Impact Hazard Communication Risk Study: 2007 VK184 Laura Delgado
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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. -
Using a Nuclear Explosive Device for Planetary Defense Against an Incoming Asteroid
Georgetown University Law Center Scholarship @ GEORGETOWN LAW 2019 Exoatmospheric Plowshares: Using a Nuclear Explosive Device for Planetary Defense Against an Incoming Asteroid David A. Koplow Georgetown University Law Center, [email protected] This paper can be downloaded free of charge from: https://scholarship.law.georgetown.edu/facpub/2197 https://ssrn.com/abstract=3229382 UCLA Journal of International Law & Foreign Affairs, Spring 2019, Issue 1, 76. This open-access article is brought to you by the Georgetown Law Library. Posted with permission of the author. Follow this and additional works at: https://scholarship.law.georgetown.edu/facpub Part of the Air and Space Law Commons, International Law Commons, Law and Philosophy Commons, and the National Security Law Commons EXOATMOSPHERIC PLOWSHARES: USING A NUCLEAR EXPLOSIVE DEVICE FOR PLANETARY DEFENSE AGAINST AN INCOMING ASTEROID DavidA. Koplow* "They shall bear their swords into plowshares, and their spears into pruning hooks" Isaiah 2:4 ABSTRACT What should be done if we suddenly discover a large asteroid on a collision course with Earth? The consequences of an impact could be enormous-scientists believe thatsuch a strike 60 million years ago led to the extinction of the dinosaurs, and something ofsimilar magnitude could happen again. Although no such extraterrestrialthreat now looms on the horizon, astronomers concede that they cannot detect all the potentially hazardous * Professor of Law, Georgetown University Law Center. The author gratefully acknowledges the valuable comments from the following experts, colleagues and friends who reviewed prior drafts of this manuscript: Hope M. Babcock, Michael R. Cannon, Pierce Corden, Thomas Graham, Jr., Henry R. Hertzfeld, Edward M. -
General Assembly Distr.: General 16 November 2012
United Nations A/AC.105/C.1/106 General Assembly Distr.: General 16 November 2012 Original: English Committee on the Peaceful Uses of Outer Space Scientific and Technical Subcommittee Fiftieth session Vienna, 11-22 February 2013 Item 12 of the provisional agenda* Near-Earth objects Information on research in the field of near-Earth objects carried out by Member States, international organizations and other entities Note by the Secretariat I. Introduction 1. In accordance with the multi-year workplan adopted by the Scientific and Technical Subcommittee of the Committee on the Peaceful Uses of Outer Space at its forty-fifth session, in 2008 (A/AC.105/911, annex III, para. 11), and extended by the Subcommittee at its forty-eighth session in 2011 (A/AC.105/987, annex III, para. 9), Member States, international organizations and other entities were invited to submit information on research in the field of near-Earth objects for the consideration of the Working Group on Near-Earth Objects, to be reconvened at the fiftieth session of the Subcommittee. 2. The present document contains information received from Germany and Japan, and the Committee on Space Research, the International Astronomical Union and the Secure World Foundation. __________________ * A/AC.105/C.1/L.328. V.12-57478 (E) 041212 051212 *1257478* A/AC.105/C.1/106 II. Replies received from Member States Germany [Original: English] [29 October 2012] The national activities listed below are based on the strong involvement of the Institute of Planetary Research of the German Aerospace Centre (DLR). DLR uses the Spitzer SpaceTelescope of the National Aeronautics and Space Administration (NASA) for an infrared survey (“ExploreNEOs”) of the physical properties of 750 near-Earth objects, as part of an international team. -
The Tumbling Spin State of (99942) Apophis
