Module Contact: Dr Mark Claire, ENV Copyright of the University of East Anglia Version 1

Size: px
Start display at page:

Download "Module Contact: Dr Mark Claire, ENV Copyright of the University of East Anglia Version 1"

Transcription

1 UNIVERSITY O EAST ANGLIA School of Environmental Sciences Main Series Postgraduate Examination EARTH AND LIE ENV-MA38 Time allowed: 2 hours. Answer TWO questions, ONE from EACH section. Write EACH answer in a SEPARATE answer book. ALL questions carry equal marks Notes are not permitted in this examination. Do not turn over until you are told to do so by the Invigilator. ENV-MA38 Module Contact: Dr Mark Claire, ENV Copyright of the University of East Anglia Version 1

2 2 SECTION A 1. Describe the major features of the carbonate-silicate feedback cycle on atmospheric CO 2 concentrations, including a feedback diagram. Describe how catastrophic breakdowns of the carbonate-silicate cycle lead to the boundaries of the classical circumstellar habitable zone. 2. Is the Gaia hypothesis consistent with the theory of evolution by natural selection? Is the Gaia hypothesis testable? If so, how? If not, why not? Your answer should start with a definition of the Gaia hypothesis, address the main biological criticisms of it, and describe evidence and models that attempt to answer the criticisms. Your answer should also draw on examples of postulated feedback mechanisms and evidence from Earth history. 3. Discuss how atmospheric oxygen concentrations have changed over Earth history, focusing on evaluating the evidence for step changes at the Great Oxidation and Cambrian Explosion events. What evidence is there that the major changes were caused by evolutionary innovations, and what evidence is there that the changes in oxygen in turn influenced the evolution of life? SECTION B 4. The Critical Step model of Carter (1983) assumes that evolution towards complex, and ultimately intelligent, observer species is governed by the necessity to pass a number of critical steps. Each step is assumed to occur with a uniform, but low probability, and cannot occur until previous steps in the sequence have occurred. Considering only the subset of planets on which observer species do evolve, the probability distribution for the evolution of such a species, that requires n critical steps, is found to be: nt Pnn / () t t n 1 n h per unit time, where t is time, measured from the point where life first becomes possible on the planet, t h is the habitable lifetime of the planet, and 0 < t < t h. a) Sketch the shape of this probability distribution as a function of t, for the cases n = 1, n = 2, and n = 3.

3 b) The expectation time <t n > (the mean time averaged over many realizations) at which the observer species evolves is given by the integral 3 t h tn tpn / n() t dt 0 Show that the solution of the integral is: t n n 1 n t h c) Assuming Earth has been habitable since the end of the late heavy bombardment 3.9 Ga ago, give estimates for the number of critical steps required for the evolution of ourselves as observer species on Earth, under each of the following two assumptions: (1) the habitable period of the Earth is 10 Ga, as Carter (1983) assumed ; and (2) the habitable period of Earth is 5 Ga, as Watson (2008) assumed. [15%] d) It has been suggested that because life became established on Earth soon after the planet became continuously habitable is evidence that the origin of life must be a common event, so that prokaryotic life should be found frequently in the universe. Comment on and contrast the implications for the likelihood of life evolving if (1) the evidence of the Isua formation rocks (3.8 Ga old) is accepted as evidence for life, and (2) if the evidence of the Swaziland formations (3.5 Ga old) is accepted as evidence for life. Assume that the end of the late heavy bombardment marks the earliest time from which the Earth could be continuously habitable. [25%] PLEASE TURN OVER

4 5. a) Briefly describe (with a chemical equation if appropriate) the effect of the following processes as sources or sinks for atmospheric oxygen, on geological time scales: 4 i) Organic carbon burial in sediments ii) Oxidative weathering of continental rock iii) Hydrogen escape iv) Reduced gases emanating from volcanoes To a first approximation, the equation for the rate of change of oxygen in the atmosphere due to geologic sources and sinks can be written. do cb oxw dt (1) where o is a non-dimensional oxygen content of the atmosphere, equal to 1 in the presentday, cb is the molar flux of carbon buried in sediments and oxw the flux of oxygen consumed by oxidative weathering of continental rocks. A similar equation for phosphorus in the oceans can be written dp dt (2) pw pb where pw is the molar flux of phosphorus released by continental weathering, ε is the fraction of pw that is biogeochemically available, and pb is the rate of burial of this material in the oceans. We further assume the following relationships: Carbon and phosphorus are buried in a constant ratio, R c/p cb pb R (3) c / p Phosphorus weathering and oxidative weathering take place in a constant ratio, R ox/p oxw pw R (4) ox/ p

