Final Copy 2020 09 29 Zhao
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Lomonosov, the Discovery of Venus's Atmosphere, and Eighteenth Century Transits of Venus
Journal of Astronomical History and Heritage, 15(1), 3-14 (2012). LOMONOSOV, THE DISCOVERY OF VENUS'S ATMOSPHERE, AND EIGHTEENTH CENTURY TRANSITS OF VENUS Jay M. Pasachoff Hopkins Observatory, Williams College, Williamstown, Mass. 01267, USA. E-mail: [email protected] and William Sheehan 2105 SE 6th Avenue, Willmar, Minnesota 56201, USA. E-mail: [email protected] Abstract: The discovery of Venus's atmosphere has been widely attributed to the Russian academician M.V. Lomonosov from his observations of the 1761 transit of Venus from St. Petersburg. Other observers at the time also made observations that have been ascribed to the effects of the atmosphere of Venus. Though Venus does have an atmosphere one hundred times denser than the Earth’s and refracts sunlight so as to produce an ‘aureole’ around the planet’s disk when it is ingressing and egressing the solar limb, many eighteenth century observers also upheld the doctrine of cosmic pluralism: believing that the planets were inhabited, they had a preconceived bias for believing that the other planets must have atmospheres. A careful re-examination of several of the most important accounts of eighteenth century observers and comparisons with the observations of the nineteenth century and 2004 transits shows that Lomonosov inferred the existence of Venus’s atmosphere from observations related to the ‘black drop’, which has nothing to do with the atmosphere of Venus. Several observers of the eighteenth-century transits, includ- ing Chappe d’Auteroche, Bergman, and Wargentin in 1761 and Wales, Dymond, and Rittenhouse in 1769, may have made bona fide observations of the aureole produced by the atmosphere of Venus. -
Is a Global Identity Possible? the Relevance of Big History to Self-Other Relations”, Refugee Watch, (13):36, 2010, Pp.53-77
On The Possibility of a Global Political Community: The Enigma of ‘Small Local Differences’ within Humanity1 Heikki Patomäki Introduction Is anything like a global political community – and thereby ideals such as global democracy and justice – achievable? This is a key question not only for political theory but also for contemporary political practices. For instance, a call for global solidarity in the face of rapid global warming (UNDP 2007), which seems ever more urgent in 2017, assumes a shared planetary identity across the currently prevailing differences and divisions. It seems that there can be no solidarity without a common identity at some level of human being. Environmentalists maintain that all humans share an important thing in common, namely planet Earth and its sphere of life, to which we essentially belong. In contrast, many political realists believe that humans are essentially tribal beings, or at least will remain so in the foreseeable future. This belief may be grounded on anything from speculative philosophical accounts of the human nature to sociobiological theories 1 This paper has been in progress for a decade. I first wrote it in 2007 and presented it in a few conferences, workshops and the like, including the Calcutta Research Group Winter School in December 2007. That presentation led eventually to a limited-circulation publication “Is a Global Identity Possible? The Relevance of Big History to Self-Other Relations”, Refugee Watch, (13):36, 2010, pp.53-77. A couple of years later I used the last two sections of this paper in a revised form in “The Problems of Legitimation and Potential Conflicts in a World Political Community”, Cooperation & Conflict, (47):2, 2012, pp.239-59. -
Bowliîo&Ebîstate University Library
