The Spatial and Temporal Distribution of the Metal Mineralisation in Eastern Australia and the Relationship of the Observed Patterns to Giant Ore Deposits

Total Page:16

File Type:pdf, Size:1020Kb

The Spatial and Temporal Distribution of the Metal Mineralisation in Eastern Australia and the Relationship of the Observed Patterns to Giant Ore Deposits The Spatial and Temporal Distribution of the Metal Mineralisation in Eastern Australia and the Relationship of the Observed Patterns to Giant Ore Deposits A thesis submitted for the degree of Doctor of Philosophy May 2007 Larry J. Robinson School of Earth Sciences Principal Advisor Associate Professor Dr. Suzanne D. Golding Associate Advisor Senior Lecturer Dr. Richard Wilson Certificate of Originality I hereby certify that the work embodied in this thesis is the result of original research and has not been submitted for a higher degree at any other University or Institution. (Signed) Larry John Robinson ABSTRACT The introduced mineral deposit model (MDM) is the product of a trans-disciplinary study, based on Complexity and General Systems Theory. Both investigate the abstract organization of phenomena, independent of their substance, type, or spatial or temporal scale of existence. The focus of the research has been on giant, hydrothermal mineral deposits. They constitute <0.001% of the total number of deposits yet contain 70-85% of the world's metal resources. Giants are the definitive exploration targets. They are more profitable to exploit and less susceptible to fluctuations of the market. Consensus has it that the same processes that generate small deposits also form giants but those processes are simply longer, vaster, and larger. Heat is the dominant factor in the genesis of giant mineral deposits. A paleothermal map shows where the vast heat required to generate a giant has been concentrated in a large space, and even allows us to deduce the duration of the process. To generate a paleothermal map acceptable to the scientific community requires reproducibility. Experimentation with various approaches to pattern recognition of geochemical data showed that the AUTOCLUST algorithm not only gave reproducibility but also gave the most consistent, most meaningful results. It automatically extracts boundaries based on Voronoi and Delaunay tessellations. The user does not specify parameters; however, the modeller does have tools to explore the data. This approach is near ideal in that it removes much of the human- generated bias. This algorithm reveals the radial, spatial distribution, of gold deposits in the Lachlan Fold Belt of southeastern Australia at two distinct scales – repeating patterns every ~80 km and ~230 km. Both scales of patterning are reflected in the geology. The ~80 km patterns are nested within the ~230 km patterns revealing a self-similar, geometrical relationship. It is proposed that these patterns originate from Rayleigh-Bénard convection in the mantle. At the Rayleigh Number appropriate for the mantle, the stable planform is the spoke pattern, where hot mantle material is moving upward near the centre of the pattern and outward along the radial arms. Discontinuities in the mantle, Rayleigh-Bénard convection in the mantle, and the spatial distribution of giant mineral deposits, are correlative. The discontinuities in the Earth are acting as platforms from which Rayleigh-Bénard convection can originate. Shallow discontinuities give rise to plumelets, which manifest at the crust as repeating patterns ranging, from ~100 to ~1,000 km in diameter. Deeper discontinuities give rise to plumes, which become apparent at i the crust as repeating patterns ranging from >1,000 to ~4,000 km in diameter. The deepest discontinuities give rise to the superplumes, which become detectable at the crust as repeating patterns ranging from >4,000 to >10,000 km in diameter. Rayleigh-Bénard convection concentrates the reservoir of heat in the mantle into specific locations in the crust; thereby providing the vast heat requirements for the processes that generate giant, hydrothermal mineral deposits. The radial spatial distribution patterns observed for gold deposits are also present for base metal deposits. At the supergiant Broken Hill deposit in far western New South Wales, Australia, the higher temperature Broken Hill-type deposits occur in a radial pattern while the lower temperature deposits occur in concentric patterns. The supergiant Broken Hill deposit occurs at the very centre of the pattern. If the supergiant Broken Hill Deposit was buried beneath alluvium, water or younger rocks, it would now be possible to predict its location with accuracy measured in tens of square kilometres. This predictive accuracy is desired by every exploration manager of every exploration company. The giant deposits at Broken Hill, Olympic Dam, and Mount Isa all occur on the edge of an annulus. There are at least two ways of creating an annulus on the Earth's surface. One is through Rayleigh-Bénard convection and the other is through meteor impact. It is likely that only 'large' meteors (those >10 km in diameter) would have any permanent impact on the mantle. Lesser meteors would leave only a superficial scar that would be eroded away. The permanent scars in the mantle act as ‘accidental templates’ consisting of concentric and possibly radial fractures that impose those structures on any rocks that were subsequently laid down or emplaced over the mantle. In southeastern Australia, the proposed Deniliquin Impact structure has been an 'accidental template' providing a 'line-of-least-resistance' for the ascent of the ~2,000 km diameter, offshore, Cape Howe Plume. The western and northwestern radial arms of this plume have created the very geometry of the Lachlan Fold Belt, as well as giving rise to the spatial distribution of the granitic rocks in that belt and ultimately to the gold deposits. The interplay between the templating of the mantle by meteor impacts and the ascent of plumelets, plumes or superplumes from various discontinuities in the mantle is quite possibly the reason that mineral deposits occur where they do. ii TABLE OF CONTENTS 1 INTRODUCTION ......................................................................................................................................... 