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East India Company - Wikipedia, the Free Encyclopedia
East India Company - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/East_India_Company From Wikipedia, the free encyclopedia The English East India Company was an English and later (from 1707) East India Company British joint-stock company[1] formed for pursuing trade with the East Indies but which ended up trading mainly with the Indian subcontinent. The East India Company traded mainly in cotton, silk, indigo dye, salt, saltpetre, tea and opium. The Company was granted a Royal Charter in 1600,[2] making it the oldest among several similarly formed European East India Companies. Shares of the company were owned by wealthy merchants and aristocrats. The government owned no shares and had only indirect control. The Company eventually came to rule large areas of India Company flag after 1801 with its own private army, exercising military power and assuming Former type Public administrative functions.[3] Company rule in India effectively began in 1757 after the Battle of Plassey and lasted until 1858 when, following the Industry International trade Indian Rebellion of 1857, the Government of India Act 1858 led to the Fate Dissolved British Crown assuming direct control of India in the new British Raj. Founded 1600 The Company was dissolved in 1874 as a result of the East India Stock Defunct June 1, 1874 Dividend Redemption Act passed one year earlier, as the Government of India Act had by then rendered it vestigal, powerless and obsolete. Its Headquarters London, England functions had been fully absorbed into official government machinery in the British Raj and its private army had been nationalized by the British Colonial India Crown. -
THE SOVIET MOON PROGRAM in the 1960S, the United States Was Not the Only Country That Was Trying to Land Someone on the Moon and Bring Him Back to Earth Safely
AIAA AEROSPACE M ICRO-LESSON Easily digestible Aerospace Principles revealed for K-12 Students and Educators. These lessons will be sent on a bi-weekly basis and allow grade-level focused learning. - AIAA STEM K-12 Committee. THE SOVIET MOON PROGRAM In the 1960s, the United States was not the only country that was trying to land someone on the Moon and bring him back to Earth safely. The Union of Soviet Socialist Republics, also called the Soviet Union, also had a manned lunar program. This lesson describes some of it. Next Generation Science Standards (NGSS): ● Discipline: Engineering Design ● Crosscutting Concept: Systems and System Models ● Science & Engineering Practice: Constructing Explanations and Designing Solutions GRADES K-2 K-2-ETS1-1. Ask questions, make observations, and gather information about a situation people want to change to define a simple problem that can be solved through the development of a new or improved object or tool. Have you ever been busy doing something when somebody challenges you to a race? If you decide to join the race—and it is usually up to you whether you join or not—you have to stop what you’re doing, get up, and start racing. By the time you’ve gotten started, the other person is often halfway to the goal. This is the sort of situation the Soviet Union found itself in when President Kennedy in 1961 announced that the United States would set a goal of landing a man on the Moon and returning him safely to the Earth before the end of the decade. -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
GRAIL-Identified Gravity Anomalies in Oceanus Procellarum: Insight Into 2 Subsurface Impact and Magmatic Structures on the Moon 3 4 Ariel N
1 GRAIL-identified gravity anomalies in Oceanus Procellarum: Insight into 2 subsurface impact and magmatic structures on the Moon 3 4 Ariel N. Deutscha, Gregory A. Neumannb, James W. Heada, Lionel Wilsona,c 5 6 aDepartment of Earth, Environmental and Planetary Sciences, Brown University, Providence, RI 7 02912, USA 8 bNASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 9 cLancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK 10 11 Corresponding author: Ariel N. Deutsch 12 Corresponding email: [email protected] 13 14 Date of re-submission: 5 April 2019 15 16 Re-submitted to: Icarus 17 Manuscript number: ICARUS_2018_549 18 19 Highlights: 20 • Four positive Bouguer gravity anomalies are analyzed on the Moon’s nearside. 21 • The amplitudes of the anomalies require a deep density contrast. 22 • One 190-km anomaly with crater-related topography is suggestive of mantle uplift. 23 • Marius Hills anomalies are consistent with intruded dike swarms. 24 • An anomaly south of Aristarchus has a crater rim and possibly magmatic intrusions. 25 26 Key words: 27 Moon; gravity; impact cratering; volcanism 1 28 Abstract 29 30 Four, quasi-circular, positive Bouguer gravity anomalies (PBGAs) that are similar in diameter 31 (~90–190 km) and gravitational amplitude (>140 mGal contrast) are identified within the central 32 Oceanus Procellarum region of the Moon. These spatially associated PBGAs are located south of 33 Aristarchus Plateau, north of Flamsteed crater, and two are within the Marius Hills volcanic 34 complex (north and south). Each is characterized by distinct surface geologic features suggestive 35 of ancient impact craters and/or volcanic/plutonic activity. -
