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Is the Universe Expanding?: an Historical and Philosophical Perspective for Cosmologists Starting Anew
Western Michigan University ScholarWorks at WMU Master's Theses Graduate College 6-1996 Is the Universe Expanding?: An Historical and Philosophical Perspective for Cosmologists Starting Anew David A. Vlosak Follow this and additional works at: https://scholarworks.wmich.edu/masters_theses Part of the Cosmology, Relativity, and Gravity Commons Recommended Citation Vlosak, David A., "Is the Universe Expanding?: An Historical and Philosophical Perspective for Cosmologists Starting Anew" (1996). Master's Theses. 3474. https://scholarworks.wmich.edu/masters_theses/3474 This Masters Thesis-Open Access is brought to you for free and open access by the Graduate College at ScholarWorks at WMU. It has been accepted for inclusion in Master's Theses by an authorized administrator of ScholarWorks at WMU. For more information, please contact [email protected]. IS THEUN IVERSE EXPANDING?: AN HISTORICAL AND PHILOSOPHICAL PERSPECTIVE FOR COSMOLOGISTS STAR TING ANEW by David A Vlasak A Thesis Submitted to the Faculty of The Graduate College in partial fulfillment of the requirements forthe Degree of Master of Arts Department of Philosophy Western Michigan University Kalamazoo, Michigan June 1996 IS THE UNIVERSE EXPANDING?: AN HISTORICAL AND PHILOSOPHICAL PERSPECTIVE FOR COSMOLOGISTS STARTING ANEW David A Vlasak, M.A. Western Michigan University, 1996 This study addresses the problem of how scientists ought to go about resolving the current crisis in big bang cosmology. Although this problem can be addressed by scientists themselves at the level of their own practice, this study addresses it at the meta level by using the resources offered by philosophy of science. There are two ways to resolve the current crisis. -
The Solar System's Extended Shelf Life
Vol 459|11 June 2009 NEWS & VIEWS PLANETARY SCIENCE The Solar System’s extended shelf life Gregory Laughlin Simulations show that orbital chaos can lead to collisions between Earth and the inner planets. But Einstein’s tweaks to Newton’s theory of gravity render these ruinous outcomes unlikely in the next few billion years. In the midst of a seemingly endless torrent of charted with confidence tens of millions of ‘disturbing function’ could not be neglected, baleful economic and environmental news, a years into the future. An ironclad evaluation and consideration of these terms revived the dispatch from the field of celestial dynamics of the Solar System’s stability, however, eluded question of orbital stability. In 1889, Henri manages to sound a note of definite cheer. On mathematicians and astronomers for nearly Poincaré demonstrated that even the gravita- page 817 of this issue, Laskar and Gastineau1 three centuries. tional three-body problem cannot be solved report the outcome of a huge array of computer In the seventeenth century, Isaac Newton by analytic integration, thereby eliminating simulations. Their work shows that the orbits was bothered by his inability to fully account any possibility that an analytic solution for of the terrestrial planets — Mercury, Venus, for the observed motions of Jupiter and Saturn. the entire future motion of the eight planets Earth and Mars — have a roughly 99% chance The nonlinearity of the gravitational few-body could be found. Poincaré’s work anticipated the of maintaining their current, well-ordered problem led him to conclude3 that, “to consider now-familiar concept of dynamical chaos and clockwork for the roughly 5 billion years that simultaneously all these causes of motion and the sensitive dependence of nonlinear systems remain before the Sun evolves into a red giant to define these motions by exact laws admit- on initial conditions5. -
Workshop on Astronomy and Dynamics at the Occasion of Jacques Laskar’S 60Th Birthday Testing Modified Gravity with Planetary Ephemerides
