Open Innovation in the Eighteenth Century: the Longitude Problem
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FROM LONGITUDE to ALTITUDE: INDUCEMENT PRIZE CONTESTS AS INSTRUMENTS of PUBLIC POLICY in SCIENCE and TECHNOLOGY Clayton Stallbau
FROM LONGITUDE TO ALTITUDE: INDUCEMENT PRIZE CONTESTS AS INSTRUMENTS OF PUBLIC POLICY IN SCIENCE AND TECHNOLOGY Clayton Stallbaumer* I. INTRODUCTION On a foggy October night in 1707, a fleet of Royal Navy warships ran aground on the Isles of Scilly, some twenty miles southwest of England.1 Believing themselves to be safely west of any navigational hazards, two thousand sailors discovered too late that they had fatally misjudged their position.2 Although the search for an accurate method to determine longitude had bedeviled Europe for several centuries, the “sudden loss of so many lives, so many ships, and so much honor all at once” elevated the discovery of a solution to a top national priority in England.3 In 1714, Parliament issued the Longitude Act,4 promising as much as £20,0005 for a “Practicable and Useful” method of determining longitude at sea; fifty-nine years later, clockmaker John Harrison claimed the prize.6 Nearly three centuries after the fleet’s tragic demise, another accident, also fatal but far removed from longitude’s terrestrial reach, struck a nation deeply. Just four days after its crew observed a moment’s silence in memory of the Challenger astronauts, the space shuttle Columbia disintegrated upon reentry, killing all on board.7 Although * J.D., University of Illinois College of Law, 2006; M.B.A., University of Illinois College of Business, 2006; B.A., Economics, B.A., History, Lake Forest College, 2001. 1. DAVA SOBEL, LONGITUDE: THE TRUE STORY OF A LONE GENIUS WHO SOLVED THE GREATEST SCIENTIFIC PROBLEM OF HIS TIME 12 (1995). -
QUICK REFERENCE GUIDE Latitude, Longitude and Associated Metadata
QUICK REFERENCE GUIDE Latitude, Longitude and Associated Metadata The Property Profile Form (PPF) requests the property name, address, city, state and zip. From these address fields, ACRES interfaces with Google Maps and extracts the latitude and longitude (lat/long) for the property location. ACRES sets the remaining property geographic information to default values. The data (known collectively as “metadata”) are required by EPA Data Standards. Should an ACRES user need to be update the metadata, the Edit Fields link on the PPF provides the ability to change the information. Before the metadata were populated by ACRES, the data were entered manually. There may still be the need to do so, for example some properties do not have a specific street address (e.g. a rural property located on a state highway) or an ACRES user may have an exact lat/long that is to be used. This Quick Reference Guide covers how to find latitude and longitude, define the metadata, fill out the associated fields in a Property Work Package, and convert latitude and longitude to decimal degree format. This explains how the metadata were determined prior to September 2011 (when the Google Maps interface was added to ACRES). Definitions Below are definitions of the six data elements for latitude and longitude data that are collected in a Property Work Package. The definitions below are based on text from the EPA Data Standard. Latitude: Is the measure of the angular distance on a meridian north or south of the equator. Latitudinal lines run horizontal around the earth in parallel concentric lines from the equator to each of the poles. -
Latitude/Longitude Data Standard
LATITUDE/LONGITUDE DATA STANDARD Standard No.: EX000017.2 January 6, 2006 Approved on January 6, 2006 by the Exchange Network Leadership Council for use on the Environmental Information Exchange Network Approved on January 6, 2006 by the Chief Information Officer of the U. S. Environmental Protection Agency for use within U.S. EPA This consensus standard was developed in collaboration by State, Tribal, and U. S. EPA representatives under the guidance of the Exchange Network Leadership Council and its predecessor organization, the Environmental Data Standards Council. Latitude/Longitude Data Standard Std No.:EX000017.2 Foreword The Environmental Data Standards Council (EDSC) identifies, prioritizes, and pursues the creation of data standards for those areas where information exchange standards will provide the most value in achieving environmental results. The Council involves Tribes and Tribal Nations, state and federal agencies in the development of the standards and then provides the draft materials for general review. Business groups, non- governmental organizations, and other interested parties may then provide input and comment for Council consideration and standard finalization. Standards are available at http://www.epa.gov/datastandards. 1.0 INTRODUCTION The Latitude/Longitude Data Standard is a set of data elements that can be used for recording horizontal and vertical coordinates and associated metadata that define a point on the earth. The latitude/longitude data standard establishes the requirements for documenting latitude and longitude coordinates and related method, accuracy, and description data for all places used in data exchange transaction. Places include facilities, sites, monitoring stations, observation points, and other regulated or tracked features. 1.1 Scope The purpose of the standard is to provide a common set of data elements to specify a point by latitude/longitude. -
