Patrick Moore's Data Book of Astronomy
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Ann Merchant Boesgaard Publications Merchant, A. E., Bodenheimer, P., and Wallerstein, G
Ann Merchant Boesgaard Publications Merchant, A. E., Bodenheimer, P., and Wallerstein, G. (1965). “The Lithium Isotope Ratio in Two Hyades F Stars.” Ap. J., 142, 790. Merchant, A. E. (1966). “Beryllium in F- and G-Type Dwarfs.” Ap. J., 143, 336. Hodge, P. W., and Merchant, A. E. (1966). “Photometry of SO Galaxies II. The Peculiar Galaxy NGC 128.” Ap. J., 144, 875. Merchant, A. E. (1967). “The Abundance of Lithium in Early M-Type Stars.” Ap. J., 147, 587. Merchant, A. E. (1967). “Measured Equivalent Widths in Early M-Type Stars.” Lick Obs. Bull. No. 595 (Univ. of California Press). Boesgaard, A. M. (1968). “Isotopes of Magnesium in Stellar Atmosphere.” Ap. J., 154, 185. Boesgaard, A. M. (1968). “Observations of Beryllium in Stars.” Highlights of Astron- omy, ed. L. Perek (Dordrecht: D. Reidel), p. 237. Boesgaard, A. M. (1969). “Intensity Variation in Ca Emission in an MS Star.” Pub. A. S. P., 81, 283. Boesgaard, A. M. (1969). “Observational Clues to the Evolution of M Giant Stars.” Pub. A. S. P., 81, 365. Boesgaard, A. M. (1970). “The Lithium Isotope Ratio in δ Sagittae.” Ap. J., 159, 727. Boesgaard, A. M. (1970). “The Ratio of Titanium to Zirconium in Late-Type Stars.” Ap. J., 161, 163. Boesgaard, A. M. (1970). “On the Lithium Content in Late-Type Giants.” Ap. Letters, 5, 145. Boesgaard, A. M. (1970). “Lithium in Heavy-Metal Red Giants.” Ap. J., 161, 1003. Boesgaard, A. M. (1971). “The Lithium Content of Capella.” Ap. J., 167, 511. Boesgaard, A. M. (1973). “Iron Emission Lines in a Orionis.” In Stellar Chromospheres, eds. -
Urania Nr 3/2005
> /2005 (717) urania 3/tom LXXVI maj—czerwiec mhćirn iVlich jp f f l owiek, który świat nauczył rnier> życe(?) wokóf planetoid Fotome anzytów za pomocą rnaiych Europejskie Obserwatorium Południowe leskopami pomocniczymi (AT) o średnicy a dalej ogromne budynki mieszczące wiel (ESO) zbudowało w latach 1988-2002, na 1,8 m, które mogą zajmować 30 różnych kie teleskopy i 2 kopuły teleskopów pomoc ściętym wierzchołku góry Cerro Paranal pozycji, będą stanowiły ciągle rozbudowy niczych (obecnie są 2 AT, będzie ich 8). (2635 m n.p.m.) na pustyni Atacama w Chi wany instrument interferometryczny (VLTI) Na górnym zdjęciu widzimy teleskop „z gó le, Bardzo Duży Teleskop (VLT). Składa o bazie sięgającej przeszło 200 m, które ry" wraz z okolicznym krajobrazem, toro się on z czterech teleskopów o średnicy go rozdzielczość (0,001 sekundy łuku) bę wiskami teleskopów AT i drogami kanałów 8,2 m, mogących kierować zebrane świa dzie tak wielka, że można by widzieć nim optycznych prowadzących zebrane świa tło do wspólnego ogniska. Razem zbierają astronautę na Księżycu. Dolne zdjęcie tło do wspólnego ogniska interferometru one tyle światła, ile zbierałby teleskop przedstawia ogólny, obecny (2005 r.) wi oznaczonego gwiazdką. Idea i zasady o średnicy 16 m, a pracując w systemie dok tego obserwatorium. Na pierwszym działania tego instrumentu wywodzą się interferometrycznym, stanowią teleskop planie widzimy torowisko i stanowiska ob z odkryć i prac Alberta Michelsona. o średnicy prawie 130 m. Wspomagane te serwacyjne dla teleskopów pomocniczych, Zdjęcia ESO U R A N IA - POSTtPY ASTRONOMII 3/2005 Szanowni i Drodzy Czytelnicy, Interferometria, jako technika badawcza, zdobywa coraz szersze pola zastosowań w astronomii. -
The Comet's Tale, and Therefore the Object As a Whole Would the Section Director Nick James Highlighted Have a Low Surface Brightness
