Asteroid Impacts Are Inevitable. What's the Plan?
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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. -
For Immediate Release
FOR IMMEDIATE RELEASE ASTRONAUTS, EXPERTS, AND SPACE AGENCIES DISCUSS ASTEROIDS, OPPORTUNITIES, AND RISKS ON ASTEROID DAY, 30 JUNE LUXEMBOURG, 22 June 2020 /PRNewswire/ -- The Asteroid Foundation returns with Asteroid Day LIVE Digital from Luxembourg. This year, the event is a fully digital celebration of asteroid science and exploration. Panel discussions and one-on-one interviews with astronauts and world experts will be broadcast on 30 June 2020. Each year Asteroid Day presents the public with a snap-shot of cutting-edge asteroid research from the largest telescopes on Earth to some of the most ambitious space missions. Topics of discussion this year include the acceleration in the rate of our asteroid discoveries and why it is set to accelerate even faster, the imminent arrival of samples from asteroid Ryugu and Bennu, the exciting preparations for the joint US-Europe mission to binary asteroid Didymos, and much more. Asteroids are the leftover remnants of the birth of the planets in the Solar System, and many are the shattered fragments of these diminutive proto-planets that never made it to maturity. “Asteroid exploration missions tell us about the birth of our own planet and reveal how asteroids can serve astronauts as stepping stones to Mars,” says Tom Jones, PhD, veteran astronaut and planetary scientist, and Asteroid Day Expert Panel member. Each asteroid is an individual with its own story to tell. And that’s what Asteroid Day is all about: bringing those stories to the widest audience possible. “Space and science have been an endless source of inspiration for SES! This is one of the reasons why we and our partners continue to do extraordinary things in space to deliver amazing experiences everywhere on earth,” says Ruy Pinto, Chief Technology Officer at SES. -
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]. -
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. -
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] -
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. -
Copernic Agent Search Results
Copernic Agent Search Results Search: sonofusion (The exact phrase) Found: 1626 result(s) on _Full.Search Date: 7/17/2010 5:51:35 AM 1. New sonofusion experiment produces results without external neutron source Mar 2009 - ...Rensselaer Polytechnic Institute New sonofusion experiment produces results without...results in 2004, suggesting that "sonofusion" may be a viable approach to producing...technique, which has been dubbed "sonofusion," produces a shock wave t http://www.eurekalert.org/pub_releases/2006-01/rpi-nse012706.php 93% 2. Bubbles feel the heat http://physicsworld.com/cws/article/news/21654 92% 3. Directory:Sonofusion - PESWiki Directory of technologies and resources relating to sonofusion, also known as bubble fusion, which involves room temperature fusion using sound frequencies " ... http://peswiki.com/index.php/Directory:Sonofusion 92% 4. Evidence bubbles over to support tabletop nuclear fusion device The researchers believe the new evidence shows that "sonofusion" generates nuclear reactions by creating tiny bubbles that implode with tremendous force. http://news.uns.purdue.edu/html4ever/2004/0400302.Taleyarkhan.fusion.html 92% 5. Research Uses Sonofusion to Generate Temperatures Hot Enough For Fusion - The Tech Mar 2009 - ...Article Tools E-Mail Print Write the Editor Research Uses Sonofusion to Generate Temperatures Hot Enough For Fusion By Kenneth Chang...tabletop. Putterman's approach is to use sound waves, called sonofusion or bubble fusion, to expand and col http://tech.mit.edu/V127/N7/long5.html 92% 6. Roger Stringham Sonofusion Jets Sonofusion is a developing alternate energy technology that has the potential to replace polluting hydrocarbons which include fossil fuels. The economics for sonofusion appear feasible now with its application to heating large structures. -
19. Near-Earth Objects Chelyabinsk Meteor: 2013 ~0.5 Megaton Airburst ~1500 People Injured
