"Ringing" from an Asteroid Collision Event Which Triggered the Flood?
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South Pole-Aitken Basin: Crater Size-Frequency Distribution Measurements
EPSC Abstracts Vol. 7 EPSC2012-832 2012 European Planetary Science Congress 2012 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2012 South Pole-Aitken Basin: Crater Size-Frequency Distribution Measurements H. Hiesinger1, C. H. van der Bogert1, J. H. Pasckert1, N. Schmedemann2, M.S. Robinson3, B. Jolliff4, and N. Petro5; 1Institut für Planetologie (IfP), WWU Münster, Wilhelm-Klemm-Straße 10, 48149 Münster, Germany ([email protected]/ +49-251-8339057), 2Institute of Geosciences, Freie Universität Berlin, Germany, 3Arizona State University, Tempe, USA, 4Dept. of Earth and Planet. Sci. Washington Univ., St. Louis, USA, 5Goddard Spaceflight Center, Greenbelt, USA. Introduction morphology and topography derived from the LROC Being the largest basin (>2500 km in diameter) WAC mosaic and LOLA. LOLA topography was and presumably the oldest preserved impact structure also used to identify old and highly degraded impact on the Moon [e.g., 1], the South Pole-Aitken (SPA) structures and to improve our statistics in areas with basin is of particular interest. SPA might have large shadows close to the pole. The CSFDs were penetrated the entire lunar crust and exposed lower plotted with CraterStats [7], applying the lunar crustal or upper mantle material, but despite its deep chronology (CF) of [8] and the production function penetration, it did not reveal KREEP-rich rocks in (PF) of [9]. From this we derived absolute model contrast with the Imbrium basin. In addition, its age ages (AMAs) for craters between ~1.5 km and 300 should shed light on the plausibility of the terminal km in diameter [9]. More details on the technique of cataclysm [e.g., 2]. -
10. Collisions • Use Conservation of Momentum and Energy and The
10. Collisions • Use conservation of momentum and energy and the center of mass to understand collisions between two objects. • During a collision, two or more objects exert a force on one another for a short time: -F(t) F(t) Before During After • It is not necessary for the objects to touch during a collision, e.g. an asteroid flied by the earth is considered a collision because its path is changed due to the gravitational attraction of the earth. One can still use conservation of momentum and energy to analyze the collision. Impulse: During a collision, the objects exert a force on one another. This force may be complicated and change with time. However, from Newton's 3rd Law, the two objects must exert an equal and opposite force on one another. F(t) t ti tf Dt From Newton'sr 2nd Law: dp r = F (t) dt r r dp = F (t)dt r r r r tf p f - pi = Dp = ò F (t)dt ti The change in the momentum is defined as the impulse of the collision. • Impulse is a vector quantity. Impulse-Linear Momentum Theorem: In a collision, the impulse on an object is equal to the change in momentum: r r J = Dp Conservation of Linear Momentum: In a system of two or more particles that are colliding, the forces that these objects exert on one another are internal forces. These internal forces cannot change the momentum of the system. Only an external force can change the momentum. The linear momentum of a closed isolated system is conserved during a collision of objects within the system. -
The Physics of a Car Collision by Andrew Zimmerman Jones, Thoughtco.Com on 09.10.19 Word Count 947 Level MAX
The physics of a car collision By Andrew Zimmerman Jones, ThoughtCo.com on 09.10.19 Word Count 947 Level MAX Image 1. A crash test dummy sits inside a Toyota Corolla during the 2017 North American International Auto Show in Detroit, Michigan. Crash test dummies are used to predict the injuries that a human might sustain in a car crash. Photo by: Jim Watson/AFP/Getty Images During a car crash, energy is transferred from the vehicle to whatever it hits, be it another vehicle or a stationary object. This transfer of energy, depending on variables that alter states of motion, can cause injuries and damage cars and property. The object that was struck will either absorb the energy thrust upon it or possibly transfer that energy back to the vehicle that struck it. Focusing on the distinction between force and energy can help explain the physics involved. Force: Colliding With A Wall Car crashes are clear examples of how Newton's Laws of Motion work. His first law of motion, also referred to as the law of inertia, asserts that an object in motion will stay in motion unless an external force acts upon it. Conversely, if an object is at rest, it will remain at rest until an unbalanced force acts upon it. Consider a situation in which car A collides with a static, unbreakable wall. The situation begins with car A traveling at a velocity (v) and, upon colliding with the wall, ending with a velocity of 0. The force of this situation is defined by Newton's second law of motion, which uses the equation of This article is available at 5 reading levels at https://newsela.com. -
