How Much Could Refuges Help Us Recover from a Global Catastrophe?
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Cross-References ASTEROID IMPACT Definition and Introduction History of Impact Cratering Studies
18 ASTEROID IMPACT Tedesco, E. F., Noah, P. V., Noah, M., and Price, S. D., 2002. The identification and confirmation of impact structures on supplemental IRAS minor planet survey. The Astronomical Earth were developed: (a) crater morphology, (b) geo- 123 – Journal, , 1056 1085. physical anomalies, (c) evidence for shock metamor- Tholen, D. J., and Barucci, M. A., 1989. Asteroid taxonomy. In Binzel, R. P., Gehrels, T., and Matthews, M. S. (eds.), phism, and (d) the presence of meteorites or geochemical Asteroids II. Tucson: University of Arizona Press, pp. 298–315. evidence for traces of the meteoritic projectile – of which Yeomans, D., and Baalke, R., 2009. Near Earth Object Program. only (c) and (d) can provide confirming evidence. Remote Available from World Wide Web: http://neo.jpl.nasa.gov/ sensing, including morphological observations, as well programs. as geophysical studies, cannot provide confirming evi- dence – which requires the study of actual rock samples. Cross-references Impacts influenced the geological and biological evolu- tion of our own planet; the best known example is the link Albedo between the 200-km-diameter Chicxulub impact structure Asteroid Impact Asteroid Impact Mitigation in Mexico and the Cretaceous-Tertiary boundary. Under- Asteroid Impact Prediction standing impact structures, their formation processes, Torino Scale and their consequences should be of interest not only to Earth and planetary scientists, but also to society in general. ASTEROID IMPACT History of impact cratering studies In the geological sciences, it has only recently been recog- Christian Koeberl nized how important the process of impact cratering is on Natural History Museum, Vienna, Austria a planetary scale. -
Geological Timeline
Geological Timeline In this pack you will find information and activities to help your class grasp the concept of geological time, just how old our planet is, and just how young we, as a species, are. Planet Earth is 4,600 million years old. We all know this is very old indeed, but big numbers like this are always difficult to get your head around. The activities in this pack will help your class to make visual representations of the age of the Earth to help them get to grips with the timescales involved. Important EvEnts In thE Earth’s hIstory 4600 mya (million years ago) – Planet Earth formed. Dust left over from the birth of the sun clumped together to form planet Earth. The other planets in our solar system were also formed in this way at about the same time. 4500 mya – Earth’s core and crust formed. Dense metals sank to the centre of the Earth and formed the core, while the outside layer cooled and solidified to form the Earth’s crust. 4400 mya – The Earth’s first oceans formed. Water vapour was released into the Earth’s atmosphere by volcanism. It then cooled, fell back down as rain, and formed the Earth’s first oceans. Some water may also have been brought to Earth by comets and asteroids. 3850 mya – The first life appeared on Earth. It was very simple single-celled organisms. Exactly how life first arose is a mystery. 1500 mya – Oxygen began to accumulate in the Earth’s atmosphere. Oxygen is made by cyanobacteria (blue-green algae) as a product of photosynthesis. -
A Dystopian Booklist* Norwell High School Library Media Center
The Worst is Yet to Come: a Dystopian Booklist* Norwell High School Library Media Center Dystopia: 1. a society characterized by human misery, squalor, oppression, disease, and overcrowding; 2. an imaginary place where everything is as bad as it can be Anthony, Joelle. Restoring Harmony - Ten years after the Great Collapse of 2031, Molly McClure leaves the safety of her family's island home to travel through a dangerous and desolate wasteland to find her grandparents and persuade them to return with her to Canada. Atwood, Margaret. Handmaid’s Tale - It is the world of the near future, and Offred is a Handmaid in the home of the Commander and his wife. She is allowed out once a day to the food market, she is not permitted to read, and she is hoping the Commander makes her pregnant, because she is only valued if her ovaries are viable. Offred can remember the years before, when she was an independent woman, had a job of her own, a husband and child. But all of that is gone now...everything has changed. (summary description from OCLN Library Catalog) Bacigalupi, Paolo. Ship Breaker - In a futuristic world, teenaged Nailer scavenges copper wiring from grounded oil tankers for a living, but when he finds a beached ship with a girl in the wreckage, he has to decide if he should strip the ship or rescue the girl. The Drowned Cities - In a future America that has devolved into unending civil wars, Mahlia and Mouse barely escape the war-torn lands of the Drowned Cities, but their safety is soon threatened and Mahlia will have to risk everything if she is to save Mouse. -
Asteroid Impact, Not Volcanism, Caused the End-Cretaceous Dinosaur Extinction
