EARTH SCIENCE CONCEPTUAL FRAMEWORK GRADES K–12 • WCCUSD/UCMP EARTH AS a SYSTEM Theme/Questions K-2 3-5 6-8 9-12

Total Page:16

File Type:pdf, Size:1020Kb

EARTH SCIENCE CONCEPTUAL FRAMEWORK GRADES K–12 • WCCUSD/UCMP EARTH AS a SYSTEM Theme/Questions K-2 3-5 6-8 9-12 EARTH SCIENCE CONCEPTUAL FRAMEWORK GRADES K–12 • WCCUSD/UCMP EARTH AS A SYSTEM Theme/Questions K-2 3-5 6-8 9-12 How is the Earth part The Earth is part of a bigger system The Earth is part of the Solar System. The Earth is part of the Solar System. The Earth is part of the Solar System. of a larger system? called the Solar System. How do the four The Earth’s position in relation to the The relative positions of Earth and The tilt of the Earth’s axis and the spheres (lithosphere, Sun changes what happens on Earth. Sun affect the dynamics of the Earth. Earth’s orbit affect Earth’s seasons, cli- atmosphere, hydro- mate belts, and global wind and ocean sphere, biosphere) currents. interact? The gravitational forces of the moon, What evidence is sun, and all other celestial bodies infl u- there of this interac- ence the Earth. tion? The planet Earth has a distinct inter- The planet Earth has distinct layers The planet Earth is made of layers dis- The planet Earth is made of layers dis- nal structure composed of the crust, (crust, mantle, and core) that look tinguished by composition, structure, tinguished by composition, structure, mantle, and core. and act differently. and temperature. and temperature. Earth is made up of land, water, air, Earth is composed of land, water, air, The planet Earth is composed of the The planet Earth is composed of litho- and living things. and living things. lithosphere, hydrosphere, atmosphere, sphere, hydrosphere, atmosphere, and and biosphere. The boundaries of biosphere. The boundaries of these these spheres are not fi xed. spheres are not fi xed. Land is solid and is made of rocks, The properties of rocks and minerals The lithosphere is composed of oce- The lithosphere is composed of oceanic soils and living things. There are dif- in the crust refl ect processes that form anic and continental plates that move and continental plates that move along ferent kinds of rocks. Land has differ- them. Different landforms result from along the plate boundaries as a result the plate boundaries as a result of con- ent shapes called landforms. wind, water, and earth movements. of convection currents in the Earth’s vection currents in the Earth’s mantle. mantle. Plate movements, along with Different landforms result from plate weathering, erosion, and deposition movements, weathering, erosion, and are responsible for many of Earth’s deposition. Minerals and rocks have landforms. The properties of rocks physical and chemical properties that and minerals in the crust refl ect pro- provide evidence of the processes cesses that form them. through which they were formed. Water forms rivers, lakes, and oceans. Water exists on the Earth’s surface Water cycles among the lithosphere, Water cycles among the lithosphere, Water can also exist as ice, mist, (oceans, rivers, ice) and in the air (at- biosphere, and atmosphere. biosphere, and atmosphere. Water, in clouds, and steam. mosphere). Water acts as an important agent of its various states, acts as an agent of Water is an important agent of change change on the Earth’s surface and change on the Earth’s surface. on the Earth’s surface. lithosphere. We live on Earth, along with all other All four spheres interact with one an- All four spheres interact with one The interaction of the four spheres living things (other plants and ani- other. These interactions are refl ected another. These interactions are impor- shape the Earth’s surface, weather, and mals). in the different biomes and ecosys- tant in determining the Earth’s sur- ecosystems. People, other animals, and plants tems. face, weather, and ecosystems. need air, food water, and a place to live. Draft of Earth Science Conceptual Framework for Grades K–12 developed by WCCUSD/AK teachers. © 2004 UC Museum of Paleontology and West Contra Costa Unifi ed School District. EARTH SCIENCE CONCEPTUAL FRAMEWORK GRADES K–12 • WCCUSD/UCMP CHANGE Theme/Questions K–2 3–5 6–8 9–12 In what ways does the The Earth changes over time. Some The Earth changes over time. Some The Earth is always changing. There The Earth is always changing. There Earth change? changes are fast and some are slow. changes take a long time (climate), are short-term and long-term, large- are short-term and long-term, large- Some changes are big and some are some changes happen more quickly scale and small-scale changes. scale and small-scale changes. Rates of What causes change small. (weather). There are large-scale change are dependent upon the agent in the Earth? changes (earthquakes, tsunami, vol- of change. cano) and more ordinary changes What is the evidence (weathering, erosion, glaciation). that change has oc- curred? Earth’s surface is always changing. Some changes build land features There