson delights in Dava Sobel’s account of a rare band of human computers. here are half a million photographic magnitude, on the as computers at Harvard, a practice unique plates in the Harvard College Observa- photographic plates to the university. Within five years, the num- tory collection, all unique. They date to and computing its ber of paid female computers, from a range Tthe mid-1880s, and each can display the light location in the sky. of backgrounds, had risen to 14. Their efforts from 50,000 stars. These fragments of the Pickering was espe- would be boosted by philanthropist Cath- cosmos furthered our understanding of the cially interested in erine Wolfe Bruce, who in 1889 donated Universe. They also reflect the dedication and variable stars, whose US$50,000 to the observatory, convinced intelligence of extraordinary women whose light would brighten that the introduction of photography and stories are more than astronomical history: and fade over a spe- spectroscopy would advance the field. ARCHIVES UNIV. HARVARD COURTESY they reveal lives of ambition, aspiration and cific period. These The Glass The Glass Universe concentrates on a few of brilliance. It takes a talented writer to inter- fluctuations, captured Universe: How the Harvard computers. Williamina Fleming, weave professional achievement with per- on the plates, required the Ladies of a Scottish school teacher, arrived at the obser- sonal insight. By the time I finished The Glass constant observation, the Harvard vatory in 1879, pregnant and abandoned by Universe, Dava Sobel’s wonderful, meticulous but he couldn’t afford Observatory Took her husband.
    [Show full text]