Asteroid impact, not volcanism, caused the end-Cretaceous dinosaur extinction Alfio Alessandro Chiarenzaa,b,1,2, Alexander Farnsworthc,1, Philip D. Mannionb, Daniel J. Luntc, Paul J. Valdesc, Joanna V. Morgana, and Peter A. Allisona aDepartment of Earth Science and Engineering, Imperial College London, South Kensington, SW7 2AZ London, United Kingdom; bDepartment of Earth Sciences, University College London, WC1E 6BT London, United Kingdom; and cSchool of Geographical Sciences, University of Bristol, BS8 1TH Bristol, United Kingdom Edited by Nils Chr. Stenseth, University of Oslo, Oslo, Norway, and approved May 21, 2020 (received for review April 1, 2020) The Cretaceous/Paleogene mass extinction, 66 Ma, included the (17). However, the timing and size of each eruptive event are demise of non-avian dinosaurs. Intense debate has focused on the highly contentious in relation to the mass extinction event (8–10). relative roles of Deccan volcanism and the Chicxulub asteroid im- An asteroid, ∼10 km in diameter, impacted at Chicxulub, in pact as kill mechanisms for this event. Here, we combine fossil- the present-day Gulf of Mexico, 66 Ma (4, 18, 19), leaving a crater occurrence data with paleoclimate and habitat suitability models ∼180 to 200 km in diameter (Fig. 1A). This impactor struck car- to evaluate dinosaur habitability in the wake of various asteroid bonate and sulfate-rich sediments, leading to the ejection and impact and Deccan volcanism scenarios. Asteroid impact models global dispersal of large quantities of dust, ash, sulfur, and other generate a prolonged cold winter that suppresses potential global aerosols into the atmosphere (4, 18–20). These atmospheric dinosaur habitats. -
Sustainable Development, Technological Singularity and Ethics
European Research Studies Journal Volume XXI, Issue 4, 2018 pp. 714- 725 Sustainable Development, Technological Singularity and Ethics Vyacheslav Mantatov1, Vitaly Tutubalin2 Abstract: The development of modern convergent technologies opens the prospect of a new technological order. Its image as a “technological singularity”, i.e. such “transhuman” stage of scientific and technical progress, on which the superintelligence will be practically implemented, seems to be quite realistic. The determination of the basic philosophical coordinates of this future reality in the movement along the path of sustainable development of mankind is the most important task of modern science. The article is devoted to the study of the basic ontological, epistemological and moral aspects in the reception of the coming technological singularity. The method of this study is integrating dialectical and system approach. The authors come to the conclusion: the technological singularity in the form of a “computronium” (superintelligence) opens up broad prospects for the sustainable development of mankind in the cosmic dimension. This superintelligence will become an ally of man in the process of cosmic evolution. Keywords: Technological Singularity, Superintelligence, Convergent Technologies, Cosmocentrism, Human and Universe JEL code: Q01, Q56. 1East Siberia State University of Technology and Management, Ulan-Ude, Russia [email protected] 2East Siberia State University of Technology and Management, Ulan-Ude, Russia, [email protected] V. Mantatov, V. Tutubalin 715 1. Introduction Intelligence organizes the world by organizing itself. J. Piaget Technological singularity is defined as a certain moment or stage in the development of mankind, when scientific and technological progress will become so fast and complex that it will be unpredictable. -
Reducing Nuclear Risks in Europe a FRAMEWORK for ACTION
Reducing A FrAmework For Action Nuclear Risks e dited by Steve AndreASen in Europe And iSAbelle williAmS Featured essay: “the race between Cooperation and catastrophe” by sam NuNN Reducing Nuclear Risks in Europe a FrameWork For acTIoN Edit eD by STeve aNDreaSeN aND ISabelle WIllIamS Featured essay: “The race between Cooperation and catastrophe” by sam NuNN Nuclear ThreaT INITIaTIve Washington, D.c. t he Nuclear threat INItIatIve NTI is a nonprofit, nonpartisan organization with a mission to strengthen global security by reducing the risk of use and preventing the spread of nuclear, biological, and chemical weapons, and to work to build the trust, transparency, and security that are preconditions to the ultimate fulfillment of the Non-Proliferation Treaty’s goals and ambitions. www.nti.org The views expressed in this publication are the authors’ own and do not reflect those of NTI, its Board of Directors, or other institutions with which the authors are associated. © 2011 the Nuclear Threat Initiative All rights reserved. No part of this publication may be reproduced, stored in a retrieval sys- tem, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, or otherwise, without written permission of the publisher and copyright holder. c over phoTo oF a u.S. aIr Force F-16 FIghTINg FalcoN aIrcraFT courTeSy oF The u.S. aIr Force. phoTo by maSTer SgT. WIllIam greer/releaSeD. ii T able oF coNTeNTS Acknowledgments v Authors and Reviewers vii summary coNteNt executive summary: Reassembling a More Credible NATO Nuclear Policy and Posture 1 Joan Rohlfing, Isabelle Williams, and Steve Andreasen featured essay: The Race Between Cooperation and Catastrophe 8 Sam Nunn chaPters 1. -
