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Edmond Halley and His Recurring Comet
EDMOND HALLEY AND HIS RECURRING COMET “They [the astronomers of the flying island of Laputa] have observed ninety-three different comets and settled their periods with great exactness. If this be true (and they affirm it with great confidence), it is much to be wished that their observations were made public, whereby the theory of comets, which at present is very lame and defective, might be brought into perfection with other parts of astronomy.” — Jonathan Swift, GULLIVER’S TRAVELS, 1726 HDT WHAT? INDEX HALLEY’S COMET EDMOND HALLEY 1656 November 8, Saturday (Old Style): Edmond Halley was born. NEVER READ AHEAD! TO APPRECIATE NOVEMBER 8TH, 1656 AT ALL ONE MUST APPRECIATE IT AS A TODAY (THE FOLLOWING DAY, TOMORROW, IS BUT A PORTION OF THE UNREALIZED FUTURE AND IFFY AT BEST). Edmond Halley “Stack of the Artist of Kouroo” Project HDT WHAT? INDEX HALLEY’S COMET EDMOND HALLEY 1671 February 2, Friday (1671, Old Style): Harvard College was given a “3 foote and a halfe with a concave ey-glasse” reflecting telescope. This would be the instrument with which the Reverends Increase and Cotton Mather would observe a bright comet of the year 1682. ASTRONOMY HALLEY’S COMET HARVARD OBSERVATORY ESSENCE IS BLUR. SPECIFICITY, THE OPPOSITE OF ESSENCE, IS OF THE NATURE OF TRUTH. Edmond Halley “Stack of the Artist of Kouroo” Project HDT WHAT? INDEX HALLEY’S COMET EDMOND HALLEY 1676 Edmond Halley was for six weeks the guest of the British East India Company at their St. Helena colony in the South Atlantic for purposes of observation of the exceedingly rare transit of the planet Venus across the face of the sun. -
Modelling and the Transit of Venus
Modelling and the transit of Venus Dave Quinn University of Queensland <[email protected]> Ron Berry University of Queensland <[email protected]> Introduction enior secondary mathematics students could justifiably question the rele- Svance of subject matter they are being required to understand. One response to this is to place the learning experience within a context that clearly demonstrates a non-trivial application of the material, and which thereby provides a definite purpose for the mathematical tools under consid- eration. This neatly complements a requirement of mathematics syllabi (for example, Queensland Board of Senior Secondary School Studies, 2001), which are placing increasing emphasis on the ability of students to apply mathematical thinking to the task of modelling real situations. Success in this endeavour requires that a process for developing a mathematical model be taught explicitly (Galbraith & Clatworthy, 1991), and that sufficient opportu- nities are provided to students to engage them in that process so that when they are confronted by an apparently complex situation they have the think- ing and operational skills, as well as the disposition, to enable them to proceed. The modelling process can be seen as an iterative sequence of stages (not ) necessarily distinctly delineated) that convert a physical situation into a math- 1 ( ematical formulation that allows relationships to be defined, variables to be 0 2 l manipulated, and results to be obtained, which can then be interpreted and a n r verified as to their accuracy (Galbraith & Clatworthy, 1991; Mason & Davis, u o J 1991). The process is iterative because often, at this point, limitations, inac- s c i t curacies and/or invalid assumptions are identified which necessitate a m refinement of the model, or perhaps even a reassessment of the question for e h t which we are seeking an answer. -
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. -
Transit of Venus Presentation
http://sunearthday.nasa.gov/2012/transit/webcast.php Venus visible Venus with the unaided eye: "morning star" or the Earth "evening star. • Similar to Earth: – diameter: 12,103 km – 0.95 Earth’s – mass 0.89 of Earth's – few craters -- young surface – densities, chemical compositions are similar • rotation unusually slow (Venus day = 243 Earth days -- longer than Venus' year) • rotation retrograde • periods of Venus' rotation and of its orbit are synchronized -- always same face toward Earth when the two planets are at their closest approach • greenhouse effect -- surface temperature hot enough to melt lead M ikhail Lomonosov, june 5, 1761 discovered, during a transit, that V enus has an atmosphere The atmosphere is is composed mostly of carbon dioxide. There are several layers of clouds, many kilometers thick, composed of sulfuric acid. Mariner 10 Image of Venus V enera 13 Venus’ orbit is inclined (by 3.39 degrees) relative to the ecliptic If in the same plane we would have 5 transits in 8 years Venus: 13 years , Earth: 8 years Each