Catalogue 03-2019 Rare and Valuable Astronomical Books, Mostly New Arrivals
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Strategies of Defending Astrology: a Continuing Tradition
Strategies of Defending Astrology: A Continuing Tradition by Teri Gee A thesis submitted in conformity with the requirements for the degree of Doctorate of Philosophy Institute for the History and Philosophy of Science and Technology University of Toronto © Copyright by Teri Gee (2012) Strategies of Defending Astrology: A Continuing Tradition Teri Gee Doctorate of Philosophy Institute for the History and Philosophy of Science and Technology University of Toronto 2012 Abstract Astrology is a science which has had an uncertain status throughout its history, from its beginnings in Greco-Roman Antiquity to the medieval Islamic world and Christian Europe which led to frequent debates about its validity and what kind of a place it should have, if any, in various cultures. Written in the second century A.D., Ptolemy’s Tetrabiblos is not the earliest surviving text on astrology. However, the complex defense given in the Tetrabiblos will be treated as an important starting point because it changed the way astrology would be justified in Christian and Muslim works and the influence Ptolemy’s presentation had on later works represents a continuation of the method introduced in the Tetrabiblos. Abû Ma‘shar’s Kitâb al- Madkhal al-kabîr ilâ ‘ilm ahk. âm al-nujûm, written in the ninth century, was the most thorough surviving defense from the Islamic world. Roger Bacon’s Opus maius, although not focused solely on advocating astrology, nevertheless, does contain a significant defense which has definite links to the works of both Abû Ma‘shar and Ptolemy. As such, he demonstrates another stage in the development of astrology. -
PHIL 339 Intro Phil of Science, UO Philosophy Dept, Winter 2018
1 PHIL 339 Intro Phil of Science, UO Philosophy Dept, Winter 2018 Albert Einstein, Marie Curie, Benjamin Franklin,Watson & Crick, Rosalind Franklin, Galileo Galilei, Dr. Linus Pauling, William Crawford Eddy, James Watt Maria Goeppert-Mayer, Charles Darwin, James Clerk Maxwell, Archimedes, Lise Meitner, Sigmund Freud, Irène Joliot-Curie Gregor Johann Mendel,Chien-Shiung Wu,Barbara McClintock, Neil DeGrasse Tyson. All Contents ©2017 Photo Researchers, Inc., 307 Fifth Avenue, New York, NY , 10016 212-758-3420 800-833- 9033 Science Source® is a registered trademark of Photo Researchers, Inc. / 2 PHIL 339 Intro Phil of Science, UO Philosophy Dept, Winter 2018 Course Data PHIL 339 Intro Phil of Science >2 4.00 cr. Grading Options: Optional for all students Instructor: Prof. N. Zack, Office: 239 SCH Phone: (541) 346-1547 Office Hours: WTh -2-3 See CRN for CommentsPrereqs/Comments: Prereq: one philosophy course (waiver available) *Note: This is a 2-hr course twice a week and discussion is built in. There will breaks and variations in subject matter to keep it interesting. OVERVIEW/DESCRIPTION (See also APPENDICES A-D AFTER SYLLABUS) Philosophy of Science is unique to philosophy. It raises questions about facts, theories, reality, explanation, and truth not often addressed by scientists or other humanistic scholars. This course will provide the basics of Philosophy of Science with concrete examples as science now applies to contemporary subjects such as Climate Change, Feminism, and Race. Students will have an opportunity to choose their own branches of inquiry for end-of-term reports. Work will consist of reading, discussion, and 4 3-page papers. -
New Force at Large Distances
New force at large distances Daniel Grumiller Institute for Theoretical Physics Vienna University of Technology TEDx Vienna, November 2010 I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? (picture by NASA) D. Grumiller | New force 2/11 I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? (picture by lifesbalancebeam) D. Grumiller | New force 2/11 Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? (picture by spacescan.org) D. Grumiller | New force 2/11 We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: D. Grumiller | New force 2/11 What is the Universe made of? D. -
Claudius Ptolemy: Tetrabiblos