2. Descriptive Astronomy (“Astronomy Without a Telescope”)
2. Descriptive Astronomy (“Astronomy Without a Telescope”) http://apod.nasa.gov/apod/astropix.html • How do we locate stars in the heavens? • What stars are visible from a given location? • Where is the sun in the sky at any given time? • Where are you on the Earth? An “asterism” is two stars that appear To be close in the sky but actually aren’t In 1930 the International Astronomical Union (IAU) ruled the heavens off into 88 legal, precise constellations. (52 N, 36 S) Every star, galaxy, etc., is a member of one of these constellations. Many stars are named according to their constellation and relative brightness (Bayer 1603). Sirius α − Centauri, α-Canis declination less http://calgary.rasc.ca/constellation.htm - list than -53o not Majoris, α-Orionis visible from SC http://www.google.com/sky/ Betelgeuse https://en.wikipedia.org/wiki/List_of_Messier_objects (1758 – 1782) Biggest constellation – Hydra – the female water snake 1303 square degrees, but Ursa Major and Virgo almost as big. Hydrus – the male water snake is much smaller – 2243 square degrees Smallest is Crux – the Southern Cross – 68 square degrees Brief History Some of the current constellations can be traced back to the inhabitants of the Euphrates valley, from whom they were handed down through the Greeks and Arabs. Few pictorial records of the ancient constellation figures have survived, but in the Almagest AD 150, Ptolemy catalogued the positions of 1,022 of the brightest stars both in terms of celestial latitude and longitude, and of their places in 48 constellations. The Ptolemaic constellations left a blank area centered not on the present south pole but on a point which, because of precession, would have been the south pole c. -
GMT and Longitude by Lunar Distance: Two Methods Compared from a Practitioner’S Point of View
THE JOURNAL OF NAVIGATION (2019), 72, 1660–1664. c The Royal Institute of Navigation 2019 doi:10.1017/S0373463319000341 FORUM GMT and Longitude by Lunar Distance: Two Methods Compared From a Practitioner’s Point of View Eric Romelczyk (E-mail: [email protected]) This article discusses the technique of observing lunar distance - that is, angular distance between the moon and another celestial body - to establish universal time and longitude, from a practitioner’s point of view. The article presents a brief overview of the principles underlying the lunar distance observation and its use in celestial navigation. A discussion follows of two different methods for finding universal time by observing lunar distance, Dr. Wendel Brunner’s calculator-based method and the specialised inspection tables created by Bruce Stark. The article compares the two methods against each other for ease of use and accuracy. The author concludes that either method will provide satisfactory results, but that the technique of observing lunar dis- tance is unlikely to regain relevance in the modern-day practice of navigation and is primarily useful as a skill-building exercise in making sextant observations. KEYWORDS 1. Navigation. 2. History. 3. Nautical. 4. Time. Submitted: 8 August 2018. Accepted: 14 April 2019. First published online: 2 May 2019. 1. INTRODUCTION. 1.1. History of the lunar distance method. For centuries of seafaring history, a method for accurately measuring time to the degree of precision necessary to establish the navigator’s longitude was out of reach for practical purposes. It had been understood since the mid-16th century that the navigator’s longitude could be established either by reference to the moon’s angular distance from other celestial bodies - the “lunar distance”, measured by careful sextant observations - or by reference to a timepiece of sufficient accuracy. -
Spherical Coordinate Systems