5 b) Show by assuming steady state of the phosphorus equation that there can be no steady state for oxygen according to the system of equations (1) (4), unless either (a) continental weathering is zero, or (b) if R c/ p Rox/ p 5 (5) c) Van Cappellen and Ingall (1994) proposed that the main feedback that stabilizes oxygen concentration is that R c/p increases with decreasing oxygen concentration. They suggest that R c/p is not constant but is a function of atmospheric oxygen, for example: R / p o 0.05 c (6) Taking R ox/p = 150, show that this function implies that steady state oxygen has the following linear dependence on ε: o (7) [20%] d) Lenton and Watson (2000) proposed that a tendency of land vegetation to increase the value of ε has been important in determining the history of atmospheric oxygen. What range of values of ε does equation (7) suggest would be appropriate to: i) The Proterozoic, before land vegetation evolved, and ii) The Phanerozoic during the period since vascular land plants evolved? [20%] PLEASE TURN OVER

6 6.a) The following circuit diagram with input, i, contains a system, with output, o, which is the linear sum of its inputs. It also contains a feedback loop with an amplifier (amp.), which multiplies the incoming signal by a gain factor, G. 6 i) Write down an expression balancing the inputs and outputs of the system and rearrange it to get the ratio of output to input (the amplification factor ) in terms of the gain. ii) iii) iv) What range of values for the gain factor gives negative feedback? What range of values for the gain factor gives positive feedback? What is the condition for runaway positive feedback? b) One postulated state for the Earth system is that an organic haze would form in the atmosphere if the CH 4 :CO 2 ratio were to reach a value of approximately 1:10. Assuming that the CH 4 flux is due to methanogenic bacteria, and that the haze regulates the temperature due to an anti-greenhouse effect leads to a biologically-modulated feedback cycle. At a fixed CO 2 concentration (5%), the surface temperature (T S ) in Celsius as a function of methane concentration (in ppm) as computed by an Archean climate model that includes the effect of organic haze (Haqq-Misra et al. 2008) is: T S (CH 4 ) = CH CH (1) Methanogens are thermophilic bacteria whose growth rate increases with temperature. Assume a linear growth rate such that CH 4 concentrations (in ppm) increase with surface temperature as: CH 4 (T S ) = (T S ) / ( ) (2)

7 7 i) Show that a temperature of 12º C forms a steady state solution to the set of equations (1) and (2). ii) The gain factor of this system is given by: G dt S dch 4 dch 4 dt S (3) where dt S /dch 4 comes from differentiating equation (1) and dch 4 /dt S from differentiating equation (2). Compute these derivatives and simplify the resulting expression for the gain factor. iii) What is the value of the gain factor at the steady state found in part (i)? What does this tell us about the sign and strength of the feedback and hence the stability of this state? iv) ind the alternate steady state solution of the system (by inserting (1) into (2), rearranging, and solving). v) What is the value of the gain factor at the state in part (iv)? What does this tell us about the sign of the feedback and the stability of this state? vi) At what temperature does the feedback change sign? [60%] c) Sketch a graph of equations (1) and (2), with annotations indicating important numbers and stability regions calculated in part b) [10%] END O PAPER

Chapter 12: Long-Term Climate Regulation. Carl Sagan and George Mullen posed the Faint Young Sun Paradox in 1972.

Chapter 12: Long-Term Climate Regulation. Carl Sagan and George Mullen posed the Faint Young Sun Paradox in 1972. Chapter 12: Long-Term Climate Regulation Carl Sagan and George Mullen posed the Faint Young Sun Paradox in 1972. What about the details? Faint young Sun paradox Solution: A greenhouse gas or a lower albedo

More information

Global Carbon Cycle - I

Global Carbon Cycle - I Global Carbon Cycle - I OCN 401 - Biogeochemical Systems Reading: Schlesinger, Chapter 11 1. Overview of global C cycle 2. Global C reservoirs Outline 3. The contemporary global C cycle 4. Fluxes and residence

More information

Global Carbon Cycle - I

Global Carbon Cycle - I Global Carbon Cycle - I Reservoirs and Fluxes OCN 401 - Biogeochemical Systems 13 November 2012 Reading: Schlesinger, Chapter 11 Outline 1. Overview of global C cycle 2. Global C reservoirs 3. The contemporary

More information

Radiative Balance and the Faint Young Sun Paradox

Radiative Balance and the Faint Young Sun Paradox Radiative Balance and the Faint Young Sun Paradox Solar Irradiance Inverse Square Law Faint Young Sun Early Atmosphere Earth, Water, and Life 1. Water - essential medium for life. 2. Water - essential

More information

PTYS 214 Spring Announcements Midterm #4: two weeks from today!