1 1.1 OBJECTIVE AND SCOPE........................................................................................................................... 1 1.2 THE MINERAL DEPOSIT MODEL............................................................................................................. 5 1.3 ORGANISATION OF THE THESIS .............................................................................................................. 6 2 GENERAL SYSTEMS APPROACH TO MODELLING ..................................................................... 10 2.1 SYSTEMS THEORY AND THE GENERAL SYSTEMS APPROACH ............................................................. 12 2.2 COMPLEXITY, EMERGENCE, MODEL BUILDING, & SIMPLICITY .......................................................... 15 2.2.1 Complexity..................................................................................................................................... 15 2.2.2 Emergence..................................................................................................................................... 18 2.2.3 Model Building.............................................................................................................................. 21 2.2.4 Simplicity....................................................................................................................................... 25 2.3 FRACTALS, CHAOS THEORY, AND NONLINEAR DYNAMICS................................................................. 27 2.3.1 Fractals ......................................................................................................................................... 27 2.3.2 Chaos Theory (Dynamical Systems Theory)................................................................................ 29 2.3.3 Nonlinear Dynamics ..................................................................................................................... 33 2.4 PATTERN FORMATION FAR-FROM-EQUILIBRIUM & SELF-ORGANISATION......................................... 34 2.4.1 Pattern Formation Far-From-Equilibrium.................................................................................. 34 2.4.2 Self-Organisation.......................................................................................................................... 39 2.5 SELF-ORGANISED CRITICALITY ........................................................................................................... 45 3 METAL MINERAL DEPOSITS MODELS............................................................................................ 53 3.1.1 An Historical Sketch of the Genesis Models of Mineral Deposits............................................... 53 3.1.2 Metal Mineral Deposit Modelling................................................................................................ 60 3.1.2.1 Descriptive Models versus Genetic Models ......................................................................................... 62 3.1.2.2 Mineral Deposit Density Models.......................................................................................................... 67 3.1.2.3 Spatial-Temporal Models...................................................................................................................... 68 3.1.2.4 Structural Models.................................................................................................................................. 69 3.1.2.5 Statistical/Probabilistic Models............................................................................................................. 70 3.1.2.6
Recommended publications
  • 2015 Summer Intern Poster Session and Abstract Proceedings
    2015 Summer Intern Poster Session and Abstract Proceedings NASA Goddard Space Flight Center 2015 Summer Intern Poster Session and Abstracts NASA Goddard Space Flight Center Greenbelt, MD, USA July 30, 2015 Director, Office of Education, Goddard Space Flight Center Dr. Robert Gabrys Deputy Director, Office of Education, Goddard Space Flight Center Dean A. Kern Acting Lead, Internships, Fellowships, and Scholarships, Goddard Space Flight Center Mablelene Burrell Prepared by USRA Republication of an article or portions thereof (e.g., extensive excerpts, figures, tables, etc.) in original form or in translation, as well as other types of reuse (e.g., in course packs) require formal permission from the Office of Education at NASA Goddard Space Flight Center. i Preface NASA Education internships provide unique NASA‐related research and operational experiences for high school, undergraduate, and graduate students. These internships immerse participants with career professionals emphasizing mentor‐directed, degree‐related, and real NASA‐mission work tasks. During the internship experience, participants engage in scientific or engineering research, technology development, and operations activities. As part of the internship enrichment activities offered by Goddard’s Office of Education, the Greenbelt Campus hosts its annual all‐intern Summer Poster Session. Here, interns from Business, Science, Computer Science, Information Technology, and Engineering and Functional Services domains showcase their completed work and research to the entire internal Goddard community and visiting guests. On July 30, 2015, more than 375 interns presented their work at Greenbelt while having the opportunity to receive feedback from scientists and engineers alike. It is this interaction with Center‐wide technical experts that contributes significantly to the interns’ professional development and represents a culminating highlight of their quality experience at NASA.
