Challenging the Paradigm: the Legacy of Galileo Symposium
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Galileo Galilei Introduction Galileo Galilei (1564–1642) Was One of The
Galileo Galilei Introduction Galileo Galilei (1564–1642) was one of the most significant figures of the Scientific Revolution. Galileo was involved in nearly all fields of natural philosophy, including astronomy, mathematics, and what we now term “physics.” He is rightly considered one of the founders of modern physics and astronomy, and one of the main originators of the modern scientific method. Galileo’s study of motion became the foundation for Newton’s laws of motion and the principles of inertia and gravity. His astronomical studies were instrumental in supporting the heliocentric model of the solar system first propounded by Copernicus. He should also be credited with making experimentation the basis of scientific study, and with the use of mathematics as the fundamental means for expressing and validating the findings of experimental investigation. Galileo’s application of mathematics to experimental results has become one of the most important aspects of modern science. Galileo made important improvements to the telescope, which enabled him to make great advances in astronomical observation. His observations emboldened him to become the most important advocate of Copernicanism—the astronomical system created by Nicolaus Copernicus (1473–1543)—and his support ultimately ushered in the Copernican revolution in astronomy. Copernicus had devised a heliocentric model in which he posited that the Earth revolved around the sun (in perfect circles). Contrary to the Ptolemaic system and Christian cosmology, Copernicus positioned the sun as a fixed center around which Mercury, Venus, Earth, Mars, Jupiter, and Saturn orbited. Furthermore, Copernicus posited the diurnal rotation of the Earth on its own axis in addition to its annual revolutions around the sun. -
The Spectrumspectrum the Calendar 2 Membership Corner 3 the Newsletter for the Buffalo Astronomical a Letter from Mike 4
Inside this issue: TheThe SpectrumSpectrum The Calendar 2 Membership Corner 3 The Newsletter for the Buffalo Astronomical A Letter from Mike 4 Obs Report 5 The Banquet 6 Stay Warm and 9 Cozy Astro Day Poster 11 March/April The Galileo Affair 12 Volume 17, Issue 2 Gallery 18 May Star Chart 19 March Star Chart 19 April Star Chart 20 Our Newly Redesigned Website is Live! If you haven’t checked out BuffaloAstronomy.com recently, it’s time for a visit. Our new site, designed by webmaster and club member Gene Timothy is up and running. The interface is clean and organized and much easier to update with club news and astronomy content. You can now register for the April Banquet, join the club and pay dues using a PayPal account or a major credit card. Coming soon is a new log-in area which will allow members to communicate with each other, share a profile and access special features, including BAA historical information and an archive of Spectrum issues dating back many decades. Come visit and share your comments, thoughts and ideas on how we can make the site better and more useful to the club. A BIG thank you to Gene and the BAA Board for their hard work and creativity! 1 BAA Schedule of Astronomy Fun for 2015 BAA Schedule of Astronomy Fun for 2015 Mar 13: BAA Meeting at 7:30pm at Buffalo State College Mar 20: New Moon Mar 20: Total Solar Eclipse (Arctic) Mar 21-22: Maple Syrup Festival at BMO 9am-3pm Need help for Solar viewing Mar 21: Messier Marathon Dusk till Dawn at Beaver Meadow Observatory Apr 4: First Public Night at Beaver Meadow Observatory April 4: Total Lunar Eclipse Apr 11: BAA Annual Dinner Meeting at Risottos April 18; New Moon Apr 18/19: NEAF who wants to car pool?? April 21-22: Lyrids Meteor Shower Apr 25: Astronomy Day at Buffalo Museum of Science details TBA May 2: Public Night BMO May 8: BAA Meeting at 7:30pm at Buffalo State College May 18: New Moon Jun 6: Public Night BMO Jun 12: BAA Meeting/Elections at 7:30pm at Buffalo State College Jun 17 New Moon July 4: Public Night BMO – I will need help as I have family obligations that day. -
JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
The Jesuits and the Galileo Affair Author(S): Nicholas Overgaard Source: Prandium - the Journal of Historical Studies, Vol
Early Modern Catholic Defense of Copernicanism: The Jesuits and the Galileo Affair Author(s): Nicholas Overgaard Source: Prandium - The Journal of Historical Studies, Vol. 2, No. 1 (Spring, 2013), pp. 29-36 Published by: The Department of Historical Studies, University of Toronto Mississauga Stable URL: http://jps.library.utoronto.ca/index.php/prandium/article/view/19654 Prandium: The Journal of Historical Studies Vol. 2, No. 1, (2013) Early Modern Catholic Defense of Copernicanism: The Jesuits and the Galileo Affair Nicholas Overgaard “Obedience should be blind and prompt,” Ignatius of Loyola reminded his Jesuit brothers a decade after their founding in 1540.1 By the turn of the seventeenth century, the incumbent Superior General Claudio Aquaviva had reiterated Loyola’s expectation of “blind obedience,” with specific regard to Jesuit support for the Catholic Church during the Galileo Affair.2 Interpreting the relationship between the Jesuits and Copernicans like Galileo Galilei through the frame of “blind obedience” reaffirms the conservative image of the Catholic Church – to which the Jesuits owed such obedience – as committed to its medieval traditions. In opposition to this perspective, I will argue that the Jesuits involved in the Galileo Affair3 represent the progressive ideas of the Church in the early seventeenth century. To prove this, I will argue that although the Jesuits rejected the epistemological claims of Copernicanism, they found it beneficial in its practical applications. The desire to solidify their status as the intellectual elites of the Church caused the Jesuits to reject Copernicanism in public. However, they promoted an intellectual environment in which Copernican studies – particularly those of Galileo – could develop with minimal opposition, theological or otherwise. -
Galileo and Bellarmine
The Inspiration of Astronomical Phenomena VI ASP Conference Series, Vol. 441 Enrico Maria Corsini, ed. c 2011 Astronomical Society of the Pacific Galileo and Bellarmine George V. Coyne, S.J. Vatican Observatory, Vatican City State Abstract. This paper aims to delineate two of the many tensions which bring to light the contrasting views of Galileo Galilei and of Cardinal Robert Bellarmine with respect to the Copernican-Ptolemaic controversies of the 16th and 17th centuries: their respective positions on Aristotle’s natural philosophy and on the interpretation of Sa- cred Scripture. Galileo’s telescopic observations, reported in his Sidereus Nuncius, were bringing about the collapse of Aristotle’s natural philosophy and he taught that there was no science in Scripture. 1. Introduction This paper investigates the tensions between two of the principal protagonists in the controversies involved in the birth of modern science, Galileo Galilei and Cardinal Robert Bellarmine, and how they were resolved or not in a spirit of accommodation. Bellarmine’s fellow Jesuits at the Roman College confirmed Galileo’s Earth-shaking observations, reported in his Sidereus Nuncius. Aristotle’s physics was crumbling. Would Aristotelian philosophy, which was at the service of theology, also collapse? Controversies over the nature of sunspots and of comets seemed to hold implications for the very foundations of Christian belief. Some Churchmen saw the threat and faced it with an astute view into the future; others, though pioneers as scientists, could not face the larger implications of the scientific revolution to which they with Galileo con- tributed. Much of what occurred can be attributed to the strong personalities of the individual antagonists and Bellarmine will prove to be one of the most important of those personages. -
Galileo's Assayer