Moon Minerals a Visual Guide
Moon Minerals a visual guide A.G. Tindle and M. Anand Preliminaries Section 1 Preface Virtual microscope work at the Open University began in 1993 meteorites, Martian meteorites and most recently over 500 virtual and has culminated in the on-line collection of over 1000 microscopes of Apollo samples. samples available via the virtual microscope website (here). Early days were spent using LEGO robots to automate a rotating microscope stage thanks to the efforts of our colleague Peter Whalley (now deceased). This automation speeded up image capture and allowed us to take the thousands of photographs needed to make sizeable (Earth-based) virtual microscope collections. Virtual microscope methods are ideal for bringing rare and often unique samples to a wide audience so we were not surprised when 10 years ago we were approached by the UK Science and Technology Facilities Council who asked us to prepare a virtual collection of the 12 Moon rocks they loaned out to schools and universities. This would turn out to be one of many collections built using extra-terrestrial material. The major part of our extra-terrestrial work is web-based and we The authors - Mahesh Anand (left) and Andy Tindle (middle) with colleague have build collections of Europlanet meteorites, UK and Irish Peter Whalley (right). Thank you Peter for your pioneering contribution to the Virtual Microscope project. We could not have produced this book without your earlier efforts. 2 Moon Minerals is our latest output. We see it as a companion volume to Moon Rocks. Members of staff -
Cretaceous - Tertiary Mass Extinction Meteoritic Versus Volcanic Causes
GENERAL I ARTICLE Cretaceous - Tertiary Mass Extinction Meteoritic Versus Volcanic Causes P V Sukumaran The bolide impact theory for mass extinctions at the Cretaceous-tertiary (K-T) boundary was a revolutionary concept. This theory was contested by short duration global volcanism as a possible alternative cause for the K-T extinction. Though there is a converging evidence for an extra-terrestrial impact coinciding with the P V Sukumaran took his terminal Cretaceous, the causative link between the M Tech degree in impact and the K-T mass extinction is debatable. Thus, Applied Geology from the while the impact theory is re-emerging, available evidence University of Saugar and has been with the is still insufficient to rule out either of the two hypotheses. Geological Survey of India since 1974. His interests Introduction include geochemistry, petrology and palae oceanography. He is It is now widely believed that life on earth began very early in presently posted to the its geological history, probably about 4000 My (million years) Marine Wing of the ago (Mojzsis and others, 1996). Since then it underwent Department and has participated in many several evolutionary branchings to the complex diversity as scientific cruises both as we see today. Nevertheless, it was not a smooth voyage for life Chief Scientist and as a all along, the evolution was punctuated by geologically participating scientist. ins tan taneous events of mass mortality. New species emerged at the expense of their predecessors following each extinction event and life went on evolving ever more vibrantly. In the geologic record of rock strata, such mass extinction events are identifiable based on sudden absence and reduction in diversity of fossil assemblage across stratigraphic boundaries. -
Lunar Meteorites: Impact Melt and Regolith Breccias and Large-Scale Heterogeneities of the Upper Lunar Crust
Meteoritics & Planetary Science 40, Nr 7, 989–1014 (2005) Abstract available online at http://meteoritics.org “New” lunar meteorites: Impact melt and regolith breccias and large-scale heterogeneities of the upper lunar crust Paul H. WARREN*, Finn ULFF-MØLLER, and Gregory W. KALLEMEYN Institute of Geophysics, University of California—Los Angeles, Los Angeles, California 90095–1567, USA *Corresponding author. E-mail: [email protected] (Received 06 May 2002; revision accepted 24 April 2005) Abstract–We have analyzed nine highland lunar meteorites (lunaites) using mainly INAA. Several of these rocks are difficult to classify. Dhofar 081 is basically a fragmental breccia, but much of its groundmass features a glassy-fluidized texture that is indicative of localized shock melting. Also, much of the matrix glass is swirly-brown, suggesting a possible regolith derivation. We interpret Dar al Gani (DaG) 400 as an extremely immature