CLAUDIUS PTOLEMY: TETRABIBLOS OR THE QUADRIPARTITE MATHEMATICAL TREATISE FOUR BOOKS OF THE INFLUENCE OF THE STARS TRANSLATED FROM THE GREEK PARAPHRASE OF PROCLUS BY J. M. ASHMAND London, Davis and Dickson [1822] This version courtesy of http://www.classicalastrologer.com/ Revised 04-09-2008 Foreword It is fair to say that Claudius Ptolemy made the greatest single contribution to the preservation and transmission of astrological and astronomical knowledge of the Classical and Ancient world. No study of Traditional Astrology can ignore the importance and influence of this encyclopaedic work. It speaks not only of the stars, but of a distinct cosmology that prevailed until the 18th century. It is easy to jeer at someone who thinks the earth is the cosmic centre and refers to it as existing in a sublunary sphere. However, our current knowledge tells us that the universe is infinite. It seems to me that in an infinite universe, any given point must be the centre. Sometimes scientists are not so scientific. The fact is, it still applies to us for our purposes and even the most rational among us do not refer to sunrise as earth set. It practical terms, the Moon does have the most immediate effect on the Earth which is, after all, our point of reference. She turns the tides, influences vegetative growth and the menstrual cycle. What has become known as the Ptolemaic Universe, consisted of concentric circles emanating from Earth to the eighth sphere of the Fixed Stars, also known as the Empyrean. This cosmology is as spiritual as it is physical. -
Download Report 2010-12
RESEARCH REPORt 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Cover: Aurora borealis paintings by William Crowder, National Geographic (1947). The International Geophysical Year (1957–8) transformed research on the aurora, one of nature’s most elusive and intensely beautiful phenomena. Aurorae became the center of interest for the big science of powerful rockets, complex satellites and large group efforts to understand the magnetic and charged particle environment of the earth. The auroral visoplot displayed here provided guidance for recording observations in a standardized form, translating the sublime aesthetics of pictorial depictions of aurorae into the mechanical aesthetics of numbers and symbols. Most of the portait photographs were taken by Skúli Sigurdsson RESEARCH REPORT 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Introduction The Max Planck Institute for the History of Science (MPIWG) is made up of three Departments, each administered by a Director, and several Independent Research Groups, each led for five years by an outstanding junior scholar. Since its foundation in 1994 the MPIWG has investigated fundamental questions of the history of knowl- edge from the Neolithic to the present. The focus has been on the history of the natu- ral sciences, but recent projects have also integrated the history of technology and the history of the human sciences into a more panoramic view of the history of knowl- edge. Of central interest is the emergence of basic categories of scientific thinking and practice as well as their transformation over time: examples include experiment, ob- servation, normalcy, space, evidence, biodiversity or force. -
James Clerk Maxwell
Conteúdo Páginas Henry Cavendish 1 Jacques Charles 2 James Clerk Maxwell 3 James Prescott Joule 5 James Watt 7 Jean-Léonard-Marie Poiseuille 8 Johann Heinrich Lambert 10 Johann Jakob Balmer 12 Johannes Robert Rydberg 13 John Strutt 14 Michael Faraday 16 Referências Fontes e Editores da Página 18 Fontes, Licenças e Editores da Imagem 19 Licenças das páginas Licença 20 Henry Cavendish 1 Henry Cavendish Referência : Ribeiro, D. (2014), WikiCiências, 5(09):0811 Autor: Daniel Ribeiro Editor: Eduardo Lage Henry Cavendish (1731 – 1810) foi um físico e químico que investigou isoladamente de acordo com a tradição de Sir Isaac Newton. Cavendish entrou no seminário em 1742 e frequentou a Universidade de Cambridge (1749 – 1753) sem se graduar em nenhum curso. Mesmo antes de ter herdado uma fortuna, a maior parte das suas despesas eram gastas em montagem experimental e livros. Em 1760, foi eleito Fellow da Royal Society e, em 1803, um dos dezoito associados estrangeiros do Institut de France. Entre outras investigações e descobertas de Cavendish, a maior ocorreu em 1781, quando compreendeu que a água é uma substância composta por hidrogénio e oxigénio, uma reformulação da opinião de há milénios de que a água é um elemento químico básico. O químico inglês John Warltire (1725/6 – 1810) realizou uma Figura 1 Henry Cavendish (1731 – 1810). experiência em que explodiu uma mistura de ar e hidrogénio, descobrindo que a massa dos gases residuais era menor do que a da mistura original. Ele atribuiu a perda de massa ao calor emitido na reação. Cavendish concluiu que algum erro substancial estava envolvido visto que não acreditava que, dentro da teoria do calórico, o calor tivesse massa suficiente, à escala em análise. -
As Above, So Below. Astrology and the Inquisition in Seventeenth-Century New Spain
