DOCSLIB.ORG

Transits of Mercury, 1605–2999 CE

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Transits of Mercury, 1605–2999 CE Appendix A Transits of Mercury, 1605–2999 CE Date (TT) Int. Offset Date (TT) Int. Offset Date (TT) Int. Offset 1605 Nov 01.84 7.0 −0.884 2065 Nov 11.84 3.5 +0.187 2542 May 17.36 9.5 −0.716 1615 May 03.42 9.5 +0.493 2078 Nov 14.57 13.0 +0.695 2545 Nov 18.57 3.5 +0.331 1618 Nov 04.57 3.5 −0.364 2085 Nov 07.57 7.0 −0.742 2558 Nov 21.31 13.0 +0.841 1628 May 05.73 9.5 −0.601 2095 May 08.88 9.5 +0.326 2565 Nov 14.31 7.0 −0.599 1631 Nov 07.31 3.5 +0.150 2098 Nov 10.31 3.5 −0.222 2575 May 15.34 9.5 +0.157 1644 Nov 09.04 13.0 +0.661 2108 May 12.18 9.5 −0.763 2578 Nov 17.04 3.5 −0.078 1651 Nov 03.04 7.0 −0.774 2111 Nov 14.04 3.5 +0.292 2588 May 17.64 9.5 −0.932 1661 May 03.70 9.5 +0.277 2124 Nov 15.77 13.0 +0.803 2591 Nov 19.77 3.5 +0.438 1664 Nov 04.77 3.5 −0.258 2131 Nov 09.77 7.0 −0.634 2604 Nov 22.51 13.0 +0.947 1674 May 07.01 9.5 −0.816 2141 May 10.16 9.5 +0.114 2608 May 13.34 3.5 +1.010 1677 Nov 07.51 3.5 +0.256 2144 Nov 11.50 3.5 −0.116 2611 Nov 16.50 3.5 −0.490 1690 Nov 10.24 13.0 +0.765 2154 May 13.46 9.5 −0.979 2621 May 16.62 9.5 −0.055 1697 Nov 03.24 7.0 −0.668 2157 Nov 14.24 3.5 +0.399 2624 Nov 18.24 3.5 +0.030 1707 May 05.98 9.5 +0.067 2170 Nov 16.97 13.0 +0.907 2637 Nov 20.97 13.0 +0.543 1710 Nov 06.97 3.5 −0.150 2174 May 08.15 3.5 +0.972 2644 Nov 13.96 7.0 −0.906 1723 Nov 09.71 13.0 +0.361 2177 Nov 09.97 3.5 −0.526 2654 May 14.61 9.5 +0.805 1736 Nov 11.44 13.0 +0.869 2187 May 11.44 9.5 −0.101 2657 Nov 16.70 3.5 −0.381 1740 May 02.96 3.5 +0.934 2190 Nov 12.70 3.5 −0.009 2667 May 17.89 9.5 −0.265 1743 Nov 05.44 3.5 −0.560 2203 Nov 16.44 13.0 +0.504 2670 Nov 19.44 3.5 +0.137 1753 May 06.26 9.5 −0.146 2210 Nov 09.43 7.0 −0.942 2683 Nov 22.17 13.0 +0.650 1756 Nov 07.17 3.5 −0.044 2220 May 09.42 9.5 +0.766 2690 Nov 15.16 7.0 −0.796 1769 Nov 09.91 13.0 +0.468 2223 Nov 12.17 3.5 −0.420 2700 May 15.89 9.5 +0.593 1776 Nov 02.90 7.0 −0.975 2233 May 12.71 9.5 −0.311 2703 Nov 18.90 3.5 −0.274 1782 Nov 12.64 6.0 +0.974 2236 Nov 13.90 3.5 +0.098 2713 May 19.17 9.5 −0.478 1786 May 04.24 3.5 +0.724 2249 Nov 16.64 13.0 +0.610 2716 Nov 20.64 3.5 +0.245 1789 Nov 05.64 3.5 −0.454 2256 Nov 09.63 7.0 −0.834 2729 Nov 23.37 13.0 +0.756 1799 May 07.54 9.5 −0.357 2266 May 10.70 9.5 +0.557 2736 Nov 16.36 7.0 −0.688 (continued) © Springer-Verlag New York 2015 627 J. Westfall, W. Sheehan, Celestial Shadows, Astrophysics and Space Science Library 410, DOI 10.1007/978-1-4939-1535-4 628 Appendix A: Transits of Mercury, 1605–2999 CE (continued) Date (TT) Int. Offset Date (TT) Int. Offset Date (TT) Int. Offset 1802 Nov 09.37 3.5 +0.063 2269 Nov 12.37 3.5 −0.312 2746 May 17.16 9.5 +0.386 1815 Nov 12.11 13.0 +0.573 2279 May 13.99 9.5 −0.525 2749 Nov 19.10 3.5 −0.165 1822 Nov 05.10 7.0 −0.866 2282 Nov 