    [Show full text]
  • SPACE NEWS Previous Page | Contents | Zoom in | Zoom out | Front Cover | Search Issue | Next Page BEF Mags INTERNATIONAL
    Contents | Zoom in | Zoom out For navigation instructions please click here Search Issue | Next Page SPACEAPRIL 19, 2010 NEWSAN IMAGINOVA CORP. NEWSPAPER INTERNATIONAL www.spacenews.com VOLUME 21 ISSUE 16 $4.95 ($7.50 Non-U.S.) PROFILE/22> GARY President’s Revised NASA Plan PAYTON Makes Room for Reworked Orion DEPUTY UNDERSECRETARY FOR SPACE PROGRAMS U.S. AIR FORCE AMY KLAMPER, COLORADO SPRINGS, Colo. .S. President Barack Obama’s revised space plan keeps Lockheed Martin working on a Ulifeboat version of a NASA crew capsule pre- INSIDE THIS ISSUE viously slated for cancellation, potentially positioning the craft to fly astronauts to the interna- tional space station and possibly beyond Earth orbit SATELLITE COMMUNICATIONS on technology demonstration jaunts the president envisions happening in the early 2020s. Firms Complain about Intelsat Practices Between pledging to choose a heavy-lift rocket Four companies that purchase satellite capacity from Intelsat are accusing the large fleet design by 2015 and directing NASA and Denver- operator of anti-competitive practices. See story, page 5 based Lockheed Martin Space Systems to produce a stripped-down version of the Orion crew capsule that would launch unmanned to the space station by Report Spotlights Closed Markets around 2013 to carry astronauts home in an emer- The office of the U.S. Trade Representative has singled out China, India and Mexico for not meet- gency, the White House hopes to address some of the ing commitments to open their domestic satellite services markets. See story, page 13 chief complaints about the plan it unveiled in Feb- ruary to abandon Orion along with the rest of NASA’s Moon-bound Constellation program.
    [Show full text]
  • Bias-Corrected Population, Size Distribution, and Impact Hazard for the Near-Earth Objects ✩
    Icarus 170 (2004) 295–311 www.elsevier.com/locate/icarus Bias-corrected population, size distribution, and impact hazard for the near-Earth objects ✩ Joseph Scott Stuart a,∗, Richard P. Binzel b a MIT Lincoln Laboratory, S4-267, 244 Wood Street, Lexington, MA 02420-9108, USA b MIT EAPS, 54-426, 77 Massachusetts Avenue, Cambridge, MA 02139, USA Received 20 November 2003; revised 2 March 2004 Available online 11 June 2004 Abstract Utilizing the largest available data sets for the observed taxonomic (Binzel et al., 2004, Icarus 170, 259–294) and albedo (Delbo et al., 2003, Icarus 166, 116–130) distributions of the near-Earth object population, we model the bias-corrected population. Diameter-limited fractional abundances of the taxonomic complexes are A-0.2%; C-10%, D-17%, O-0.5%, Q-14%, R-0.1%, S-22%, U-0.4%, V-1%, X-34%. In a diameter-limited sample, ∼ 30% of the NEO population has jovian Tisserand parameter less than 3, where the D-types and X-types dominate. The large contribution from the X-types is surprising and highlights the need to better understand this group with more albedo measurements. Combining the C, D, and X complexes into a “dark” group and the others into a “bright” group yields a debiased dark- to-bright ratio of ∼ 1.6. Overall, the bias-corrected mean albedo for the NEO population is 0.14 ± 0.02, for which an H magnitude of 17.8 ± 0.1 translates to a diameter of 1 km, in close agreement with Morbidelli et al. (2002, Icarus 158 (2), 329–342).