THE DRAMATURGY OF LUDVIG HOLBERG'S COMEDIES Gerald S. Argetsinger A Dissertation Submitted to the Graduate School of Bowling Green State University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY August 1975 BOWLIÎO&EBÎ STATE UNIVERSITY LIBRARY © 1975 GERALD SCOTT ARGETSINGER ALL RIGHTS RESERVED il ABSTRACT This study first described Ludvig Holberg's dramaturgy and then identified the characteristics which • have engendered the comedies' continued popularity. All of the prior Holberg research was studied, but most of the understanding of the comedies came through the careful studying of the playscripts. Holberg's form was greatly influenced by the comedies of Moliere and the Commedia dell' Arte. The content and tone were influenced by the comedies of Ben Jonson and George Farquhar. Holberg wrote for, and was best liked by, the middle class. At first, scholars found his plays crass and inferior. But only twenty years after his death, the plays were accepted as the foundation of the Royal Danish Theatre’s repertory. Holberg created comic characters based upon middle class types. The characters’ speech is almost strictly everyday, Copenhagen Danish. Little was done to linguistically individualize speech except when it was an integral part of the satire of the play. Holberg was also adept at writing jokes. He was a master at creating comic situations. These situations give the characters a setting in which to be funny and provide a foundation for intrigues and other comic business. The visual aspects of the early productions were not important. After careful investigation, it was concluded that Holberg's plays did not succeed, as previous writings tend to assume, because of the "Danishness” of the characters. -
Satire and the Enlightenment Scandinavian R5B, Spring 2017
Satire and the Enlightenment Scandinavian R5B, Spring 2017 GSI: Zachary Blinkinsop Office: Dwinelle 6414 Office Hours: Monday and Wednesday 1200-1345 or by appointment Satire flourished during the eighteenth century when heavy-hitting writers across Europe penned droll attacks on superstition, intolerance, and vice. In this course, we will explore how the satirical mode functioned as part of the Enlightenment project. Particular emphasis will placed on the literary history of Sweden and Denmark-Norway from 1720 to 1792 and Ludvig Holberg’s satirical writings will comprise the mainstay of readings. Guiding questions in the course include: when is satire subversive and when does it reinforce the status quo? How do Scandinavian satires differ from their contemporaries in Great Britain, France, and colonial America/the United States? Is there a taxonomy of satire and what formal elements are ubiquitous across satirical sub-genres? Students will write a term paper that incorporates scholarship, historical material, and one or more of the course texts. All readings are in English. Course Texts (* indicates texts to purchase) Ogbord & Buckroyd * Satire Ebenezer Cooke “The Sot-Weed Factor” American, 1708 Ludvig Holberg Erasmus Montanus Danish, 1722 Ludvig Holberg Jeppe of the Hill Danish, 1723 Jonathan Swift Gulliver’s Travels Anglo-Irish, 1726 Jonathan Swift “A Modest Proposal” Anglo-Irish, 1729 Benjamin Franklin “The Witch Trial at Mount Holly” American, 1730 Olof Dalin “Proof of Wisdom: Mr. Arngrim Beserk” Swedish, 1739 Ludvig Holberg * The -
Reposs #19: Newtonianism in the Scandinavian Countries, 1690–1790
RePoSS: Research Publications on Science Studies RePoSS #19: Newtonianism in the Scandinavian Countries, 1690–1790 Helge Kragh August 2012 Centre for Science Studies, University of Aarhus, Denmark Research group: History and philosophy of science Please cite this work as: Helge Kragh (Aug. 2012). Newtonianism in the Scandinavian Countries, 1690–1790. RePoSS: Research Publications on Sci- ence Studies 19. Aarhus: Centre for Science Studies, University of Aarhus. url: http://www.css.au.dk/reposs. Copyright c Helge Kragh, 2012 1 Newtonianism in the Scandinavian Countries, 1690-1790 HELGE KRAGH 1 Introduction In the present context, the Scandinavian countries refer to two national or administrative units, the one being Denmark and the other Sweden. In the period here considered, largely the century from 1690 to 1790, ‘Denmark’ means really Denmark-Norway, for until 1814 Norway was part of the double monarchy ruled by the king and his government in Copenhagen. It should also be kept in mind that parts of what is today Germany, namely Schleswig-Holstein, belonged to the kingdom. However, as far as language and culture were concerned, these parts of southern Denmark were more German than Danish, and they played no important role in the scientific life of the kingdom. Sweden covered a much larger geographical area than it does today. The country had expanded greatly during the seventeenth century, when not only Finland but also parts of the Baltic area and northern Germany came under Swedish rule. About 1720, after the Great Northern War, Sweden lost most of its possessions, but the major part of Finland remained as part of the country until Centre for Science Studies, Department of Physics and Astronomy, Aarhus University, Denmark. -