15.11 3.5 +0.204 2759 May 20.45 9.5 −0.693 1832 May 05.52 9.5 +0.510 2295 Nov 17.84 13.0 +0.716 2762 Nov 21.84 3.5 +0.352 1835 Nov 07.84 3.5 −0.347 2302 Nov 11.83 7.0 −0.725 2775 Nov 24.57 13.0 +0.862 1845 May 08.82 9.5 −0.576 2312 May 11.97 9.5 +0.348 2782 Nov 17.56 7.0 −0.575 1848 Nov 09.58 3.5 +0.168 2315 Nov 14.57 3.5 −0.206 2792 May 17.44 9.5 +0.174 1861 Nov 12.31 13.0 +0.678 2325 May 15.27 9.5 −0.738 2795 Nov 20.30 3.5 −0.058 1868 Nov 05.30 7.0 −0.759 2328 Nov 16.31 3.5 +0.311 2805 May 20.73 9.5 −0.907 1878 May 06.79 9.5 +0.302 2341 Nov 19.04 13.0 +0.822 2808 Nov 22.04 3.5 +0.458 1881 Nov 08.04 3.5 −0.239 2348 Nov 12.03 7.0 −0.616 2815 Nov 16.02 7.0 −0.998 1891 May 10.10 9.5 −0.793 2358 May 13.25 9.5 +0.136 2821 Nov 24.77 6.0 +0.968 1894 Nov 10.77 3.5 +0.275 2361 Nov 14.77 3.5 −0.097 2828 Nov 17.77 7.0 −0.471 1907 Nov 14.15 13.0 +0.782 2371 May 16.55 9.5 −0.954 2838 May 18.71 9.5 −0.033 1914 Nov 07.50 7.0 −0.651 2374 Nov 17.51 3.5 +0.417 2841 Nov 20.50 3.5 +0.049 1924 May 08.07 9.5 +0.089 2387 Nov 20.24 13.0 +0.926 2854 Nov 23.24 13.0 +0.564 1927 Nov 10.24 3.5 −0.133 2391 May 11.44 3.5 +0.991 2861 Nov 16.22 7.0 −0.887 1937 May 11.38 9.5 −1.006 2394 Nov 13.23 3.5 −0.508 2871 May 16.71 9.5 +0.818 1940 Nov 11.97 3.5 +0.380 2404 May 13.52 9.5 −0.075 2874 Nov 18.97 3.5 −0.363 1953 Nov 14.70 13.0 +0.888 2407 Nov 15.97 3.5 +0.011 2884 May 18.99 9.5 −0.246 1957 May 06.05 3.5 +0.954 2420 Nov 17.71 13.0 +0.525 2887 Nov 21.70 3.5 +0.156 1960 Nov 07.70 3.5 −0.545 2427 Nov 11.69 7.0 −0.925 2900 Nov 24.44 13.0 +0.671 1970 May 09.35 9.5 −0.120 2437 May 11.52 9.5 +0.782 2907 Nov 18.43 7.0 −0.778 1973 Nov 10.44 3.5 −0.027 2440 Nov 13.43 3.5 −0.401 2917 May 17.98 9.5 +0.615 1986 Nov 13.17 13.0 +0.485 2450 May 14.80 9.5 −0.290 2920 Nov 20.17 3.5 −0.254 1993 Nov 06.17 7.0 −0.957 2453 Nov 1617 3.5 +0.118 2930 May 21.26 9.5 −0.456 1999 Nov 15.90 6.0 +0.992 2466 Nov 1891 13.0 +0.631 2933 Nov 22.90 3.5 +0.264 2003 May 07.33 3.5 +0.745 2473 Nov 11.90 7.0 −0.816 2946 Nov 25.64 13.0 +0.777 2006 Nov 08.90 3.5 −0.437 2483 May 12.79 9.5 +0.576 2953 Nov 18.63 7.0 −0.668 2016 May 09.62 9.5 −0.335 2486 Nov 14.64 3.5 −0.293 2963 May 19.25 9.5 +0.406 2019 Nov 11.64 3.5 +0.078 2496 May 15.08 9.5 −0.502 2966 Nov 21.37 3.5 −0.146 2032 Nov 13.37 13.0 +0.590 2499 Nov 17.37 3.5 +0.224 2976 May 21.54 9.5 −0.667 2039 Nov 07.37 7.0 −0.849 2512 Nov 20.11 13.0 +0.737 2979 Nov 24.11 3.5 +0.371 2049 May 07.60 9.5 +0.538 2519 Nov 14.10 7.0 −0.707 2992 Nov 25.84 13.0 +0.883 2052 Nov 09.11 3.5 −0.329 2529 May 14.07 9.5 +0.365 2999 Nov 19.83 7.0 −0.561 2062 May 10.90 9.5 −0.548 2532 Nov 15.84 3.5 −0.185 Notes : TT represents Terrestrial Time; Int . is the number of years since the last previous transit of Mercury; Offset is the number of solar semidiameters that Mercury passes north (+) or south (−) of the apparent solar center (geocentric view).
