Unraveling Earth's Early History
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The History of Planet Earth
SECOND EDITION Earth’s Evolving The History of Systems Planet Earth Ronald Martin, Ph.D. University of Delaware Newark, Delaware © Jones & Bartlett Learning, LLC, an Ascend Learning Company. NOT FOR SALE OR DISTRIBUTION 9781284457162_FMxx_00i_xxii.indd 1 07/11/16 1:46 pm World Headquarters Jones & Bartlett Learning 5 Wall Street Burlington, MA 01803 978-443-5000 [email protected] www.jblearning.com Jones & Bartlett Learning books and products are available through most bookstores and online booksellers. To contact Jones & Bartlett Learning directly, call 800-832-0034, fax 978-443-8000, or visit our website, www.jblearning.com. Substantial discounts on bulk quantities of Jones & Bartlett Learning publications are available to corporations, professional associations, and other qualified organizations. For details and specific discount information, contact the special sales department at Jones & Bartlett Learning via the above contact information or send an email to [email protected]. Copyright © 2018 by Jones & Bartlett Learning, LLC, an Ascend Learning Company All rights reserved. No part of the material protected by this copyright may be reproduced or utilized in any form, electronic or mechanical, including photocopying, recording, or by any information storage and retrieval system, without written permission from the copyright owner. The content, statements, views, and opinions herein are the sole expression of the respective authors and not that of Jones & Bartlett Learning, LLC. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not constitute or imply its endorsement or recommendation by Jones & Bartlett Learning, LLC, and such reference shall not be used for advertis- ing or product endorsement purposes. -
Foundations of Complex Life: Evolution, Preservation and Detection on Earth and Beyond
National Aeronautics and Space Administration NASA Astrobiology Institute Annual Science Report 2016 Team Report: Foundations of Complex Life: Evolution, Preservation and Detection on Earth and Beyond, Massachusetts Institute of Technology Foundations of Complex Life Evolution, Preservation and Detection on Earth and Beyond Lead Institution: Massachusetts Institute of Technology Team Overview Foundations of Complex Life is a research project investigating the early evolution and preservation of complex life on Earth. We seek insight into the early evolution and preservation of complex life by refining our ability to identify evidence of environmental and biological change in the late Mesoproterozoic to Neoproterozoic eras. Better understanding how signatures of life and environment are preserved will guide how and where to look for evidence for life elsewhere in the universe—directly supporting the Curiosity mission on Mars and helping set strategic goals for future explorations of the Solar System and studies of the early Earth. Our Team pursues these questions under five themes: I. The earliest history of animals: We use methods from molecular biology, experimental taphonomy, and paleontology to explore what caused the early divergence of animals. Principal Investigator: II. Paleontology, sedimentology, and geochemistry: We track the origin of complex Roger Summons protists and animals from their biologically simple origins by documenting the stratigraphy, isotopic records, and microfossil assemblages of well-preserved rock successions from 1200 to 650 million years ago. III. A preservation-induced oxygen tipping point: We investigate how changes in the preservation of organic carbon may have driven the Neoproterozoic oxygenation of the oceans coincident with the appearance of complex life. -
Nature Based Solutions FEMA