University of Nevada, Reno Galileo's Assayer: Sense and Reason in the Epistemic Balance A thesis submitted in partial fulfillment of the requirements for the degree of Master of Arts in History. by James A Smith Dr. Bruce Moran/Thesis Advisor May 2018 c by James A Smith 2018 All Rights Reserved THE GRADUATE SCHOOL We recommend that the thesis prepared under our supervision by JAMES A. SMITH entitled Galileo's Assayer: Sense and Reason in the Epistemic Balance be accepted in partial fulfillment of the requirements for the degree of MASTER OF ARTS Bruce Moran, Ph.D., Advisor Edward Schoolman, Ph.D., Committee Member Carlos Mariscal, Ph.D., Committee Member Stanislav Jabuka, Ph.D., Graduate School Representative David W. Zeh, Ph.D., Dean, Graduate School May, 2018 i Abstract Galileo's The Assayer, published in 1623, represents a turning point in Galileo's philo- sophical work. A highly polemical \scientific manifesto," The Assayer was written after his astronomical discoveries of the moons of Jupiter and sunspots on a rotating sun, but before his mature Copernican work on the chief world systems (Ptolemaic versus Copernican). The Assayer included major claims regarding the place of math- ematics in natural philosophy and how the objects of the world and their properties can be known. It's in The Assayer that Galileo wades into the discussion about the ultimate constituents of matter and light, namely, unobservable particles and atoms. Galileo stressed the equal roles that the senses and reason served in the discovery of knowledge, in contradistinction to Aristotelian authoritarian dogma that he found to hinder the processes of discovery and knowledge acquisition. -
Article De Fond, Réalisation
ARTICLE DE FOND, RÉA LISATION QUATOR PLANETIS CIRCUM IOVIS : MEDICEA SIDERA Pierre Le Fur (MPSI, Institut Supérieur d'Électronique et du Numérique Toulon, formateur académique en astronomie –Nice) Résumé : Suivons les traces de Galilée en étudiant ses observations sur les quatre satellites médicéens de Jupiter telles qu’elles furent décrites dans le "sidereus nuncius". Nous montrerons qu’à partir de ces relevés on peut retrouver certaines lois ignorées du savant Toscan. Enfin nous proposerons la construction d’un "Jovilab" qualitatif, sorte de tables d’éphémérides de positions de ces quatre satellites. Si, en l’an de grâce 2009, nous souhaitons fêter quasi impossible à déterminer, aurait été dignement l’Année Mondiale de l’Astronomie, immédiate par simple différence entre l’heure la lecture de " sidereus nuncius ", œuvre solaire locale et cette "heure universelle jo- étincelante de Galileo Galilei, s’impose à nous. vienne"; cela aurait constitué une deuxième Elle constitue l’allumette déclenchant l’incendie révolution, moins intellectuelle mais économi- qui embrasa la physique aristotélicienne et ses quement et militairement exceptionnelle. partisans religieux. Les observations récoltées par Galilée pendant Cette œuvre peut être facilement consultée sur les années qui suivirent la publication de le site de l’Université de Strasbourg à "sidereus nuncius " lui permettront d’obtenir un l’adresse [10]. La force et la simplicité de cet outil de prévisions de la position de ces ouvrage apparaît d’emblée, même si l’on ignore satellites : le Jovilab. tout du latin… Les gravures intégrées au texte Je vous propose de suivre les traces de Galilée ; nous suggèrent autant le contenu des d’examiner ses observations médicéennes ; de découvertes décrites par Galilée que le génie de montrer comment on peut retrouver certaines son interprétation. -
Galilei-1632 Dialogue Concerning the Two Chief World Systems
Galileo di Vincenzo Bonaulti de Galilei ([ɡaliˈlɛːo ɡaliˈlɛi]; 15 February 1564 – 8 January 1642) was an Italian astronomer, physicist and engineer, sometimes described as a polymath, from Pisa. Galileo has been called the "father of observational astronomy", the "father of modern physics", the "father of the scientific method", and the "father of modern science". Galileo studied speed and velocity, gravity and free fall, the principle of relativity, inertia, projectile motion and also worked in applied science and technology, describing the properties of pendulums and "hydrostatic balances", inventing the thermoscope and