Workshop on Astronomy and Dynamics at the occasion of Jacques Laskar's 60th birthday Testing Modified Gravity with Planetary Ephemerides Luc Blanchet Gravitation et Cosmologie (GR"CO) Institut d'Astrophysique de Paris 29 avril 2015 Luc Blanchet (IAP) Testing Modified Gravity Colloque Jacques Laskar 1 / 25 Evidence for dark matter in astrophysics 1 Oort [1932] noted that the sum of observed mass in the vicinity of the Sun falls short of explaining the vertical motion of stars in the Milky Way 2 Zwicky [1933] reported that the velocity dispersion of galaxies in galaxy clusters is far too high for these objects to remain bound for a substantial fraction of cosmic time 3 Ostriker & Peebles [1973] showed that to prevent the growth of instabilities in cold self-gravitating disks like spiral galaxies, it is necessary to embed the disk in the quasi-spherical potential of a huge halo of dark matter 4 Bosma [1981] and Rubin [1982] established that the rotation curves of galaxies are approximately flat, contrarily to the Newtonian prediction based on ordinary baryonic matter Luc Blanchet (IAP) Testing Modified Gravity Colloque Jacques Laskar 2 / 25 Evidence for dark matter in astrophysics 1 Oort [1932] noted that the sum of observed mass in the vicinity of the Sun falls short of explaining the vertical motion of stars in the Milky Way 2 Zwicky [1933] reported that the velocity dispersion of galaxies in galaxy clusters is far too high for these objects to remain bound for a substantial fraction of cosmic time 3 Ostriker & Peebles [1973] showed that to -
Writing the History of Dynamical Systems and Chaos
Historia Mathematica 29 (2002), 273–339 doi:10.1006/hmat.2002.2351 Writing the History of Dynamical Systems and Chaos: View metadata, citation and similar papersLongue at core.ac.uk Dur´ee and Revolution, Disciplines and Cultures1 brought to you by CORE provided by Elsevier - Publisher Connector David Aubin Max-Planck Institut fur¨ Wissenschaftsgeschichte, Berlin, Germany E-mail: [email protected] and Amy Dahan Dalmedico Centre national de la recherche scientifique and Centre Alexandre-Koyre,´ Paris, France E-mail: [email protected] Between the late 1960s and the beginning of the 1980s, the wide recognition that simple dynamical laws could give rise to complex behaviors was sometimes hailed as a true scientific revolution impacting several disciplines, for which a striking label was coined—“chaos.” Mathematicians quickly pointed out that the purported revolution was relying on the abstract theory of dynamical systems founded in the late 19th century by Henri Poincar´e who had already reached a similar conclusion. In this paper, we flesh out the historiographical tensions arising from these confrontations: longue-duree´ history and revolution; abstract mathematics and the use of mathematical techniques in various other domains. After reviewing the historiography of dynamical systems theory from Poincar´e to the 1960s, we highlight the pioneering work of a few individuals (Steve Smale, Edward Lorenz, David Ruelle). We then go on to discuss the nature of the chaos phenomenon, which, we argue, was a conceptual reconfiguration as -
A Long Term Numerical Solution for the Insolation Quantities of the Earth Jacques Laskar, Philippe Robutel, Frédéric Joutel, Mickael Gastineau, A.C.M
A long term numerical solution for the insolation quantities of the Earth Jacques Laskar, Philippe Robutel, Frédéric Joutel, Mickael Gastineau, A.C.M. Correia, Benjamin Levrard To cite this version: Jacques Laskar, Philippe Robutel, Frédéric Joutel, Mickael Gastineau, A.C.M. Correia, et al.. A long term numerical solution for the insolation quantities of the Earth. 2004. hal-00001603 HAL Id: hal-00001603 https://hal.archives-ouvertes.fr/hal-00001603 Preprint submitted on 23 May 2004 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Astronomy & Astrophysics manuscript no. La˙2004 May 23, 2004 (DOI: will be inserted by hand later) A long term numerical solution for the insolation quantities of the Earth. J. Laskar1, P. Robutel1, F. Joutel1, M. Gastineau1, A.C.M. Correia1,2, and B. Levrard1 1 Astronomie et Syst`emesDynamiques, IMCCE-CNRS UMR8028, 77 Av. Denfert-Rochereau, 75014 Paris, France 2 Departamento de F´ısica da Universidade de Aveiro, Campus Universit´ario de Santiago, 3810-193 Aveiro, Portugal May 23, 2004 Abstract. We present here a new solution for the astronomical computation of the insolation quantities on Earth spanning from -250 Myr to 250 Myr. -