PROMOTING NATURE-BASED HAZARD MITIGATION THROUGH FEMA MITIGATION GRANTS ABBREVIATIONS ADCIRC – Advanced Circulation Model HGM Approach – Hydrogeomorphic Approach BCA – Benefit-Cost Analysis HMA – Hazard Mitigation Assistance BCR – Benefit-Cost Ratio HMGP – Hazard Mitigation Grant Program BRIC – Building Resilient Infrastructure and MSCP – Multiple Species Conservation Program Communities NBS – Nature-Based Solution C&CB – Capability- and Capacity-Building NFIP – National Flood Insurance Program CDBG-DR – Community Development Block Grant- Disaster Recovery NFWF – National Fish and Wildlife Foundation CDBG-MIT – Community Development Block NOAA – National Oceanic and Atmospheric Grant-Mitigation Administration D.C. – District of Columbia NOFO – Notice of Funding Opportunity DEM – Department of Emergency Management NPV – Net Present Value DOI – Department of the Interior SCC – State Coastal Conservancy EDYS – Ecological Dynamics Simulation SDG&E – San Diego Gas & Electric EMA – Emergency Management Agency SFHA – Special Flood Hazard Area EPA SWMM – Environmental Protection Agency SHMO – State Hazard Mitigation Officer Storm Water Management Model SLAMM – Sea Level Affecting Marshes Model FEMA – Federal Emergency Management Agency SRH-2D – Sedimentation and River Hydraulics – FIRM – Flood Insurance Rate Map Two-Dimension FMA – Flood Mitigation Assistance STWAVE – Steady-State Spectral Wave Model FMAG – Fire Management Assistance Grant TNC – The Nature Conservancy HAZUS – Hazards US USACE – U.S. Army Corps of Engineers HEC-HMS – Hydrologic -
Hutton, Kelvin, and the Great Earth Debates. • the Beginnings of Modern Geology “All Natural Processes That Affect the Earth’S Crust (Erosion, Deposition, • Ca
Chapter 1 The Science of Geology An Introduction to Geology • Geology - the science that pursues an understanding of planet Earth • Physical geology - examines the materials composing Earth and seeks to understand the many processes that operate beneath and upon its surface • Historical geology - seeks an understanding of the origin of “If there is an interesting place you want to go, there is Earth and its development interesting geology that you can study there” through time Mersin ophiolite, (Cappadocia, Central Turkey). Turkey The Science of Geology The Science of Geology 1.3: satellite image of Mt. Vesuvius, Italy. • Some historical views • Geology, people, and the environment of the Earth • Many important relationships exist between • Aristotle, 300 BC; people and the natural environment • James Ussher, ca. 1600, ‘Earth was created in Problems and issues 4004 BC;’ addressed by • Catastrophism geology include • Earth’s features formed through • Natural hazards, sudden and violent resources, world changes. ‘The Dog population growth, of and environmental Pompeii’ issues Dwelling in Goreme, Cappadocia The Science of Geology Hutton, Kelvin, and the great Earth debates. • The beginnings of modern geology “All natural processes that affect the Earth’s crust (erosion, deposition, • ca. 1780, James Huton’s volcanic eruptions, faulting, glaciation Theory of the Earth; etc.) operate with the same intensity • Uniformitarianism: “the and under the same set of physical processes that operate constraints now as in the geologic past.” today have operated in “(as to the age of Earth) we see no the past.” vestige of a beginning, no prospect of • a uniformitarian view of an end.” Earth requires a vast These points are incorrect - why? amount of time…. -
Elliptical Instability in Terrestrial Planets and Moons
A&A 539, A78 (2012) Astronomy DOI: 10.1051/0004-6361/201117741 & c ESO 2012 Astrophysics Elliptical instability in terrestrial planets and moons D. Cebron1,M.LeBars1, C. Moutou2,andP.LeGal1 1 Institut de Recherche sur les Phénomènes Hors Equilibre, UMR 6594, CNRS and Aix-Marseille Université, 49 rue F. Joliot-Curie, BP 146, 13384 Marseille Cedex 13, France e-mail: [email protected] 2 Observatoire Astronomique de Marseille-Provence, Laboratoire d’Astrophysique de Marseille, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, France Received 21 July 2011 / Accepted 16 January 2012 ABSTRACT Context. The presence of celestial companions means that any planet may be subject to three kinds of harmonic mechanical forcing: tides, precession/nutation, and libration. These forcings can generate flows in internal fluid layers, such as fluid cores and subsurface oceans, whose dynamics then significantly differ from solid body rotation. In particular, tides in non-synchronized bodies and libration in synchronized ones are known to be capable of exciting the so-called elliptical instability, i.e. a generic instability corresponding to the destabilization of two-dimensional flows with elliptical streamlines, leading to three-dimensional turbulence. Aims. We aim here