are constructive and recon- There are constructive and reconstruc- Rocks break down into smaller pieces. (mountain building), some changes structive changes. tive changes, sometimes occurring con- tear them down (mountains/rocks/ currently (e.g., volcanic eruption). sand—rock cycle). There are many kinds of energy at work: heat, chemical, kinetic, potential, radioactive. Land changes as a result of earth- Water, wind, ice, temperature changes Changes occur due to the transfer of Changes occur due to the transfer of quakes, volcanoes, and wind and wa- and vegetation are forces that change energy. energy. ter activity. the Earth’s surface and crust. The sun affects changes in tempera- The sun is the source of temperature The sun is the external source of en- The sun is the primary external source ture, weather, and the seasons. change. Temperature changes affect ergy driving changes on the Earth’s of energy driving changes on the Water can change into different forms weather and distribution of organ- surface. Earth’s surface, hydrosphere, and at- when the temperature changes. isms. mosphere. The Earth’s interior is the internal The Earth’s interior contains sources of source of energy driving large-scale heat energy driving large-scale changes changes in the lithosphere (plate tec- in the lithosphere (plate tectonics) and tonics) and Earth’s surface. Earth’s surface. Internal and external convection cur- Internal and external convection cur- rents are caused by an unequal distri- rents are caused by an unequal distribu- bution of heat. tion of heat. Convection currents drive movements Convection currents drive movements within the lithosphere, hydrosphere, within the lithosphere, hydrosphere, and atmosphere. and atmosphere. The transfer from potential to kinetic energy is responsible for changes in the Earth’s surface. Life has changed through time. Fos- Life has changed through time. Fos- Life has changed through time. Life has changed through time. There sils provide evidence that life has sils provided evidence that life has There are multiple lines of evidence are multiple lines of evidence for evolu- changed. changed. for evolution: fossils, anatomy, mol- tion: fossils, anatomy, molecules, devel- ecules, development, and geology. opment, geology, geographic distribu- tion, and experimentation. The biosphere infl uences and is infl u- enced by both internal and external energy transfers. Draft of Earth Science Conceptual Framework for Grades K–12 developed by WCCUSD/AK teachers. © 2004 UC Museum of Paleontology and West Contra Costa Unifi ed School District. EARTH SCIENCE CONCEPTUAL FRAMEWORK GRADES K–12 • WCCUSD/UCMP MATERIALS ARE CONSERVED AND RECYCLED Theme/Questions K–2 3–5 6–8 9–12 How are materials in Rocks break down into smaller pieces. Rocks are recycled from one type to Rocks are recycled from one type to All materials on Earth, including water, the Earth conserved When rocks get hot enough, they another. another (the rock cycle). rock, carbon, and nitrogen, are con- and recycled? melt. served and recycled through the four spheres. What is our evidence that materials are con- Magma is a source of new rocks. Cooling of magma near the Earth’s Plate tectonics is an essential force Formation, weathering, sedimentation, served and recycled? surface creates rock in the Earth’s that drives the rock cycle. New rock and reformation constitute a continuing crust. is created at divergent boundaries by “rock cycle” in which the total amount Where do rocks come magma pushing up from the mantle. of material is conserved and recycled. from? At subduction zones, existing rocks Plate tectonics and weathering drive the can be melted and recycled. Heat and rock cycle. What are the respon- pressure associated with plate interac- sibilities of humans tion can change existing rock. toward natural re- sources? Rocks break down into smaller pieces Surface rocks break down as a result as a result of the action of waves, of the action of waves, wind, water, wind, water, and ice (weathering). and ice (weathering) and are then Once rocks are broken down, they are carried by gravity, wind, and water carried by wind and water (erosion) (erosion) and deposited elsewhere and deposited elsewhere (deposition). (deposition). There are different kinds of rocks. We group rocks based on the way We classify rocks based on the way Properties of rocks are determined by We group rocks based on their char- they were formed. There are three they were formed: igneous, metamor- the physical and chemical conditions acteristics. types of rock: igneous, sedimentary, phic, and sedimentary. Properties of under which they formed. and metamorphic. rocks are determined by the physical Rocks are classifi ed by the processes and chemical conditions under which that formed them. they formed. Water freezes when it is very cold. Water exists on Earth as liquid (lakes, Water exists on Earth as liquid (lakes, There are different physical forms of Ice/snow melts when it gets warmer.
