The Hard Rain: Impacts, Events and Canadian Security
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
Lindley Johnson (NASA HQ) – NASA HEOMD – – NASA STMD – Tibor Balint (NASA HQ) – SSERVI – Greg Schmidt (NASA ARC) 19
September 4, 2014: Planetary Science Subcommittee Nancy Chabot, SBAG Chair 11th SBAG Meeting • July 29-31, 2014: Washington, DC • Highlights of SBAG meeting presentations from major projects • Discussion of findings • New steering committee members • Future meetings 1 NEOWISE Reac,va,on • Reac,vated in Dec 2013, NEOWISE is observing, discovering, and characterizing asteroids & comets using 3.4 and 4.6 µm channels • 7239 minor planets observed, including 157 near-Earth objects (NEOs). • 89 discoveries, including 26 NEOs and 3 comets. • NEO discoveries are large, dark • First data delivery from Reac9vaon: March 2015 to IRSA: • hp://irsa.ipac.caltech.edu/Missions/wise.html • All data from prime WISE/NEOWISE mission are publicly available through IRSA and team Comet P/2014 L2 NEOWISE papers; derived physical proper9es heading to PDS Dawn prepares to encounter Ceres PI: Alan Stern (SwRI) New Horizons Status PM: JHU-APL • Spacecraft is healthy & On-Course for Pluto (Radio) § 1.3x more fuel available for KBO Extended (High-E Plasma) NH Payload Mission phase than originally expected • Payload is healthy and well-calibrated § Finishing final Annual Checkout (ACO-8) • First Pluto OpNav Campaign conducted (UV Spectral) § See image below • Enter final Hibernation on Aug 29th (Vis-Color + IR Spectral) • Pluto Encounter begins on 2015-Jan-15 (Low-E Plasma) • Pluto Closest Approach: 2015-Jul-14 (Pan Imager) Intensive searches with ground-based facilities over the past Pluto OpNav Campaign: 2 years have not yet yielded a KBO target for NH. A 194- Cleanly separate Pluto & orbit Hubble program was started in June; below Charon shows the first potentially targetable KBO found. -
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. -
The Militarisation of Space 14 June 2021
By, Claire Mills The militarisation of space 14 June 2021 Summary 1 Space as a new military frontier 2 Where are military assets in space? 3 What are counterspace capabilities? 4 The regulation of space 5 Who is leading the way on counterspace capabilities? 6 The UK’s focus on space commonslibrary.parliament.uk Number 9261 The militarisation of space Contributing Authors Patrick Butchard, International Law, International Affairs and Defence Section Image Credits Earth from Space / image cropped. Photo by ActionVance on Unsplash – no copyright required. Disclaimer The Commons Library does not intend the information in our research publications and briefings to address the specific circumstances of any particular individual. We have published it to support the work of MPs. You should not rely upon it as legal or professional advice, or as a substitute for it. We do not accept any liability whatsoever for any errors, omissions or misstatements contained herein. You should consult a suitably qualified professional if you require specific advice or information. Read our briefing ‘Legal help: where to go and how to pay’ for further information about sources of legal advice and help. This information is provided subject to the conditions of the Open Parliament Licence. Feedback Every effort is made to ensure that the information contained in these publicly available briefings is correct at the time of publication. Readers should be aware however that briefings are not necessarily updated to reflect subsequent changes. If you have any comments on our briefings please email [email protected]. Please note that authors are not always able to engage in discussions with members of the public who express opinions about the content of our research, although we will carefully consider and correct any factual errors. -
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. -
Foi-R--5077--Se
Omvärldsanalys Rymd 2020 Fokus på försvar och säkerhet Sandra Lindström (red.), Kristofer Hallgren, Seméli Papadogiannakis, Ola Rasmusson, John Rydqvist och Jonatan Westman FOI-R--5077--SE Januari 2021 Sandra Lindström (red.), Kristofer Hallgren, Seméli Papadogiannakis, Ola Rasmusson, John Rydqvist och Jonatan Westman Omvärldsanalys Rymd 2020 Fokus på försvar och säkerhet FOI-R--5077--SE Titel Omvärldsanalys Rymd 2020 – Fokus på försvar och säkerhet Title Global Space Trends 2020 for Defence and Security Rapportnr/Report no FOI-R--5077--SE Månad/Month Januari Utgivningsår/Year 2021 Antal sidor/Pages 127 ISSN 1650-1942 Kund/Customer Försvarsmakten Forskningsområde Flygsystem och rymdfrågor FoT-område Sensorer och signaturanpassningsteknik Projektnr/Project no E60966 Godkänd av/Approved by