at confirming the relevance of such an elliptical instability in terrestrial bodies by determining its growth rate, as well as its consequences on energy dissipation, on magnetic field induction, and on heat flux fluctuations on planetary scales. Methods. Previous studies and theoretical results for the elliptical instability are re-evaluated and extended to cope with an astro- physical context. In particular, generic analytical expressions of the elliptical instability growth rate are obtained using a local WKB approach, simultaneously considering for the first time (i) a local temperature gradient due to an imposed temperature contrast across the considered layer or to the presence of a volumic heat source and (ii) an imposed magnetic field along the rotation axis, coming from an external source. -
The Solar System
5 The Solar System R. Lynne Jones, Steven R. Chesley, Paul A. Abell, Michael E. Brown, Josef Durech,ˇ Yanga R. Fern´andez,Alan W. Harris, Matt J. Holman, Zeljkoˇ Ivezi´c,R. Jedicke, Mikko Kaasalainen, Nathan A. Kaib, Zoran Kneˇzevi´c,Andrea Milani, Alex Parker, Stephen T. Ridgway, David E. Trilling, Bojan Vrˇsnak LSST will provide huge advances in our knowledge of millions of astronomical objects “close to home’”– the small bodies in our Solar System. Previous studies of these small bodies have led to dramatic changes in our understanding of the process of planet formation and evolution, and the relationship between our Solar System and other systems. Beyond providing asteroid targets for space missions or igniting popular interest in observing a new comet or learning about a new distant icy dwarf planet, these small bodies also serve as large populations of “test particles,” recording the dynamical history of the giant planets, revealing the nature of the Solar System impactor population over time, and illustrating the size distributions of planetesimals, which were the building blocks of planets. In this chapter, a brief introduction to the different populations of small bodies in the Solar System (§ 5.1) is followed by a summary of the number of objects of each population that LSST is expected to find (§ 5.2). Some of the Solar System science that LSST will address is presented through the rest of the chapter, starting with the insights into planetary formation and evolution gained through the small body population orbital distributions (§ 5.3). The effects of collisional evolution in the Main Belt and Kuiper Belt are discussed in the next two sections, along with the implications for the determination of the size distribution in the Main Belt (§ 5.4) and possibilities for identifying wide binaries and understanding the environment in the early outer Solar System in § 5.5. -
Chapter 8: Geologic Time
Chapter 8: Geologic Time 1. The Art of Time 2. The History of Relative Time 3. Geologic Time 4. Numerical Time 5. Rates of Change Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Geologic Time How long has this landscape looked like this? How can you tell? Will your grandchildren see this if they hike here in 80 years? The Good Earth/Chapter 8: Geologic Time The Art of Time How would you create a piece of art to illustrate the passage of time? How do you think the Earth itself illustrates the passage of time? What time scale is illustrated in the example above? How well does this relate to geological time/geological forces? The Good Earth/Chapter 8: Geologic Time Go back to the Table of Contents Go to the next section: The History of (Relative) Time The Good Earth/Chapter 8: Geologic Time The History of (Relative) Time Paradigm shift: 17th century – science was a baby and geology as a discipline did not exist. Today, hypothesis testing method supports a geologic (scientific) age for the earth as opposed to a biblical age. Structures such as the oldest Egyptian pyramids (2650-2150 B.C.) and the Great Wall of China (688 B.C.) fall within a historical timeline that humans can relate to, while geological events may seem to have happened before time existed! The Good Earth/Chapter 8: Geologic Time The History of (Relative) Time • Relative Time = which A came first, second… − Grand Canyon – B excellent model − Which do you think happened first – the The Grand Canyon – rock layers record thousands of millions of years of geologic history. -