The tumbling spin state of (99942) Apophis P. Pravec a, P. Scheirich a, J. Durechˇ b, J. Pollock c, P. Kuˇsnir´ak a, K. Hornoch a, A. Gal´ad a, D. Vokrouhlick´y b, A.W. Harris d, E. Jehin e, J. Manfroid e, C. Opitom e, M. Gillon e, F. Colas g, J. Oey h, J. Vraˇstil a,b, D. Reichart f, K. Ivarsen f, J. Haislip f, A. LaCluyze f aAstronomical Institute, Academy of Sciences of the Czech Republic, Friˇcova 1, CZ-25165 Ondˇrejov, Czech Republic bInstitute of Astronomy, Faculty of Mathematics and Physics, Charles University, Prague, V Holeˇsoviˇck´ach 2, CZ-18000 Prague 8, Czech Republic cPhysics and Astronomy Department, Appalachian State University, Boone, NC 28608, U.S.A. dMoreData! Inc., 4603 Orange Knoll Avenue, La Ca˜nada, CA 91011, U.S.A. eInstitut d’Astrophysique de l’Universit´ede Li`ege, Alle du 6 Aout 17, B-4000 Li`ege, Belgium f Physics and Astronomy Department, University of North Carolina, Chapel Hill, NC 27514, U.S.A. gIMCCE-CNRS-Observatoire de Paris, 77 avenue Denfert Rochereau, 75014 Paris, France hLeura Observatory, Leura, N.S.W., Australia 2014 January 22 Preprint submitted to Elsevier 22 January 2014 Proposed running head: Apophis tumbling Editorial correspondence to: Dr. Petr Pravec Astronomical Institute AS CR Friˇcova 1 Ondˇrejov CZ-25165 Czech Republic Phone: 00420-323-620352 Fax: 00420-323-620263 E-mail address: [email protected] 2 Abstract Our photometric observations of asteroid (99942) Apophis from December 2012 to April 2013 revealed it to be in a state of non-principal axis rotation (tumbling). -
Negotiating Uncertainty: Asteroids, Risk and the Media Felicity Mellor
Accepted pre-publication version Published at: Public Understanding of Science 19(1): (2010) 16-33. Negotiating Uncertainty: Asteroids, Risk and the Media Felicity Mellor ABSTRACT Natural scientists often appear in the news media as key actors in the management of risk. This paper examines the way in which a small group of astronomers and planetary scientists have constructed asteroids as risky objects and have attempted to control the media representation of the issue. It shows how scientists negotiate the uncertainties inherent in claims about distant objects and future events by drawing on quantitative risk assessments even when these are inapplicable or misleading. Although the asteroid scientists worry that media coverage undermines their authority, journalists typically accept the scientists’ framing of the issue. The asteroid impact threat reveals the implicit assumptions which can shape natural scientists’ public discourse and the tensions which arise when scientists’ quantitative uncertainty claims are re-presented in the news media. Keywords: asteroids, impact threat, astronomy, risk, uncertainty, science journalism, media, science news Introduction Over the past two decades, British newspapers have periodically announced the end of the world. Playful headlines such as “The End is Nigh” and “Armageddon Outta Here!” are followed a few days later by reports that there’s no danger after all: “PHEW. The end of the world has been cancelled” (Britten, 1998; Wickham, 2002; Evening Standard , 1998). These stories, and others like them appearing in news media around the world, deal with the possibility that an asteroid or comet may one day collide with the Earth causing global destruction. The threat posed by near-Earth objects (NEOs) has been actively promoted by a group of astronomers and planetary scientists since the late 1980s. -
Revised Asteroid Scale Aids Understanding of Impact Risk 12 April 2005
Revised asteroid scale aids understanding of impact risk 12 April 2005 Astronomers led by an MIT professor have revised object is almost always likely to reduce the hazard the scale used to assess the threat of asteroids level to 0, once sufficient data are obtained." The and comets colliding with Earth to better general process of classifying NEO hazards is communicate those risks with the public. roughly analogous to hurricane forecasting. The overall goal is to provide easy-to-understand Predictions of a storm's path are updated as more information to assuage concerns about a potential and more tracking data are collected. doomsday collision