Modeling and Mapping of the Structural Deformation of Large Impact Craters on the Moon and Mercury
MODELING AND MAPPING OF THE STRUCTURAL DEFORMATION OF LARGE IMPACT CRATERS ON THE MOON AND MERCURY by JEFFREY A. BALCERSKI Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Department of Earth, Environmental, and Planetary Sciences CASE WESTERN RESERVE UNIVERSITY August, 2015 CASE WESTERN RESERVE UNIVERSITY SCHOOL OF GRADUATE STUDIES We hereby approve the thesis/dissertation of Jeffrey A. Balcerski candidate for the degree of Doctor of Philosophy Committee Chair Steven A. Hauck, II James A. Van Orman Ralph P. Harvey Xiong Yu June 1, 2015 *we also certify that written approval has been obtained for any proprietary material contained therein ~ i ~ Dedicated to Marie, for her love, strength, and faith ~ ii ~ Table of Contents 1. Introduction ............................................................................................................1 2. Tilted Crater Floors as Records of Mercury’s Surface Deformation .....................4 2.1 Introduction ..............................................................................................5 2.2 Craters and Global Tilt Meters ................................................................8 2.3 Measurement Process...............................................................................12 2.3.1 Visual Pre-selection of Candidate Craters ................................13 2.3.2 Inspection and Inclusion/Exclusion of Altimetric Profiles .......14 2.3.3 Trend Fitting of Crater Floor Topography ................................16 2.4 Northern -
Lunar Impact Basins Revealed by Gravity Recovery and Interior
Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, Sean Solomon, David Smith, Frank Lemoine, Erwan Mazarico, Terence Sabaka, et al. To cite this version: Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, et al.. Lunar im- pact basins revealed by Gravity Recovery and Interior Laboratory measurements. Science Advances , American Association for the Advancement of Science (AAAS), 2015, 1 (9), pp.e1500852. 10.1126/sci- adv.1500852. hal-02458613 HAL Id: hal-02458613 https://hal.archives-ouvertes.fr/hal-02458613 Submitted on 26 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. RESEARCH ARTICLE PLANETARY SCIENCE 2015 © The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. Distributed Lunar impact basins revealed by Gravity under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). Recovery and Interior Laboratory measurements 10.1126/sciadv.1500852 Gregory A. Neumann,1* Maria T. Zuber,2 Mark A. Wieczorek,3 James W. Head,4 David M. H. Baker,4 Sean C. Solomon,5,6 David E. Smith,2 Frank G. -
Unit 11: Exploration of the Americas
Unit 11: Exploration of the Americas Name: ________________________________________ Teacher: _____________________________ IB/AP World History 9 Commack High School Please Note: You are responsible for all information in this packet, supplemental handouts provided in class as well as your homework, class webpage and class discussions. A Changing Map and Protection to the North Directions: As you read, look for advantages and disadvantages of the land controlled by each dynasty. When the Yuan dynasty ruled China, the Mongols controlled land that The early Ming emperors pushed the Mongols and other nomadic included their homeland to the north. Through trade routes they were tribes north and secured their borders. They reinforced and expanded connected to the rest of the Mongol empires that lay to the west and to the Great Wall of China (video) continuously throughout their the Middle East and Europe. Since the Mongols and their allies ruled dynasty’s reign. Much of the Great Wall as we know it today was most of central Asia, they had little need to reinforce their defenses and built during the Ming dynasty. did little to maintain the Great Wall. Source: http://archive.artsmia.org/art-of-asia/history/images/maps/china-yuan-large.gif Source: http://archive.artsmia.org/art-of-asia/history/images/maps/china-ming-large.gif 1. What is the difference between these two maps? 2. What advantages did the Yuan Dynasty gain from the land it 3. What advantages did the Ming Dynasty gain from the land it controlled? What disadvantage came from controlling this land? controlled? What disadvantage came from controlling this land? Voyages of Zheng He Source: Elisabeth Ellis and Anthony esler, World History: Connection to Today, Prentice Hall (adapted) from the NYS Global History and Geography Regents Examination, June 2004 Watch this excerpt from a History Channel Video on 4. -
GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins. -
Arxiv:0706.3947V1