Astronomy 241: Foundations of Astrophysics I 19. Near-Earth Objects Chelyabinsk Meteor: 2013 ~0.5 megaton airburst ~1500 people injured (C) Don Davis Asteroids 101 — B612 Foundation Great Daylight Fireball: 1972 Earthgrazer: The Great Daylight Fireball of 1972 Tunguska Meteor: 1908 Asteroid or comet: D ~ 40 m ~10 megaton airburst ~40 km destruction radius The Tunguska Impact Tunguska: The Largest Recent Impact Event Barringer Crater: ~50 ky BP M-type asteroid: D ~ 50 m ~10 megaton impact 1.2 km crater diameter Meteor Crater — Wikipedia Chicxulub Crater: ~65 My BP Asteroid: D ~ 10 km 180 km crater diameter Chicxulub Crater— Wikipedia Comets and Meteor Showers Comets shed dust and debris which slowly spread out as they move along the comet’s orbit. If the Earth encounters one of these trails, we get a Breakup of a Comet meteor shower. Meteor Stream Perseid Meteor Shower Raining Perseids Major Meteor Showers Forty Thousand Meteor Origins Across the Sky Known Potentially-Hazardous Objects Near-Earth object — Wikipedia Near-Earth object — Wikipedia Origin of Near-Earth Objects (NEOs) ! WHAM Mars Some fragments wind up on orbits which are resonant with Jupiter. Their orbits grow more elliptical, finally entering the inner solar system. Wikipedia: Asteroid belt Asteroid Families Many asteroids are members of families; they have similar orbits and compositions (indicated by colors). Asteroid Belt Populations Inner belt asteroids (left) and families (right). Origin of Key Stages in the Evolution of the Asteroid Vesta Processed Family Members Crust Surface Magnesium-Sliicate Lavas Meteorites Mantle (Olivine) Iron-Nickle Core Stony Irons? As smaller bodies in the early Solar System Heavier elements sink to the Occasional impacts with other bodies fall together, the asteroid agglomerates. -
Educator's Guide
educator’s guide Table of Contents INTRODUCTION . 3 ACTIVITY FOR GRADES 3-5 Introduction for Educator . 4 Asteroids in Orbit Student Activity . 5 ACTIVITIES FOR GRADES 6-8 Introduction for Educator . 7 What Are Asteroids? Instructions for Educator . 7 Making a Splash Instructions for Educator . 7 Working Together Instructions for Educator . 8 What Are Asteroids? Student Activity . 9 Making a Splash Student Activity . 11 Working Together Student Activity . 13 ACTIVITIES FOR GRADES 9-12 Introduction for Educator . 15 Tracing the Past Instructions for Educator . 15 Defending the Future Instructions for Educator . 16 Tracing the Past Student Activity . 17 Defending the Future Student Activity . 18 EDUCATIONAL STANDARDS ALIGNMENT . 19 ACKNOWLEDGEMENTS . 20 2 Introduction AN EXTRAORDINARY FIELD TRIP AND LEARNING EXPERIENCE! Dear Educator, Planetary defense is a relatively new science . Only a few decades ago did we become certain Earth’s history of asteroid impacts was sure to repeat itself . Could we save our world today from a cosmic threat? You bet we can . But to tend to this problem, we must first understand it . That’s where Asteroid Hunters comes in . Asteroid Hunters will take your students on an exciting field trip across the Solar System and to the dawn of time . They’ll watch how gravity spun gas and dust into our Solar System, how rocky debris gathered into worlds, and how the planet-building leftovers became asteroids . They’ll learn that these natural wonders of deep space brought water to planets, and the building blocks of life itself . They will also see how we possess the technological know-how to keep an asteroid from hitting our planet– unlike the doomed dinosaurs of 65 million years ago . -
Assessment of Morelian Meteoroid Impact on Mexican Environment
atmosphere Article Assessment of Morelian Meteoroid Impact on Mexican Environment Maria A. Sergeeva 1,2,*, Vladislav V. Demyanov 3,4, Olga A. Maltseva 5 , Artem Mokhnatkin 6, Mario Rodriguez-Martinez 7 , Raul Gutierrez 7, Artem M. Vesnin 3, Victor Jose Gatica-Acevedo 1,8, Juan Americo Gonzalez-Esparza 1 , Mark E. Fedorov 4, Tatiana V. Ishina 4, Marni Pazos 9, Luis Xavier Gonzalez 1,2, Pedro Corona-Romero 1,2, Julio Cesar Mejia-Ambriz 1,2, Jose Juan Gonzalez-Aviles 1,2, Ernesto Aguilar-Rodriguez 1, Enrique Cabral-Cano 10 , Blanca Mendoza 11, Esmeralda Romero-Hernandez 12, Ramon Caraballo 1 and Isaac David Orrala-Legorreta 1,13 1 SCiESMEX, LANCE, Instituto de Geofisica, Unidad Michoacan, Universidad Nacional Autonoma de Mexico, Morelia, Michoacan C.P. 58089, Mexico; [email protected] (V.J.G.-A.); americo@igeofisica.unam.mx (J.A.G.-E.); xavier@igeofisica.unam.mx (L.X.G.); p.coronaromero@igeofisica.unam.mx (P.C.-R.); jcmejia@geofisica.unam.mx (J.C.M.