1 Diebold Schilling, Disaster in connection with two comets sighted in 1456, Lucerne Chronicle, 1513 (Wikimedia Commons) THE COMET’S TALE Comet Section – British Astronomical Association Journal – Number 38 2019 June britastro.org/comet Evolution of the comet C/2016 R2 (PANSTARRS) along a total of ten days on January 2018. Composition of pictures taken with a zoom lens from Teide Observatory in Canary Islands. J.J Chambó Bris 2 Table of Contents Contents Author Page 1 Director’s Welcome Nick James 3 Section Director 2 Melvyn Taylor’s Alex Pratt 6 Observations of Comet C/1995 01 (Hale-Bopp) 3 The Enigma of Neil Norman 9 Comet Encke 4 Setting up the David Swan 14 C*Hyperstar for Imaging Comets 5 Comet Software Owen Brazell 19 6 Pro-Am José Joaquín Chambó Bris 25 Astrophotography of Comets 7 Elizabeth Roemer: A Denis Buczynski 28 Consummate Comet Section Secretary Observer 8 Historical Cometary Amar A Sharma 37 Observations in India: Part 2 – Mughal Empire 16th and 17th Century 9 Dr Reginald Denis Buczynski 42 Waterfield and His Section Secretary Medals 10 Contacts 45 Picture Gallery Please note that copyright 46 of all images belongs with the Observer 3 1 From the Director – Nick James I hope you enjoy reading this issue of the We have had a couple of relatively bright Comet’s Tale. Many thanks to Janice but diffuse comets through the winter and McClean for editing this issue and to Denis there are plenty of images of Buczynski for soliciting contributions. 46P/Wirtanen and C/2018 Y1 (Iwamoto) Thanks also to the section committee for in our archive. -
ESO's VLT Sphere and DAMIT
ESO’s VLT Sphere and DAMIT ESO’s VLT SPHERE (using adaptive optics) and Joseph Durech (DAMIT) have a program to observe asteroids and collect light curve data to develop rotating 3D models with respect to time. Up till now, due to the limitations of modelling software, only convex profiles were produced. The aim is to reconstruct reliable nonconvex models of about 40 asteroids. Below is a list of targets that will be observed by SPHERE, for which detailed nonconvex shapes will be constructed. Special request by Joseph Durech: “If some of these asteroids have in next let's say two years some favourable occultations, it would be nice to combine the occultation chords with AO and light curves to improve the models.” 2 Pallas, 7 Iris, 8 Flora, 10 Hygiea, 11 Parthenope, 13 Egeria, 15 Eunomia, 16 Psyche, 18 Melpomene, 19 Fortuna, 20 Massalia, 22 Kalliope, 24 Themis, 29 Amphitrite, 31 Euphrosyne, 40 Harmonia, 41 Daphne, 51 Nemausa, 52 Europa, 59 Elpis, 65 Cybele, 87 Sylvia, 88 Thisbe, 89 Julia, 96 Aegle, 105 Artemis, 128 Nemesis, 145 Adeona, 187 Lamberta, 211 Isolda, 324 Bamberga, 354 Eleonora, 451 Patientia, 476 Hedwig, 511 Davida, 532 Herculina, 596 Scheila, 704 Interamnia Occultation Event: Asteroid 10 Hygiea – Sun 26th Feb 16h37m UT The magnitude 11 asteroid 10 Hygiea is expected to occult the magnitude 12.5 star 2UCAC 21608371 on Sunday 26th Feb 16h37m UT (= Mon 3:37am). Magnitude drop of 0.24 will require video. DAMIT asteroid model of 10 Hygiea - Astronomy Institute of the Charles University: Josef Ďurech, Vojtěch Sidorin Hygiea is the fourth-largest asteroid (largest is Ceres ~ 945kms) in the Solar System by volume and mass, and it is located in the asteroid belt about 400 million kms away. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
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. -
Dynamical Evolution of the Cybele Asteroids
MNRAS 451, 244–256 (2015) doi:10.1093/mnras/stv997 Dynamical evolution of the Cybele asteroids Downloaded from https://academic.oup.com/mnras/article-abstract/451/1/244/1381346 by Universidade Estadual Paulista J�lio de Mesquita Filho user on 22 April 2019 V. Carruba,1‹ D. Nesvorny,´ 2 S. Aljbaae1 andM.E.Huaman1 1UNESP, Univ. Estadual Paulista, Grupo de dinamicaˆ Orbital e Planetologia, 12516-410 Guaratingueta,´ SP, Brazil 2Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA Accepted 2015 May 1. Received 2015 May 1; in original form 2015 April 1 ABSTRACT The Cybele region, located between the 2J:-1A and 5J:-3A mean-motion resonances, is ad- jacent and exterior to the asteroid main belt. An increasing density