Ludvig Holberg O Ne I N No Other Light We Wan T You English to See Him
L U DVI G H O LB E RG TH E FOU NDER OF N ORW EG IAN LITERATU RE AND AN OXFO RD STUDENT H A MM E R M A . S . C . , . OXFORD D . B A KW ELL BR A TREET B. H L C , O S LU DVI G HOLB ERG TH E FOU NDER OF N ORW EGIAN LITERAT U R E A ND AN OX FORD STU DENT A . H A MM E R M . c . s . L , OXFO RD B A D TREET B . EL RO ' H BLAC KW L, S MC MXX LU DVI G H OLB E R G I NTRODU CTORY NOTE TH E lec tu re w as 23rd 1 919 following delivered on May , , at i o f Sir Magdalen College , Oxford , by invitat on the President , Herbert Warren , and in the presence , among others , of the L N . orwegian Minister in ondon , Mr Benjamin Vogt In revising the manuscript I have thought it necessary to enlarge it o n a few points where I had to condense the lecture W I in order to keep it ithin the confin es Of an hour . have also added a few supplementary footnotes and a brief reference to the bulky Holberg literature which m a y perhaps prove o f interest to Holberg students in England . In paying my respectful thanks to the President Of Magdalen College and the distinguished audience for their kind reception I beg to sum up my feelings in the words o f Holberg ' himself ' M u ms san e n ominibu s devin ctu m Oxoniensibu s me ’ tenerz fateor . -
FERDINAND QUENISSET's ASTROPHOTOGRAPHIC PLATES ) L I a T E D (
FERDINAND QUENISSET'S ASTROPHOTOGRAPHIC PLATES ) l i a t e d ( 5 ° n , 6 3 9 1 , r e i t l e P t e m o C Weekly transmission 36-2018 presents: Ferdinand Quénisset, French astrophotographer II Camille Flammarion’s Observatory in Juvisy III Weekly Drawing by éophile Bouchet: “A S.E.T.I. is born ” VII Seven astrophotographic plates, positives and negatives 1-7 Previous transmissions can be found at: www.plantureux.fr ) l i a t e d ( 3 ° n , n o o M e h T Ferdinand Quénisset (1872–1951), French astrophotographer Quénisset was born on 8 August 1872 in Paris, the son of Gatien Jules Quénisset, an assistant director of Monnaies et Médailles in Paris, and Juliette Antonia Mallard, a dressmaker. Ferdinand became interested in astronomy by reading Camille Flammarion‘s books. In 1891, Quénisset, 19 years old, joined Flamamrion’s Society Astronomique de France as assistant librarian. At the time, the SAF was located at 28 rue Serpente in Paris. Soon, Quenisset worked also as an observer at Flammarion’s observatory in Juvisy-sur-Orge, where he discovered a comet in 1893. He was forced to abandon astronomy for several years while he performed his military service, but then returned to Juvisy to resume his post at the observatory until 1947. The e-bulletins present articles as well as selections of books, albums, photographs and documents as they have been handed down to the actual owners by their creators and by amateurs from past generations. The glass plates are available, price is 800 euros for the group (8), 400 euros for the drawing. -
Monte Carlo Simulations of Atmospheric Loss by Stellar Winds from Exoplanets Daniel Violette University of Connecticut - Storrs, [email protected]
University of Connecticut OpenCommons@UConn Honors Scholar Theses Honors Scholar Program Spring 5-19-2014 Monte Carlo Simulations of Atmospheric Loss by Stellar Winds from Exoplanets Daniel Violette University of Connecticut - Storrs, [email protected] Follow this and additional works at: https://opencommons.uconn.edu/srhonors_theses Part of the Astrophysics and Astronomy Commons, and the Atomic, Molecular and Optical Physics Commons Recommended Citation Violette, Daniel, "Monte Carlo Simulations of Atmospheric Loss by Stellar Winds from Exoplanets" (2014). Honors Scholar Theses. 