Load more

Recommended publications
  • KAREN J. MEECH February 7, 2019 Astronomer
    BIOGRAPHICAL SKETCH – KAREN J. MEECH February 7, 2019 Astronomer Institute for Astronomy Tel: 1-808-956-6828 2680 Woodlawn Drive Fax: 1-808-956-4532 Honolulu, HI 96822-1839 [email protected] PROFESSIONAL PREPARATION Rice University Space Physics B.A. 1981 Massachusetts Institute of Tech. Planetary Astronomy Ph.D. 1987 APPOINTMENTS 2018 – present Graduate Chair 2000 – present Astronomer, Institute for Astronomy, University of Hawaii 1992-2000 Associate Astronomer, Institute for Astronomy, University of Hawaii 1987-1992 Assistant Astronomer, Institute for Astronomy, University of Hawaii 1982-1987 Graduate Research & Teaching Assistant, Massachusetts Inst. Tech. 1981-1982 Research Specialist, AAVSO and Massachusetts Institute of Technology AWARDS 2018 ARCs Scientist of the Year 2015 University of Hawai’i Regent’s Medal for Research Excellence 2013 Director’s Research Excellence Award 2011 NASA Group Achievement Award for the EPOXI Project Team 2011 NASA Group Achievement Award for EPOXI & Stardust-NExT Missions 2009 William Tylor Olcott Distinguished Service Award of the American Association of Variable Star Observers 2006-8 National Academy of Science/Kavli Foundation Fellow 2005 NASA Group Achievement Award for the Stardust Flight Team 1996 Asteroid 4367 named Meech 1994 American Astronomical Society / DPS Harold C. Urey Prize 1988 Annie Jump Cannon Award 1981 Heaps Physics Prize RESEARCH FIELD AND ACTIVITIES • Developed a Discovery mission concept to explore the origin of Earth’s water. • Co-Investigator on the Deep Impact, Stardust-NeXT and EPOXI missions, leading the Earth-based observing campaigns for all three. • Leads the UH Astrobiology Research interdisciplinary program, overseeing ~30 postdocs and coordinating the research with ~20 local faculty and international partners.
    [Show full text]
  • 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.
    [Show full text]
  • Explore the Universe Observing Certificate Second Edition
    RASC Observing Committee Explore the Universe Observing Certificate Second Edition Explore the Universe Observing Certificate Welcome to the Explore the Universe Observing Certificate Program. This program is designed to provide the observer with a well-rounded introduction to the night sky visible from North America. Using this observing program is an excellent way to gain knowledge and experience in astronomy. Experienced observers find that a planned observing session results in a more satisfying and interesting experience. This program will help introduce you to amateur astronomy and prepare you for other more challenging certificate programs such as the Messier and Finest NGC. The program covers the full range of astronomical objects. Here is a summary: Observing Objective Requirement Available Constellations and Bright Stars 12 24 The Moon 16 32 Solar System 5 10 Deep Sky Objects 12 24 Double Stars 10 20 Total 55 110 In each category a choice of objects is provided so that you can begin the certificate at any time of the year. In order to receive your certificate you need to observe a total of 55 of the 110 objects available. Here is a summary of some of the abbreviations used in this program Instrument V – Visual (unaided eye) B – Binocular T – Telescope V/B - Visual/Binocular B/T - Binocular/Telescope Season Season when the object can be best seen in the evening sky between dusk. and midnight. Objects may also be seen in other seasons. Description Brief description of the target object, its common name and other details. Cons Constellation where object can be found (if applicable) BOG Ref Refers to corresponding references in the RASC’s The Beginner’s Observing Guide highlighting this object.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • The Observer's Handbook for 1912
    T he O bservers H andbook FOR 1912 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA E d i t e d b y C. A, CHANT FOURTH YEAR OF PUBLICATION TORONTO 198 C o l l e g e St r e e t Pr in t e d fo r t h e So c ie t y 1912 T he Observers Handbook for 1912 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA TORONTO 198 C o l l e g e St r e e t Pr in t e d fo r t h e S o c ie t y 1912 PREFACE Some changes have been made in the Handbook this year which, it is believed, will commend themselves to observers. In previous issues the times of sunrise and sunset have been given for a small number of selected places in the standard time of each place. On account of the arbitrary correction which must be made to the mean time of any place in order to get its standard time, the tables given for a particualar place are of little use any­ where else, In order to remedy this the times of sunrise and sunset have been calculated for places on five different latitudes covering the populous part of Canada, (pages 10 to 21), while the way to use these tables at a large number of towns and cities is explained on pages 8 and 9. The other chief change is in the addition of fuller star maps near the end. These are on a large enough scale to locate a star or planet or comet when its right ascension and declination are given.