Chapter 7: the Age of Earth
Earth and Life History Ancient Carvings These beautiful formations in Paria Canyon, along the boder of Arizona and Utah, were carved by the Paria River about 5.4 million years ago. 40,000–12,000 1875 Years Ago Henry Hancock discovers that a Organisms are trapped tooth more than 23 cm long and in tar pits found at La 9 cm wide may be from a saber- Brea (Los Angeles, tooth cat; realizes the bones at California). La Brea could be ancient. A.D. 1 1750 1800 1850 1900 1795 1896 James Hutton pro- Henri Becquerel dis- poses idea that covers radioactivity of natural processes uranium salts not long forming rock layers after Wilhelm Conrad occur uniformly Roentgen discovers throughout time. the X ray in 1895. 278 (bkgd)Layne Kennedy/CORBIS, (t)Albert Copley/Visuals Unlimited, (b)American Institute of Physics/Emilio Segrè Visual Archives To learn more about geologists and paleontologists and their work, visit ca7.msscience.com. Interactive Time Line To learn more about these events and others, visit ca7.msscience.com. c. 1910–1915 1980 1990 First scientific digs of the La Luis and Walter Alvarez from UC NASA researchers Kevin Pope, Brea Tar Pits are made by Berkeley propose that an asteroid Adriana Ocampo, and Charles scientists from the Univer- crashed into Earth 65 million years Duller, identify a huge crater sity of California; about ago, causing the sudden extinction in the Yucatan, Mexico, that 170,000 fossils found. of dinosaurs and many other living they think is the site of the things. asteroid crash. 1900 1920 1940 1960 1980 2000 2020 1913 1967 November 2002 First numeric time scale of geo- Richard Leakey finds two The National Science Founda- logic ages is proposed by skulls and uses new technol- tion launches a program, sci- Arthur Holmes of Great Britain; ogy to date objects more entists from around the world he used radioactive means to accurately; one is 195,000 will verify dates and class of measure the age of Earth years old, the oldest for a old specimens and analyze (about 4 billion years old). -
A Christian Physicist Examines Noah's Flood and Plate Tectonics
A Christian Physicist Examines Noah’s Flood and Plate Tectonics by Steven Ball, Ph.D. September 2003 Dedication I dedicate this work to my friend and colleague Rodric White-Stevens, who delighted in discussing with me the geologic wonders of the Earth and their relevance to Biblical faith. Cover picture courtesy of the U.S. Geological Survey, copyright free 1 Introduction It seems that no subject stirs the passions of those intending to defend biblical truth more than Noah’s Flood. It is perhaps the one biblical account that appears to conflict with modern science more than any other. Many aspiring Christian apologists have chosen to use this account as a litmus test of whether one accepts the Bible or modern science as true. Before we examine this together, let me clarify that I accept the account of Noah’s Flood as completely true, just as I do the entirety of the Bible. The Bible demonstrates itself to be reliable and remarkably consistent, having numerous interesting participants in various stories through which is interwoven a continuous theme of God’s plan for man’s redemption. Noah’s Flood is one of those stories, revealing to us both God’s judgment of sin and God’s over-riding grace and mercy. It remains a timeless account, for it has much to teach us about a God who never changes. It is one of the most popular Bible stories for children, and the truth be known, for us adults as well. It is rather unfortunate that many dismiss the account as mythical, simply because it seems to be at odds with a scientific view of the earth. -
The Composition of Planetary Atmospheres 1