    [Show full text]
  • Galileo Reveals Best-Yet Europa Close-Ups Stone Projects A
    II Stone projects a prom1s1ng• • future for Lab By MARK WHALEN Vol. 28, No. 5 March 6, 1998 JPL's future has never been stronger and its Pasadena, California variety of challenges never broader, JPL Director Dr. Edward Stone told Laboratory staff last week in his annual State of the Laboratory address. The Laboratory's transition from an organi­ zation focused on one large, innovative mission Galileo reveals best-yet Europa close-ups a decade to one that delivers several smaller, innovative missions every year "has not been easy, and it won't be in the future," Stone acknowledged. "But if it were easy, we would­ n't be asked to do it. We are asked to do these things because they are hard. That's the reason the nation, and NASA, need a place like JPL. ''That's what attracts and keeps most of us here," he added. "Most of us can work elsewhere, and perhaps earn P49631 more doing so. What keeps us New images taken by JPL's The Conamara Chaos region on Europa, here is the chal­ with cliffs along the edges of high-standing Galileo spacecraft during its clos­ lenge and the ice plates, is shown in the above photo. For est-ever flyby of Jupiter's moon scale, the height of the cliffs and size of the opportunity to do what no one has done before­ Europa were unveiled March 2. indentations are comparable to the famous to search for life elsewhere." Europa holds great fascination cliff face of South Dakota's Mount To help achieve success in its series of pro­ for scientists because of the Rushmore.
    [Show full text]
  • Radar Observations and a Physical Model of Asteroid 4660 Nereus, a Prime Space Mission Target ∗ Marina Brozovic A, ,Stevenj.Ostroa, Lance A.M
    Icarus 201 (2009) 153–166 Contents lists available at ScienceDirect Icarus www.elsevier.com/locate/icarus Radar observations and a physical model of Asteroid 4660 Nereus, a prime space mission target ∗ Marina Brozovic a, ,StevenJ.Ostroa, Lance A.M. Benner a, Jon D. Giorgini a, Raymond F. Jurgens a,RandyRosea, Michael C. Nolan b,AliceA.Hineb, Christopher Magri c, Daniel J. Scheeres d, Jean-Luc Margot e a Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109-8099, USA b Arecibo Observatory, National Astronomy and Ionosphere Center, Box 995, Arecibo, PR 00613, USA c University of Maine at Farmington, Preble Hall, 173 High St., Farmington, ME 04938, USA d Aerospace Engineering Sciences, University of Colorado, Boulder, CO 80309-0429, USA e Department of Astronomy, Cornell University, 304 Space Sciences Bldg., Ithaca, NY 14853, USA article info abstract Article history: Near–Earth Asteroid 4660 Nereus has been identified as a potential spacecraft target since its 1982 Received 11 June 2008 discovery because of the low delta-V required for a spacecraft rendezvous. However, surprisingly little Revised 1 December 2008 is known about its physical characteristics. Here we report Arecibo (S-band, 2380-MHz, 13-cm) and Accepted 2 December 2008 Goldstone (X-band, 8560-MHz, 3.5-cm) radar observations of Nereus during its 2002 close approach. Available online 6 January 2009 Analysis of an extensive dataset of delay–Doppler images and continuous wave (CW) spectra yields a = ± = ± Keywords: model that resembles an ellipsoid with principal axis dimensions X 510 20 m, Y 330 20 m and +80 Radar observations Z = 241− m.