time Earth completes 1.6 orbits, Venus catches up to it after 2.6 of its orbits Progress of the 2004 Transit of Venus pictured from NASA's Soho solar observatory. Credit: NASA Ascending (A) or Duration since last transit Date of transit Descending (D) node (years and months) 6 December 1631 A 4 December 1639 A 8 yrs 6 June 1761 D 121 yrs 6 months 3 June 1769 D 8 yrs 9 December 1874 A 105 yrs 6 months 6 December 1882 A 8 yrs 8 June 2004 D 121 yrs 6 months 5 June 2012 D 8 yrs 11 December 2117 A 105 yrs 6 months 8 December 2125 A 8 yrs In 6000 years 81 transits only Venus’ Role in History Copernican System vs Ptolemaic System http://astro.unl.edu/classaction/animations/renaissance/venusphases.html Venus’ Role in History Size of the Solar System - Revealed! • Kepler predicted the transit of December 1631 (though not observed!) and 120 year cycle. -
History of Science Society Annual Meeting San Diego, California 15-18 November 2012
History of Science Society Annual Meeting San Diego, California 15-18 November 2012 Session Abstracts Alphabetized by Session Title. Abstracts only available for organized sessions. Agricultural Sciences in Modern East Asia Abstract: Agriculture has more significance than the production of capital along. The cultivation of rice by men and the weaving of silk by women have been long regarded as the two foundational pillars of the civilization. However, agricultural activities in East Asia, having been built around such iconic relationships, came under great questioning and processes of negation during the nineteenth and twentieth centuries as people began to embrace Western science and technology in order to survive. And yet, amongst many sub-disciplines of science and technology, a particular vein of agricultural science emerged out of technological and scientific practices of agriculture in ways that were integral to East Asian governance and political economy. What did it mean for indigenous people to learn and practice new agricultural sciences in their respective contexts? With this border-crossing theme, this panel seeks to identify and question the commonalities and differences in the political complication of agricultural sciences in modern East Asia. Lavelle’s paper explores that agricultural experimentation practiced by Qing agrarian scholars circulated new ideas to wider audience, regardless of literacy. Onaga’s paper traces Japanese sericultural scientists who adapted hybridization science to the Japanese context at the turn of the twentieth century. Lee’s paper investigates Chinese agricultural scientists’ efforts to deal with the question of rice quality in the 1930s. American Motherhood at the Intersection of Nature and Science, 1945-1975 Abstract: This panel explores how scientific and popular ideas about “the natural” and motherhood have impacted the construction and experience of maternal identities and practices in 20th century America. -
The Earth Observer. July
National Aeronautics and Space Administration The Earth Observer. July - August 2012. Volume 24, Issue 4. Editor’s Corner Steve Platnick obser ervth EOS Senior Project Scientist The joint NASA–U.S. Geological Survey (USGS) Landsat program celebrated a major milestone on July 23 with the 40th anniversary of the launch of the Landsat-1 mission—then known as the Earth Resources and Technology Satellite (ERTS). Landsat-1 was the first in a series of seven Landsat satellites launched to date. At least one Landsat satellite has been in operation at all times over the past four decades providing an uninter- rupted record of images of Earth’s land surface. This has allowed researchers to observe patterns of land use from space and also document how the land surface is changing with time. Numerous operational applications of Landsat data have also been developed, leading to improved management of resources and informed land use policy decisions. (The image montage at the bottom of this page shows six examples of how Landsat data has been used over the last four decades.) To commemorate the anniversary, NASA and the USGS helped organize and participated in several events on July 23. A press briefing was held over the lunch hour at the Newseum in Washington, DC, where presenta- tions included the results of a My American Landscape contest. Earlier this year NASA and the USGS sent out a press release asking Americans to describe landscape change that had impacted their lives and local areas. Of the many responses received, six were chosen for discussion at the press briefing with the changes depicted in time series or pairs of Landsat images. -
Venus Transit 5−6 June 2012 (From 22:00 to 4:56 UT) Australia, Japan, Norway
