Acta Universitatis Carolinae. Mathematica Et Physica
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Publikationen Dr. Rita Haub M.A
Publikationen Rita Haub 1. Die Motetten in der Notre-Dame-Handschrift Mü A (Bayerische Staatsbibliothek, Cod. gall. 42) (= Münchner Editionen zur Musikgeschichte Band 8), Tutzing 1986. 2. Die Geschichtlichen Hilfswissenschaften stellen sich vor (Redaktion u. Layout: Wolfgang Bildt und Rita Haub), München 21987. 3. 7 Katalogartikel (Urkunden und Siegel) in: Kilian. Mönch aus Irland – aller Franken Patron. 689-1989. (Katalog der Sonderausstellung zur 1300-Jahr-Feier des Kiliansmartyriums), München 1989. 4. Das Urkundenwesen in der Diözese Eichstätt bis zur Mitte des 13. Jahrhunderts, München 1993 (Selbstverlag). 5. Die Urkunden des Klosters Weihenstephan bis zum Jahre 1381, bearb. von Bodo Uhl, mit den Registern zu Teil 1 und 2, bearb. von Rita Haub (= Quellen und Erörterungen zur Bayerischen Geschichte, Neue Folge Band XXVII Zweiter Teil), München 1993. 6. Die Urbare des Kollegiatstifts St. Johann in Regensburg bis zum Jahre 1400, bearb. von Matthias Thiel, mit den Registern zu Teil 1 und 2, bearb. von Rita Haub (=Quellen und Erörterungen zur Bayerischen Geschichte, Neue Folge Band XXVIII Zweiter Teil), München 1994. 7. Georgius Victorinus und der Triumphus Divi Michaelis Archangeli Bavarici, in: Musik in Bayern 51 (1995), 79-85. 8. Matthäus Rader im Spiegel seiner Briefe, in: Stimmen der Zeit 214 (1996), Umschau 209-212. 9. Eine Urkunde Oswalds von Wolkenstein im Bestand der Klosterurkunden Beuerberg im Bayerischen Hauptstaatsarchiv München, in: Zeitschrift für bayerische Landesgeschichte 59 (1996), 177-183. 10. Petrus Canisius als Schriftsteller, in: Julius Oswald und Peter Rummel (Hgg.), Petrus Canisius – Reformer der Kirche. Festschrift zum 400. Todestag des zweiten Apostels Deutschlands (= Jahrbuch des Vereins für Augsburger Bistumsgeschichte e.V. -
Prehistory of Transit Searches Danielle BRIOT1 & Jean
Prehistory of Transit Searches Danielle BRIOT1 & Jean SCHNEIDER2 1) GEPI, UMR 8111, Observatoire de Paris, 61 avenue de l’Observatoire, F- 75014, Paris, France [email protected] 2) LUTh, UMR 8102, Observatoire de Paris, 5 place Jules Janssen, F-92195 Meudon Cedex, France [email protected] Abstract Nowadays the more powerful method to detect extrasolar planets is the transit method, that is to say observations of the stellar luminosity regularly decreasing when the planet is transiting the star. We review the planet transits which were anticipated, searched, and the first ones which were observed all through history. Indeed transits of planets in front of their star were first investigated and studied in the solar system, concerning the star Sun. The first observations of sunspots were sometimes mistaken for transits of unknown planets. The first scientific observation and study of a transit in the solar system was the observation of Mercury transit by Pierre Gassendi in 1631. Because observations of Venus transits could give a way to determine the distance Sun-Earth, transits of Venus were overwhelmingly observed. Some objects which actually do not exist were searched by their hypothetical transits on the Sun, as some examples a Venus satellite and an infra-mercurial planet. We evoke the possibly first use of the hypothesis of an exoplanet transit to explain some periodic variations of the luminosity of a star, namely the star Algol, during the eighteen century. Then we review the predictions of detection of exoplanets by their transits, those predictions being sometimes ancient, and made by astronomers as well as popular science writers. -
Catholic Christian Christian
Religious Scientists (From the Vatican Observatory Website) https://www.vofoundation.org/faith-and-science/religious-scientists/ Many scientists are religious people—men and women of faith—believers in God. This section features some of the religious scientists who appear in different entries on these Faith and Science pages. Some of these scientists are well-known, others less so. Many are Catholic, many are not. Most are Christian, but some are not. Some of these scientists of faith have lived saintly lives. Many scientists who are faith-full tend to describe science as an effort to understand the works of God and thus to grow closer to God. Quite a few describe their work in science almost as a duty they have to seek to improve the lives of their fellow human beings through greater understanding of the world around them. But the people featured here are featured because they are scientists, not because they are saints (even when they are, in fact, saints). Scientists tend to be creative, independent-minded and confident of their ideas. We also maintain a longer listing of scientists of faith who may or may not be discussed on these Faith and Science pages—click here for that listing. Agnesi, Maria Gaetana (1718-1799) Catholic Christian A child prodigy who obtained education and acclaim for her abilities in math and physics, as well as support from Pope Benedict XIV, Agnesi would write an early calculus textbook. She later abandoned her work in mathematics and physics and chose a life of service to those in need. Click here for Vatican Observatory Faith and Science entries about Maria Gaetana Agnesi. -