regolith breccia consisting mainly of impact-melt breccia clasts; we interpret Dhofar 026 as an unusually complex anorthositic impact-melt breccia with scattered ovoid globules that formed as clasts of mafic, subophitic impact melt. The presence of mafic crystalline globules in a lunar material, even one so clearly impact-heated, suggests that it may have originated as a regolith. Our new data and a synthesis of literature data suggest a contrast in Al2O3- incompatible element systematics between impact melts from the central nearside highlands, where Apollo sampling occurred, and those from the general highland surface of the Moon. Impact melts from the general highland surface tend to have systematically lower incompatible element concentration at any given Al2O3 concentration than those from Apollo 16. -
Carbon Monoxide in Jupiter After Comet Shoemaker-Levy 9
ICARUS 126, 324±335 (1997) ARTICLE NO. IS965655 Carbon Monoxide in Jupiter after Comet Shoemaker±Levy 9 1 1 KEITH S. NOLL AND DIANE GILMORE Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218 E-mail: [email protected] 1 ROGER F. KNACKE AND MARIA WOMACK Pennsylvania State University, Erie, Pennsylvania 16563 1 CAITLIN A. GRIFFITH Northern Arizona University, Flagstaff, Arizona 86011 AND 1 GLENN ORTON Jet Propulsion Laboratory, Pasadena, California 91109 Received February 5, 1996; revised November 5, 1996 for roughly half the mass. In high-temperature shocks, Observations of the carbon monoxide fundamental vibra- most of the O is converted to CO (Zahnle and MacLow tion±rotation band near 4.7 mm before and after the impacts 1995), making CO one of the more abundant products of of the fragments of Comet Shoemaker±Levy 9 showed no de- a large impact. tectable changes in the R5 and R7 lines, with one possible By contrast, oxygen is a rare element in Jupiter's upper exception. Observations of the G-impact site 21 hr after impact atmosphere. The principal reservoir of oxygen in Jupiter's do not show CO emission, indicating that the heated portions atmosphere is water. The Galileo Probe Mass Spectrome- of the stratosphere had cooled by that time. The large abun- ter found a mixing ratio of H OtoH of X(H O) # 3.7 3 dances of CO detected at the millibar pressure level by millime- 2 2 2 24 P et al. ter wave observations did not extend deeper in Jupiter's atmo- 10 at P 11 bars (Niemann 1996). -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
Lap02205 Lunar Meteorite: Lunar Mare Basalt with Similarities to the Apollo 12 Ilmenite Basalt
Lunar and Planetary Science XXXV (2004) 1548.pdf LAP02205 LUNAR METEORITE: LUNAR MARE BASALT WITH SIMILARITIES TO THE APOLLO 12 ILMENITE BASALT. T. Mikouchi1, J. Chokai1, T. Arai2, E. Koizumi1, A. Monkawa1, M. Miyamoto1, 1Dept. of Earth and Planetary Science, University of Tokyo, Hongo, Tokyo 113-0033, Japan ([email protected]), 2Lunar Exploration Tech. Office, Japan Aerospace Exploration Agency (JAXA), Tsukuba, Ibaraki, 305-8505, Japan. Introduction: LAP02205 is a new lunar meteorite and then decreases. The plagioclase composition recovered from the Antarctica. Although most lunar ranges from An91Or0 to An80Or7 (Fig. 2b). Plagioclase meteorites are brecciated, LAP02205 is a crystalline contains 0.5-2.5 wt% FeO and 0-0.5 wt% MgO. Oli- rock showing a basaltic texture, thus offering useful vine is remarkably zoned (Fo67-48) as pyroxenes (Fig. information to understand crystallization of lunar mare 2c). Minor elements in olivines are 0.3-0.4 wt% CaO basalt. In this abstract, we present initial results of our and 0.1-0.4 wt% Cr2O3. Most ilmenite grains contain ongoing petrological and mineralogical study of this very small amounts (~0.1 wt%) of MgO and Cr2O3. meteorite and discuss its relationship to other lunar Silica contains ~1 wt% Al2O3 and ~0.3 wt% TiO2. meteorites and Apollo samples. Spinels in LAP02205 are chemically zoned from the Petrography: The thin section (LAP02205,34) chromite core (6 wt% TiO2, 44 wt% Cr2O3, and 12 shows a medium-grained subophitic texture (Fig. 1a) wt% Al2O3) to thin ulvöspinel rim (32-25 wt% TiO2, 3- with evidence for moderate shock metamorphism (e.g., 14 wt% Cr2O3, and 2-4 wt% Al2O3). -
Relativistic Kinematics of Particle Interactions Introduction
