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Basic Principles of Celestial Navigation James A
Basic principles of celestial navigation James A. Van Allena) Department of Physics and Astronomy, The University of Iowa, Iowa City, Iowa 52242 ͑Received 16 January 2004; accepted 10 June 2004͒ Celestial navigation is a technique for determining one’s geographic position by the observation of identified stars, identified planets, the Sun, and the Moon. This subject has a multitude of refinements which, although valuable to a professional navigator, tend to obscure the basic principles. I describe these principles, give an analytical solution of the classical two-star-sight problem without any dependence on prior knowledge of position, and include several examples. Some approximations and simplifications are made in the interest of clarity. © 2004 American Association of Physics Teachers. ͓DOI: 10.1119/1.1778391͔ I. INTRODUCTION longitude ⌳ is between 0° and 360°, although often it is convenient to take the longitude westward of the prime me- Celestial navigation is a technique for determining one’s ridian to be between 0° and Ϫ180°. The longitude of P also geographic position by the observation of identified stars, can be specified by the plane angle in the equatorial plane identified planets, the Sun, and the Moon. Its basic principles whose vertex is at O with one radial line through the point at are a combination of rudimentary astronomical knowledge 1–3 which the meridian through P intersects the equatorial plane and spherical trigonometry. and the other radial line through the point G at which the Anyone who has been on a ship that is remote from any prime meridian intersects the equatorial plane ͑see Fig. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
Summer 2021 Edition of Aries
Summer 2021 Aries derbyastronomy.org © Peter Hill © Rob Seymour Derby & District Astronomical Society Society Astronomical & District Derby Member Gallery— Peter Hill Visit the D.D.A.S website for more informaon on how Peter obtained these wonderful images. H Alpha Ca K White Light Images © Peter Hill Emerging Sunspot AR2827 ….. Peter Hill 1. Front Cover Member’s Gallery ….. Peter Hill 2. Inside front cover Index & Newsletter Information 3 COVID Statement & Committee Member Details 4 EDITORIAL ….. Anthony Southwell 5-6 Meet your Committee ….. Vice Chair & Ordinary Member 7-8 Chairman’s Challenge ….. Peter Branson 9 NEW - Chairman’s Challenge Competition 9 Derby Ram Trail and the Flamstead Ram ….. Anthony Southwell 10 Astro News - China on Mars: Zhurong Rover 11 Astro News - Dark Matter Map Reveals Cosmic Mystery 12 Astro News - James Webb Space Telescope Launch Delay “Likely,” 13 Astro News - Ingenuity set for 7th Red Planet flight 14 Astro News - NASA Announces Two New Missions to Venus 15 Observatory Rules & Regulations 16-17 BOOK REVIEW ….. The Apollo Guidance Computer ….. Reviewed by Malcolm Neal 18 What’s inside this issue... this inside What’s Library List ….. Titles for loan from the society library 19 inside back cover Programme of events ….. Rolling Calendar of DDAS Meengs and Events 20 back cover Member Gallery Book Reviewers WANTED Did you win a book in the Raffle? Or have you borrowed one from the Society Library. Each issue we would like to feature some of the fantastic Why not tell us what you thought about it in our Book Review . photos taken by members of Guide others through the maze the society. -
Prime Meridian ×
This website would like to remind you: Your browser (Apple Safari 4) is out of date. Update your browser for more × security, comfort and the best experience on this site. Encyclopedic Entry prime meridian For the complete encyclopedic entry with media resources, visit: http://education.nationalgeographic.com/encyclopedia/prime-meridian/ The prime meridian is the line of 0 longitude, the starting point for measuring distance both east and west around the Earth. The prime meridian is arbitrary, meaning it could be chosen to be anywhere. Any line of longitude (a meridian) can serve as the 0 longitude line. However, there is an international agreement that the meridian that runs through Greenwich, England, is considered the official prime meridian. Governments did not always agree that the Greenwich meridian was the prime meridian, making navigation over long distances very difficult. Different countries published