Pure and Fundamental
PURE AND FUNDAMENTAL THE LARGEST RESEARCH CENTRE IN QUÉBEC The CenTre de reCherChes maThémaTiques (crm) is the largest research centre in Québec and one of the most important mathematics research centres in the world. The crm was created in 1968 at the Université de montréal and gathers all the stakeholders in mathematical research at Québec universities and some other canadian universities. The crm organizes events attended by researchers from all over the globe and representing all mathematical disciplines. The crm focuses on pure and applied mathematics in all areas of human activity, for instance theoretical physics, brain and molecular imaging, quantum information, statistics, and genomics. Indeed mathematics is both the first science and the 1 servant of experimental science, which draws upon its new concepts, its language, and its methods. Fonds de recherche sur la nature et les technologies Plenary speakers A short course on SFT Organizers will be given by: P. Biran (Tel Aviv) M. Abreu (Instituto Superior F. Bourgeois (Université Libre O. Cornea (Montréal) Técnico) de Bruxelles) D. Gabai (Princeton) R. Cohen (Stanford) K. Cieliebak (München) E. Ghys (ENS, Lyon) A. Givental (Berkeley) T. Ekholm (Southern California) E. Giroux (ENS, Lyon) F. Lalonde (Montréal) E. Katz (Duke) R. Gompf (Austin, Texas) R. Lipshitz (Stanford) J. Sabloff (Haverford College) H. Hofer (Courant Institute) L. Polterovich (Tel Aviv) K. Wehrheim (MIT) K. Honda (Southern California) R. Schoen (Stanford) E. Ionel (Stanford) D. McDuff (Stony Brook) T. Mrowka (MIT) Y.-G. Oh (Wisconsin-Madison) K. Ono (Hokkaido) P. Ozsvath (Columbia) R. Pandharipande (Princeton) D. Salamon (ETH, Zurich) 0 Thematic Program 8 A bird eye’s view of the CRM 9 4 M. -
Avenir De La Terre
Avenir de la Terre L'avenir biologique et géologique de la Terre peut être extrapolé à partir de plusieurs facteurs, incluant la chimie de la surface de la Terre, la vitesse de refroidissement de l'intérieur de la Terre, les interactions gravitationnelles avec les autres objets du Système solaire et une augmentation constante de la luminosité solaire. Un facteur d'incertitude dans cette extrapolation est l'influence des 2 technologies introduites par les êtres humains comme la géo-ingénierie , qui 3, 4 peuvent causer des changements significatifs sur la planète . Actuellement, 5 6 l'extinction de l'Holocène est provoquée par la technologie et ses effets peuvent 7 durer cinq millions d'années . À son tour, la technologie peut provoquer l'extinction Illustration montrant la Terre après la transformation du Soleil engéante de l'humanité, laissant la Terre revenir graduellement à un rythme d'évolution plus 8, 9 rouge, scénario devant se dérouler lent résultant uniquement de processus naturels à long terme . 1 dans sept milliards d'années . Au cours d'intervalles de plusieurs millions d'années, des événements célestes aléatoires présentent un risque global pour la biosphère, pouvant aboutir à des extinctions massives. Ceci inclut les impacts provoqués par des comètes et des astéroïdes avec des diamètres de 5 à 10 km ou plus et les supernovas proches de la Terre. D'autres événements géologiques à grandes échelles sont plus facilement prédictibles. Si les effets du réchauffement climatique sur le long terme ne sont pas pris en compte, les paramètres de Milanković prédisent que la planète continuera à subir des périodes glaciaires au moins jusqu'à la fin des glaciations quaternaires. -
Glossary of Terms Absorption Line a Dark Line at a Particular Wavelength Superimposed Upon a Bright, Continuous Spectrum