Lars Höstbeck Ansvarig avdelning Försvars- och säkerhetssystem Bild/Cover: Tre gröna lasrar från Starfire Optical Range på Kirtland Air Force Base i New Mexico, USA. Anläggningen används bland annat för inmätning av objekt i låga satellitbanor. Den allmänna uppfattningen (men ej officiell) är att lasern även kan användas som ASAT-vapen. Källa: Directed Energy Directorate, US Air Force. Detta verk är skyddat enligt lagen (1960:729) om upphovsrätt till litterära och konstnärliga verk, vilket bl.a. innebär att citering är tillåten i enlighet med vad som anges i 22 § i nämnd lag. För att använda verket på ett sätt som inte medges direkt av svensk lag krävs särskild överenskommelse. This work is protected by the Swedish Act on Copyright in Literary and Artistic Works (1960:729). Citation is permitted in accordance with article 22 in said act. Any form of use that goes beyond what is permitted by Swedish copyright law, requires the written permission of FOI. -
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). -
Direct Fusion Drive Rocket for Asteroid Deflection
Direct Fusion Drive Rocket for Asteroid Deflection IEPC-2013-296 Presented at the 33rd International Electric Propulsion Conference, The George Washington University, Washington, D.C., USA October 6{10, 2013 Joseph B. Mueller∗ and Yosef S. Raziny and Michael A. Paluszek z and Amanda J. Knutson x and Gary Pajer { Princeton Satellite Systems, 6 Market St, Suite 926, Plainsboro, NJ, 08536, USA Samuel A. Cohenk Plasma Physics Laboratory, 100 Stellarator Road, Princeton, NJ, 08540 and Allan H. Glasser∗∗ University of Washington, Department of Aeronautics and Astronautics, Guggenheim Hall, Seattle, WA 98195 Traditional thinking presumes that planetary defense is only achievable with years of warning, so that a mission can launch in time to deflect the asteroid. However, the danger posed by hard-to-detect small meteors was dramatically demonstrated by the 20 meter Chelyabinsk meteor that exploded over Russia in 2013 with the force of 440 kilotons of TNT. A 5-MW Direct Fusion Drive (DFD) engine allows rockets to rapidly reach threaten- ing asteroids that and deflect them using clean burning deuterium-helium-3 fuel, a compact field-reversed configuration, and heated by odd-parity rotating magnetic fields. This paper presents the latest development of the DFD rocket engine based on recent simulations and experiments as well as calculations for an asteroid deflection envelope and a mission plan to deflect an Apophis-type asteroid given just one year of warning. Armed with this new defense technology, we will finally have achieved a vital capability for ensuring our planet's safety from impact threats. ∗Senior Technical Staff, [email protected]. -
Aas 21-290 Cislunar Space Situational Awareness
AAS 21-290 CISLUNAR SPACE SITUATIONAL AWARENESS Carolin Frueh*, Kathleen Howell†, Kyle J. DeMars‡, Surabhi Bhadauria§ Classically, space situational awareness (SSA) and space traffic management (STM) focus on the near-Earth region, which is highly populated by satellites and space debris objects. With the expansion of space activities further in the cislunar space, the problems of SSA and STM arise anew in regions far away from the near-Earth realm. This paper investigates the conditions for successful Space Situational Awareness and Space Traffic Management in the cislunar region by drawing a direct comparison to the known challenges and solutions in the near-Earth realm, highlighting similarities and differences and their implications on Space Traffic Management engineering solutions. INTRODUCTION Space Situational Awareness (SSA), sometimes called Space Domain Awareness (SDA), can be understood as summary terms for the comprehensive knowledge on all objects in a specific region without necessarily having direct communication to those objects. Space Traffic Management (STM), as an extrapolatory term, is applying the SSA knowledge to manage this said region to enable sustainable use. All three of those terms have traditionally been applied to the realm of the near-Earth space, usually expanding from low Earth orbit (LEO) to hyper geostationary orbit (hyper-GEO), and the objects of interest are objects in orbital motion for which the dominant astrodynamical term is the central gravitational potential of the Earth. Space Traffic Management (STM) aims at engineering solutions, methods, and protocols that allow regulating space fairing in a manner enabling the sustainable use of space. SSA and SDA thereby provide the knowledge-base for STM, and the areas are heavily intertwined. -
Planetary Defence Activities Beyond NASA and ESA