various military compasses, and using the telescope for scientific observations of celestial objects. His contributions to observational astronomy include the telescopic confirmation of the phases of Venus, the observation of the four largest satellites of Jupiter, the observation of Saturn's rings, and the analysis of sunspots. Galileo's championing of heliocentrism and Copernicanism was controversial during his lifetime, when most subscribed to geocentric models such as the Tychonic system. He met with opposition from astronomers, who doubted heliocentrism because of the absence of an observed stellar parallax. The matter was investigated by the Roman Inquisition in 1615, which concluded that heliocentrism was "foolish and absurd in philosophy, and formally heretical since it explicitly contradicts in many places the sense of Holy Scripture". Galileo later defended his views in Dialogue Concerning the Two Chief World Systems (1632), which appeared to attack Pope Urban VIII and thus alienated him and the Jesuits, who had both supported Galileo up until this point. He was tried by the Inquisition, found "vehemently suspect of heresy", and forced to recant. -
Mars Reconnaissance Orbiter and Opportunity Observations Of
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Mars Reconnaissance Orbiter and Opportunity 10.1002/2014JE004686 observations of the Burns formation: Crater Key Point: hopping at Meridiani Planum • Hydrated Mg and Ca sulfate Burns formation minerals mapped with MRO R. E. Arvidson1, J. F. Bell III2, J. G. Catalano1, B. C. Clark3, V. K. Fox1, R. Gellert4, J. P. Grotzinger5, and MER data E. A. Guinness1, K. E. Herkenhoff6, A. H. Knoll7, M. G. A. Lapotre5, S. M. McLennan8, D. W. Ming9, R. V. Morris9, S. L. Murchie10, K. E. Powell1, M. D. Smith11, S. W. Squyres12, M. J. Wolff3, and J. J. Wray13 1 2 Correspondence to: Department of Earth and Planetary Sciences, Washington University in Saint Louis, Missouri, USA, School of Earth and Space R. E. Arvidson, Exploration, Arizona State University, Tempe, Arizona, USA, 3Space Science Institute, Boulder, Colorado, USA, 4Department of [email protected] Physics, University of Guelph, Guelph, Ontario, Canada, 5Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 6U.S. Geological Survey, Astrogeology Science Center, Flagstaff, Arizona, USA, 7 8 Citation: Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts, USA, Department Arvidson, R. E., et al. (2015), Mars of Geosciences, Stony Brook University, Stony Brook, New York, USA, 9NASA Johnson Space Center, Houston, Texas, USA, Reconnaissance Orbiter and Opportunity 10Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA, 11NASA Goddard Space Flight Center, observations of the Burns formation: Greenbelt, Maryland, USA, 12Department of Astronomy, Cornell University, Ithaca, New York, USA, 13School of Earth and Crater hopping at Meridiani Planum, J. -
PDF Program Book
46th Meeting of the Division for Planetary Sciences with Historical Astronomy Division (HAD) 9-14 November 2014 | Tucson, AZ OFFICERS AND MEMBERS ........ 2 SPONSORS ............................... 2 EXHIBITORS .............................. 3 FLOOR PLANS ........................... 5 ATTENDEE SERVICES ................. 8 Session Numbering Key SCHEDULE AT-A-GLANCE ........ 10 100s Monday 200s Tuesday SUNDAY ................................. 20 300s Wednesday 400s Thursday MONDAY ................................ 23 500s Friday TUESDAY ................................ 44 Sessions are numbered in the program book by day and time. WEDNESDAY .......................... 75 All posters will be on display Monday - Friday THURSDAY.............................. 85 FRIDAY ................................. 119 Changes after 1 October are included only in the online program materials. AUTHORS INDEX .................. 137 1 DPS OFFICERS AND MEMBERS Current DPS Officers Heidi Hammel Chair Bonnie Buratti Vice-Chair Athena Coustenis Secretary Andrew Rivkin Treasurer Nick Schneider Education and Public Outreach Officer Vishnu Reddy Press Officer Current DPS Committee Members Rosaly Lopes Term Expires November 2014 Robert Pappalardo Term Expires November 2014 Ralph McNutt Term Expires November 2014 Ross Beyer Term Expires November 2015 Paul Withers Term Expires November 2015 Julie Castillo-Rogez Term Expires October 2016 Jani Radebaugh Term Expires October 2016 SPONSORS 2 EXHIBITORS Platinum Exhibitor Silver Exhibitors 3 EXHIBIT BOOTH ASSIGNMENTS 206 Applied -