maps and charts with longitude based on the meridian passing through their capital city. France would publish maps with 0 longitude running through Paris. Cartographers in China would publish maps with 0 longitude running through Beijing. Even different parts of the same country published materials based on local meridians. Finally, at an international convention called by U.S. President Chester Arthur in 1884, representatives from 25 countries agreed to pick a single, standard meridian. They chose the meridian passing through the Royal Observatory in Greenwich, England. The Greenwich Meridian became the international standard for the prime meridian. UTC The prime meridian also sets Coordinated Universal Time (UTC). UTC never changes for daylight savings or anything else. Just as the prime meridian is the standard for longitude, UTC is the standard for time. -
Early Maritime Navigation Unit Plan
EARLY MARITIME NAVIGATION UNIT PLAN Compelling How did advances in marine navigation, from the 13th century C.E. through the 18th century Question C.E., help to catapult Western Europe into global preeminence? C3 Historical Thinking Standards – D2.His.1.9-12. Evaluate how historical events and developments were shaped by unique circumstances of time and place as well as broader historical contexts. Standards C3 Historical Thinking Standards – D2.His.2.9-12. and Analyze change and continuity in historical eras. Practices Common Core Content Standards – CCSS.ELA-LITERACY.WHST.9-10.1.B Develop claim(s) and counterclaims fairly, supplying data and evidence for each while pointing out the strengths and limitations of both claim(s) and counterclaims in a discipline-appropriate form and in a manner that anticipates the audience's knowledge level and concerns. Staging the How do advances in marine navigation technology help nations develop and sustain world Question influence? Supporting Supporting Supporting Supporting Question 1 Question 2 Question 3 Question 4 Why has the sea been What is navigation and How does being posed How did STEM confer crucial to the fate of what special challenges with a challenge lead us to advantages to a society’s nations, empires, and does the sea pose to innovation and progress? ability to navigate the civilizations? travelers? world’s oceans? Formative Formative Formative Formative Performance Task 1 Performance Task 2 Performance Task 3 Performance Task 4 1) Look at the planet’s 1) In pairs ask your 1) Compass Lesson Plan 1) Drawing connections to physical geography, partner to draw you a (Lesson is located below the last three questions, all the Print Documents) build an argument that map from school to a view the Longitude video the sea was better at specific location in your Discover how the (07:05 min) connecting cultures town. -
Kew Observatory and the Evolution of Victorian Science, 1840–1910
introduction Kew Observatory, Victorian Science, and the “Observatory Sciences” One more recent instance of the operations of this Society in this respect I may mention, in addition to those I have slightly enumerated. I mean the important accession to the means of this Society of a fixed position, a place for deposit, regula- tion, and comparison of instruments, and for many more purposes than I could name, perhaps even more than are yet contemplated, in the Observatory at Kew. Address by Lord Francis Egerton to British Association for the Advancement of Science, June 1842 When in 1842 Lord Egerton, president of the British Association for the Advancement of Science (BAAS), announced the association’s acquisition of Kew Observatory (figure I.1), he heralded the inaugura- tion of what would become one of the major institutions of nineteenth- century British—indeed international—science. Originally built as a pri- vate observatory for King George III and long in a moribund state, after 1842 the Kew building would, as Egerton predicted, become a multi- functional observatory, put to more purposes than were even imagined in 1842. It became distinguished in several sciences: geomagnetism, me- teorology, solar astronomy, and standardization—the latter term being used in this book to refer to testing scientific instruments and develop- ing prototypes of instruments to be used elsewhere, as well as establish- ing and refining constants and standards of measurement. Many of the major figures in the physical sciences of the nineteenth century were in some way involved with Kew Observatory. For the first twenty months of the twentieth century, Kew was the site of the National Physical Labora- 3 © 2018 University of Pittsburgh Press. -