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Geologic, Climatic, and Vegetation History of California
    GEOLOGIC, CLIMATIC, AND VEGETATION HISTORY OF CALIFORNIA Constance I. Millar I ntroduction The dawning of the “Anthropocene,” the era of human-induced climate change, exposes what paleoscientists have documented for decades: earth’s environment—land, sea, air, and the organisms that inhabit these—is in a state of continual flux. Change is part of global reality, as is the relatively new and disruptive role humans superimpose on environmental and climatic flux. Historic dynamism is central to understanding how plant lineages exist in the present—their journey through time illuminates plant ecology and diversity, niche preferences, range distributions, and life-history characteristics, and is essential grounding for successful conservation planning. The editors of the current Manual recognize that the geologic, climatic, and vegetation history of California belong together as a single story, reflecting their interweaving nature. Advances in the sci- ences of geology, climatology, and paleobotany have shaken earlier interpretations of earth’s history and promoted integrated understanding of the origins of land, climate, and biota of western North America. In unraveling mysteries about the “what, where, and when” of California history, the respec- tive sciences have also clarified the “how” of processes responsible for geologic, climatic, and vegeta- tion change. This narrative of California’s prehistory emphasizes process and scale while also portraying pic- tures of the past. The goal is to foster a deeper understanding of landscape dynamics of California that will help toward preparing for changes coming in the future. This in turn will inform meaningful and effective conservation decisions to protect the remarkable diversity of rock, sky, and life that is our California heritage.
    [Show full text]
  • Plate Tectonics
    Plate tectonics tive motion determines the type of boundary; convergent, divergent, or transform. Earthquakes, volcanic activity, mountain-building, and oceanic trench formation occur along these plate boundaries. The lateral relative move- ment of the plates typically varies from zero to 100 mm annually.[2] Tectonic plates are composed of oceanic lithosphere and thicker continental lithosphere, each topped by its own kind of crust. Along convergent boundaries, subduction carries plates into the mantle; the material lost is roughly balanced by the formation of new (oceanic) crust along divergent margins by seafloor spreading. In this way, the total surface of the globe remains the same. This predic- The tectonic plates of the world were mapped in the second half of the 20th century. tion of plate tectonics is also referred to as the conveyor belt principle. Earlier theories (that still have some sup- porters) propose gradual shrinking (contraction) or grad- ual expansion of the globe.[3] Tectonic plates are able to move because the Earth’s lithosphere has greater strength than the underlying asthenosphere. Lateral density variations in the mantle result in convection. Plate movement is thought to be driven by a combination of the motion of the seafloor away from the spreading ridge (due to variations in topog- raphy and density of the crust, which result in differences in gravitational forces) and drag, with downward suction, at the subduction zones. Another explanation lies in the different forces generated by the rotation of the globe and the tidal forces of the Sun and Moon. The relative im- portance of each of these factors and their relationship to each other is unclear, and still the subject of much debate.
    [Show full text]
  • Plate Tectonics Research Rewrites History of Earth's Continents 8 July 2020
    Plate tectonics research rewrites history of Earth's continents 8 July 2020 of the rock fragments was not consistent with what we would usually see when subduction occurs. If the continents were formed through subduction and plate tectonics we would expect the ratio of iron and zinc isotopes to be either very high or very low, but our analyses instead found the ratio of isotopes was similar to that found in non-subduction rocks." Dr. Doucet said the team used a relatively new technique known as the non-traditional stable isotope method, which has been used to pinpoint the processes that formed continental and mantle Credit: Pixabay rocks. "Our research provides a new, but unknown theory as to how the Earth's continents formed more than Curtin University-led research has found new three billion years ago. Further research will be evidence to suggest that the Earth's first continents needed to determine what the unknown explanation were not formed by subduction in a modern-like is," Dr. Doucet said. plate tectonics environment as previously thought, and instead may have been created by an entirely The research was co-authored by researchers from different process. Curtin's Earth Dynamics Research Group, Université Libre de Bruxelles in Belgium, Institute Published in the journal Geology, the research for Geochemistry and Petrology in Switzerland, and team measured the iron and zinc isotopes in rock Université de Montpellier in France. sourced from central Siberia and South Africa and determined that the composition of these rocks The full paper is titled "Archean lithospheric may have formed in a non-subduction differentiation: Insights from Fe and Zn isotopes." environment.