of three-body resonances makes the region between the Cybele and Hilda populations dynamically unstable, so that the Cybele zone could be considered the last outpost of an extended main belt. The presence of binary asteroids with large primaries and small secondaries suggested that asteroid families should be found in this region, but only relatively recently the first dynamical groups were identified in this area. Among these, the Sylvia group has been proposed to be one of the oldest families in the extended main belt. In this work we identify families in the Cybele region in the context of the local dynamics and non-gravitational forces such as the Yarkovsky and stochastic Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effects. We confirm the detec- tion of the new Helga group at 3.65 au, which could extend the outer boundary of the Cybele region up to the 5J:-3A mean-motion resonance. -
Occultation Newsletter Volume 8, Number 4
Volume 12, Number 1 January 2005 $5.00 North Am./$6.25 Other International Occultation Timing Association, Inc. (IOTA) In this Issue Article Page The Largest Members Of Our Solar System – 2005 . 4 Resources Page What to Send to Whom . 3 Membership and Subscription Information . 3 IOTA Publications. 3 The Offices and Officers of IOTA . .11 IOTA European Section (IOTA/ES) . .11 IOTA on the World Wide Web. Back Cover ON THE COVER: Steve Preston posted a prediction for the occultation of a 10.8-magnitude star in Orion, about 3° from Betelgeuse, by the asteroid (238) Hypatia, which had an expected diameter of 148 km. The predicted path passed over the San Francisco Bay area, and that turned out to be quite accurate, with only a small shift towards the north, enough to leave Richard Nolthenius, observing visually from the coast northwest of Santa Cruz, to have a miss. But farther north, three other observers video recorded the occultation from their homes, and they were fortuitously located to define three well- spaced chords across the asteroid to accurately measure its shape and location relative to the star, as shown in the figure. The dashed lines show the axes of the fitted ellipse, produced by Dave Herald’s WinOccult program. This demonstrates the good results that can be obtained by a few dedicated observers with a relatively faint star; a bright star and/or many observers are not always necessary to obtain solid useful observations. – David Dunham Publication Date for this issue: July 2005 Please note: The date shown on the cover is for subscription purposes only and does not reflect the actual publication date. -
(704) Interamnia from Its Occultations and Lightcurves
International Journal of Astronomy and Astrophysics, 2014, 4, 91-118 Published Online March 2014 in SciRes. http://www.scirp.org/journal/ijaa http://dx.doi.org/10.4236/ijaa.2014.41010 A 3-D Shape Model of (704) Interamnia from Its Occultations and Lightcurves Isao Satō1*, Marc Buie2, Paul D. Maley3, Hiromi Hamanowa4, Akira Tsuchikawa5, David W. Dunham6 1Astronomical Society of Japan, Yamagata, Japan 2Southwest Research Institute, Boulder, USA 3International Occultation Timing Association, Houston, USA 4Hamanowa Astronomical Observatory, Fukushima, Japan 5Yanagida Astronomical Observatory, Ishikawa, Japan 6International Occultation Timing Association, Greenbelt, USA Email: *[email protected], [email protected], [email protected], [email protected], [email protected], [email protected] Received 9 November 2013; revised 9 December 2013; accepted 17 December 2013 Copyright © 2014 by authors and Scientific Research Publishing Inc. This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/ Abstract A 3-D shape model of the sixth largest of the main belt asteroids, (704) Interamnia, is presented. The model is reproduced from its two stellar occultation observations and six lightcurves between 1969 and 2011. The first stellar occultation was the occultation of TYC 234500183 on 1996 De- cember 17 observed from 13 sites in the USA. An elliptical cross section of (344.6 ± 9.6 km) × (306.2 ± 9.1 km), for position angle P = 73.4 ± 12.5˚ was fitted. The lightcurve around the occulta- tion shows that the peak-to-peak amplitude was 0.04 mag. and the occultation phase was just be- fore the minimum. -