    [Show full text]
  • Ebook < Impact Craters on Mars # Download
    7QJ1F2HIVR # Impact craters on Mars « Doc Impact craters on Mars By - Reference Series Books LLC Mrz 2012, 2012. Taschenbuch. Book Condition: Neu. 254x192x10 mm. This item is printed on demand - Print on Demand Neuware - Source: Wikipedia. Pages: 50. Chapters: List of craters on Mars: A-L, List of craters on Mars: M-Z, Ross Crater, Hellas Planitia, Victoria, Endurance, Eberswalde, Eagle, Endeavour, Gusev, Mariner, Hale, Tooting, Zunil, Yuty, Miyamoto, Holden, Oudemans, Lyot, Becquerel, Aram Chaos, Nicholson, Columbus, Henry, Erebus, Schiaparelli, Jezero, Bonneville, Gale, Rampart crater, Ptolemaeus, Nereus, Zumba, Huygens, Moreux, Galle, Antoniadi, Vostok, Wislicenus, Penticton, Russell, Tikhonravov, Newton, Dinorwic, Airy-0, Mojave, Virrat, Vernal, Koga, Secchi, Pedestal crater, Beagle, List of catenae on Mars, Santa Maria, Denning, Caxias, Sripur, Llanesco, Tugaske, Heimdal, Nhill, Beer, Brashear Crater, Cassini, Mädler, Terby, Vishniac, Asimov, Emma Dean, Iazu, Lomonosov, Fram, Lowell, Ritchey, Dawes, Atlantis basin, Bouguer Crater, Hutton, Reuyl, Porter, Molesworth, Cerulli, Heinlein, Lockyer, Kepler, Kunowsky, Milankovic, Korolev, Canso, Herschel, Escalante, Proctor, Davies, Boeddicker, Flaugergues, Persbo, Crivitz, Saheki, Crommlin, Sibu, Bernard, Gold, Kinkora, Trouvelot, Orson Welles, Dromore, Philips, Tractus Catena, Lod, Bok, Stokes, Pickering, Eddie, Curie, Bonestell, Hartwig, Schaeberle, Bond, Pettit, Fesenkov, Púnsk, Dejnev, Maunder, Mohawk, Green, Tycho Brahe, Arandas, Pangboche, Arago, Semeykin, Pasteur, Rabe, Sagan, Thira, Gilbert, Arkhangelsky, Burroughs, Kaiser, Spallanzani, Galdakao, Baltisk, Bacolor, Timbuktu,... READ ONLINE [ 7.66 MB ] Reviews If you need to adding benefit, a must buy book. Better then never, though i am quite late in start reading this one. I discovered this publication from my i and dad advised this pdf to find out. -- Mrs. Glenda Rodriguez A brand new e-book with a new viewpoint.
    [Show full text]
  • Optimal Flight to Near-Earth Asteroids with Using Electric Propulsion and Gravity Maneuvers
    OPTIMAL FLIGHT TO NEAR-EARTH ASTEROIDS WITH USING ELECTRIC PROPULSION AND GRAVITY MANEUVERS A. V. Chernov Keldysh Institute of Applied Mathematics, Miusskaya Sq. 4, Moscow, 125047, Russia, E-mail: [email protected] ABSTRACT Optimal space flight to near-Earth asteroid for using low thrust and gravity assist maneuver near Mars or Venus is investigated in this paper. The main deflection asteroids from the Earth and prevention their possible collision is investigated. The deflection is attention is given a case of the ideal low thrust. Besides realized by means of impact-kinetic effect of the optimal trajectories with the constrained low trust spacecraft on the asteroid and changing the asteroid appropriate to electric engine SPT-140 and solar orbit. The effectiveness of this method for preventing batteries as energy sources are received in vicinity of the optimal trajectories for ideal thrust. asteroid-Earth collision is estimated by means of optimal space flights, which are found. The flight of spacecraft (SC) is realized by means of using electric 2. THE PROBLEM STATEMENT propulsion system. To increase effectiveness the optimal gravity maneuvers of spacecraft near Mars and At first the SC with mass M0 moves along an initial Venus are using. Criterion of the space flight circular near-Earth parking orbit with radius R0. The optimization is maximal deflection of the asteroid from geocentric motion is realized by means of high thrust the Earth at the moment of asteroid-Earth nearest engine with the gas exhaust velocity c1. At moment t1 approach. For determination of optimal trajectories the the SC is applied the velocity impulse ∆V and the SC is maximum Pontrjagin principle is used.