    [Show full text]
  • Early Earth - W
    EARTH SYSTEM: HISTORY AND NATURAL VARIABILITY - Vol. I - Early Earth - W. Bleeker EARLY EARTH W. Bleeker Continental Geoscience Division, Geological Survey of Canada, Ottawa, Canada Keywords: early Earth, accretion, planetesimals, giant impacts, Moon, Hadean, Archaean, Proterozoic, late heavy bombardment, origin of life, mantle convection, mantle plumes, plate tectonics, geological time-scale, age dating Contents 1. Introduction 2. Early Earth: Concepts 2.1. Divisions of Geological Time 2.2. Definition of the“Early Earth” 2.3. Age Dating 3. Early Earth Evolution 3.1. Origin of the Universe and Formation of the Elements 3.2. Formation of the Solar System 3.3. Accretion, Differentiation, and Formation of the Earth–Moon System 3.4. Oldest Rocks and Minerals 3.5. The Close of the Hadean: the Late Heavy Bombardment 3.6. Earth’s Oldest Supracrustal Rocks and the Origin of Life 3.7. Settling into a Steady State: the Archean 4. Conclusions Acknowledgements Glossary Bibliography Biographical Sketch Summary The “ early Earth” encompasses approximately the first gigayear (Ga, 109 y) in the evolution of our planet, from its initial formation in the young Solar System at about 4.55 Ga to sometimeUNESCO in the Archean eon at about 3.5– Ga. EOLSS This chapter describes the evolution of the early Earth and reviews the evidence that pertains to this interval from both planetary and geological science perspectives. Such a description, even in general terms, can only be given with some background knowledge of the origin and calibration of the geological timescale, modernSAMPLE age-dating techniques, the foCHAPTERSrmation of solar systems, and the accretion of terrestrial planets.
    [Show full text]
  • History of the Earth's Climate, We Must First Understand Something About the Age of the Earth and How Various Events Have Been Dated
    The history of Earth climate In order to understand the history of the Earth's climate, we must first understand something about the age of the Earth and how various events have been dated. Some fundamental questions: .How old is the Earth? . How do we know the age of the Earth?? . What was the origin of the Earth's atmosphere? . What was the Earth's early climate like? . How has the Earth's climate changed over geologic time? The Radiometric Time Scale: Key to age of Earth and geologic time . 1896, discovery of natural radioactive decay of Uranium by Henry Becquerel, French physicist . 1905 British physicist Lord Rutherford described the structure of the atom and suggested radioactive decay for measuring geologic time . 1907 Yale Prof. B.B. Boltwood published first chronology of Earth based on radioactivity . 1950... first more-or-less accurate age dating. Principles of radiometric dating . elements distinguished by number of protons in the nucleus. Proton + neutron combination = nuclide . same no. protons but different no. neutrons = isotopes. e.g., isotopes of C with 6, 7, or 8 neutrons designated 12C, 13C, 14C. radioactive decay of less stable nuclides is statistically determined. The number of radioactive nuclei that decay in a given unit of time is directly proportional to the number of nuclei present at that time—first-order kinetics. ∂N =−λN ∂t where ∂N = rateofchangeovertimeofradioactivenuclei() N ∂t λ = decayconst., uniqueforeachradioactivenuclide Rearrangeto : ∂N =−λ∂t N Integratefromtimeoto timet2 toget : =−λ ln(NNto2 / ) t N −λ t2 = e t No takingnaturallog ofbothsides : =−λ lnNNtto2 ln A plot of ln N versus time will give a straight line with slope = -λ With radioactive nuclides, we often speak of half-life, the length of time required to diminish the original # of radioactive nuclei by 1/2: N = 1/2No λ 1/2 = e- t1/2 λ 2 = e t1/2 t1/2 = ln2 = 0.693/λ λ By various rearrangements, we can use a measured concentration of a radioactive element at the current time to determine the age.
