Oral Histories in Meteoritics and Planetary Science – Xxxx: Dale
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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. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars
SPIRIT AT CUSEV CRATER RESEARCH ARTICLE The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars S. W. Squyres,^* R. E. Arvidson,^ J. F. Bell III/ J. Bruckner,' N. A. Cabrol,'* W. Calvîn,= M. H. Carr,® P. R. Christensen/ B. C. Clark,® L Crumpler,® D. J. Des Marais,^" C. d'Uston,''^ T. Economou,^^ J. Farmer,^ W. Farrand," W. Folkner,^^ M. Colombek,^'* S. Corevan," J. A. Crant,^^ R. Creeley,'^ J. Crotzinger,^'^ L Haskin,^ K. E. Herkenhoff,^® S. Hvîid," J. Johnson,^® C. Klîngelhofer,^" A. Knoll,^^ C. Landis,^^ M. Lemmon,^' R. Li,^* M. B. Madsen,2= M. C. Malin,^^ s. M. McLennan,^^ H. Y. McSween,^« D. W. Ming,^^ J. Moersch,^« R. V. Morris,^^ T. Parker,^'* J. W. Rice Jr.,' L Richter,'" R. Rieder,' M. Sims,^° M. Smitli,'^ P. Smith,'^ L A. Soderblom,^® R. Sullivan,^ H. Wanke,' T. Wdowiak," M. Wolff,'^ A. Yen^'* The Mars Exploration Rover Spirit and its Atliena science payload liave been used to sediment carried by the water that cut investigate a landing site in Gusev crater. Gusev is hypothesized to be the site of a Ma'adim before it overflowed and exited former lake, but no clear evidence for lacustrine sedimentation has been found to through a gap in the northern rim of the date. Instead, the dominant lithology is basalt, and the dominant geologic processes are impact events and eolian transport. I^jany rocks exhibit coatings and other characteristics that may be evidence for minor aqueous alteration. Any lacustrine ^Department of Astronomy, Cornell University, Ithaca, NY 14853, USA. ^Department of Earth and sediments that may exist at this location within Gusev apparently have been buried Planetary Sciences, Washington University, St. -
Its Founding and Early Years Ewen A. Whitaker
The University of Arizona's LUNAR AND PLANETARY LABORATORY Its Founding and Early Years Ewen A. Whitaker Set in Varityper Times Roman and printed at the University of Arizona Printing-Reproductions Department Equal Employment Opportunity· Affirmative Action Employer CONTENTS THE PRE-TUCSON ERA Historical background ........................................ I Enter Gerard P. Kuiper ....................................... 2 The Moon enters the picture ................................... 3 A call for suggestions ......................................... 5 The Harold Urey affair ....................................... 6 Preliminaries for the Lunar Atlas ............................... 7 1957 - a dream begins to take shape ............................. 7 The shot that was seen (and heard) around the world ............... 8 Other irons in the fire ......................................... 9 Kuiper seeks full-time help for the Lunar Project .................. 9 1959 - the Lunar Project gathers momentum ..................... 11 A new factor in the Lunar Project LPL story ................... 12 The Air Force enters the lunar cartography business ............... 13 The Lunar Atlas published at last .............................. 14 Big problems with the Yerkes set-up ............................ : 6 The southwestern U.S. begins to beckon ........................ 17 "There is a tide in the affairs of men ..." ....................... 18 Preparing for the move ...................................... 23 THE TUCSON ERA The Lunar Project makes the transfer -
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. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
The Adventures of a Citizen Scientist
