The Search for Life and a New Logic
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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. -
Chapter Two: the Astronomers and Extraterrestrials
Warning Concerning Copyright Restrictions The Copyright Law of the United States (Title 17, United States Code) governs the making of photocopies or other reproductions of copyrighted materials, Under certain conditions specified in the law, libraries and archives are authorized to furnish a photocopy or other reproduction, One of these specified conditions is that the photocopy or reproduction is not to be used for any purpose other than private study, scholarship, or research , If electronic transmission of reserve material is used for purposes in excess of what constitutes "fair use," that user may be liable for copyright infringement. • THE EXTRATERRESTRIAL LIFE DEBATE 1750-1900 The idea of a plurality of worlds from Kant to Lowell J MICHAEL]. CROWE University of Notre Dame TII~ right 0/ ,It, U,,;v"Jily 0/ Camb,idg4' to P'''''' a"d s,1I all MO""" of oooks WM grattlrd by H,rr,y Vlf(;ff I $J4. TM U,wNn;fyltas pritr"d and pu"fisllrd rOffti",.ously sincr J5U. Cambridge University Press Cambridge London New York New Rochelle Melbourne Sydney Published by the Press Syndicate of the University of Cambridge In lovi ng The Pirr Building, Trumpingron Srreer, Cambridge CB2. I RP Claire H 32. Easr 57th Streer, New York, NY 1002.2., U SA J 0 Sramford Road, Oakleigh, Melbourne 3166, Australia and Mi ha © Cambridge Univ ersiry Press 1986 firsr published 1986 Prinred in rh e Unired Srares of America Library of Congress Cataloging in Publication Data Crowe, Michael J. The exrrarerresrriallife debare '750-1900. Bibliography: p. Includes index. I. Pluraliry of worlds - Hisrory. -
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. -
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere A Constellation of Rare Books from the History of Science Collection The exhibition was made possible by generous support from Mr. & Mrs. James B. Hebenstreit and Mrs. Lathrop M. Gates. CATALOG OF THE EXHIBITION Linda Hall Library Linda Hall Library of Science, Engineering and Technology Cynthia J. Rogers, Curator 5109 Cherry Street Kansas City MO 64110 1 Thinking Outside the Sphere is held in copyright by the Linda Hall Library, 2010, and any reproduction of text or images requires permission. The Linda Hall Library is an independently funded library devoted to science, engineering and technology which is used extensively by The exhibition opened at the Linda Hall Library April 22 and closed companies, academic institutions and individuals throughout the world. September 18, 2010. The Library was established by the wills of Herbert and Linda Hall and opened in 1946. It is located on a 14 acre arboretum in Kansas City, Missouri, the site of the former home of Herbert and Linda Hall. Sources of images on preliminary pages: Page 1, cover left: Peter Apian. Cosmographia, 1550. We invite you to visit the Library or our website at www.lindahlll.org. Page 1, right: Camille Flammarion. L'atmosphère météorologie populaire, 1888. Page 3, Table of contents: Leonhard Euler. Theoria motuum planetarum et cometarum, 1744. 2 Table of Contents Introduction Section1 The Ancient Universe Section2 The Enduring Earth-Centered System Section3 The Sun Takes -
The History of Optical Astronomy, by Caroline Herschel and Lyman Spitzer
Online Modules from The University of Chicago Multiwavelength Astronomy: The History of Optical Astronomy, by Caroline Herschel and Lyman Spitzer http://ecuip.lib.uchicago.edu/multiwavelength-astronomy/optical/history/index.html Subject(s): Astronomy/Space Science Grade(s) Level: 9-12 Duration: One Class Period Objectives: As a result of reading The History of Optical Astronomy, students will be able to • Discriminate between reflecting and refracting telescope designs and describe the differences between them; • Explain how a telescope focuses light; • Articulate the limitations of ground-based telescopes and propose solutions to these limitations; • Identify important astronomical discoveries made and personages working in the optical regime; • Discuss examples of problem-solving and creativity in astronomy. Materials: Internet connection and browser for displaying the lesson. Pre-requisites: Students should be familiar with the Electromagnetic Spectrum. Before using the lesson, students should familiarize themselves with all vocabulary terms. Procedures: Students will