    [Show full text]
  • Earth History: Historical Geology and Paleontology
    Earth History: Historical Geology and Paleontology College of Natural Sciences and Mathematics Department of Environmental Sciences EEES 2230-001 CRM 10170 Instructor: Email: [email protected] Office Hours: 8:30-9:25 MW, 12-2M, 8:30-9:30TR Office Location: 3022 BO Office Phone: 419-530-2398 Term: Spring 2015 Class Location: BO 1006 Class Day/Time: MW 11-11:50 Lab Location: BO1006 Lab Day/Time: 2-3:50M Credit Hours: 3 EEES – 2230 EARTH HISTORY: HISTORICAL GEOLOGY AND PALEONTOLOGY [3 hours] The morphology and paleoecology of fossil taxa, significant strata, and tectonic events important to the interpretation of paleoenvironments and Earth history are stressed. Field trip(s) required. [Spring] Prerequisite: EEES 2100 (Taught as a writing intensive course—WAC) COURSE OVERVIEW Ever wonder about what the earth was like before the time of humans or maybe during the time of dinosaurs? What about the different rocks you see? Ever been to the Grand Canyon? What about fossils? By the end of this course you will be well versed in the geologic and biologic history of Earth. STUDENT LEARNING OUTCOMES Apply the scientific method to concepts of historical geology and paleontology Us the principles of relative dating and absolute dating to chart the history of Earth and its organisms through geologic time Understand the development of the geologic time scale Become familiar with the use of geologic maps, cross sections, and stratigraphic columns to interpret Earth history Identify important fossil forms from each period and master selected index fossils Understand the concepts of evolution Understand the physical, chemical, and tectonic evolution of Earth through geologic time Understand sequence stratigraphy Related TAGs: Geology Students will be able to: 1.
    [Show full text]
  • Fossils, Rocks, and Time
    * W T' U.S. Department of the Interior / U.S. Geological Survey Fossils, Rocks, and Time ' Sfi 0. Front and back cover: This photographic collage of fossils shows the amazing diversity of plant and animal life on Earth over the last 600 million years. Fossils, Rocks, and Time by Lucy E. Edwards and John Pojeta, Jr. A scientist examines and compares fossil shells. Introduction e study our Earth for many reasons: to find water to drink or oil to run our cars Earth is Wor coal to heat our homes, to know constantly where to expect earthquakes or landslides or floods, and to try to understand our natural sur­ changing roundings. Earth is constantly changing nothing nothing on its on its surface is truly permanent. Rocks that are now on top of a mountain may once have been surface is truly at the bottom of the sea. Thus, to understand permanent. the world we live on, we must add the dimension of time. We must study Earth's history. When we talk about recorded history, time is measured in years, centuries, and tens of cen­ turies. When we talk about Earth history, time is measured in millions and billions of years. Time is an everyday part of our lives. We keep track of time with a marvelous invention, the cal­ endar, which is based on the movements of Earth in space. One spin of Earth on its axis is a day, and one trip around the Sun is a year. The modern calendar is a great achievement, developed over many thousands of years as theory and technology improved.
    [Show full text]
  • Origin of Evolution
    Evolution Origin of Life Dr Seema Makhija Department of Zoology Deshbandhu College Kalkaji New Delhi – 110 019 Contents: Mythological Approach Theory of Special Creation Ancient and Medieval Approach Theory of Panspermia Cosmozoic theory Theory of Spontaneous generation or Abiogenesis Theory of Biogenesis Redi’s Experiment Biochemical Origin Origin of earth and its primitive atmosphere: Source and forms of energy on primitive earth: Chemical origin of life or Chemogeny Step I: Origin of organic compounds Step II: Formation of Macromolecules or complex organic molecules (polymerization) (a) Proteins (b) Polysaccharides (c) Lipids (d) Nucleic acids Biological Evolution or Biogeny Step III: Formation of primary organisms or Eubionts Step IV: Evolution of modes of nutrition: Step V: Oxygen revolution and the present day atmosphere Experimental Evidence of Biochemical Origin of life Origin of Life Life is tenacious, and it completely permeates the surface layer of the planet. We find life beneath the deepest ocean, on the highest mountain, in the driest desert and the coldest glacier, and deep down in the rocks and sediments Not knowing what conditions are needed for the emergence of life, it is only possible to speculate about its existence elsewhere in the universe. Man has always been perplexed about the origin of life on earth. For centuries, a number of theories/hypotheses has been suggested to explain the origin. Mythological Approach Theory of Special Creation Earlier, life was thought to be created by some supernatural force in a very short time. Most of the major religions of the world and civilization believe it to be a supernatural phenomenon of the past.