A Critical Look at Catastrophe Risk Assessments
CERN-TH/2000-029 DAMTP-2000-105 hep-ph/0009204 A critical look at catastrophe risk assessments Adrian Kent Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge CB3 9EW, U.K. (September 15, 2000) Recent papers by Busza et al. (BJSW) and Dar et al. (DDH) argue that astrophysical data can be used to establish small bounds on the risk of a \killer strangelet" catastrophe scenario in forthcoming collider experiments. The case for the safety of the experiments set out by BJSW does not rely on these bounds, but on theoretical arguments, which BJSW find sufficiently compelling to firmly exclude any possibility of catastrophe. However, DDH and other commentators (initially including BJSW) have suggested that these empirical bounds alone do give sufficient reassurance. We note that this seems unsupportable when the bounds are expressed in terms of expected cost | a good measure, according to standard risk 8 analysis arguments. For example, DDH's main bound, pcatastrophe < 2 10− , implies only that the expectation value of the number of deaths is bounded by 120. × We thus reappraise the DDH and BJSW risk bounds by comparing risk policy in other areas. 15 We find that requiring a catastrophe risk of no higher than 10− per year is necessary to be consistent with established policy for risk optimisation from radiation≈ hazards, even if highly risk tolerant assumptions are made and no value is placed on the lives of future generations. A respectable case can be made for requiring a bound many orders of magnitude smaller. We conclude that the costs of small risks of catastrophe have been significantly underestimated in the physics literature, with obvious implications for future policy. -
Hayles Program in Literature, Duke University, North Carolina
Response Essay After shocks: Posthuman ambivalence N. Katherine Hayles Program in Literature, Duke University, North Carolina. postmedieval: a journal of medieval cultural studies (2010) 1, 262–271. doi:10.1057/pmed.2010.28 When I began writing How We Became Posthuman (1999), I was drawn to the topic in part because of the intense ambivalence I felt toward the idea of the posthuman. I thought, no doubt naively, that writing would help me resolve it. Far from overcoming mixed feelings, the writing intensified my emotions by bringing the issues into sharper focus. As David Gary Shaw rightly observes, the book is drenched in feelings – feelings of dread, possibility and hope. More than a decade later, my ambivalence remains unresolved. I do not doubt that coming decades will see us plunging deeper into what I have elsewhere called the regime of computation, creating more intelligent machines and more pervasive data systems that, having already transformed the meaning of ‘human,’ will continue to do so with increasing urgency and momentum. What are we to make of this trajectory, and what are the possibilities for constructive interventions? While I have not escaped dread in contemplating these questions, I want to focus in this inaugural issue of postmedieval on what posthumanism can offer to premodern studies, and what premodern studies can offer to posthumanism. In my view, we cannot prevent the regime of computation from continuing to expand, but we have an opportunity to interpret it in ways that may help to maximize its positive potential and minimize its risks. With this objective in mind, I want to focus on three areas that seem to me particularly promising, richly explored in the essays in this collection: futurity, non-human others and distributed cognition. -
16401729.Pdf
............. C/86-1 Neither MAD nor Starstruck -- and Doubts, Too, About Arms Control by George W. Rathjens and Laura Reed Defense and Arms Control Studies Program Massachusetts Institute of Technology Center for International Studies Cambridge, Massachusetts 02139 March 1986 2/26/86 Neither MAD nor Starstruck -- and Doubts, Too, About Arms Control* George W. Rathjens Laura Reed Throughout the whole of the post-World War II period there have been strong differences over aspects of American nuclear policy; notably, about the sizing of nuclear forces, about particular weapons systems (e.g. the B-1 bomber and the MX missile), and most significantly about the role of nuclear weapons in dealing with threats other than that of a direct attack on the United States (i.e., about "extended deterrence" and "nuclear war fighting"). But there were also broad elements of consensus, at least from the Kennedy through the Carter Administrations, on several fundamental points: 1.) There could be no effective defense of the American population and social infrastructure against Soviet nuclear weapons. Cities and most other works of humanity were seen to be so fragile and nuclear weapons so powerful that the offense would likely always have the advantage over the defense. Any effort to defend the whole country could be negated by improvements, at less cost, in Soviet offensive capabilities, and likely would be, leaving the U.S. vulnerable to total destruction. 2.) This meant that the only real hope of dealing with a possible direct Soviet attack against the United States lay in deterrence through the threat of inflicting punitive damage on the Soviet Union. -