Spherical Coordinate Systems Exploring Space Through Math Pre-Calculus let's examine the Earth in 3-dimensional space. The Earth is a large spherical object. In order to find a location on the surface, The Global Pos~ioning System grid is used. The Earth is conventionally broken up into 4 parts called hemispheres. The North and South hemispheres are separated by the equator. The East and West hemispheres are separated by the Prime Meridian. The Geographic Coordinate System grid utilizes a series of horizontal and vertical lines. The horizontal lines are called latitude lines. The equator is the center line of latitude. Each line is measured in degrees to the North or South of the equator. Since there are 360 degrees in a circle, each hemisphere is 180 degrees. The vertical lines are called longitude lines. The Prime Meridian is the center line of longitude. Each hemisphere either East or West from the center line is 180 degrees. These lines form a grid or mapping system for the surface of the Earth, This is how latitude and longitude lines are represented on a flat map called a Mercator Projection. Lat~ude , l ong~ude , and elevalion allows us to uniquely identify a location on Earth but, how do we identify the pos~ion of another point or object above Earth's surface relative to that I? NASA uses a spherical Coordinate system called the Topodetic coordinate system. Consider the position of the space shuttle . The first variable used for position is called the azimuth. Azimuth is the horizontal angle Az of the location on the Earth, measured clockwise from a - line pointing due north. -
Rewarding Energy Innovation to Achieve Climate Stabilization
Case Western Reserve University School of Law Scholarly Commons Faculty Publications 2011 Eyes on a Climate Prize: Rewarding Energy Innovation to Achieve Climate Stabilization Jonathan H. Adler Case Western University School of Law, [email protected] Follow this and additional works at: https://scholarlycommons.law.case.edu/faculty_publications Part of the Environmental Law Commons, and the Science and Technology Law Commons Repository Citation Adler, Jonathan H., "Eyes on a Climate Prize: Rewarding Energy Innovation to Achieve Climate Stabilization" (2011). Faculty Publications. 656. https://scholarlycommons.law.case.edu/faculty_publications/656 This Article is brought to you for free and open access by Case Western Reserve University School of Law Scholarly Commons. It has been accepted for inclusion in Faculty Publications by an authorized administrator of Case Western Reserve University School of Law Scholarly Commons. \\jciprod01\productn\H\HLE\35-1\HLE101.txt unknown Seq: 1 14-MAR-11 12:33 EYES ON A CLIMATE PRIZE:REWARDING ENERGY INNOVATION TO ACHIEVE CLIMATE STABILIZATION Jonathan H. Adler* Stabilizing atmospheric concentrations of greenhouse gases at double their pre-in- dustrial levels (or lower) will require emission reductions far in excess of what can be achieved at a politically acceptable cost with current or projected levels of tech- nology. Substantial technological innovation is required if the nations of the world are to come anywhere close to proposed emission reduction targets. Neither tradi- tional federal support for research and development of new technologies nor tradi- tional command-and-control regulations are likely to spur sufficient innovation. Technology inducement prizes, on the other hand, have the potential to significantly accelerate the rate of technological innovation in the energy sector. -
Lunar Distances Final
A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem. -
Overruling As a Speech Act: Performativity and Normative Discourse
Prepublication Draft 2009 Overruling as a speech act: performativity and normative discourse Ross CHARNOCK Université de Paris Abstract: In the common law system, judges are said to be bound by precedents decided in courts of the same level or above. However, in higher courts, under certain conditions, they have the right to overrule. Overruling declarations may be analysed as performative speech acts, having the effect of changing the law. This analysis raises both linguistic and legal problems, discussed with reference to English and American law and language. As the judges are reluctant to be seen to be assuming a legislative function, they tend to use indirect rather than explicit language, especially in the most significant cases. Alternatively, they present their overruling decisions not as new legislation, but rather as declarations of the true state of the unchanging common law. However, this view implies increased illocutionary force, as it may involve retrospective application. Secondly, the legal validity of overruling declarations depends to a large extent on their perlocutionary effects. Even after successful performance, these effects may be cancelled by later decisions in higher courts. Finally, the legal effect of overruling decisions suggests a close relation between performativity and normativity. However, this relation does not in itself provide a satisfactory explanation of the normativity of judicial discourse. 1. Introduction It is trivially true that legal procedure involves performative utterances. In criminal trials, in the common law system at least, the accused is required to plead guilty or not guilty. During the interrogation of witnesses, legal representatives may declare an objection to a particular line of questioning, using either the explicit performative form (“I object”), or, perhaps more typically through the conventional use of the single word “objection”. -
Navigation and the Age of Exploration