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”, -
The British Astronomical Association Handbook 2017
THE HANDBOOK OF THE BRITISH ASTRONOMICAL ASSOCIATION 2017 2016 October ISSN 0068–130–X CONTENTS PREFACE . 2 HIGHLIGHTS FOR 2017 . 3 CALENDAR 2017 . 4 SKY DIARY . .. 5-6 SUN . 7-9 ECLIPSES . 10-15 APPEARANCE OF PLANETS . 16 VISIBILITY OF PLANETS . 17 RISING AND SETTING OF THE PLANETS IN LATITUDES 52°N AND 35°S . 18-19 PLANETS – EXPLANATION OF TABLES . 20 ELEMENTS OF PLANETARY ORBITS . 21 MERCURY . 22-23 VENUS . 24 EARTH . 25 MOON . 25 LUNAR LIBRATION . 26 MOONRISE AND MOONSET . 27-31 SUN’S SELENOGRAPHIC COLONGITUDE . 32 LUNAR OCCULTATIONS . 33-39 GRAZING LUNAR OCCULTATIONS . 40-41 MARS . 42-43 ASTEROIDS . 44 ASTEROID EPHEMERIDES . 45-50 ASTEROID OCCULTATIONS .. ... 51-53 ASTEROIDS: FAVOURABLE OBSERVING OPPORTUNITIES . 54-56 NEO CLOSE APPROACHES TO EARTH . 57 JUPITER . .. 58-62 SATELLITES OF JUPITER . .. 62-66 JUPITER ECLIPSES, OCCULTATIONS AND TRANSITS . 67-76 SATURN . 77-80 SATELLITES OF SATURN . 81-84 URANUS . 85 NEPTUNE . 86 TRANS–NEPTUNIAN & SCATTERED-DISK OBJECTS . 87 DWARF PLANETS . 88-91 COMETS . 92-96 METEOR DIARY . 97-99 VARIABLE STARS (RZ Cassiopeiae; Algol; λ Tauri) . 100-101 MIRA STARS . 102 VARIABLE STAR OF THE YEAR (T Cassiopeiæ) . .. 103-105 EPHEMERIDES OF VISUAL BINARY STARS . 106-107 BRIGHT STARS . 108 ACTIVE GALAXIES . 109 TIME . 110-111 ASTRONOMICAL AND PHYSICAL CONSTANTS . 112-113 INTERNET RESOURCES . 114-115 GREEK ALPHABET . 115 ACKNOWLEDGEMENTS / ERRATA . 116 Front Cover: Northern Lights - taken from Mount Storsteinen, near Tromsø, on 2007 February 14. A great effort taking a 13 second exposure in a wind chill of -21C (Pete Lawrence) British Astronomical Association HANDBOOK FOR 2017 NINETY–SIXTH YEAR OF PUBLICATION BURLINGTON HOUSE, PICCADILLY, LONDON, W1J 0DU Telephone 020 7734 4145 PREFACE Welcome to the 96th Handbook of the British Astronomical Association. -
The Minor Planet Bulletin 44 (2017) 142
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 44, NUMBER 2, A.D. 2017 APRIL-JUNE 87. 319 LEONA AND 341 CALIFORNIA – Lightcurves from all sessions are then composited with no TWO VERY SLOWLY ROTATING ASTEROIDS adjustment of instrumental magnitudes. A search should be made for possible tumbling behavior. This is revealed whenever Frederick Pilcher successive rotational cycles show significant variation, and Organ Mesa Observatory (G50) quantified with simultaneous 2 period software. In addition, it is 4438 Organ Mesa Loop useful to obtain a small number of all-night sessions for each Las Cruces, NM 88011 USA object near opposition to look for possible small amplitude short [email protected] period variations. Lorenzo Franco Observations to obtain the data used in this paper were made at the Balzaretto Observatory (A81) Organ Mesa Observatory with a 0.35-meter Meade LX200 GPS Rome, ITALY Schmidt-Cassegrain (SCT) and SBIG STL-1001E CCD. Exposures were 60 seconds, unguided, with a clear filter. All Petr Pravec measurements were calibrated from CMC15 r’ values to Cousins Astronomical Institute R magnitudes for solar colored field stars. Photometric Academy of Sciences of the Czech Republic measurement is with MPO Canopus software. To reduce the Fricova 1, CZ-25165 number of points on the lightcurves and make them easier to read, Ondrejov, CZECH REPUBLIC data points on all lightcurves constructed with MPO Canopus software have been binned in sets of 3 with a maximum time (Received: 2016 Dec 20) difference of 5 minutes between points in each bin.