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 -
A New Vision of the Senses in the Work of Galileo Galilei
Perception, 2008, volume 37, pages 1312 ^ 1340 doi:10.1068/p6011 Galileo's eye: A new vision of the senses in the work of Galileo Galilei Marco Piccolino Dipartimento di Biologia, Universita© di Ferrara, I 44100 Ferrara, Italy; e-mail: [email protected] Nicholas J Wade University of Dundee, Dundee DD1 4HN, Scotland, UK Received 4 December 2007 Abstract. Reflections on the senses, and particularly on vision, permeate the writings of Galileo Galilei, one of the main protagonists of the scientific revolution. This aspect of his work has received scant attention by historians, in spite of its importance for his achievements in astron- omy, and also for the significance in the innovative scientific methodology he fostered. Galileo's vision pursued a different path from the main stream of the then contemporary studies in the field; these were concerned with the dioptrics and anatomy of the eye, as elaborated mainly by Johannes Kepler and Christoph Scheiner. Galileo was more concerned with the phenomenology rather than with the mechanisms of the visual process. His general interest in the senses was psychological and philosophical; it reflected the fallacies and limits of the senses and the ways in which scientific knowledge of the world could be gathered from potentially deceptive appearances. Galileo's innovative conception of the relation between the senses and external reality contrasted with the classical tradition dominated by Aristotle; it paved the way for the modern understanding of sensory processing, culminating two centuries later in Johannes Mu« ller's elaboration of the doctrine of specific nerve energies and in Helmholtz's general theory of perception. -
THE STUDY of SATURN's RINGS 1 Thesis Presented for the Degree Of
1 THE STUDY OF SATURN'S RINGS 1610-1675, Thesis presented for the Degree of Doctor of Philosophy in the Field of History of Science by Albert Van Haden Department of History of Science and Technology Imperial College of Science and Teohnology University of London May, 1970 2 ABSTRACT Shortly after the publication of his Starry Messenger, Galileo observed the planet Saturn for the first time through a telescope. To his surprise he discovered that the planet does.not exhibit a single disc, as all other planets do, but rather a central disc flanked by two smaller ones. In the following years, Galileo found that Sa- turn sometimes also appears without these lateral discs, and at other times with handle-like appendages istead of round discs. These ap- pearances posed a great problem to scientists, and this problem was not solved until 1656, while the solution was not fully accepted until about 1670. This thesis traces the problem of Saturn, from its initial form- ulation, through the period of gathering information, to the final stage in which theories were proposed, ending with the acceptance of one of these theories: the ring-theory of Christiaan Huygens. Although the improvement of the telescope had great bearing on the problem of Saturn, and is dealt with to some extent, many other factors were in- volved in the solution of the problem. It was as much a perceptual problem as a technical problem of telescopes, and the mental processes that led Huygens to its solution were symptomatic of the state of science in the 1650's and would have been out of place and perhaps impossible before Descartes. -
On the Alleged Use of Keplerian Telescopes in Naples in the 1610S
On the Alleged Use of Keplerian Telescopes in Naples in the 1610s By Paolo Del Santo Museo Galileo: Institute and Museum of History of Science – Florence (Italy) Abstract The alleged use of Keplerian telescopes by Fabio Colonna (c. 1567 – 1640), in Naples, since as early as October 1614, as claimed in some recent papers, is shown to be in fact untenable and due to a misconception. At the 37th Annual Conference of the Società Italiana degli Storici della Fisica e dell'Astronomia (Italian Society of the Historians of Physics and Astronomy, SISFA), held in Bari in September 2017, Mauro Gargano gave a talk entitled Della Porta, Colonna e Fontana e le prime osservazioni astronomiche a Napoli. This contribution, which appeared in the Proceedings of the Conference (Gargano, 2019a), was then followed by a paper —actually, very close to the former, which, in turn, is very close to a previous one (Gargano, 2017)— published, in the same year, in the Journal of Astronomical History and Heritage (Gargano, 2019b). In both of these writings, Gargano