    [Show full text]
  • Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling
    Dissertation zur Erlangung des akademischen Grades Doktor der Naturwissenschaften (doctor rerum naturalium) Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling Dipl.-Phys. Michael M¨uller 2007 Eingereicht und verteidigt am Fachbereich Geowissenschaften der Freien Universit¨atBerlin. Angefertigt am Institut f¨ur Planetenforschung des Deutschen Zentrums f¨urLuft- und Raumfahrt e.V. (DLR) in Berlin-Adlershof. arXiv:1208.3993v1 [astro-ph.EP] 20 Aug 2012 Gutachter Prof. Dr. Ralf Jaumann (Freie Universit¨atBerlin, DLR Berlin) Prof. Dr. Tilman Spohn (Westf¨alische Wilhems-Universit¨atM¨unster,DLR Berlin) Tag der Disputation 6. Juli 2007 In loving memory of Felix M¨uller(1948{2005). Wish you were here. Abstract The subject of this work is the physical characterization of asteroids, with an emphasis on the thermal inertia of near-Earth asteroids (NEAs). Thermal inertia governs the Yarkovsky effect, a non-gravitational force which significantly alters the orbits of asteroids up to ∼ 20 km in diameter. Yarkovsky-induced drift is important in the assessment of the impact hazard which NEAs pose to Earth. Yet, very little has previously been known about the thermal inertia of small asteroids including NEAs. Observational and theoretical work is reported. The thermal emission of aster- oids has been observed in the mid-infrared (5{35 µm) wavelength range using the Spitzer Space Telescope and the 3.0 m NASA Infrared Telescope Facility, IRTF; techniques have been established to perform IRTF observations remotely from Berlin. A detailed thermophysical model (TPM) has been developed and exten- sively tested; this is the first detailed TPM shown to be applicable to NEA data.
    [Show full text]
  • EUROMARGINS Final Report - Thursday, September 11, 2008 Page 1
    EUROMARGINS Final Report - Thursday, September 11, 2008 Page 1 European Science Foundation (ESF) The European Science Foundation (ESF) was established in 1974 to create a common European platform for cross‐border cooperation in all aspects of scientific research. With its emphasis on a multidisciplinary and pan‐European approach, the Foundation provides the leadership necessary to open new frontiers in European science. Its activities include providing science policy advice (Science Strategy); stimulating co‐operation between researchers and organisations to explore new directions (Science Synergy); and the administration of externally funded programmes (Science Management). These take place in the following areas: Physical and engineering sciences; Medical sciences; Life, earth and environmental sciences; Humanities; Social sciences; Polar; Marine; Space sciences; Radio astronomy frequencies; Nuclear physics. Headquartered in Strasbourg with offices in Brussels, the ESF’s membership comprises 75 national funding agencies, research performing organisations and academies from 30 European nations. The Foundation’s independence allows the ESF to objectively represent the priorities of all these members. What is a EUROCORES? The EUROCORES (ESF Collaborative Research) Scheme is an ESF instrument to stimulate collaboration between researchers based in Europe, and to maintain European research at an international competitive level. The EUROCORES Scheme provides a framework for national research funding agencies (research councils and academies and other funding organisations) to fund collaborative research, in and across all scientific areas. Participating funding agencies jointly define a research programme, specify the type of proposals to be requested and agree on the peer‐review procedure. The ESF, with funds from the EC Sixth Framework Programme under Contract no.