Glossary of terms absorption line A dark line at a particular wavelength superimposed upon a bright, continuous spectrum. Such a spectral line can be formed when electromag- netic radiation, while travelling on its way to an observer, meets a substance; if that substance can absorb energy at that particular wavelength then the observer sees an absorption line. Compare with emission line. accretion disk A disk of gas or dust orbiting a massive object such as a star, a stellar-mass black hole or an active galactic nucleus. An accretion disk plays an important role in the formation of a planetary system around a young star. An accretion disk around a supermassive black hole is thought to be the key mecha- nism powering an active galactic nucleus. active galactic nucleus (agn) A compact region at the center of a galaxy that emits vast amounts of electromagnetic radiation and fast-moving jets of particles; an agn can outshine the rest of the galaxy despite being hardly larger in volume than the Solar System. Various classes of agn exist, including quasars and Seyfert galaxies, but in each case the energy is believed to be generated as matter accretes onto a supermassive black hole. adaptive optics A technique used by large ground-based optical telescopes to remove the blurring affects caused by Earth’s atmosphere. Light from a guide star is used as a calibration source; a complicated system of software and hardware then deforms a small mirror to correct for atmospheric distortions. The mirror shape changes more quickly than the atmosphere itself fluctuates. -
Finding the Radiation from the Big Bang
Finding The Radiation from the Big Bang P. J. E. Peebles and R. B. Partridge January 9, 2007 4. Preface 6. Chapter 1. Introduction 13. Chapter 2. A guide to cosmology 14. The expanding universe 19. The thermal cosmic microwave background radiation 21. What is the universe made of? 26. Chapter 3. Origins of the Cosmology of 1960 27. Nucleosynthesis in a hot big bang 32. Nucleosynthesis in alternative cosmologies 36. Thermal radiation from a bouncing universe 37. Detecting the cosmic microwave background radiation 44. Cosmology in 1960 52. Chapter 4. Cosmology in the 1960s 53. David Hogg: Early Low-Noise and Related Studies at Bell Lab- oratories, Holmdel, N.J. 57. Nick Woolf: Conversations with Dicke 59. George Field: Cyanogen and the CMBR 62. Pat Thaddeus 63. Don Osterbrock: The Helium Content of the Universe 70. Igor Novikov: Cosmology in the Soviet Union in the 1960s 78. Andrei Doroshkevich: Cosmology in the Sixties 1 80. Rashid Sunyaev 81. Arno Penzias: Encountering Cosmology 95. Bob Wilson: Two Astronomical Discoveries 114. Bernard F. Burke: Radio astronomy from first contacts to the CMBR 122. Kenneth C. Turner: Spreading the Word — or How the News Went From Princeton to Holmdel 123. Jim Peebles: How I Learned Physical Cosmology 136. David T. Wilkinson: Measuring the Cosmic Microwave Back- ground Radiation 144. Peter Roll: Recollections of the Second Measurement of the CMBR at Princeton University in 1965 153. Bob Wagoner: An Initial Impact of the CMBR on Nucleosyn- thesis in Big and Little Bangs 157. Martin Rees: Advances in Cosmology and Relativistic Astro- physics 163. -
Observational Cosmology - 30H Course 218.163.109.230 Et Al
Observational cosmology - 30h course 218.163.109.230 et al. (2004–2014) PDF generated using the open source mwlib toolkit. See http://code.pediapress.com/ for more information. PDF generated at: Thu, 31 Oct 2013 03:42:03 UTC Contents Articles Observational cosmology 1 Observations: expansion, nucleosynthesis, CMB 5 Redshift 5 Hubble's law 19 Metric expansion of space 29 Big Bang nucleosynthesis 41 Cosmic microwave background 47 Hot big bang model 58 Friedmann equations 58 Friedmann–Lemaître–Robertson–Walker metric 62 Distance measures (cosmology) 68 Observations: up to 10 Gpc/h 71 Observable universe 71 Structure formation 82 Galaxy formation and evolution 88 Quasar 93 Active galactic nucleus 99 Galaxy filament 106 Phenomenological model: LambdaCDM + MOND 111 Lambda-CDM model 111 Inflation (cosmology) 116 Modified Newtonian dynamics 129 Towards a physical model 137 Shape of the universe 137 Inhomogeneous cosmology 143 Back-reaction 144 References Article Sources and Contributors 145 Image Sources, Licenses and Contributors 148 Article Licenses License 150 Observational cosmology 1 Observational cosmology Observational cosmology is the study of the structure, the evolution and the origin of the universe through observation, using instruments such as telescopes and cosmic ray detectors. Early observations The science of physical cosmology as it is practiced today had its subject material defined in the years following the Shapley-Curtis debate when it was determined that the universe had a larger scale than the Milky Way galaxy. This was precipitated by observations that established the size and the dynamics of the cosmos that could be explained by Einstein's General Theory of Relativity. -