400. https://opencommons.uconn.edu/srhonors_theses/400 Monte Carlo Simulations of Atmospheric Loss by Stellar Winds from Exoplanets Daniel Violette University of Connecticut, Department of Physics ii Abstract Hot Jupiters are a class of extra-solar planets. Massive gas giants on the same size scale as Jupiter, they orbit their host stars closely. This proximity results in large stellar winds capable of stripping away a planet’s atmosphere. Developing a more complete understanding of atmospheric mass loss and evolution in planetary bodies is critical, and Hot Jupiter systems are accessible analogues. This project will seek to create a computational model capable of estimating mass loss rates due to stellar winds. A Monte Carlo method is utilized to take an ensemble of single, high-energy energetic neutral particles, produced by kilo-electronvolt stellar wind ions, and and trace their path through theoretical atmospheres. As these particles travel, they collide many times, imparting energy to the atmospheric molecules and potentially exciting them to high enough energies to escape the planetary gravity. Different mechanisms for particle interaction and escape will also be analyzed in order to determine their impact on the mass loss rates. -
Sophie's World
Sophie’s World Jostien Gaarder Reviews: More praise for the international bestseller that has become “Europe’s oddball literary sensation of the decade” (New York Newsday) “A page-turner.” —Entertainment Weekly “First, think of a beginner’s guide to philosophy, written by a schoolteacher ... Next, imagine a fantasy novel— something like a modern-day version of Through the Looking Glass. Meld these disparate genres, and what do you get? Well, what you get is an improbable international bestseller ... a runaway hit... [a] tour deforce.” —Time “Compelling.” —Los Angeles Times “Its depth of learning, its intelligence and its totally original conception give it enormous magnetic appeal ... To be fully human, and to feel our continuity with 3,000 years of philosophical inquiry, we need to put ourselves in Sophie’s world.” —Boston Sunday Globe “Involving and often humorous.” —USA Today “In the adroit hands of Jostein Gaarder, the whole sweep of three millennia of Western philosophy is rendered as lively as a gossip column ... Literary sorcery of the first rank.” —Fort Worth Star-Telegram “A comprehensive history of Western philosophy as recounted to a 14-year-old Norwegian schoolgirl... The book will serve as a first-rate introduction to anyone who never took an introductory philosophy course, and as a pleasant refresher for those who have and have forgotten most of it... [Sophie’s mother] is a marvelous comic foil.” —Newsweek “Terrifically entertaining and imaginative ... I’ll read Sophie’s World again.” — Daily Mail “What is admirable in the novel is the utter unpretentious-ness of the philosophical lessons, the plain and workmanlike prose which manages to deliver Western philosophy in accounts that are crystal clear. -
“Religion in the Public Sphere” This Publication Is a Seminar Report from the Holberg Prize Seminar 2005
The Holberg Prize Seminar 2005, Holberg Prize Laureate Professor Jürgen Habermas: “Religion in the Public Sphere” This publication is a seminar report from the Holberg Prize Seminar 2005 The main lecture at the seminar was held by the Holberg International Memorial Prize laureate 2005 Professor Jürgen Habermas. In addition to the main lecture four scholars were invited to give a lecture which theme was in relation to the topic of Jürgen Habermas’s lecture. These lectures had a timeframe of 30 minutes. All of the main lectures were commented by additional scholars, the comments had a timeframe of 10 minutes. The scholars were asked to contribute their papers as they where given at the seminar. Contents Award Announcement 4 About the Ludvig Holberg Memorial Fund 5 Greetings from the Ludvig Holberg Memorial Fund 6 Jürgen Habermas’s speech at the award seremony 30 November 2005 8 Jürgen Habermas: Religion in the public sphere. 10 Arne Johan Vetlesen: Faith in religion. Habermas’s post-secular search for Meaning and Solidarity. 22 Gunnar Skirbekk: The Critically Ambiguous Idea of a “Modernization of (Religious) Consciousness”. 27 Cristina Lafont: The Burdens of the Public Use of Reason. 32 Cathrine Holst: Secular Worries. 48 Helge Høibraaten: Post-metaphysical thought, religion and secular society. 52 Craig Calhoun: Religion, Secularism, and Public Reason. 64 Thomas M. Schmidt: The Discourse of Religion in the Post-Secular Society. 80 Jon Hellesnes: On Artificially Moralising the Morally Irrelevant. 90 Hauke Brunkhorst: Hard Times for Democracy. 92 Tore Lindholm: Challenging Habermas on the Moral Legitimacy of Religious Voices in Democratic Politics. -