Department of History and Civilization As Above, So Below. Astrology and the Inquisition in Seventeenth-Century New Spain Ana Avalos Thesis submitted for assessment with a view to obtaining the degree of Doctor of History and Civilization of the European University Institute Florence, February 2007 EUROPEAN UNIVERSITY INSTITUTE Department of History and Civilization As Above, So Below. Astrology and the Inquisition in Seventeenth-Century New Spain Ana Avalos Thesis submitted for assessment with a view to obtaining the degree of Doctor of History and Civilization of the European University Institute Examining Board: Prof. Peter Becker, Johannes-Kepler-Universität Linz Institut für Neuere Geschichte und Zeitgeschichte (Supervisor) Prof. Víctor Navarro Brotons, Istituto de Historia de la Ciencia y Documentación “López Piñero” (External Supervisor) Prof. Antonella Romano, European University Institute Prof. Perla Chinchilla Pawling, Universidad Iberoamericana © 2007, Ana Avalos No part of this thesis may be copied, reproduced or transmitted without prior permission of the author A Bernardo y Lupita. ‘That which is above is like that which is below and that which is below is like that which is above, to achieve the wonders of the one thing…’ Hermes Trismegistus Contents Acknowledgements 4 Abbreviations 5 Introduction 6 1. The place of astrology in the history of the Scientific Revolution 7 2. The place of astrology in the history of the Inquisition 13 3. Astrology and the Inquisition in seventeenth-century New Spain 17 Chapter 1. Early Modern Astrology: a Question of Discipline? 24 1.1. The astrological tradition 27 1.2. Astrological practice 32 1.3. Astrology and medicine in the New World 41 1.4. -
The Humanities in Deconstruction: Raising the Question of the Post-Colonial University
ACCESS: CONTEMPORARY ISSUES IN EDUCATION 2007, VOL. 26, NO. 1, 1–10 The humanities in deconstruction: Raising the question of the post-colonial university Michael A. Peters University of Illinois at Urbana-Champaign ABSTRACT Derrida is, perhaps, the foremost philosopher of the humanities and of its place in the university. Over the long period of his career he has been concerned with the fate, status, place and contribution of the humanities. Through his deconstructive readings and writings he has done much not only to reinvent the Western tradition by attending closely to those texts which constitute it but also he has redefined its procedures and protocols, questioning and commenting upon the relationship between commentary and interpretation, the practice of quotation, the delimitation of a work and its singularity, its signature, and its context – the whole form of life of literary culture, together with textual practices and conventions that shape it. From his very early work he has occupied a marginal in-between space – simultaneously, textual, literary, philosophical, and political – a space that permitted him a freedom to question, to speculate and to draw new limits to humanitas. Derrida has demonstrated his power to reconceptualise and to reimagine the humanities in the space of the contemporary university. This paper discusses Derrida’s tasks for the new humanities (Trifonas & Peters, 2005). 1. Fundamentalisms and the need for a deconstructive humanities An appreciation of Derrida’s work can shed light on the growth and clash -
Recent News 28,270 MILES - WAY to GO!
Number 62 Spring 2017 TREASURE HUNT – 16 Where is this bridge (hint: it is not in the UK) and who designed it? Can you see the parabola and its tangent? Recent News 28,270 MILES - WAY TO GO! In October last year a record was set for the longest single road route ever worked out. The Travelling Salesperson Problem (TSP) was first posed in the 1930’s by Merrill Flood who was looking to solve a school bus routing problem in the US and it asks the following question: "Given a list of cities and the distances between each pair of cities, what is the shortest possible route that visits each city exactly once and returns to the origin city?" This is an example of an optimisation problem and is of immense importance to businesses who need to make deliveries to many places as the shortest route between the warehouse and drop off points generally means considerable saving in time and money. The TSP also has applications in computing DNA sequences, aiming telescopes and designing computer chip circuits. William Cook and a team of researchers at the University of Waterloo in Ontario, Canada calculated a round route that starts in Portland, Dorset and finishes in Weymouth, four miles away has at least 100 times more stops than the previous longest TSP. It links 24,727 hostelries in the UK. EDITORIAL SQUARE NUMBERS Welcome back to a new term and a new year! We In SYMmetryplus 61, Autumn 2016, modular arithmetic congratulate Mathematical Pie for their 200th edition was used to find a prime factor of 283 1. -
The Mystery and Majesty