Transient Lunar Phenomena: Regularity and Reality Arlin P.S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is still controversial. Nonetheless, a review of TLP data shows regularities in the observations; a key question is whether this structure is imposed by human observer effects, terrestrial atmospheric effects or processes tied to the lunar surface. I interrogate an extensive catalog of TLPs to determine if human factors play a determining role in setting the distribution of TLP reports. We divide the sample according to variables which should produce varying results if the determining factors involve humans e.g., historical epoch or geographical location of the observer, and not reflecting phenomena tied to the lunar surface. Specifically, we bin the reports into selenographic areas (300 km on a side), then construct a robust average count for such “pixels” in a way discarding discrepant counts. Regardless of how we split the sample, the results are very similar: roughly 50% of the report count originate from the crater Aristarchus and vicinity, 16% from Plato, 6% from recent, major impacts (Copernicus, ∼ ∼ Kepler and Tycho - beyond Aristarchus), plus a few at Grimaldi. Mare Crisium produces a robust signal for three of five averages of up to 7% of the reports (however, Crisium subtends more than one pixel). The consistency in TLP report counts for specific features on this list indicate that 80% of the reports arXiv:0706.3947v1 [astro-ph] 27 Jun 2007 ∼ are consistent with being real (perhaps with the exception of Crisium). -
Download 1 File
CORNELL UNIVERSITY LIBRARY BOUGHT WITH THE INCOME OF THE SAGE ENDOWMENT FUND GIVEN IN 1 89 1 BY HENRY WILLIAMS SAGE Date Due -ARR-l 9 1 'mmm -^iU. tiiV'Sc.i'isf IrotT ri j; mr f]It ¥. r NOV 1 4 959 BS $KP2 6 mQE§ •^^N 2 -^Tre^ fV! ah M si p;^^^^ ^HLZ^um Z 32 3 3 G Cornell University Library F7.A21 F7 The founding of New England 3 1924 030 933 927 olin Cornell University Library The original of tiiis bool< is in tine Cornell University Library. There are no known copyright restrictions in the United States on the use of the text. http://www.archive.org/details/cu31924030933927 THE FOUNDING OF NEW ENGLAND New England in i 640. (Inset shows Labrador Current) THE FOUNDING OF NEW ENGLAND BY JAMES TRUSLOW ADAMS Illustrated THE ATLANTIC MONTHLY PRESS BOSTON ^ K >/ Copyright, 1921 By JAMES TRUSLOW ADAMS '^ To A. L. A. 3 One duty that was always incumbent on the historian has now become a duty of deeper significance and stronger obli- gation. Truth, and Truth only, is our aim. We are bound as historians to examine and record facts without favor or affection to our own nation or to any other. Lord Bryce, Presidential Address, at the International Congress of Historical Studies, 191 PREFACE The following account of the founding of New England is intended to serve as an introduction to the later history of that section, and to the study of its relations with other por- tions of the Empire and with the mother-country, as well as of the section's influence upon the nation formed from such of the colonies as subsequently revolted. -
From Natural History to Orientalism, the Russell Brothers on the Cusp of Empire
From Natural History to Orientalism, The Russell Brothers on the Cusp of Empire Author: Jenna Larson Boyle Persistent link: http://hdl.handle.net/2345/3052 This work is posted on eScholarship@BC, Boston College University Libraries. Boston College Electronic Thesis or Dissertation, 2010 Copyright is held by the author, with all rights reserved, unless otherwise noted. Boston College The Graduate School of Arts and Sciences Department of History FROM NATURAL HISTORY TO ORIENTALISM: THE RUSSELL BROTHERS ON THE CUSP OF EMPIRE a thesis by JENNA LARSON BOYLE submitted in partial fulfillment of the requirements For the degree of Master of Arts May 2009 ! ! copyright by JENNA LARSON BOYLE 2010 ! ABSTRACT FROM NATURAL HISTORY TO ORIENTALISM: THE RUSSELL BROTHERS ON THE CUSP OF EMPIRE Jenna Larson Boyle Thesis Chair: Dana Sajdi The British physicians Dr. Alexander Russell M.D., FRS (c.1715 – 1768)!and Dr. Patrick Russell M.D., FRS (1726/7 – 1805), both British Levant Company servants, wrote and published two editions in 1756 and 1794, respectively. These brothers resided in Aleppo, Syria, when it was a provincial capital of the Ottoman Empire and recorded their observations and empirical observations in a literary work that would later become the two editions of The Natural History of Aleppo. These editions are vital references for modern scholars concerned with Ottoman Syria, Levantine commercial activity and European presence, and the city of Aleppo. However, these very scholars ignore the significant fact that these two editions were written by two different individuals at two different points in history. Thus, this MA thesis aims to investigate the two editions and illustrate how the variations in these publications were the result of both coexisting and correlated processes that culminated in an eighteenth-century phenomenon of the transformation of British global presence from a commercial power to a modern empire.