claimed that the Neapolitan naturalist Fabio Colonna (c. 1567 – 1640), member of the Accademia dei Lincei, would have made observations with a so-called “Keplerian” or “astronomical” telescope (i.e. with converging eyepiece), in the early autumn of 1614. The events related to the birth and development of Keplerian telescope —named after Johannes Kepler, who theorised this optical configuration in his Dioptrice, published in 1611— are complex and not well-documented, and their examination lies beyond the scope of this paper. However, from a historiographical point of view, the news that someone was already using such a configuration since as early as autumn 1614 for astronomical observations, if true, would have not negligible implications, which Gargano himself does not seem to realize. -
Sunspot Positions, Areas, and Group Tilt Angles for 1611−1631 from Observations by Christoph Scheiner? R
A&A 595, A104 (2016) Astronomy DOI: 10.1051/0004-6361/201629000 & c ESO 2016 Astrophysics Sunspot positions, areas, and group tilt angles for 1611−1631 from observations by Christoph Scheiner? R. Arlt1, V. Senthamizh Pavai1; 2, C. Schmiel1, and F. Spada1 1 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [email protected] 2 Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, 14476 Potsdam, Germany Received 25 May 2016 / Accepted 5 August 2016 ABSTRACT Aims. Digital images of observations printed in the books Rosa Ursina sive solis and Prodromus pro sole mobili by Christoph Scheiner, as well as the drawings from Scheiner’s letters to Marcus Welser, are analysed to obtain information on the positions and sizes of sunspots that appeared before the Maunder minimum. Methods. In most cases, the given orientation of the ecliptic is used to set up the heliographic coordinate system for the drawings. Positions and sizes are measured manually on screen. Very early drawings have no indication of their orientation. A rotational match- ing using common spots of adjacent days is used in some cases, while in other cases, the assumption that images were aligned with a zenith-horizon coordinate system appeared to be the most probable. Results. In total, 8167 sunspots were measured. A distribution of sunspot latitudes versus time (butterfly diagram) is obtained for Scheiner’s observations. The observations of 1611 are very inaccurate, the drawings of 1612 have at least an indication of their orientation, while the remaining part of the spot positions from 1618−1631 have good to very good accuracy. -
Historical Sunspot Records
Living Reviews in Solar Physics (2020) 17:1 https://doi.org/10.1007/s41116-020-0023-y REVIEW ARTICLE Historical sunspot records Rainer Arlt1 · José M. Vaquero2 Received: 10 May 2019 / Accepted: 22 January 2020 © The Author(s) 2020 Abstract Sunspot observations are available in fairly good numbers since 1610, after the inven- tion of the telescope. This review is concerned with those sunspot observations of which longer records and drawings in particular are available. Those records bear information beyond the classical sunspot numbers or group sunspot numbers. We begin with a brief summary on naked-eye sunspot observations, in particular those with drawings. They are followed by the records of drawings from 1610 to about 1900. The review is not a compilation of all known historical sunspot information. Some records contributing substantially to the sunspot number time series may there- fore be absent. We also glance at the evolution of the understanding of what sunspots actually are, from 1610 to the 19th century. The final part of the review illuminates the physical quantities that can be derived from historical drawings. Keywords Sunspots · Sunspot drawings · Sunspot positions Contents 1 Introduction ............................................... 2 Pre-telescopic observations ....................................... 2.1 Naked-eye observations: difficulties of interpretation ....................... 2.2 Evaluation of historical naked-eye observations of sunspots .................... 2.3 Observations using a camera obscura ................................ 3 Sunspot positions and areas from historical reports ........................... 3.1 Presence of orientation lines .................................... 3.2 Rotational matching ......................................... 3.3 Measurements rather than drawings ................................. 3.4 Not-to-scale areas .......................................... 4 The period before the Maunder minimum ................................ 4.1 Thomas Harriot (1560–1621) ................................... -
How to Make the Earth Orbit the Sun in 1614