Testable Hypotheses for Opportunity's Traverse
42nd Lunar and Planetary Science Conference (2011) 2199.pdf TESTABLE HYPOTHESES FOR OPPORTUNITY’S TRAVERSE FROM SANTA MARIA TO THE RIM OF ENDEAVOUR CRATER. A. A. Fraeman1, R. E. Arvidson1, S. L. Murchie2, F. P. Seelos2, and J. A. McGo- vern2, 1Washington University in St. Louis, Dept. of Earth and Planetary Science, St. Louis, MO (afrae- [email protected]), 2Johns Hopkins University Applied Physics Laboratory, Laurel, MD Introduction: As of January 2011, the Mars rover Botany Bay and the southern tip of Cape York: Opportunity was located at Santa Maria crater, ~6 km In contrast to the plains, CRISM normal [1] and over- away from the closest rim segment of the ~20 km di- sampled FRT data show signatures of hydrated phases, ameter Noachian-aged impact crater Endeavour (Fig. including hydrated sulfates, present throughout Botany 1). Endeavour predates the sedimentary rocks ex- Bay and the southern point of Cape York (Fig. 3). amined by Opportunity for the past 7 years, and Com- These phases have not been detected from orbit at any pact Reconnaissance Imaging Spectrometer for Mars other location along Opportunity’s ~26km traverse (CRISM) data indicate that Fe-Mg smectites are (with the exception of a small group of CRISM pixels present on the rim of this highly degraded crater [1]. on the SE rim of Santa Maria crater [3]), and suggests The purpose of this abstract is to present working a change in mineralogy occurs, probably at a strati- hypotheses to help guide the acquisition and analysis of graphic contact within Botany Bay. Opportunity’s continued Mars Reconnaissance Orbiter (MRO) cover- ground-truth observations will be essential in determin- age and Opportunity observations as the rover departs ing the nature of these phases as the rover approaches Santa Maria, traverses across the plains, and ascends Cape York, the closest rim segment. -
High-Resolution Mosaics of the Galilean Satellites from Galileo SSI
Lunar and Planetary Science XXIX 1833.pdf High-Resolution Mosaics of the Galilean Satellites from Galileo SSI. M. Milazzo, A. McEwen, C. B. Phillips, N. Dieter, J. Plassmann. Planetary Image Research Laboratory, LPL, University of Arizona, Tucson, AZ 85721; [email protected] The Galileo Spacecraft began mapping the Jovian orthographic projection centered at the latitude and system in June 1996. Twelve orbits of Jupiter and more longitude coordinates of the sub-spacecraft point to than 1000 images later, the Solid State Imager (SSI) is still preserve their perspective. Depending on the photometric collecting images, most far superior in resolution to geometry and scale, it may be necessary to apply a anything collected by the Voyager spacecraft. The data photometric normalization to the images. Next, the collected includes: low to medium resolution color data, individual frames are mosaicked together, and mosaicked medium resolution data to fill gaps in Voyager coverage, and onto a portion of the base map for regional context. Once very high-resolution data over selected areas. We have the mosaic is finished, it is checked to make sure that the tie been systematically processing the SSI images of the and match points were correct, and that the frames mesh. Galilean satellites to produce high-resolution mosaics and to We produce 3 final products: (i) an SSI-only mosaic, (ii) SSI place them into the regional context provided by medium- images mosaicked onto regional context, and (iii) the resolution mosaics from Voyager and/or Galileo. addition of a latitude-longitude grid to the context mosaic. Production of medium-resolution global mosaics is The purpose of this poster is to show the mosa- described in a companion abstract [1].