with our planet. The Torino scale, a risk-assessment system similar According to Dr. Donald K. Yeomans, manager of to the Richter scale used for earthquakes, was NASA's Near Earth Object Program Office, "The adopted by a working group of the International revisions in the Torino Scale should go a long way Astronomical Union (IAU) in 1999 at a meeting in toward assuring the public that while we cannot Torino, Italy. On the scale, zero means virtually no always immediately rule out Earth impacts for chance of collision, while 10 means certain global recently discovered near-Earth objects, additional catastrophe. observations will almost certainly allow us to do so." "The idea was to create a simple system The highest Torino level ever given an asteroid was conveying clear, consistent information about near- a 4 last December, with a 2 percent chance of Earth objects [NEOs]," or asteroids and comets hitting Earth in 2029. And after extended tracking of that appear to be heading toward the planet, said the asteroid's orbit, it was reclassified to level 0, Richard Binzel, a professor in MIT's Department of effectively no chance of collision, "the outcome Earth, Atmospheric and Planetary Sciences and correctly emphasized by level 4 as being most the creator of the scale. -
Planetary Defense: Near-Earth Objects, Nuclear Weapons, and International Law James A
Hastings International and Comparative Law Review Volume 42 Article 2 Number 1 Winter 2019 Winter 2019 Planetary Defense: Near-Earth Objects, Nuclear Weapons, and International Law James A. Green Follow this and additional works at: https://repository.uchastings.edu/ hastings_international_comparative_law_review Part of the Comparative and Foreign Law Commons, and the International Law Commons Recommended Citation James A. Green, Planetary Defense: Near-Earth Objects, Nuclear Weapons, and International Law, 42 Hastings Int'l & Comp.L. Rev. 1 (2019). Available at: https://repository.uchastings.edu/hastings_international_comparative_law_review/vol42/iss1/2 This Article is brought to you for free and open access by the Law Journals at UC Hastings Scholarship Repository. It has been accepted for inclusion in Hastings International and Comparative Law Review by an authorized editor of UC Hastings Scholarship Repository. Planetary Defense: Near-Earth Objects, Nuclear Weapons, and International Law BY JAMES A. GREEN ABSTRACT The risk of a large Near-Earth Object (NEO), such as an asteroid, colliding with the Earth is low, but the consequences of that risk manifesting could be catastrophic. Recent years have witnessed an unprecedented increase in global political will in relation to NEO preparedness, following the meteoroid impact in Chelyabinsk, Russia in 2013. There also has been an increased focus amongst states on the possibility of using nuclear detonation to divert or destroy a collision- course NEO—something that a majority of scientific opinion now appears to view as representing humanity’s best, or perhaps only, option in extreme cases. Concurrently, recent developments in nuclear disarmament and the de-militarization of space directly contradict the proposed “nuclear option” for planetary defense. -
Defending Earth: the Threat from Asteroid and Comet Impact
Defending Earth: The Threat from Asteroid and Comet Impact Version A | 05 September 2009 Mr. A.C. Charania President, Commercial Division | SpaceWorks Engineering, Inc. (SEI) | [email protected] | 1+770.379.8006 Acknowledgments: Multiple slides from Dr. Clark Chapman, Southwest Research Institute Boulder, Colorado, USA, URL: www.boulder.swri.edu/~cchapman 1 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero Source: NASA/JPL/Infrared Telescope Facility 2009 Jupiter Impact Event: 19 July 2009 (1 km Sized Object) 2 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero Source: JPL / NASA Spitzer Space Telescope 95 Light Years Away (Star HD 172555): Moon-Sized Object Impacts Mercury-Sized Object at 10 km/s (5.8+/-0.6 AU Orbit) 3 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero SPACEWORKS 4 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero KEY CUSTOMERS AND PRODUCTS 5 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero DOMAIN OF EXPERTISE: ADVANCED CONCEPTS 6 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero INTRODUCTION 7 Copyright 2009, SpaceWorks Engineering, Inc. (SEI) | www.sei.aero − Asteroid - A relatively small, inactive, rocky body orbiting the Sun − Comet - A relatively small, at times active, object whose ices can vaporize in sunlight forming an atmosphere (coma) of dust and gas and, sometimes, a tail of dust and/or gas − Meteoroid - A small particle from a comet or asteroid orbiting the Sun − Meteor - The light phenomena which results when a meteoroid enters the Earth's atmosphere and vaporizes; a shooting star − Meteorite -A meteoroid that survives its passage through the Earth's atmosphere and lands upon the Earth's surface − NEO - Near Earth Object (within 0.3 AU) − PHOs - Potentially Hazardous Objects (within 0.025 AU) COMMON DEFINITIONS 8 Copyright 2009, SpaceWorks Engineering, Inc. -
NASA's Near-Earth Object Program Overview Don Yeomans/JPL
NASA’sNational Aeronautics and Near-Earth Object Program Overview Space Administration Jet Propulsion Laboratory California Institute of Technology Don Yeomans/JPL Pasadena, California National Aeronautics and Space Administration The Population of Near-Earth Objects is Jet Propulsion Laboratory California Institute of Technology Pasadena, California Made Up of Active Comets (1%) and Asteroids (99%) Comets (Weak and very black icy dust balls) •Weak collection of talcum-powder sized silicate dust •About 30% ices (mostly water) just below surface dust •Fairly recent resurfacing and few impact craters •Some evidence that comet Tempel 1 does not have a uniform composition (i.e., more CO2 in south) Asteroids (run the gamut from wimpy ex-comet fluff balls to slabs of iron •Most are shattered fragments of larger asteroids •Rubble rock piles - like Itokawa •Shattered (but coherent) rock - like Eros •Solid rock •Solid slabs of iron - like Meteor crater object National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology History of Known NEO Population Pasadena, California 201018001900195019901999 The Inner Solar System in 2006 Known • 500,000 minor planets Earth • 7100 NEOs • ~1100 PHOs Crossing New Survey Will Outside Likely Find Earth’s • 25,000+ NEOs Orbit (> 140m) • 5,000+ PHOs Scott Manley Armagh Observatory National Aeronautics and Space Administration NASA’s Current Jet Propulsion Laboratory California Institute of Technology Pasadena, California NEO Search Surveys NEO Program Office @ JPL LINEAR, Socorro NM • Program coordination • Automated SENTRY http://neo.jpl.nasa.gov/ Minor Planet Center (MPC) • IAU sanctioned • Discovery Clearinghouse • Initial Orbit Determination Spacewatch Tucson, AZ NASA’s NEO Observations Catalina Sky Program run by Lindley Johnson Survey (SMD) Tucson AZ & Australia National Aeronautics and Space Administration Jet Propulsion Laboratory NASA NEO Survey California Institute of Technology Pasadena, California Discoveries NASA goal is to discover 90% of NEAs larger than 1 km. -
NASA's Near-Earth Object Program
NASA’s Near-Earth Object Program (Spaceguard) Don Yeomans Manager, NASA Near-Earth Object Program Office Meteor Crater Arizona History of Known NEO Population The Inner Solar System in 2006 201118001900195019901999 Known • 500,000 Earth minor planets Crossing •7750 NEOs Outside • 1200 PHAs Earth’s Orbit Scott Manley Armagh Observatory NASA’s NEO Search Program (Current Systems) Minor Planet Center (MPC) • IAU sanctioned NEO-WISE • Int’l observation database • Initial orbit determination www.cfa.harvard.edu/iau/mpc. html NEO Program Office @ JPL • Program coordination JPL • Precision orbit determination Sun-synch LEO • Automated SENTRY www.neo.jpl.nasa.gov Catalina Sky Pan-STARRS LINEAR Survey MIT/LL UofAZ Arizona & Australia Uof HI Soccoro, NM Haleakula, Maui3 The Importance of Near-Earth Objects •Science •Future Space Resources •Planetary Defense •Exploration