MODULE 3: NAVIGATION AND THE AGE OF EXPLORATION OVERVIEW Since ancient times, humans have looked up at the stars. The patterns they saw appeared unchanging; Greek and Roman observers grouped the stars in constellations that looked exactly the same from year to year. They saw their gods, heroes, and animals in the heavens: Orion the Hunter, Cassiopeia the Queen, the Great and Small Bears, Leo the Lion, Cygnus the Swan; and so forth. The stars’ constancy supported Aristotle’s theory of the earth-centered universe; more practically, the stars’ positions enabled early travelers to navigate at night. The Romans used the stars chiefly to determine direction (rather than position). The most important of the stars was the North Star, or Polaris. In the northern hemisphere, it never changed its position; it seemed to be a fixed point in the heavens. The North Star is not the brightest star in the northern sky, but it is still easy to locate: it is the last star in the tail of the constellation known as Ursa Minor, the Small Bear (or Little Dipper). Nearby is the Great Bear, Ursa Major (or Big Dipper). The two stars farthest from the tail of the Big Dipper are the pointer stars: they always point to the North Star. The Big Dipper appears to wheel around the North Star as the seasons change, high above it in the summer and below it in the winter; but the pointer stars always direct the eye to the one star whose position in the night sky never changes. For a picture showing the relative position of both the Big and Little Dippers, go to the Mystic Seaport website: www.mysticseaport.org/public/education/planetarium. -
John Harrison (1693-1776) and the Heroics of Longitude
DOI 10.6094/helden.heroes.heros./2014/02/09 Ulrike Zimmermann 119 John Harrison (1693-1776) and the Heroics of Longitude 1. A Symposium and a Rediscovery bestseller, and Dava Sobel embarked on a car eer as a wellknown and respected author of 2 When American journalist Dava Sobel attended popular science books. the Longitude Symposium of Harvard Univer Dava Sobel’s first subject already was his sity at Cambridge, Massachusetts, in November tory, albeit part of an unaccountably hidden or 1993, she did not expect anything decisive to at least underrated history. John Harrison was a come out of either the conference or her attend carpenter and selftaught clockmaker, who was ance. “500 people from seventeen countries” born in Yorkshire and spent his early life in Bar came together to hold “a conference about the rowuponHumber, North Lincolnshire. He would history of finding longitude at sea,” W. H. An prob ably have spent his life in obscur ity had he drewes, curator of the scientific instruments col not solved one of the major techno logical prob lec tion at Harvard, notes in his introduction to lems of his time, the problem of how to determine the conference proceedings (Andrewes, Intro a ship’s eastwest position, its longitude, at sea. duction 1). Despite the sizable number of par Harrison has a firm place in the his tory of navi ticipants, the Longitude Symposium was at first gation, and would have been known amongs t sight a convention of specialists sharing their horologists, clock and watch makers, and nava l knowledge and discussing finer points of their historians. -
Types of Coordinate Systems What Are Map Projections?
What are map projections? Page 1 of 155 What are map projections? ArcGIS 10 Within ArcGIS, every dataset has a coordinate system, which is used to integrate it with other geographic data layers within a common coordinate framework such as a map. Coordinate systems enable you to integrate datasets within maps as well as to perform various integrated analytical operations such as overlaying data layers from disparate sources and coordinate systems. What is a coordinate system? Coordinate systems enable geographic datasets to use common locations for integration. A coordinate system is a reference system used to represent the locations of geographic features, imagery, and observations such as GPS locations within a common geographic framework. Each coordinate system is defined by: Its measurement framework which is either geographic (in which spherical coordinates are measured from the earth's center) or planimetric (in which the earth's coordinates are projected onto a two-dimensional planar surface). Unit of measurement (typically feet or meters for projected coordinate systems or decimal degrees for latitude–longitude). The definition of the map projection for projected coordinate systems. Other measurement system properties such as a spheroid of reference, a datum, and projection parameters like one or more standard parallels, a central meridian, and possible shifts in the x- and y-directions. Types of coordinate systems There are two common types of coordinate systems used in GIS: A global or spherical coordinate system such as latitude–longitude. These are often referred to file://C:\Documents and Settings\lisac\Local Settings\Temp\~hhB2DA.htm 10/4/2010 What are map projections? Page 2 of 155 as geographic coordinate systems.