Planetary Defence Activities Beyond NASA and ESA Brent W. Barbee 1. Introduction The collision of a significant asteroid or comet with Earth represents a singular natural disaster for a myriad of reasons, including: its extraterrestrial origin; the fact that it is perhaps the only natural disaster that is preventable in many cases, given sufficient preparation and warning; its scope, which ranges from damaging a city to an extinction-level event; and the duality of asteroids and comets themselves---they are grave potential threats, but are also tantalising scientific clues to our ancient past and resources with which we may one day build a prosperous spacefaring future. Accordingly, the problems of developing the means to interact with asteroids and comets for purposes of defence, scientific study, exploration, and resource utilisation have grown in importance over the past several decades. Since the 1980s, more and more asteroids and comets (especially the former) have been discovered, radically changing our picture of the solar system. At the beginning of the year 1980, approximately 9,000 asteroids were known to exist. By the beginning of 2001, that number had risen to approximately 125,000 thanks to the Earth-based telescopic survey efforts of the era, particularly the emergence of modern automated telescopic search systems, pioneered by the Massachusetts Institute of Technology’s (MIT’s) LINEAR system in the mid-to-late 1990s.1 Today, in late 2019, about 840,000 asteroids have been discovered,2 with more and more being found every week, month, and year. Of those, approximately 21,400 are categorised as near-Earth asteroids (NEAs), 2,000 of which are categorised as Potentially Hazardous Asteroids (PHAs)3 and 2,749 of which are categorised as potentially accessible.4 The hazards posed to us by asteroids affect people everywhere around the world. -
Nova Notes June 2013 Final
Volume 44 Number 3 of 5 June / July 2013 E mail: [email protected] In this issue: Meeting Announcements 2 Nova East 2013 3 A Spring Comet 4 April Meeting Report 6 May Meeting Report 7 Keji DSP—An update 8 GA 2015—Update 8 Featured Photo of the Month 9 St. Croix Observatory 10 Cosmic Debris 12 Front Page Photo: M51 Chris Turner Imaged: April 17 2013, Camera: Canon T1i OTA: Mak Newt 190mm Guided: PHD FWHM 3.5. Nebulosity (36 X 300s, 12 Dark, 51 Flat, 51 Bias, ISO 3200), Workflow: align_recon_norm_pproc / digital development/curves/tighten star edges From the editor Quinn Smith As the June approaches, our last meeting for the summer will be held at the Centre’s observatory at St Croix, on the summer solstice (June 21st). For those of you who had not had an opportunity to visit the St Croix Observatory (SCO), this would be a great opportunity to see what you’ve been missing. Details will be posted on the “chat list”, and a final decision (based on weather) will be made on Thursday June 20th. If the weather is bad, we will meet in our usual room at St Mary’s University. In July the RASC will be meeting for the annual General Assembly. This year it is being hosted by the Thunder Bay Centre. In 2015 it will hosted by the Halifax Centre (see page 8). Due to changes in Federal laws, the governing structure of the RASC is being changed and there are several key motions that need to be voted on. -
Asteroid Retrieval Feasibility Study
Asteroid Retrieval Feasibility Study 2 April 2012 Prepared for the: Keck Institute for Space Studies California Institute of Technology Jet Propulsion Laboratory Pasadena, California 1 2 Authors and Study Participants NAME Organization E-Mail Signature John Brophy Co-Leader / NASA JPL / Caltech [email protected] Fred Culick Co-Leader / Caltech [email protected] Co -Leader / The Planetary Louis Friedman [email protected] Society Carlton Allen NASA JSC [email protected] David Baughman Naval Postgraduate School [email protected] NASA ARC/Carnegie Mellon Julie Bellerose [email protected] University Bruce Betts The Planetary Society [email protected] Mike Brown Caltech [email protected] Michael Busch UCLA [email protected] John Casani NASA JPL [email protected] Marcello Coradini ESA [email protected] John Dankanich NASA GRC [email protected] Paul Dimotakis Caltech [email protected] Harvard -Smithsonian Center for Martin Elvis [email protected] Astrophysics Ian Garrick-Bethel UCSC [email protected] Bob Gershman NASA JPL [email protected] Florida Institute for Human and Tom Jones [email protected] Machine Cognition Damon Landau NASA JPL [email protected] Chris Lewicki Arkyd Astronautics [email protected] John Lewis University of Arizona [email protected] Pedro Llanos USC [email protected] Mark Lupisella NASA GSFC [email protected] Dan Mazanek NASA LaRC [email protected] Prakhar Mehrotra Caltech [email protected]