le kin rel.tex Relativistic Kinematics of Particle Interactions byW von Schlipp e, March2002 1. Notation; 4-vectors, covariant and contravariant comp onents, metric tensor, invariants. 2. Lorentz transformation; frequently used reference frames: Lab frame, centre-of-mass frame; Minkowski metric, rapidity. 3. Two-b o dy decays. 4. Three-b o dy decays. 5. Particle collisions. 6. Elastic collisions. 7. Inelastic collisions: quasi-elastic collisions, particle creation. 8. Deep inelastic scattering. 9. Phase space integrals. Intro duction These notes are intended to provide a summary of the essentials of relativistic kinematics of particle reactions. A basic familiarity with the sp ecial theory of relativity is assumed. Most derivations are omitted: it is assumed that the interested reader will b e able to verify the results, which usually requires no more than elementary algebra. Only the phase space calculations are done in some detail since we recognise that they are frequently a bit of a struggle. For a deep er study of this sub ject the reader should consult the monograph on particle kinematics byByckling and Ka jantie. Section 1 sets the scene with an intro duction of the notation used here. Although other notations and conventions are used elsewhere, I present only one version which I b elieveto b e the one most frequently encountered in the literature on particle physics, notably in such widely used textb o oks as Relativistic Quantum Mechanics by Bjorken and Drell and in the b o oks listed in the bibliography. This is followed in section 2 by a brief discussion of the Lorentz transformation. -
Cosmic Collisions” Planetarium Show
“Cosmic Collisions” Planetarium Show Theme: A Tour of the Universe within the context of “Things Colliding with Other Things” The educational value of NASM Theater programming is that the stunning visual images displayed engage the interest and desire to learn in students of all ages. The programs do not substitute for an in-depth learning experience, but they do facilitate learning and provide a framework for additional study elaborations, both as part of the Museum visit and afterward. See the “Alignment with Standards” table for details regarding how Cosmic Collisions and its associated classroom extensions meet specific national standards of learning (SoL’s). Cosmic Collisions takes its audience on a tour of the Universe, from the very small (nuclear fusion processes powering our Sun) to the very large (galaxies), all in the context of the role “collisions” have in the overall scheme of things. Since the concept of large-scale collisions engages the attention of most learners of any age, Cosmic Collisions can be the starting point of a broader learning experience. What you will see in the Cosmic Collisions program: • Meteors (“shooting stars”) – fragments of a comet colliding with Earth’s atmosphere • The Impact Theory of the formation of the Moon • Collisions between hydrogen atoms in solar interior, resulting in nuclear fusion • Charged particles in the Solar Wind creating an aurora display when they hit Earth’s atmosphere • The very large impact that “killed the dinosaurs” • Future impact risk?!? – Perhaps flying a spaceship alongside would deflect enough… • Stellar collisions within a globular cluster • The Milky Way and Andromeda galaxies collide Learning Elaboration While Visiting the National Air and Space Museum Thousands of books and articles have been written about astronomy, but a good starting point is the many books and related materials available at the Museum Store in each NASM building. -
Stratigraphy of Barmer Basin, Rajasthan: Implications on Cretaceous-Tertiary Boundary*
828 NOTES STRATIGRAPHY OF BARMER BASIN, RAJASTHAN: IMPLICATIONS ON CRETACEOUS-TERTIARY BOUNDARY* M.S. SISODIA Department of Geology, J.N.Vyas University, Jodhpur - 342 005 Email: [email protected] EXTENDED ABSTRACT Earth scientistshave been in pursuit for 'longto frnd the anoma\iesmd as bi-stoPtion in the morphology ofthe EaTth. tn~tliabout: (1) What killed dinosaurs at the end-Cretaceous? If we imagine a scenario of the post 65 Ma era, it is possible and (2) Had the mass extinction during the geological history that the intelligent being of the future era may find these been abrupt or is a gradual process? The objective of this changes incorporated in a thin sedimentary layer with no paper is an attempt on the basis of data collected fiom lateral continuity, and may fall into the trap of interprcting the Barmer Basin, Rajasthan, to find a plausible answer to tens of thousand years as a very very small time period. It is these two questions. to be noted that the enormity of dinosaurs must have caused The palaeontological analysis done by Sepkoski (I 992) extinction of many of the species of the Cretaceous Period. reveals that the Earth has suffered five major mass Though, final blow responsible for complete deterioration extinctions during its history: during Late Ordovician, the in the environment could be an impact that led to the death Devonian, the Pertnian, the Triassic and the Cretaceous. It of dinosaurs. is generally believed that the species become extinct when The Banner Basin is a narrow N-S trending graben. Its their rate of adaptation is not able to compete with the western margin is defined by a NNW-SSE trending fault environrnei~talstress.