The mystery and majesty Nearly 40 years after THE SPACE AGE BLASTED off when the Soviet Union launched the Voyager 2 visited Uranus world’s first artificial satellite in 1957. Since then, humanity has explored our cosmic and Neptune, scientists are backyard with vigor — and yet two planets have fallen to the planetary probe wayside. eager for new expeditions. In the 63 years since Sputnik, humanity has only visited Neptune and Uranus once BY JOEL DAVIS — when Voyager 2 flew past Uranus in January 1986 and Neptune in August 1989 40 ASTRONOMY • DECEMBER 2020 of the ICE GIANTS — and even that wasn’t entirely pre- interstellar mission, more than a dozen pro- In 1781, Uranus became the first planet planned. The unmitigated success of posals have been offered for return missions ever discovered using a telescope. Nearly 200 years later, Voyager 2 Voyager 1 and 2 on their original mission to one or both ice giants. So far, none have became the first spacecraft to visit to explore Jupiter and Saturn earned the made it past the proposal stage due to lack Uranus and Neptune, in 1986 and 1989 respectively. NASA/JPL twin spacecrafts further missions in our of substantial scientific interest. Effectively, solar system and beyond, with Neptune and the planetary research community has been Uranus acting as the last stops on a Grand giving the ice giants the cold shoulder. Tour of the outer solar system. But recently, exoplanet data began In the 31 years since Voyager 2 left the revealing the abundance of icy exoplanets Neptune system in 1989 and began its in our galaxy “and new questions about WWW.ASTRONOMY.COM 41 With a rotation axis tilted more than 90 degrees compared to its orbital plane, Neptune likewise has a highly tilted rotation axis and tilted magnetic axis. -
The Astronomical Work of Carl Friedrich Gauss
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector HISTORIA MATHEMATICA 5 (1978), 167-181 THE ASTRONOMICALWORK OF CARL FRIEDRICH GAUSS(17774855) BY ERIC G, FORBES, UNIVERSITY OF EDINBURGH, EDINBURGH EH8 9JY This paper was presented on 3 June 1977 at the Royal Society of Canada's Gauss Symposium at the Ontario Science Centre in Toronto [lj. SUMMARIES Gauss's interest in astronomy dates from his student-days in Gattingen, and was stimulated by his reading of Franz Xavier von Zach's Monatliche Correspondenz... where he first read about Giuseppe Piazzi's discovery of the minor planet Ceres on 1 January 1801. He quickly produced a theory of orbital motion which enabled that faint star-like object to be rediscovered by von Zach and others after it emerged from the rays of the Sun. Von Zach continued to supply him with the observations of contemporary European astronomers from which he was able to improve his theory to such an extent that he could detect the effects of planetary perturbations in distorting the orbit from an elliptical form. To cope with the complexities which these introduced into the calculations of Ceres and more especially the other minor planet Pallas, discovered by Wilhelm Olbers in 1802, Gauss developed a new and more rigorous numerical approach by making use of his mathematical theory of interpolation and his method of least-squares analysis, which was embodied in his famous Theoria motus of 1809. His laborious researches on the theory of Pallas's motion, in whi::h he enlisted the help of several former students, provided the framework of a new mathematical formu- lation of the problem whose solution can now be easily effected thanks to modern computational techniques. -
Thermodynamic Temperature
Thermodynamic temperature Thermodynamic temperature is the absolute measure 1 Overview of temperature and is one of the principal parameters of thermodynamics. Temperature is a measure of the random submicroscopic Thermodynamic temperature is defined by the third law motions and vibrations of the particle constituents of of thermodynamics in which the theoretically lowest tem- matter. These motions comprise the internal energy of perature is the null or zero point. At this point, absolute a substance. More specifically, the thermodynamic tem- zero, the particle constituents of matter have minimal perature of any bulk quantity of matter is the measure motion and can become no colder.[1][2] In the quantum- of the average kinetic energy per classical (i.e., non- mechanical description, matter at absolute zero is in its quantum) degree of freedom of its constituent particles. ground state, which is its state of lowest energy. Thermo- “Translational motions” are almost always in the classical dynamic temperature is often also called absolute tem- regime. Translational motions are ordinary, whole-body perature, for two reasons: one, proposed by Kelvin, that movements in three-dimensional space in which particles it does not depend on the properties of a particular mate- move about and exchange energy in collisions. Figure 1 rial; two that it refers to an absolute zero according to the below shows translational motion in gases; Figure 4 be- properties of the ideal gas. low shows translational motion in solids. Thermodynamic temperature’s null point, absolute zero, is the temperature The International System of Units specifies a particular at which the particle constituents of matter are as close as scale for thermodynamic temperature.