Cosmological Sources of Critical Cosmopolitanism
Review of International Studies (2010), 36, 181–200 2010 British International Studies Association doi:10.1017/S0260210510001063 First published online 2 Sep 2010 Cosmological sources of critical cosmopolitanism HEIKKI PATOMÄKI* Abstract. Critical cosmopolitan orientation has usually been embedded in a non-geocentric physical (NGP) cosmology that locates the human drama on the surface of planet Earth within wide scales of time and space. Although neither a necessary nor a sufficient condition for critical cosmopolitanism, NGP cosmology provides a contrast to the underpinnings of centric cosmologies, such as those of Aristotle, which see the world as revolving around a particular observer, theorist and/or communal identity. NGP cosmology makes it plausible to envisage all humans as part of the same species. The connection works also through homology and analogy. An astronomic theory can be isomorphic with an ethico-political theory, that is, a structure-preserving mapping from one to the other is possible. Key cosmopolitan theorists have situated morality within a cosmic framework. However, the ethico-political implications of the NGP cosmology are ambiguous. Nietzsche was among the first to articulate its sceptical and nihilist implications. Various reactions have encouraged territorial nationalism and geopolitics. I suggest that critical cosmopolitical orientation should now be grounded on the notion of cosmic evolution, which is not only contextual, historical, pluralist and open-ended but also suggests that humanity is not a mere accident of the cosmos. Heikki Patomäki is Professor of World Politics and the Vice Director of the Centre of Excellence in Global Governance Research at the University of Helsinki, Finland. He is also an Innovation Professor of Human Security – Globalisation and Global Institutions at the RMIT University in Melbourne, Australia. -
Download/Hc:27894/CONTENT/ How to Read Neanderthal for Sapiens.Pdf
DO THE INTERACTIONS BETWEEN ASTRONOMY AND RELIGION, BEGINNING IN PREHISTORY, FORM A DISTINCT RELIGIOUS TRADITION? by Brandon Reece Taylor (a.k.a. Brandon Taylorian / Cometan) A Dissertation Submitted to the School of Humanities, Language and Global Studies University of Central Lancashire In Partial Fulfilment of the Requirements for the Degree of Master of Arts August 2020 Word count: 14,856 1 of 96 Abstract –––––––––––––––––––––––––––––––––– Astronomy and religion have long been intertwined with their interactions resembling a symbiotic relationship since prehistoric times. Building on existing archaeological research, this study asks: do the interactions between astronomy and religion, beginning from prehistory, form a distinct religious tradition? Prior research exploring the prehistoric origins of religion has unearthed evidence suggesting the influence of star worship and night sky observation in the development of religious sects, beliefs and practices. However, there does not yet exist a historiography dedicated to outlining why astronomy and religion mutually developed, nor has there been a proposal set forth asserting that these interactions constitute a religious tradition; proposed herein as the Astronic tradition, or Astronicism. This paper pursues the objective of arguing for the Astronic tradition to be treated, firstly, as a distinct religious tradition and secondly, as the oldest archaeologically-verifiable religious tradition. To achieve this, the study will adopt a multidisciplinary approach involving archaeology, anthropology, geography, psychology, mythology, archaeoastronomy and comparative religion. After proposing six characteristics inherent to a religious tradition, the paper will assemble a historiography for astronomical religion. As a consequence of the main objective, this study also asserts that astronomical religion, most likely astrolatry, has its origins in the Upper Palaeolithic period of the Stone Age based on specimens from the archaeological record.