The Adventures of a Citizen Scientist Perhaps one never knows one’s parents, really knows them. You never know their early lives and, as a kid, you’re living inside your own skin, not theirs. After that you’re out of there. Growing up in Chicago, I never knew my dad was famous. He was just a firm, affectionate, if too busy father figure, who loved music and the outdoors, played tennis better than I could, was awfully good with tools, and could explain scientific ideas so well that I almost understood them. I knew he was a physicist and taught at the University, and he and mother often took me on lecture or research trips, but I didn’t know what it was all about. During the war, when he was one of those in charge of the bomb project and we’d moved to Oak Ridge, he was just a hard-working ordinary man doing a job like everybody else. August 6th, 1945, brought a dramatically different perspective, as you might expect. My father was suddenly a national and world figure. That fall, as I went off to college, I began to hear something of his achievements — not only the bomb, but the cosmic ray studies and the Nobel Prize, with all that seemed to entail. At that moment, too, he’d become Chancellor of Washington University in St. Louis, and my college was his college, where his father had been Professor of Philosophy and Psychology and Dean. I was in Wooster, Ohio, the town in which my father had grown up, with his childhood house just down College Avenue. -
History of Space-Based Infrared Astronomy and the Air Force Infrared Celestial Backgrounds Program
AFRL-RV-HA-TR-2008-1039 History of Space-Based Infrared Astronomy and the Air Force Infrared Celestial Backgrounds Program S. D. Price 18 April 2008 Approved for Public Release: Distribution Unlimited AIR FORCE RESEARCH LABORATORY Space Vehicles Directorate 29 Randolph Rd. Hanscom AFB, MA 01731-3010 AFRL-RV-HA-TR-2008-1039 This Technical Report has been reviewed and is approved for publication. / signed / ____________________________ Robert A. Morris, Chief Battlespace Environment Division / signed / / signed / _________________ _______________________________ Stephan D. Price Paul Tracy, Acting Chief Author Battlespace Surveillance Innovation Center This report has been reviewed by the ESC Public Affairs Office (PA) and is releasable to the National Technical Information Service. Qualified requestors may obtain additional copies from the Defense Technical Information Center (DTIC). All others should apply to the National Technical Information Service (NTIS). If your address has changed, if you wish to be removed from the mailing list, of if the address is no longer employed by your organization, please notify AFRL/VSIM, 29 Randolph Rd., Hanscom AFB, MA 01731-3010. This will assist us in maintaining a current mailing list. Do not return copies of this report unless contractual obligations or notices on a specific document require that it be returned. Form Approved REPORT DOCUMENTATION PAGE OMB No. 0704-0188 The public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, searching existing data sources, gathering and maintaining the data needed, and completing and reviewing the collection of information. Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing the burden, to Department of Defense, Washington Headquarters Services, Directorate for Information Operations and Reports (0704-0188), 1215 Jefferson Davis Highway, Suite 1204, Arlington, VA 22202-4302. -
Astronomy Alphabet
Astronomy Alphabet Educational video for children Teacher https://vimeo.com/77309599 & Learner Guide This guide gives background information about the astronomy topics mentioned in the video, provides questions and answers children may be curious about, and suggests topics for discussion. Alhazen A Alhazen, called the Father of Optics, performed NASA/Goddard/Lunar Reconnaissance Orbiter, Apollo 17 experiments over a thousand years ago Can you find Alhazen crater when you look at the Moon? to learn about how light travels and Why does the Moon look bigger near the behaves. He also studied astronomy, horizon? separated light into colors, and sought to Believe it or not, scientists still don’t know for sure why explain why the Moon looks bigger near we perceive the Moon to be larger when it lies near to the the horizon. horizon. Though photos of the Moon at different points in the sky show it to be the same size, we humans think we I’ve never heard of Abu Ali al-Hasan ibn al- see something quite different. Try this experiment yourself Hasan ibn al-Hatham (Alhazen). sometime! One possibility is that objects we see next to the Tell me more about him. Moon when it’s near to them give us the illusion that it’s We don’t know that much about Alhazen be- bigger, because of a sense of scale and reference. cause he lived so long ago, but we do know that he was born in Persia in 965. He wrote hundreds How many craters does the Moon have, and what of books on math and science and pioneered the are their names? scientific method of experimentation. -