Venus Transit 5−6 June 2012 (from 22:00 to 4:56 UT) Australia, Japan, Norway Objective The main objective of the venus-2012.org project is the observation of the Venus Transit that will take place on 5th/6th June 2012 (see Fig. 1) from three locations: Australia, Japan and Norway. In particular the project will: 1) Perform live broadcasting of the event (sky-live.tv). 2) Promote educational activities usingFIGURE images 1 obtained during the transit (astroaula.net). Global Visibility of the Transit of Venus of 2012 June 05/06 Region X* Greatest Transit Transit at Zenith Transit Sunset Sunset Begins Ends at at IV I IV I Transit at at Entire Ends No Transit III II III II Sunrise in Progress Begins Transit Sunrise in Progress Transit at Sunset Visible Transit Visible at Sunrise Transit (June 05) (June 06) Region Y* F. Espenak, NASAs GSFC eclipse.gsfc.nasa.gov/OH/transit12.html * Region X - Beginning and end of Transit are visible, but the Sun sets for a short period around maximum transit. * Region Y - Beginning and end of Transit are NOT visible, but the Sun rises for a short period around maximum transit. Figure 1. Earth map showing visibility of the Venus transit in 2012 (credit F. Espenak, NASA/GSFC). The Phenomenon A transit of an astronomical object occurs when it appears to move across the disc of another object which has a larger apparent size. There are different types of transits, like the Galilean moons on Jupiter’s disc, and exoplanets moving across their mother star. -
Bibliography from ADS File: Gingerich.Bib June 27, 2021 1
Bibliography from ADS file: gingerich.bib Gingerich, O., “Year of astronomy: Mankind’s place in the Universe”, August 16, 2021 2009Natur.457...28G ADS Gingerich, O., “Book Review: Mikołaj Kopernik Dzieła Wszystkie, iii”, 2008JHA....39..416G ADS Gingerich, O., “The Role of Ephemerides from Ptolemy to Kepler”, Gingerich, O., “Not so amateur”, 2008Natur.453..156G ADS 2017ASSP...50...17G ADS Gingerich, O.: 2007a, Revisiting The Fitness of the Environment, 20 Gingerich, O., “Book Review: The Abridged Almagest”, 2007fcl..book...20G ADS 2016JHA....47..448G ADS Gingerich, O., “Publish or Perish: The Case of Thomas Harriot”, Gingerich, O.: 2016b, Copernicus: A Very Short Introduction 2007AAS...211.3401G ADS 2016cvsi.book.....G ADS Gingerich, O., “Quests of a theoretical astronomer”, 2007Natur.450..480G Gingerich, O., “Book Review: Longitude for the Coffee Table”, ADS 2016JHA....47..224G ADS Gingerich, O., “Book review: Heinrich Rantzau und die Astrologie / Disqui- Gingerich, O., “Letter: On Galileo and the Moon”, 2016JRASC.110...95G sitiones Historiae Scientiarum, Braunschweiger Beiträge zur Wissenschafts- ADS geschichte, Band 2; Braunschweig, 318 pp., 2004, ISBN 3-927939-65-X.”, Gingerich, O., “Book Review: Studien zur ”Sphaera’ des Johannes de Sacro- 2007JHA....38..510G ADS bosco”, 2015JHA....46..101G ADS Gingerich, O., “Gutenberg’s Gift”, 2007ASPC..377..319G ADS Pasachoff, J. M., Needham, P. S., Wright, E. T., & Gingerich, O., “Recreating Gingerich, O., “Book Review: le Conflit Entre L’astronomie Nouvelle et Galileo’s 1609 Discovery of Lunar Mountains”, -
Who Invented the Calculus? - and Other 17Th Century Topics Transcript
Who invented the calculus? - and other 17th century topics Transcript Date: Wednesday, 16 November 2005 - 12:00AM Location: Barnard's Inn Hall WHO INVENTED THE CALCULUS? Professor Robin Wilson Introduction We’ve now covered two-thirds of our journey ‘From Caliphs to Cambridge’, and in this lecture I want to try to survey the mathematical achievements of the seventeenth century – a monumental task. I’ve divided my talk into four parts – first, the movement towards the practical sciences, as exemplified by the founding of Gresham College and the Royal Society. Next, we’ll gravitate towards astronomy, from Copernicus to Newton. Thirdly, we visit France and the gradual movement from geometry to algebra (with a brief excursion into some new approaches to pi) – and finally, the development of the calculus. So first, let’s make an excursion to Gresham College. Practical science The Gresham professorships arose from the will of Sir Thomas Gresham, which provided for £50 per year for each of seven professors to read lectures in Divinity, Astronomy, Music, Geometry, Law, Physic and Rhetoric. As the Ballad of Gresham College later described it: If to be rich and to be learn’d Be every Nation’s cheifest glory, How much are English men concern’d, Gresham to celebrate thy story Who built th’Exchange t’enrich the Citty And a Colledge founded for the witty. From its beginning, Gresham College encouraged the practical sciences, rather than the Aristotelian studies still pursued at the ancient universities: Thy Colledg, Gresham, shall hereafter Be the whole world’s Universitie, Oxford and Cambridge are our laughter; Their learning is but Pedantry. -
