MOON FORMATION at the END of a COLLISION CHAIN Erik Asphaug
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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. -
How Earth Got Its Moon Article
FEATURE How Earth Got its MOON Standard formation tale may need a rewrite By Thomas Sumner he moon’s origin story does not add up. Most “Multiple impacts just make more sense,” says planetary scientists think that the moon formed in the earli- scientist Raluca Rufu of the Weizmann Institute of Science in est days of the solar system, around 4.5 billion years Rehovot, Israel. “You don’t need this one special impactor to Tago, when a Mars-sized protoplanet called Theia form the moon.” whacked into the young Earth. The collision sent But Theia shouldn’t be left on the cutting room floor just debris from both worlds hurling into orbit, where the rubble yet. Earth and Theia were built largely from the same kind of eventually mingled and combined to form the moon. material, new research suggests, and so had similar composi- If that happened, scientists expect that Theia’s contribution tions. There is no sign of “other” material on the moon, this would give the moon a different composition from Earth’s. perspective holds, because nothing about Theia was different. Yet studies of lunar rocks show that Earth and its moon are “I’m absolutely on the fence between these two opposing compositionally identical. That fact throws a wrench into the ideas,” says UCLA cosmochemist Edward Young. Determining planet-on-planet impact narrative. which story is correct is going to take more research. But the Researchers have been exploring other scenarios. Maybe answer will offer profound insights into the evolution of the the Theia impact never happened (there’s no direct evidence early solar system, Young says. -
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). -
"Ringing" from an Asteroid Collision Event Which Triggered the Flood?
The Proceedings of the International Conference on Creationism Volume 6 Print Reference: Pages 255-261 Article 23 2008 Is the Moon's Orbit "Ringing" from an Asteroid Collision Event which Triggered the Flood? Ronald G. Samec Bob Jones University Follow this and additional works at: https://digitalcommons.cedarville.edu/icc_proceedings DigitalCommons@Cedarville provides a publication platform for fully open access journals, which means that all articles are available on the Internet to all users immediately upon publication. However, the opinions and sentiments expressed by the authors of articles published in our journals do not necessarily indicate the endorsement or reflect the views of DigitalCommons@Cedarville, the Centennial Library, or Cedarville University and its employees. The authors are solely responsible for the content of their work. Please address questions to [email protected]. Browse the contents of this volume of The Proceedings of the International Conference on Creationism. Recommended Citation Samec, Ronald G. (2008) "Is the Moon's Orbit "Ringing" from an Asteroid Collision Event which Triggered the Flood?," The Proceedings of the International Conference on Creationism: Vol. 6 , Article 23. Available at: https://digitalcommons.cedarville.edu/icc_proceedings/vol6/iss1/23 In A. A. Snelling (Ed.) (2008). Proceedings of the Sixth International Conference on Creationism (pp. 255–261). Pittsburgh, PA: Creation Science Fellowship and Dallas, TX: Institute for Creation Research. Is the Moon’s Orbit “Ringing” from an Asteroid Collision Event which Triggered the Flood? Ronald G. Samec, Ph. D., M. A., B. A., Physics Department, Bob Jones University, Greenville, SC 29614 Abstract We use ordinary Newtonian orbital mechanics to explore the possibility that near side lunar maria are giant impact basins left over from a catastrophic impact event that caused the present orbital configuration of the moon. -
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. -
Way-Out World
Non-fiction: Way-Out World Way-Out World By Hugh Westrup What strange satellite circles the visible edge of the solar system? The detonation of a single nuclear bomb can do catastrophic damage. So imagine the power of more than one bomb—not just two or 10 or even 10 million, but 10 billion. Astronomers have evidence that a collision with enough force to equal the explosion of 10 billion nuclear bombs once happened in the solar system. Out of that crack-up was born one of the oddest things in space. Its name is Haumea. “There is so much to learn about this newfound object, and we keep finding surprises,” says Mike Brown, an astronomer at the California Institute of Technology. “It’s just crazy.” ODD Balls The solar system is always changing. What astronomers know about it is changing even faster. Advances in telescope technology keep deepening their view of space, continually revealing new objects and new features on old objects. One example of that change in perspective is Pluto. For more than 70 years, astronomers considered it the ninth planet. Then, in 2007, the International Astronomical Union reclassified it as a dwarf planet. Like a planet, a dwarf planet orbits the sun. It also has enough mass, and therefore enough gravity, to give it a rounded shape. But it lacks pull; its gravity isn’t strong enough to clear its neighborhood of most smaller objects the way that planets do. A year later Pluto was reclassified again. Now it’s a plutoid. A plutoid is simply a dwarf planet that exists beyond Neptune, the eighth planet. -
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. -
Waves, Sampling) Our Solar System: Sizes Are to Scale; Distances Are Not!