    [Show full text]
  • The History of Life 347 DO NOT EDIT--Changes Must Be Made Through “File Info” Correctionkey=A
    DO NOT EDIT--Changes must be made through “File info” CorrectionKey=A The History CHAPTER 12 of Life BIg IdEa Scientists use many types of data collection and experimentation to form hypotheses and theories about how life formed on Earth. 12.1 The Fossil Record 12.2 The geologic Time Scale 12.3 Origin of Life 9d 12.4 Early Single-Celled Organisms 7F, 7g, 11C data analysis CalcuLaTINg axes IntervaLS 2g 12.5 Radiation of Multicellular Life 7E 12.6 Primate Evolution Online BiOlOgy HMDScience.com ONLINE Labs ■■ Video Lab Model of Rock Strata ■■ Radioactive Decay ■■ QuickLab Geologic Clock ■■ Stride Inferences ■■ Understanding Geologic Time ■■ Comparing Indexes Among Primates ■■ Virtual Lab Comparing Hominoid Skulls (t) ©Silkeborg Denmark Museum, 346 Unit 4: Evolution DO NOT EDIT--Changes must be made through “File info” CorrectionKey=A Q What can fossils teach us about the past? This man, known only as Tollund Man, died about 2200 years ago in what is now Denmark. Details such as his skin and hair were preserved by the acid of the bog in which he was found. A bog is a type of wetland that accumulates peat, the deposits of dead plant material. older remains from bogs can add information to the fossil record, which tends to consist mostly of hard shells, teeth, and bones. RE a d IN g T o o L b o x This reading tool can help you learn the material in the following pages. uSINg LaNGUAGE YOuR TuRN describing Time Certain words and phrases can help Read the sentences below, and write the specific time you get an idea of a past event’s time frame (when it markers.
    [Show full text]
  • Modeling Pn2 Through Geological Time: Implications for Planetary Climates and Atmospheric Biosignatures
    Modeling pN2 Through Geological Time: Implications for Planetary Climates and Atmospheric Biosignatures E.E. Stüeken1,2,3,4*, M.A. Kipp1,4, M.C. Koehler1,4, E.W. Schwieterman2,4,5, B. Johnson6, R. Buick1,4 1. Dept. of Earth & Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195, USA 2. Dept. of Earth Sciences, University of California, Riverside, CA 92521, USA 3. Department of Earth & Environmental Sciences, University of St Andrews, St Andrews KY16 9AL, Scotland, UK 4. NASA Astrobiology Institute’s Virtual Planetary Laboratory, Seattle, WA 981195, USA 5. Dept. of Astronomy and Astrobiology Program, University of Washington, Seattle, WA 98195, USA 6. School of Earth & Ocean Sciences, University of Victoria, Victoria, BC V8P 5C2, Canada * corresponding author ([email protected]) Astrobiology, Volume 16, Number 12, doi: 10.1089/ast.2016.1537 Abstract Nitrogen is a major nutrient for all life on Earth and could plausibly play a similar role in extraterrestrial biospheres. The major reservoir of nitrogen at Earth’s surface is atmospheric N2, but recent studies have proposed that the size of this reservoir may have fluctuated significantly over the course of Earth’s history with particularly low levels in the Neoarchean – presumably as a result of biological activity. We used a biogeochemical box model to test which conditions are necessary to cause large swings in atmospheric N2 pressure. Parameters for our model are constrained by observations of the modern Earth and reconstructions of biomass burial and oxidative weathering in deep time. A 1-D climate model was used to model potential effects on atmospheric climate.
    [Show full text]