    [Show full text]
  • 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.
    [Show full text]
  • Comet Section Observing Guide
    Comet Section Observing Guide 1 The British Astronomical Association Comet Section www.britastro.org/comet BAA Comet Section Observing Guide Front cover image: C/1995 O1 (Hale-Bopp) by Geoffrey Johnstone on 1997 April 10. Back cover image: C/2011 W3 (Lovejoy) by Lester Barnes on 2011 December 23. © The British Astronomical Association 2018 2018 December (rev 4) 2 CONTENTS 1 Foreword .................................................................................................................................. 6 2 An introduction to comets ......................................................................................................... 7 2.1 Anatomy and origins ............................................................................................................................ 7 2.2 Naming .............................................................................................................................................. 12 2.3 Comet orbits ...................................................................................................................................... 13 2.4 Orbit evolution .................................................................................................................................... 15 2.5 Magnitudes ........................................................................................................................................ 18 3 Basic visual observation ........................................................................................................
    [Show full text]
  • The Maunder Minimum and the Variable Sun-Earth Connection
    The Maunder Minimum and the Variable Sun-Earth Connection (Front illustration: the Sun without spots, July 27, 1954) By Willie Wei-Hock Soon and Steven H. Yaskell To Soon Gim-Chuan, Chua Chiew-See, Pham Than (Lien+Van’s mother) and Ulla and Anna In Memory of Miriam Fuchs (baba Gil’s mother)---W.H.S. In Memory of Andrew Hoff---S.H.Y. To interrupt His Yellow Plan The Sun does not allow Caprices of the Atmosphere – And even when the Snow Heaves Balls of Specks, like Vicious Boy Directly in His Eye – Does not so much as turn His Head Busy with Majesty – ‘Tis His to stimulate the Earth And magnetize the Sea - And bind Astronomy, in place, Yet Any passing by Would deem Ourselves – the busier As the Minutest Bee That rides – emits a Thunder – A Bomb – to justify Emily Dickinson (poem 224. c. 1862) Since people are by nature poorly equipped to register any but short-term changes, it is not surprising that we fail to notice slower changes in either climate or the sun. John A. Eddy, The New Solar Physics (1977-78) Foreword By E. N. Parker In this time of global warming we are impelled by both the anticipated dire consequences and by scientific curiosity to investigate the factors that drive the climate. Climate has fluctuated strongly and abruptly in the past, with ice ages and interglacial warming as the long term extremes. Historical research in the last decades has shown short term climatic transients to be a frequent occurrence, often imposing disastrous hardship on the afflicted human populations.
    [Show full text]
  • 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”,
    [Show full text]
  • Instrumental Methods for Professional and Amateur
    Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, Francois Colas, Alain Klotz, Christophe Pellier, Jean-Marc Petit, Philippe Rousselot, et al. To cite this version: Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, et al.. Instru- mental Methods for Professional and Amateur Collaborations in Planetary Astronomy. Experimental Astronomy, Springer Link, 2014, 38 (1-2), pp.91-191. 10.1007/s10686-014-9379-0. hal-00833466 HAL Id: hal-00833466 https://hal.archives-ouvertes.fr/hal-00833466 Submitted on 3 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy O. Mousis, R. Hueso, J.-P. Beaulieu, S. Bouley, B. Carry, F. Colas, A. Klotz, C. Pellier, J.-M. Petit, P. Rousselot, M. Ali-Dib, W. Beisker, M. Birlan, C. Buil, A. Delsanti, E. Frappa, H. B. Hammel, A.-C. Levasseur-Regourd, G. S. Orton, A. Sanchez-Lavega,´ A. Santerne, P. Tanga, J. Vaubaillon, B. Zanda, D. Baratoux, T. Bohm,¨ V. Boudon, A. Bouquet, L. Buzzi, J.-L. Dauvergne, A.
    [Show full text]
  • 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.
    [Show full text]