OCN 201: Origin of the Earth and Oceans Waimea Bay, Jan 2002 Periodic Table of the Elements Noble IA IIA IIIA IVA VA VIA VIIA VIIIA IB IIB IIIB IVB VB VIB VIIB gases H He Li Be B C N O FNe Na Mg Al Si P S Cl Ar K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr RbSrY ZrNbMoTcRuRhPdAgCdInSnSbTeI Xe Cs Ba La Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn Fr Ra Ac Lanthanides: Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Actinides: Th Pa U Sun Earth Oceans Atmosphere Life H, He Fe, O, Si, Mg O, H N, O H2O, C Ni, Ca, S, Al Cl, Na, Mg, S, Ca, K Ar, H2O, CO2 N, P With only a few exceptions, each of these reservoirs is made up of a different set of elements. This implies CHEMICAL DIFFERENTIATION. CHEMICAL DIFFERENTIATION: --large-scale separation of chemical elements on the basis of their physical and chemical properties, by a variety of processes Solar System:Sun Inner rocky planets (Mercury, Venus, Earth, Mars, asteroid belt) Outer gas-giant planets (Jupiter, Saturn) Outer ice-giant planets (Uranus, Neptune) Earth: *Core of iron *Mantle and crust of rock Oceans Atmosphere (*How do we know? Meteorites, bulk density, seismic waves, sampling) Our Solar System: sizes are to scale; distances are not! Inner rocky planets: Mercury, Venus, Earth, Mars, asteroid belt Outer gas-giants: Jupiter, Saturn Outer ice-giants: Uranus, Neptune (Pluto is rocky and about the size of Earth’s Moon. -
April 15, 2017 How Earth Got Its Moon
April 15, 2017 IN HIGH SCHOOLS How Earth Got its Moon Article-Based Observation Directions: After reading the article “How Earth got its moon,” answer these questions: 1. What was the moon-formation idea proposed in the mid-1970s? 2. Why does the author describe Earth’s moon as an “oddball”? 3. A study in 2001 analyzed rocks collected during the Apollo mission to the moon. How did these lunar rocks support the hypothesis that the moon was formed by multiple impacts and contradict the giant-impact hypothesis? 4. What did planetary scientist Raluca Rufu and her colleagues learn recently that supports the multi-impact hypothesis? Explain how their findings support this hypothesis and why scientists were not able to figure this out previously. 5. According to planetary scientist Nicolas Dauphas, how does the isotopic combination of materials that make up Earth tell a story that supports the idea of a single impact? What does Dauphas say supplied the Earth’s mass? BLACKLINE MASTER 1, P. 1 6. Planetary scientist Sarah Stewart states that we need to test all the new ideas about the moon’s formation. Describe the recent test that used temperature to help explain how the moon formed, and explain which moon-formation idea is consistent with the results. 7. Explain the similarities and differences between the graphic titled “Making moons” and the com- puter simulation images shown below. R. CANUP/SWRI Making moons The multi-impact hypothesis says several small hits sent terrestrial materials into orbit that eventually formed our large moon. First Disk of debris Moonlet drifts Subsequent Disk formation Moonlets merge in impact forms outward impact far-out orbit (Repeat) Millions Days Centuries of years Days Centuries R. -
Light Hydrogen in the Lunar Interior: No One Expects the Theia Contribution
EPSC Abstracts Vol. 13, EPSC-DPS2019-2056, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Light Hydrogen in the Lunar Interior: No One Expects the Theia Contribution Steven J. Desch (1), Katharine L. Robinson (2) (1) School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA, (2) Lunar and Planetary Institute, Houston, TX, USA ([email protected]) Abstract × 1021 kg) solar nebula hydrogen with D/H=21 × 10-6, combined with ~8 oceans of chondritic water with D/H=140 × 10-6, leading to some materials with The Moon is thought to have formed after a planetary -6 embryo, known as Theia, collided with the proto- D/H=120 × 10 (δD≈-230‰) that should reside at the Earth over 4.5 billion years ago. For the first time, we Earth’s core-mantle boundary. The discovery of samples with δD≈-218‰ in terrestrial lavas sampling use H isotopes to help constrain the composition of deep-mantle plumes [8] may support this hypothesis. Theia. We suggest the Moon incorporated very low- D/H (δD ≈ -750‰) hydrogen derived from solar nebula H2 ingassed into the magma ocean of a large (~0.4 ME), enstatite chondrite-like planetary embryo that was largely devoid of chondritic water. These new constraints have profound implications for the Moon-forming impact and the evolution of the Earth- Moon system. 1. Introduction Apatite [Ca5(PO4)3(OH,F,Cl) is the only water- bearing mineral found in lunar samples. Hydrogen isotopic measurements of apatites in lunar rocks show that there seem to be multiple H reservoirs with diverse D/H ratios within the lunar interior, e.g. -
Collision-Free Kinematics for Redundant Manipulators in Dynamic Scenes Using Optimal Reciprocal Velocity Obstacles*
Collision-Free Kinematics for Redundant Manipulators in Dynamic Scenes using Optimal Reciprocal Velocity Obstacles* Liangliang Zhao1, Jingdong Zhao1, Hong Liu1, and Dinesh Manocha2 Abstract— We present a novel algorithm for collision-free kinematics of multiple manipulators in a shared workspace with moving obstacles. Our optimization-based approach simultaneously handles collision-free constraints based on reciprocal velocity obstacles and inverse kinematics constraints for high-DOF manipulators. We present an efficient method based on particle swarm optimization that can generate collision-free configurations for each redundant manipulator. Furthermore, our approach can be used to compute safe and oscillation-free trajectories in a few milli-seconds. We highlight the real-time performance of our algorithm on multiple Baxter robots with 14-DOF manipulators operating in a workspace with dynamic obstacles. Videos are available at https://sites.google.com/view/collision-free-kinematics I. INTRODUCTION Redundant manipulators are widely used in complex and cluttered environments for various kinds of tasks. Moreover, Fig 1. Solving inverse kinematics on a Baxter robots many applications use multiple manipulators that work manipulator (7-DOF) in the workspace. Our algorithm can cooperatively in an environment with moving obstacles (e.g. compute the inverse kinematics solutions for these humans). To perform the tasks, the planning algorithms must redundant manipulators, and avoid collisions (red sphere) compute trajectories that simultaneously satisfy two sets of between the robots. The blue line is the desired path of the constraints: end effector. 1. Inverse Kinematics Constraints: Given the pose of workspace among other redundant manipulators and static or each end-effector, we need to compute joint dynamic obstacles.