The National Aeronautics and Space Administration Planetary Astronomy Program
FRS 347320 FINAL REPORT FOR GRANT NAG5-3938 SUBMITTED TO: The National Aeronautics and Space Administration Planetary Astronomy Program TITLE: Beginning Research with the 1.8-meter Spacewatch Telescope ORGANIZATION: The University of Arizona Lunar and Planetary Laboratory PERIOD OF GRANT: 1996 Dec. 1 - 2000 Nov. 30 PERIOD REPORTED ON: 1996 Dec. I - 2001 Feb. 9 2._o[ PRINCIPAL INVESTIGATOR: Tom Gehrels Date Professor Lunar and Planetary Laboratory University of Arizona Kuiper Space Sciences Building 1629 East University Boulevard Tucson, AZ 85721-0092 Phone: 520/621-6970 FAX: 520/621-1940 Email: [email protected] BUSINESS REPRESENTATIVE: Ms. Lynn A. Lane Senior Business Manager Lunar and Planetary Laboratory University of Arizona Kuiper Space Sciences Building 1629 East University Boulevard Tucson, AZ 85721-0092 Phone: 520/621-6966 FAX: 520/621-4933 Email: [email protected] c:_w_nnsaknag53938.fnl Participating Professionals (all at the Lunar and Planetary Laboratory): Terrence H. Bressi (B. S., Astron. & Physics) Engineer Anne S. Descour (M. S., Computer Science) Senior Systems Programmer Tom Gehrels (Ph. D., Astronomy) Professor, observer, and PI Robert Jedicke (Ph.D., Physics) Principal Research Specialist Jeffrey A. Larsen (Ph. D., Astronomy) Principal Research Specialist and observer Robert S. McMiUan (Ph.D., Astronomy) Associate Research Scientist & observer Joseph L. Montani (M. S., Astronomy) Senior Research Specialist and observer Marcus L. Perry (B. A., Astronomy) (Chief) Staff Engineer James V. Scotti (B. S., Astronomy) Senior Research Specialist and observer PROJECT SUMMARY The purpose of this grant was to bring the Spacewatch 1.8-m telescope to operational status for research on asteroids and comets. -
Asteroids and Comets: U.S
Columbia Law School Scholarship Archive Faculty Scholarship Faculty Publications 1997 Asteroids and Comets: U.S. and International Law and the Lowest-Probability, Highest Consequence Risk Michael B. Gerrard Columbia Law School, [email protected] Anna W. Barber Follow this and additional works at: https://scholarship.law.columbia.edu/faculty_scholarship Part of the Environmental Law Commons, and the International Law Commons Recommended Citation Michael B. Gerrard & Anna W. Barber, Asteroids and Comets: U.S. and International Law and the Lowest- Probability, Highest Consequence Risk, 6 N.Y.U. ENVTL. L. J. 4 (1997). Available at: https://scholarship.law.columbia.edu/faculty_scholarship/697 This Article is brought to you for free and open access by the Faculty Publications at Scholarship Archive. It has been accepted for inclusion in Faculty Scholarship by an authorized administrator of Scholarship Archive. For more information, please contact [email protected]. COLLOQUIUM ARTICLES ASTEROIDS AND COMETS: U.S. AND INTERNATIONAL LAW AND THE LOWEST-PROBABILITY, HIGHEST ICONSEQUENCE RISK MICHAEL B. GERRARD AND ANNA W. BARBER* INTRODUCrION Asteroids' and comets2 pose unique policy problems. They are the ultimate example of a low probability, high consequence event: no one in recorded human history is confirmed to have ever died from an asteroid or a comet, but the odds are that at some time in the next several centuries (and conceivably next year) an asteroid or a comet will cause mass localized destruction and that at some time in the coming half million years (and con- ceivably next year), an asteroid or a comet will kill several billion people.