Beagle Run Farm Beagle Run Farm
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Celestial Coordinate Systems
Celestial Coordinate Systems Craig Lage Department of Physics, New York University, [email protected] January 6, 2014 1 Introduction This document reviews briefly some of the key ideas that you will need to understand in order to identify and locate objects in the sky. It is intended to serve as a reference document. 2 Angular Basics When we view objects in the sky, distance is difficult to determine, and generally we can only indicate their direction. For this reason, angles are critical in astronomy, and we use angular measures to locate objects and define the distance between objects. Angles are measured in a number of different ways in astronomy, and you need to become familiar with the different notations and comfortable converting between them. A basic angle is shown in Figure 1. θ Figure 1: A basic angle, θ. We review some angle basics. We normally use two primary measures of angles, degrees and radians. In astronomy, we also sometimes use time as a measure of angles, as we will discuss later. A radian is a dimensionless measure equal to the length of the circular arc enclosed by the angle divided by the radius of the circle. A full circle is thus equal to 2π radians. A degree is an arbitrary measure, where a full circle is defined to be equal to 360◦. When using degrees, we also have two different conventions, to divide one degree into decimal degrees, or alternatively to divide it into 60 minutes, each of which is divided into 60 seconds. These are also referred to as minutes of arc or seconds of arc so as not to confuse them with minutes of time and seconds of time. -
Cambridge University Press 978-0-521-76518-3 — the Making of the Modern Admiralty C
Cambridge University Press 978-0-521-76518-3 — The Making of the Modern Admiralty C. I. Hamilton Index More Information Index Accountant-General, 60; of the Navy Arbuthnot, Charles, 97–8 (from 1832): 65, 125, 138, 146, Army Staff, 222 189–93, 295 (see also estimates); Arnold-Forster, H. O., 198, 217 staff, 164, 188, 192 Asquith, H. H., 224 administrative board, 31 Assistant Secretary for Finance Duties Admiralty (see also Admiralty Office; (see also Secretariat), 192 Board of Admiralty; Childers, H. C. E.; Aube, H.-L.-T., 172 First and Second (Permanent) Auckland, George Eden, Earl of, 119, 134 Secretaries; Geddes, E.; Goschen, Awdry, Richard, 191, 201, 205 George; Graham, Sir James; ‘mob from the North’; Naval Staff; Navy Bacon, Sir Reginald, (Kt. 1916), 215 Board; Navy Pay Office; Principal Baddeley, Vincent, (Kt. 1921), 205, 206, 259 Officers; Private Office; Victualling Balfour, A. J., 237, 238 Board; Secretariat; Sick and Hurt Ballard, G. A., 222, 223 Office; Sixpenny Office; Transport Bank of England, 28 Office; War Staff): administration/ Barham, Lord, see Middleton, Charles policy divide, 266–7, 275, 279, 288, Barnaby, Nathaniel (Kt. 1885), 136, 162, 307; attacks on, 312; civil–military 173, 194–5 division in (see also Godfrey, John), Barrow, John (cr. baronet, 1835) (see also 68–9, 279, 289, 297–302, 313, 314; Second Secretary): 6, 12, 52, 57, 63; committees, 110–11, 120–3, 186–9, administration and policy of, 41, 51, 215; communications, 176, 220, 64, 68–9, 75, 93, 100–1, 103, 152, 248–50; demobilisation, 274, 276; 163; and Benthamism, 54; and development, 2–3, 23, 234–6; J. -
Memoirs of Hydrography
MEMOIRS 07 HYDROGRAPHY INCLUDING Brief Biographies of the Principal Officers who have Served in H.M. NAVAL SURVEYING SERVICE BETWEEN THE YEARS 1750 and 1885 COMPILED BY COMMANDER L. S. DAWSON, R.N. I 1s t tw o PARTS. P a r t II.