The Composition of Planetary Atmospheres 1 All of the planets in our solar system, and some of its smaller bodies too, have an outer layer of gas we call the atmosphere. The atmosphere usually sits atop a denser, rocky crust or planetary core. Atmospheres can extend thousands of kilometers into space. The table below gives the name of the kind of gas found in each object’s atmosphere, and the total mass of the atmosphere in kilograms. The table also gives the percentage of the atmosphere composed of the gas. Object Mass Carbon Nitrogen Oxygen Argon Methane Sodium Hydrogen Helium Other (kilograms) Dioxide Sun 3.0x1030 71% 26% 3% Mercury 1000 42% 22% 22% 6% 8% Venus 4.8x1020 96% 4% Earth 1.4x1021 78% 21% 1% <1% Moon 100,000 70% 1% 29% Mars 2.5x1016 95% 2.7% 1.6% 0.7% Jupiter 1.9x1027 89.8% 10.2% Saturn 5.4x1026 96.3% 3.2% 0.5% Titan 9.1x1018 97% 2% 1% Uranus 8.6x1025 2.3% 82.5% 15.2% Neptune 1.0x1026 1.0% 80% 19% Pluto 1.3x1014 8% 90% 2% Problem 1 – Draw a pie graph (circle graph) that shows the atmosphere constituents for Mars and Earth. Problem 2 – Draw a pie graph that shows the percentage of Nitrogen for Venus, Earth, Mars, Titan and Pluto. Problem 3 – Which planet has the atmosphere with the greatest percentage of Oxygen? Problem 4 – Which planet has the atmosphere with the greatest number of kilograms of oxygen? Problem 5 – Compare and contrast the objects with the greatest percentage of hydrogen, and the least percentage of hydrogen. -
Origins of Life in the Universe Zackary Johnson
11/4/2007 Origins of Life in the Universe Zackary Johnson OCN201 Fall 2007 [email protected] Zackary Johnson http://www.soest.hawaii.edu/oceanography/zij/education.html Uniiiversity of Hawaii Department of Oceanography Class Schedule Nov‐2Originsof Life and the Universe Nov‐5 Classification of Life Nov‐7 Primary Production Nov‐9Consumers Nov‐14 Evolution: Processes (Steward) Nov‐16 Evolution: Adaptation() (Steward) Nov‐19 Marine Microbiology Nov‐21 Benthic Communities Nov‐26 Whale Falls (Smith) Nov‐28 The Marine Food Web Nov‐30 Community Ecology Dec‐3 Fisheries Dec‐5Global Ecology Dec‐12 Final Major Concepts TIMETABLE Big Bang! • Life started early, but not at the beginning, of Earth’s Milky Way (and other galaxies formed) history • Abiogenesis is the leading hypothesis to explain the beginning of life on Earth • There are many competing theories as to how this happened • Some of the details have been worked out, but most Formation of Earth have not • Abiogenesis almost certainly occurred in the ocean 20‐15 15‐94.5Today Billions of Years Before Present 1 11/4/2007 Building Blocks TIMETABLE Big Bang! • Universe is mostly hydrogen (H) and helium (He); for Milky Way (and other galaxies formed) example –the sun is 70% H, 28% He and 2% all else! Abundance) e • Most elements of interest to biology (C, N, P, O, etc.) were (Relativ 10 produced via nuclear fusion Formation of Earth Log at very high temperature reactions in large stars after Big Bang 20‐13 13‐94.7Today Atomic Number Billions of Years Before Present ORIGIN OF LIFE ON EARTH Abiogenesis: 3 stages Divine Creation 1. -
Internal Constitution of Mars
Journalof GeophysicalResearch VOLUME 77 FEBRUARY 10., 1972 NUMBER 15 Internal Constitution of Mars Do• L. ANDERSON SeismologicalLaboratory, California Institute o/ Technology Pasadena, California 91109 Models for the internal structure of Mars that are consistentwith its mass, radius, and moment of inertia have been constructed.Mars cannot be homogeneousbut must have a core, the size of which dependson its density and, therefore, on its composition.A meteorite model for Mars implies an Fe-S-Ni core (12% by massof the planet) and an Fe- or FeO-rich mantle with a zero-pressuredensity of approximately 3.54 g/cm•. Mars has an iron content of 25 wt %, which is significantly less than the iron content of the earth, Mercury, or Venus but is close to the total iron content of ordinary and carbonaceouschondrites. A satisfactory model for Mars can be obtained by exposing ordinary chondrites to relatively modest temperatures. Core formation will start when temperaturesexceed the cutecftc temperature in the system Fe-FeS (•990øC) but will not go to completionunless temperatures exceed the liquidus through- out most of the planet. No high-temperature reduction stage is required. The size and density of the core and the density of the mantle indicate that approximately63% of the potential core-forming material (Fe-S-Ni) has entered the core. Therefore, Mars, in contrast to the earth, is an incompletely differentiated planet, and its core is substantially richer in sulfur than the earth's core. The thermal energy associated with core formation in Mars is negligible. The absenceof a magnetic field can be explained by lack of lunar precessional torques and by the small size and high resistivity of the Martian core.