    [Show full text]
  • Robotic Asteroid Prospector (RAP) NASA Contract NNX12AR04G -- 9 July 2013, REV 12 Dec 2013 ©
    Phase I Final Report to NASA Innovative and Advanced Concepts (NIAC) Robotic Asteroid Prospector (RAP) NASA Contract NNX12AR04G -- 9 July 2013, REV 12 Dec 2013 © PI: Marc M. Cohen, Arch.D; Marc M. Cohen Architect P. C. Astrotecture™ http://www.astrotecture.com CoI for Mission and Spacecraft Design: Warren W. James, V Infinity Research LLC. CoI for Mining and Robotics: Kris Zacny, PhD, with Jack Craft and Philip Chu, Honeybee Robotics. Consultant for Mining Economics: Brad Blair, New Space Analytics LLC Table of Contents Abstract ............................................................................................................................. 5 Executive Summary ............................................................................................................ 6 1 Introduction ............................................................................................................... 10 1.1 Mineral Economics Strategy ............................................................................................................................ 10 1.2 Asteroids, Meteorites, and Metals ................................................................................................................. 10 1.2.1 Families of Metals ................................................................................................................................................ 10 1.2.2 Water from Carbonaceous Chondrites ....................................................................................................... 10 1.3
    [Show full text]
  • Origin and Evolution of Near-Earth Objects 409
    Morbidelli et al.: Origin and Evolution of Near-Earth Objects 409 Origin and Evolution of Near-Earth Objects A. Morbidelli Observatoire de la Côte d’Azur, Nice, France W. F. Bottke Jr. Southwest Research Institute, Boulder, Colorado Ch. Froeschlé Observatoire de la Côte d’Azur, Nice, France P. Michel Observatoire de la Côte d’Azur, Nice, France Asteroids and comets on orbits with perihelion distance q < 1.3 AU and aphelion distance Q > 0.983 AU are usually called near-Earth objects (NEOs). It has long been debated whether the NEOs are mostly of asteroidal or cometary origin. With improved knowledge of resonant dynamics, it is now clear that the asteroid belt is capable of supplying most of the observed NEOs. Particular zones in the main belt provide NEOs via powerful and diffusive resonances. Through the numerical integration of a large number of test asteroids in these zones, the pos- sible evolutionary paths of NEOs have been identified and the statistical properties of NEOs dynamics have been quantified. This work has allowed the construction of a steady-state model of the orbital and magnitude distribution of the NEO population, dependent on parameters that are quantified by calibration with the available observations. The model accounts for the exist- ence of ~1000 NEOs with absolute magnitude H < 18 (roughly 1 km in size). These bodies carry a probability of one collision with the Earth every 0.5 m.y. Only 6% of the NEO popu- lation should be of Kuiper Belt origin. Finally, it has been generally believed that collisional activity in the main belt, which continuously breaks up large asteroids, injects a large quantity of fresh material into the NEO source regions.
    [Show full text]
  • Scientific Rationale for Mobility in Planetary Environments
    Scientific Rationale for Mobility in Planetary Environments Committee on Planetary and Lunar Exploration Space Studies Board Commission on Physical Sciences, Mathematics, and Applications National Research Council NATIONAL ACADEMY PRESS Washington, D.C. 1999 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special competences and with regard for appropriate balance. The National Academy of Sciences is a private, nonprofit, self-perpetuating society of distinguished scholars engaged in scientific and engineering research, dedicated to the furtherance of science and technology and to their use for the general welfare. Upon the authority of the charter granted to it by the Congress in 1863, the Academy has a mandate that requires it to advise the federal government on scientific and technical matters. Dr. Bruce Alberts is president of the National Academy of Sciences. The National Academy of Engineering was established in 1964, under the charter of the National Academy of Sciences, as a parallel organization of outstanding engineers. It is autonomous in its administration and in the selection of its members, sharing with the National Academy of Sciences the responsibility for advising the federal government. The National Academy of Engineering also sponsors engineering programs aimed at meeting national needs, encourages education and research, and recognizes the superior achievements of engineers. Dr. William A. Wulf is president of the National Academy of Engineering.
    [Show full text]