Efficient Responses to Catastrophic Risk Richard A
University of Chicago Law School Chicago Unbound Journal Articles Faculty Scholarship 2006 Efficient Responseso t Catastrophic Risk Richard A. Posner Follow this and additional works at: https://chicagounbound.uchicago.edu/journal_articles Part of the Law Commons Recommended Citation Richard A. Posner, "Efficient Responseso t Catastrophic Risk," 6 Chicago Journal of International Law 511 (2006). This Article is brought to you for free and open access by the Faculty Scholarship at Chicago Unbound. It has been accepted for inclusion in Journal Articles by an authorized administrator of Chicago Unbound. For more information, please contact [email protected]. Efficient Responses to Catastrophic Risk Richard A. Posner* The Indian Ocean tsunami of December 2004 has focused attention on a type of disaster to which policymakers pay too little attention-a disaster that has a very low or unknown probability of occurring but that if it does occur creates enormous losses. Great as the death toll, physical and emotional suffering of survivors, and property damage caused by the tsunami were, even greater losses could be inflicted by other disasters of low (but not negligible) or unknown probability. The asteroid that exploded above Siberia in 1908 with the force of a hydrogen bomb might have killed millions of people had it exploded above a major city. Yet that asteroid was only about two hundred feet in diameter, and a much larger one (among the thousands of dangerously large asteroids in orbits that intersect the earth's orbit) could strike the earth and cause the total extinction of the human race through a combination of shock waves, fire, tsunamis, and blockage of sunlight wherever it struck. -
What Killed the Dinosaurs?
What killed the dinosaurs? The impact theory The impact theory was beautifully simple and appealing. Much of its evidence was drawn from a thin layer of rock known as the 'KT boundary'. This layer is 65 million years old (which is around the time when the dinosaurs disappeared) and is found around the world exposed in cliffs and mines. For supporters of the impact theory, the KT boundary layers contained two crucial clues. In 1979 scientists discovered that there were high concentrations of a rare element called iridium, which they thought could only have come from an asteroid. Right underneath the iridium was a layer of 'spherules', tiny balls of rock which seemed to have been condensed from rock which had been vapourised by a massive impact. On the basis of the spherules and a range of other evidence, Dr Alan Hildebrand of the University of Calgary deduced that the impact must have happened in the Yucatan peninsula, at the site of a crater known as Chicxulub. Chemical analysis later confirmed that the spherules had indeed come from rocks within the crater. The impact theory seemed to provide the complete answer. In many locations around the world, the iridium layer (evidence of an asteroid impact) sits right on top of the spherule layer (evidence that the impact was at Chicxulub). So Hildebrand and other supporters of the impact theory argued that there was one massive impact 65 million years ago, and that it was at Chicxulub. This, they concluded, must have finished off the dinosaurs by a variety of mechanisms. -
A Retrospective of Cobalt-60 Radiation Therapy: “The Atom Bomb That Saves Lives”
MEDICAL PHYSICS INTERNATIONAL Journal, Special Issue, History of Medical Physics 4, 2020 A RETROSPECTIVE OF COBALT-60 RADIATION THERAPY: “THE ATOM BOMB THAT SAVES LIVES” J. Van Dyk1, J. J. Battista1, and P.R. Almond2 1 Departments of Medical Biophysics and Oncology, Western University, London, Ontario, Canada 2 University of Texas, MD Anderson Cancer Center, Houston, Texas, United States Abstract — The first cancer patients irradiated with CONTENTS cobalt-60 gamma rays using external beam I. INTRODUCTION radiotherapy occurred in 1951. The development of II. BRIEF HISTORY OF RADIOTHERAPY cobalt-60 machines represented a momentous III. LIMITATIONS OF RADIATION THERAPY breakthrough providing improved tumour control UNTIL THE 1950s and reduced complications, along with much lower skin reactions, at a relatively low cost. This article IV. RADIOACTIVE SOURCE DEVELOPMENT provides a review of the historic context in which the V. THE RACE TO FIRST CANCER TREATMENTS advances in radiation therapy with megavoltage VI. COBALT TRUTHS AND CONSEQUENCES gamma rays occurred and describes some of the VII. COBALT TELETHERAPY MACHINE DESIGNS physics and engineering details of the associated VIII. GROWTH AND DECLINE OF COBALT-60 developments as well as some of the key locations and TELETHERAPY people involved in these events. It is estimated that IX. COBALT VERSUS LINAC: COMPETING over 50 million patients have benefited from cobalt-60 teletherapy. While the early growth in the use of MODALITIES cobalt-60 was remarkable, linear accelerators (linacs) X. OTHER USES OF COBALT-60 provided strong competition such that in the mid- XI. SUMMARY AND CONCLUSIONS 1980s, the number of linacs superseded the number of ACKNOWLEDGEMENTS cobalt machines.