—1830 t o 1885. EASTBOURNE: HENRY W. KEAY, THE “ IMPERIAL LIBRARY.” iI i / PREF A CE. N the compilation of Part II. of the Memoirs of Hydrography, the endeavour has been to give the services of the many excellent surveying I officers of the late Indian Navy, equal prominence with those of the Royal Navy. Except in the geographical abridgment, under the heading of “ Progress of Martne Surveys” attached to the Memoirs of the various Hydrographers, the personal services of officers still on the Active List, and employed in the surveying service of the Royal Navy, have not been alluded to ; thereby the lines of official etiquette will not have been over-stepped. L. S. D. January , 1885. CONTENTS OF PART II ♦ CHAPTER I. Beaufort, Progress 1829 to 1854, Fitzroy, Belcher, Graves, Raper, Blackwood, Barrai, Arlett, Frazer, Owen Stanley, J. L. Stokes, Sulivan, Berard, Collinson, Lloyd, Otter, Kellett, La Place, Schubert, Haines,' Nolloth, Brock, Spratt, C. G. Robinson, Sheringham, Williams, Becher, Bate, Church, Powell, E. J. Bedford, Elwon, Ethersey, Carless, G. A. Bedford, James Wood, Wolfe, Balleny, Wilkes, W. Allen, Maury, Miles, Mooney, R. B. Beechey, P. Shortland, Yule, Lord, Burdwood, Dayman, Drury, Barrow, Christopher, John Wood, Harding, Kortright, Johnson, Du Petit Thouars, Lawrance, Klint, W. Smyth, Dunsterville, Cox, F. W. L. Thomas, Biddlecombe, Gordon, Bird Allen, Curtis, Edye, F. -
Section II: Summary of the Periodic Report on the State of Conservation, 2006
State of Conservation of World Heritage Properties in Europe SECTION II workmanship, and setting is well documented. UNITED KINGDOM There are firm legislative and policy controls in place to ensure that its fabric and character and Maritime Greenwich setting will be preserved in the future. b) The Queen’s House by Inigo Jones and plans for Brief description the Royal Naval College and key buildings by Sir Christopher Wren as masterpieces of creative The ensemble of buildings at Greenwich, an genius (Criterion i) outlying district of London, and the park in which they are set, symbolize English artistic and Inigo Jones and Sir Christopher Wren are scientific endeavour in the 17th and 18th centuries. acknowledged to be among the greatest The Queen's House (by Inigo Jones) was the first architectural talents of the Renaissance and Palladian building in England, while the complex Baroque periods in Europe. Their buildings at that was until recently the Royal Naval College was Greenwich represent high points in their individual designed by Christopher Wren. The park, laid out architectural oeuvres and, taken as an ensemble, on the basis of an original design by André Le the Queen’s House and Royal Naval College Nôtre, contains the Old Royal Observatory, the complex is widely recognised as Britain’s work of Wren and the scientist Robert Hooke. outstanding Baroque set piece. Inigo Jones was one of the first and the most skilled 1. Introduction proponents of the new classical architectural style in England. On his return to England after having Year(s) of Inscription 1997 travelled extensively in Italy in 1613-14 he was appointed by Anne, consort of James I, to provide a Agency responsible for site management new building at Greenwich. -
Download DARWIN, Beagle Diary.Pdf
CHARLES DARWIN'S BEAGLE DIARY Edited by Richard Darwin Keynes, CBE, ScD, FRS Emeritus Professor of Physiology in the University of Cambridge, and Fellow of Churchill College CAMBRIDGE UNIVERSITY PRESS [page iv] PUBLISHED BY THE PRESS SYNDICATE OF THE UNIVERSITY OF CAMBRIDGE The Pitt Building, Trumpington Street, Cambridge, United Kingdom CAMBRIDGE UNIVERSITY PRESS The Edinburgh Building, Cambridge CB2 2RU, UK 40 West 20th Street, New York, NY 10011–4211, USA 10 Stamford Road, Oakleigh, VIC 3166, Australia Ruiz de Alarcón 13, 28014 Madrid, Spain Dock House, The Waterfront, Cape Town 8001, South Africa http://www.cambridge.org © Cambridge University Press 1988 September 7th, 1835 The Beagle sailed for the Galapagos: 15th on the 15th she was employed in surveying the outer coast of Chatham Isd1 the S. Eastern one of the Archipelago. |604| 1 The Spanish name of Chatham Island now used is Isla San Cristobal. 16th The next day we ran near Hoods Isd1 & there left a Whale boat. — In the evening the Yawl was also sent away on a surveying cruize of some length. — The weather, now & during the passage, has continued as on the coast of Peru, a steady, gentle breeze of wind & gloomy sky. — We landed for an hour on the NW end of Chatham Isd. — These islands at a distance have a sloping uniform outline, excepting where broken by sundry paps & hillocks. — The whole is black Lava, completelycovered by small leafless brushwood & low trees. — The fragments of Lava where most porous are reddish & like cinders; the stunted trees show [page] 352 GALAPAGOS ISDS SEPTEMBER 1835 Chart of the Galapagos Islands (from part of a map in Narrative 1).