HOW TO MAKE THE EARTH ORBIT THE SUN IN 1614 Originally submitted version of the paper published in the Journal for the History of Astronomy, Volume 50, number 1 (February 2019), posted to arXiv.org per SAGE Publishing’s Archiving and Sharing Policy (https://us.sagepub.com/en-us/nam/journal-author-archiving-policies-and-re-use) Christopher M. Graney Jefferson Community & Technical College 1000 Community College Drive Louisville, Kentucky 40272 (USA) [email protected] ABSTRACT In 1614 Johann Georg Locher, a student of the Jesuit astronomer Christoph Scheiner, proposed a physical mechanism to explain how the Earth could orbit the sun. An orbit, Locher said, is a perpetual fall. He proposed this despite the fact that he rejected the Copernican system, citing problems with falling bodies and the sizes of stars under that system. In 1651 and again in 1680, Jesuit writers Giovanni Battista Riccioli and Athanasius Kircher, respectively, considered and rejected outright Locher’s idea of an orbit as a perpetual fall. Thus this important concept of an orbit was proposed, considered, and rejected well before Isaac Newton would use an entirely different physics to make the idea that an orbit is a perpetual fall the common way of envisioning and explaining orbits. KEY WORDS: orbit, gravity, Locher, Scheiner, Riccioli, Kircher, Newton, Jesuit In the second decade of the seventeenth century, well before the birth of Isaac Newton, a student of a German Jesuit astronomer proposed a physical mechanism to explain how the Earth could orbit the sun: Earth could be likened, said this student, to a massive ball, perpetually falling toward the sun. -
The Reception of the Copernican Revolution Among Provençal Humanists of the Sixteenth and Seventeenth Centuries*
The Reception of the Copernican Revolution Among Provençal Humanists of the Sixteenth and Seventeenth Centuries* Jean-Pierre Luminet Laboratoire d'Astrophysique de Marseille (LAM) CNRS-UMR 7326 & Centre de Physique Théorique de Marseille (CPT) CNRS-UMR 7332 & Observatoire de Paris (LUTH) CNRS-UMR 8102 France E-mail: [email protected] Abstract We discuss the reception of Copernican astronomy by the Provençal humanists of the XVIth- XVIIth centuries, beginning with Michel de Montaigne who was the first to recognize the potential scientific and philosophical revolution represented by heliocentrism. Then we describe how, after Kepler’s Astronomia Nova of 1609 and the first telescopic observations by Galileo, it was in the south of France that the New Astronomy found its main promotors with humanists and « amateurs écairés », Nicolas-Claude Fabri de Peiresc and Pierre Gassendi. The professional astronomer Jean-Dominique Cassini, also from Provence, would later elevate the field to new heights in Paris. Introduction In the first book I set forth the entire distribution of the spheres together with the motions which I attribute to the earth, so that this book contains, as it were, the general structure of the universe. —Nicolaus Copernicus, Preface to Pope Paul III, On the Revolution of the Heavenly Spheres, 1543.1 Written over the course of many years by the Polish Catholic canon Nicolaus Copernicus (1473–1543) and published following his death, De revolutionibus orbium cœlestium (On the Revolutions of the Heavenly Spheres) is regarded by historians as the origin of the modern vision of the universe.2 The radical new ideas presented by Copernicus in De revolutionibus * Extended version of the article "The Provençal Humanists and Copernicus" published in Inference, vol.2 issue 4 (2017), on line at http://inference-review.com/. -
Die Jesuitische Weltkarte : Johann Baptist Cysats Von 1619
Die jesuitische Weltkarte : Johann Baptist Cysats von 1619 Autor(en): Höhener, Hans-Peter Objekttyp: Article Zeitschrift: Cartographica Helvetica : Fachzeitschrift für Kartengeschichte Band (Jahr): - (2019) Heft 58: Missionskartographie PDF erstellt am: 09.10.2021 Persistenter Link: http://doi.org/10.5169/seals-842079 Nutzungsbedingungen Die ETH-Bibliothek ist Anbieterin der digitalisierten Zeitschriften. Sie besitzt keine Urheberrechte an den Inhalten der Zeitschriften. Die Rechte liegen in der Regel bei den Herausgebern. Die auf der Plattform e-periodica veröffentlichten Dokumente stehen für nicht-kommerzielle Zwecke in Lehre und Forschung sowie für die private Nutzung frei zur Verfügung. Einzelne Dateien oder Ausdrucke aus diesem Angebot können zusammen mit diesen Nutzungsbedingungen und den korrekten Herkunftsbezeichnungen weitergegeben werden. Das Veröffentlichen von Bildern in Print- und Online-Publikationen ist nur mit vorheriger Genehmigung der Rechteinhaber erlaubt. Die systematische Speicherung von Teilen des elektronischen Angebots auf anderen Servern bedarf ebenfalls des schriftlichen Einverständnisses der Rechteinhaber. Haftungsausschluss Alle Angaben erfolgen ohne Gewähr für Vollständigkeit oder Richtigkeit. Es wird keine Haftung übernommen für Schäden durch die Verwendung von Informationen aus diesem Online-Angebot oder durch das Fehlen von Informationen. Dies gilt auch für Inhalte Dritter, die über dieses Angebot zugänglich sind. Ein Dienst der ETH-Bibliothek ETH Zürich, Rämistrasse 101, 8092 Zürich, Schweiz, www.library.ethz.ch