Women in Astronomy: an Introductory Resource Guide
Women in Astronomy: An Introductory Resource Guide by Andrew Fraknoi (Fromm Institute, University of San Francisco) [April 2019] © copyright 2019 by Andrew Fraknoi. All rights reserved. For permission to use, or to suggest additional materials, please contact the author at e-mail: fraknoi {at} fhda {dot} edu This guide to non-technical English-language materials is not meant to be a comprehensive or scholarly introduction to the complex topic of the role of women in astronomy. It is simply a resource for educators and students who wish to begin exploring the challenges and triumphs of women of the past and present. It’s also an opportunity to get to know the lives and work of some of the key women who have overcome prejudice and exclusion to make significant contributions to our field. We only include a representative selection of living women astronomers about whom non-technical material at the level of beginning astronomy students is easily available. Lack of inclusion in this introductory list is not meant to suggest any less importance. We also don’t include Wikipedia articles, although those are sometimes a good place for students to begin. Suggestions for additional non-technical listings are most welcome. Vera Rubin Annie Cannon & Henrietta Leavitt Maria Mitchell Cecilia Payne ______________________________________________________________________________ Table of Contents: 1. Written Resources on the History of Women in Astronomy 2. Written Resources on Issues Women Face 3. Web Resources on the History of Women in Astronomy 4. Web Resources on Issues Women Face 5. Material on Some Specific Women Astronomers of the Past: Annie Cannon Margaret Huggins Nancy Roman Agnes Clerke Henrietta Leavitt Vera Rubin Williamina Fleming Antonia Maury Charlotte Moore Sitterly Caroline Herschel Maria Mitchell Mary Somerville Dorrit Hoffleit Cecilia Payne-Gaposchkin Beatrice Tinsley Helen Sawyer Hogg Dorothea Klumpke Roberts 6. -
Table of Contents
AAS Newsletter July/August 2011, Issue 159 - The Online Publication for the members of the American Astronomical Society Table of Contents President's Column 2 2011 Chrétien Grant Winner 11 From the Executive Office 4 IAU Membership Deadline 11 Secretary's Corner 5 Highlights from the Hub of the Council Actions 6 Universe 12 Journals Update 8 SPD Meeting 23 25 Things About... 9 Washington News Back Page A A S American Astronomical Society AAS Officers President's Column Debra M. Elmegreen, President David J. Helfand, President-Elect Debra Meloy Elmegreen, [email protected] Lee Anne Willson, Vice-President Nicholas B. Suntzeff, Vice-President Edward B. Churchwell, Vice-President Hervey (Peter) Stockman, Treasurer G. Fritz Benedict, Secretary Richard F. Green, Publications Board Chair We hit a homerun in Boston with Timothy F. Slater, Education Officer one of our biggest summer meetings Councilors ever, including over 1300 registrants; Bruce Balick still, it had the more intimate feel that Richard G. French Eileen D. Friel characterizes our summer gatherings. It Edward F. Guinan was a privilege to share our 218th meeting Patricia Knezek James D. Lowenthal with the American Association of Robert Mathieu Variable Star Observers on the occasion Angela Speck th Jennifer Wiseman of their 100 anniversary, and to present them a certificate to commemorate Executive Office Staff the long-time professional-amateur Kevin B. Marvel, Executive Officer Tracy Beale, Membership Services collaboration we have all enjoyed. Administrator Margaret Geller gave a stirring Henry Chris Biemesderfer, Director of Publishing Laronda Boyce, Meetings & Exhibits Norris Russell Lecture on her discovery Coordinator of large-scale structure in the Universe.