-A.); jjgonzalez@igeofisica.unam.mx (J.J.G.-A.); ernesto@igeofisica.unam.mx (E.A.-R.); rcaraballo@igeofisica.unam.mx (R.C.); [email protected] (I.D.O.-L.) 2 CONACYT, Instituto de Geofisica, Unidad Michoacan, Universidad Nacional Autonoma de Mexico, Morelia, Michoacan C.P. 58089, Mexico 3 Institute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, 664033 Irkutsk, Russia; [email protected] (V.V.D.); [email protected] (A.M.V.) 4 Irkutsk State Transport University, 664074 Irkutsk, Russia; [email protected] (M.E.F.); [email protected] (T.V.I.) 5 Institute for Physics, Southern Federal University, 344090 Rostov-on-Don, Russia; [email protected] Citation: Sergeeva, M.A.; Demyanov, 6 Keldysh Institute of Applied Mathematics of the Russian Academy of Sciences, 125047 Moscow, Russia; V.V.; Maltseva, O.A.; Mokhnatkin, A.; [email protected] 7 Rodriguez-Martinez, M.; Gutierrez, Escuela Nacional de Estudios Superiores Unidad Morelia, Universidad Nacional Autonoma de Mexico, Morelia, Michoacan C.P. -
Planetary Defense Final Report I
Team Project - Planetary Defense Final Report i Team Project - Planetary Defense Final Report ii Team Project - Planetary Defense Cover designed by: Tihomir Dimitrov Images courtesy of: Earth Image - NASA US Geological Survey Detection Image - ESA's Optical Ground Station Laser Tags ISS Deflection Image - IEEE Space Based Lasers Collaboration Image - United Nations General Assembly Building Outreach Image - Dreamstime teacher with students in classroom Evacuation Image - Libyan City of Syrte destroyed in 2011 Shield Image - Silver metal shield PNG image The cover page was designed to include a visual representation of the roadmap for a robust Planetary Defense Program that includes five elements: detection, deflection, global collaboration, outreach, and evacuation. The shield represents the idea of defending our planet, giving confidence to the general public that the Planetary Defense elements are reliable. The orbit represents the comet threat and how it is handled by the shield, which represents the READI Project. The curved lines used in the background give a sense of flow representing the continuation and further development for Planetary Defense programs after this team project, as we would like for everyone to be involved and take action in this noble task of protecting Earth. The 2015 Space Studies Program of the International Space University was hosted by the Ohio University, Athens, Ohio, USA. While all care has been taken in the preparation of this report, ISU does not take any responsibility for the accuracy of its content. -
Required Deflection Impulses As a Function of Time Before Impact for Earth-Impacting Asteroids
Icarus 347 (2020) 113792 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Required deflection impulses as a function of time before impact for Earth-impacting asteroids Sarah Greenstreet a,b,<, Ed Lu a, Mike Loucks a,c, John Carrico a,c, Tatiana Kichkaylo a, Mario Juri¢ b a Asteroid Institute, 20 Sunnyside Ave, Suite 427, Mill Valley, CA 94941, USA b Department of Astronomy and the DIRAC Institute, University of Washington, 3910 15th Avenue, NE, Seattle, WA 98195, USA c Space Exploration Engineering LLC, 687 Chinook Way, Friday Harbor, WA 98250, USA ARTICLEINFO ABSTRACT Keywords: For any asteroid on an impact trajectory, the amount of time prior to impact a deflection can be implemented Asteroids can drastically change the amount of deflection impulse required. In this study we use the precision cloud- Dynamics based asteroid orbit propagation and targeting capabilities of the Asteroid Institute's Asteroid Decision Analysis and Mapping (ADAM) platform to investigate the distribution of deflection 훥푣 required to divert asteroids on Earth-impacting trajectories (Chesley and Spahr, 2004) as a function of time prior to impact for 10,000 synthetic impacting asteroids. We target a miss distance of one Earth radius above the surface of the Earth and calculate the distribution of deflection 훥푣 required if applied 10, 20, 30, 40, and 50 years prior to impact. We find that the median required deflection impulse decreases as approximately t*1 for increasing time before impact (Ahrens and Harris, 1992), where the median required 훥푣 is 1.4 cm/s, 0.76 cm/s, 0.55 cm/s, 0.46 cm/s, and 0.38 cm/s for 10, 20, 30, 40, & 50 years before impact, respectively.