read the lesson and answer assessment questions (listed under evaluation). Introduction: In reading this lesson, you will meet important individuals in the History of Optical Astronomy. They are: Caroline Lucretia Herschel was a German-born British astronomer and the sister of astronomer Sir William Herschel. She is the discoverer of several comets, in particular, the periodic comet 35P/Herschel-Rigollet, which bears her name. Lyman Strong Spitzer, Jr. was an American theoretical physicist, astronomer and mountaineer. He carried out research into star formation, plasma physics, and in 1946, conceived the idea of telescopes operating in outer space. Spitzer is the namesake of NASA's Spitzer Space Telescope. 1 Online Modules from The University of Chicago William Herschel was an astronomer and composer. -
Sensing the Invisible: the Herschel Experiment
MESS E N G E R S ENSIN G THE I NVISIB L E Y R HE ERSCHEL XPERIMENT U T H E C R E M TO N M I S S I O L E S S O N O V E RV I E W GRADE LEVEL 5 - 8 L ESSON S UMMARY In this lesson, students find out that there is radiation other than visible light arriving from the Sun. The students reproduce a version of William DURATION 1-2 hours Herschel’s experiment of 800 that discovered the existence of infrared radiation. The process of conducting the experiment and placing it in the historical context illustrates how scientific discoveries are often made ESSENTIAL QUESTION via creative thinking, careful design of the experiment, and adaptation of Are there forms of light other than visible light the experiment to accommodate unexpected results. Students discuss emitted by the Sun? current uses of infrared radiation and learn that it is both very beneficial and a major concern for planetary explorations such as the MESSENGER mission to Mercury. Lesson 1 of Grades 5-8 Component of Staying Cool O BJECTIVES Students will be able to: ▼ Construct a device to measure the presence of infrared radiation in sunlight. ▼ Explain that visible light is only part of the electromagnetic spectrum of radiation emitted by the Sun. ▼ Follow the path taken by Herschel through scientific discovery. ▼ Explain why we would want to use infrared radiation to study Mercury and other planets. ▼ Explain how excess infrared radiation is a concern for the MESSENGER mission. -
The Herschels and Their Astronomy
The Herschels and their Astronomy Mary Kay Hemenway 24 March 2005 outline • William Herschel • Herschel telescopes • Caroline Herschel • Considerations of the Milky Way • William Herschel’s discoveries • John Herschel Wm. Herschel (1738-1822) • Born Friedrich Wilhelm Herschel in Hanover, Germany • A bandboy with the Hanoverian Guards, later served in the military; his father helped him to leave Germany for England in 1757 • Musician in Bath • He read Smith's Harmonies, and followed by reading Smith's Optics - it changed his life. Miniature portrait from 1764 Discovery of Uranus 1781 • William Herschel used a seven-foot Newtonian telescope • "in the quartile near zeta Tauri the lowest of the two is a curious either Nebulous Star or perhaps a Comet” • He called it “Georgium Sidus" after his new patron, George Ill. • Pension of 200 pounds a year and knighted, the "King's Astronomer” -- now astronomy full time. Sir William Herschel • Those who had received a classical education in astronomy agreed that their job was to study the sun, moon, planets, comets, individual stars. • Herschel acted like a naturalist, collecting specimens in great numbers, counting and classifying them, and later trying to organize some into life cycles. • Before his discovery of Uranus, Fellows of the Royal Society had contempt for his ignorance of basic procedures and conventions. Isaac Newton's reflecting telescope 1671 William Herschel's 20-foot, 1783 Account of some Observations tending to investigate the Construction of the Heavens Philosophical Transactions of the Royal Society of London (1784) vol. 74, pp. 437-451 In a former paper I mentioned, that a more powerful instrument was preparing for continuing my reviews of the heavens. -
The Astronomy of Sir John Herschel