The Icha Newsletter Newsletter of the Inter-Union Commission For
International Astronomical Union International Union of the History and Philosophy of Science DHS/IUHPS ______________________________________________________________________________________________________________________ THE ICHA NEWSLETTER NEWSLETTER OF THE INTER-UNION COMMISSION FOR HISTORY OF ASTRONOMY* ____________________________________________________________ __________________________________________________________ No. 12 – November 2011 SUMMARY A. C41/ICHA Programme at the 2012 Beijing IAU General Assembly by C. Ruggles ............................................................................................................ 2 B. 2012-2015 C41 Organizing Committee Elections by C. Ruggles ……...…… 3 C. Journals and Publications: - Acta Historica Astronomiae by H.W. Duerbeck ........................................ 4 Books 2011 …………………………………………………………………. 5 Some research papers by C41/ICHA members – 2011…… ........................... 5 D. News - Formation of Johannes Kepler Working Group by A. E. L. Davis ………. 5 - The Transit of Venus Working Group Activities by H. W. Duerbeck ….. 6 o Solar parallax Conference (Announcement) o Venus Transit Conference (Announcement) o Special Venus Transit issue of JAHH (Announcement) - Sullivan Papers Available by E. N. Bouton ..…………………………… 7 - History of astronomy in India by B. S. Shylaja …………….………….… 8 - 3 rd Conference on Cultural Astronomy by E. Badolati…………..………. 9 - Nexus International Conference on Architecture and Mathematics by G. Magli ……………………………………………………………………. 10 E. ICHA Member -
Transit of Venus M
National Aeronautics and Space Administration The Transit of Venus June 5/6, 2012 HD209458b (HST) The Transit of Venus June 5/6, 2012 Transit of Venus Mathof Venus Transit Top Row – Left image - Photo taken at the US Naval Math Puzzler 3 - The duration of the transit depends Observatory of the 1882 transit of Venus. Middle on the relative speeds between the fast-moving image - The cover of Harpers Weekly for 1882 Venus in its orbit and the slower-moving Earth in its showing children watching the transit of Venus. orbit. This speed difference is known to be 5.24 km/sec. If the June 5, 2012, transit lasts 24,000 Right image – Image from NASA's TRACE satellite seconds, during which time the planet moves an of the transit of Venus, June 8, 2004. angular distance of 0.17 degrees across the sun as Middle - Geometric sketches of the transit of Venus viewed from Earth, what distance between Earth and by James Ferguson on June 6, 1761 showing the Venus allows the distance traveled by Venus along its shift in the transit chords depending on the orbit to subtend the observed angle? observer's location on Earth. The parallax angle is related to the distance between Earth and Venus. Determining the Astronomical Unit Bottom – Left image - NOAA GOES-12 satellite x-ray image showing the Transit of Venus 2004. Middle Based on the calculations of Nicolas Copernicus and image – An observer of the 2004 transit of Venus Johannes Kepler, the distances of the known planets wearing NASA’s Sun-Earth Day solar glasses for from the sun could be given rather precisely in terms safe viewing. -
Photogenic Venus: the "Cinematographic Turn" and Its Alternatives in Nineteenth-Century France
Photogenic Venus: The "Cinematographic Turn" and Its Alternatives in Nineteenth-Century France The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Canales, Jimena. 2002. Photogenic Venus: The "cinematographic turn" and its alternatives in nineteenth-century France. Isis 93, no. 4: 585-613. Published Version http://dx.doi.org/10.1086/375953 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:3210601 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Photogenic Venus The “Cinematographic Turn” and Its Alternatives in Nineteenth-Century France By Jimena Canales* ABSTRACT During the late nineteenth century, scientists around the world disagreed as to the types of instruments and methods that should be used for determining the most important con- stant of celestial mechanics: the solar parallax. Venus’s 1874 transit across the sun was seen as the best opportunity for ending decades of debate. However, a mysterious “black drop” that appeared between Venus and the sun and individual differences in observations of the phenomenon brought traditional methods into disrepute. To combat these difficulties, the astronomer Jules Janssen devised a controversial new instrument, the “photographic revolver,” that photographed Venus at regular intervals. Another solution came from phys- icists, who rivaled the astronomers’ dominance in precision measurements by deducing the solar parallax from physical measurements of the speed of light.