NASA’s NEO Program Office at JPL Coordination and Metrics Automatic orbit updates as new data arrive SENTRY system Relational database for NEO orbits & characteristics Conduct research on: Discovery efficiency Improving observational data Modeling dynamics Optimal mitigation processes Impact warnings & outreach http://www.jpl.nasa.gov/asteroidwatch / NEO Program Office: http://neo.jpl.nasa.gov/ Near-Earth Asteroid Discoveries Start of NASA NEO Program Discovery Completion Within Size Intervals 40% 8% <1% 87% JPL’s SENTY NEO Risk Page http://neo.jpl.nasa.gov/risk/ Object Year Potential Impact Velocity H Estimated Palermo Torino Designation Range Impacts Prob. (km/s) (mag.) Diameter -
Russian Networks Capable to Observe Neos at Near Space
52-th Session of STSC UN COPUOS Vienna, Austria, February 3, 2015 The NEO problem: current activities in Russia V.Emel’yanenko Basic aspects of the NEO problem Major constituents of the NEO (Asteroid/Comet Impact Hazard - ACH) problem are: Detection and characterization Risk assessment Protection and mitigation We work in all areas at both national and international levels. 2 General activities (Feb 2014 – Feb 2015) Studies of the Chelyabinsk meteorite; Completion of the 1.6 m telescope for NEO detection; Work on the development of a moderate aperture telescope national network aimed to detection and monitoring of NEOs; Various projects of space based means to detect and to counteract dangerous bodies; Construction of a data-bank on impact consequences . 3 Some lessons of the Chelyabinsk event (15 Feb, 2013): Asteroids of decameter size could be very dangerous; We need to know about coming threat reasonably in advance; Day time asteroids are unobservable by any ground based facilities. 4 En route to the NEO detection AZT-33IR AZT-33VM The telescope АZТ-33VM ( ∅ 1.6 m) for the mass detection of NEOs at large distances is nearing completion. First light is expected in the fall of 2015. 5 ISON telescopes for NEO surveys and follow- up observations ISON (International Scientific Optical Network) – one of the largest Russian networks capable to observe NEOs at near space. 6 ISON : results on asteroids Hundreds of light curves were constructed for tens of NEAs (3122) Florence, (20187) Janapittichova, (25916) 2001 CP44, (162004) 1991 VE, (7888) -
Modelización De Cráteres De Impacto
–– Modelización de cráteres de impacto Autores: Jesús Ordoño y Carlos Tadeo Tutor: Joan Alberich Institut Frederic Mompou Sant Vicenç dels Horts Modelización de cráteres de impacto Jesús Ordoño, Carlos Tadeo ÍNDICE Motivación y agradecimientos 2 Proceso de elaboración del Trabajo de Investigación y objetivos científicos alcanzados 4 1. Asteroides, meteoritos, cometas y cráteres de impacto 6 2. Modelización de cráteres de impacto 13 2.1. Introducción 13 2.2. Material utilizado 16 2.2.1. Datos de las canicas 17 2.2.2. Datos de la superficie de impacto 22 2.2.3. Dispositivo de lanzamiento 23 2.3. Procedimiento 25 2.4. Resultados obtenidos 28 2.4.1. Relación de los cráteres con el diámetro de las canicas 28 2.4.2. Relación de los cráteres con la masa y la densidad de las canicas 40 2.4.3. Relación de los cráteres con la energía cinética de las canicas 42 2.4.4. Relación de la profundidad de los cráteres con el diámetro de los mismos 45 3. Aplicación del modelo de cráteres de impacto a cráteres reales de la Tierra 47 3.1 Aplicación del modelo de cráteres de impacto en meteor Crater de Arizona: parámetro de control 48 3.2. Determinación del diámetro del meteorito en cráteres terrestres 51 3.3. Peligros espaciales: medidas de posibles cráteres producidos por asteroides cercanos a la Tierra 69 4. Aplicación del modelo de cráteres de impacto en otros cuerpos del Sistema Solar 81 4.1. Cráteres en planetas interiores 81 4.2. Cráteres en satélites de planetas exteriores 85 Conclusiones 89 Bibliografía 91 1 Modelización de cráteres de impacto Jesús Ordoño, Carlos Tadeo Motivación y agradecimientos Este estudio de los cráteres de impacto se gestó a raíz de nuestro interés por temas de astrofísica.