Introduction m m m m m m m m m m m Herschel’s Stars The Stars flourish, and in spite of all my attempts to thin them and . stuff them in my pockets, continue to afford a rich harvest. John Herschel to James Calder Stewart, July 17, 1834 n 2017, TRAPPIST-1, a red dwarf star forty light years from Earth, made headlines as the center of a system with not one or two but Iseven potentially habitable exoplanets.1 This dim, nearby star offers only the most recent example of verification of the sort of planetary system common in science fiction: multiple temperate, terrestrial worlds within a single star’s family of planets. Indeed, this discovery followed the an- nouncement only a few years earlier of the very first Earth-sized world orbiting within the habitable zone of its star, Kepler-186, five hundred light years from Earth.2 Along with other ongoing surveys and advanced instruments, the Kepler mission, which recently added an additional 715 worlds to a total of over five thousand exoplanet candidates, is re- vealing a universe in which exoplanets proliferate, Earth-like worlds are common, and planets within the habitable zone of their host star are far from rare.3 Exoplanetary astronomy has developed to the point that as- tronomers can not only detect these objects but also describe the phys- ical characteristics of many with a high degree of confidence and pre- cision, gaining information on their composition, atmospheric makeup, temperature, and even weather patterns. 3 © 2018 University of Pittsburgh Press. All rights reserved. -
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. -
Changing Concepts of Heat in the Early Nineteenth Century ROBERT JAMES MORRIS, JR., University of Oklahoma, Norma
SOCIAL SCIENCES 19~ Changing Concepts of Heat in the Early Nineteenth Century ROBERT JAMES MORRIS, JR., University of Oklahoma, Norma. Rival theories developed early in the nineteenth century, concerning the nature of heat, may be grouped into two opposing camps. Although perhaps differing in detail among themselves, the theories in one camp were unanimous in agreement on one fundamental point: heat phenomena were to be explained by a subtle, imponderable fluid called caloric. The other camp agreed that heat was due to vibrations of tbe particle. of matter. The caloric theory was orthodox and held by the great majority 196 PROC. OF THE OKLA. ACAD. OF SCI. FOR 1961 ot 1C1entists. This concept ot heat provided a simple, common·sense, easily vtsuaUzed explanation of most common heat phenomena. The exceptional case was that of frictional heat. In 1798, Benjamin Thompson (Count Rumford), the American sclen· tist and soldier of fortune, pUblished an account of his experiments con· ducted in a cannon·boring factory in Bavaria.' The results of these experi ments showed that an apparently unlimited amount of heat could be pro duced by friction. Caloricists, caught unawares by the impressive results ot Thompson's experiment, could offer no immediate explanation of this phenomenon. These data led Thompson to reject the idea that heat was a material substance and to propound the theory that heat was nothing more than the vibrations of the particles ot matter. With these seemingly irrefutable data, Thompson converted a few persons to his vibratory theory. However, in applying the new theory to other heat phenomena, this minority group got into trouble. -
Torrens, Hugh
BSHS Monographs publishes work of lasting scholarly value that might not otherwise be made available, and aids the dissemination of innovative projects advancing scholarship or education in the field. 13. Chang, Hasok and Jackson, 06. Morris, PJT, and Russell, CA; Catherine (eds.). 2007. An Smith, JG (ed.). 1988. Archives of Element of Controversy: The Life the British Chemical Industry, of Chlorine in Science, Medicine, 1750‐1914: A Handlist. Technology and War. ISBN 0‐0906450‐06‐3. ISBN: 978‐0‐906450‐01‐7. 05. Rees, Graham. 1984. Francis 12. Thackray, John C. (ed.). 2003. Bacon's Natural Philosophy: A To See the Fellows Fight: Eye New Source. Witness Accounts of Meetings of ISBN 0‐906450‐04‐7. the Geological Society of London 04. Hunter, Michael. 1994. The and Its Club, 1822‐1868. 2003. Royal Society and Its Fellows, ISBN: 0‐906450‐14‐4. 1660‐1700. 2nd edition. 11. Field, JV and James, Frank ISBN 978‐0‐906450‐09‐3. AJL. 1997. Science in Art. 03. Wynne, Brian. 1982. ISBN 0‐906450‐13‐6. Rationality and Ritual: The 10. Lester, Joe and Bowler, Windscale Inquiry and Nuclear Peter. E. Ray Lankester and the Decisions in Britain. Making of Modern British ISBN 0‐906450‐02‐0 Biology. 1995. 02. Outram, Dorinda (ed.). 2009. ISBN 978‐0‐906450‐11‐6. The Letters of Georges Cuvier. 09. Crosland, Maurice. 1994. In reprint of 1980 edition. the Shadow of Lavoisier: ISBN 0‐906450‐05‐5. ISBN 0‐906450‐10‐1. 01. Jordanova, L. and Porter, Roy 08. Shortland, Michael (ed.). (eds.). 1997. Images of the Earth: 1993.