PTYS 214 Spring Announcements Midterm #4: two weeks from today! PTYS 214 Spring 2018 Announcements Midterm #4: two weeks from today! 1 Previously Radiometric Dating Compare parent / daughter to determine # of half lives 14C, 40K, 238U, 232Th, 87Ru Evidence for Early

More information

Lecture 20. Origin of the atmosphere (Chap. 10) The carbon cycle and long-term climate (Chap. 8 of the textbook: p )

Lecture 20. Origin of the atmosphere (Chap. 10) The carbon cycle and long-term climate (Chap. 8 of the textbook: p ) Lecture 20 Origin of the atmosphere (Chap. 10) The carbon cycle and long-term climate (Chap. 8 of the textbook: p.158-170) end of last ice-age; begin civilization beginning of modern era of ice-ages asteroid

More information

Global Carbon Cycle - I Systematics: Reservoirs and Fluxes

Global Carbon Cycle - I Systematics: Reservoirs and Fluxes OCN 401-10 Nov. 16, 2010 KCR Global Carbon Cycle - I Systematics: Reservoirs and Fluxes The Global carbon cycle Reservoirs: biomass on land in the oceans, atmosphere, soil and rocks, waters Processes:

More information

Chapter 12 Long-Term Climate Regulation

Chapter 12 Long-Term Climate Regulation Chapter 12 Long-Term Climate Regulation Sun about 30% less luminous than today - Ts would have been below freezing - Earth seems to have had liquid water nonetheless - Faint Young Sun Paradox (FYSP) Warm

More information

Effect of Life on the Atmosphere: The Rise of Oxygen and Ozone

Effect of Life on the Atmosphere: The Rise of Oxygen and Ozone Some preliminary chemistry Chapter 11 Effect of Life on the Atmosphere: The Rise of Oxygen and Ozone Chemical reactions involve the giving and taking of electrons between atoms. the nucleus is not affected

More information

Earth History & Geobiology. O. Jagoutz

Earth History & Geobiology. O. Jagoutz Earth History & Geobiology O. Jagoutz 12.001 Intro: Earth differs from other rocky planets by the presence of the hydrosphere, free oxygen and the presence of complex life. It is a major scientific challenge

More information

Chapter Introduction. Chapter Wrap-Up. Explosion

Chapter Introduction. Chapter Wrap-Up. Explosion Chapter Introduction Lesson 1 Lesson 2 Lesson 3 Chapter Wrap-Up Geologic Time Ancient Earth The Cambrian Explosion How have natural events changed Earth over time? What do you think? Before you begin,

More information

XI. the natural carbon cycle. with materials from J. Kasting (Penn State)

XI. the natural carbon cycle. with materials from J. Kasting (Penn State) XI. the natural carbon cycle with materials from J. Kasting (Penn State) outline properties of carbon the terrestrial biological cycle of carbon the ocean cycle of carbon carbon in the rock cycle overview

More information

PTYS 214 Spring Announcements. Get exam from Kyle!

PTYS 214 Spring Announcements. Get exam from Kyle! PTYS 214 Spring 2018 Announcements Get exam from Kyle! 1 Midterm #3 Total Students: 24 Class Average: 78 Low: 32 High: 100 If you have questions see one of us! 2 All exams Top 2 exams 3 Previously Feedbacks

More information

Lecture 3. - Global Sulfur, Nitrogen, Carbon Cycles - Short-term vs. Long-term carbon cycle - CO 2 & Temperature: Last 100,000+ years

Lecture 3. - Global Sulfur, Nitrogen, Carbon Cycles - Short-term vs. Long-term carbon cycle - CO 2 & Temperature: Last 100,000+ years Lecture 3 - Global Sulfur, Nitrogen, Carbon Cycles - Short-term vs. Long-term carbon cycle - CO 2 & Temperature: Last 100,000+ years METR 113/ENVS 113 Spring Semester 2011 March 1, 2011 Suggested Reading

More information

Phys 214. Planets and Life

Phys 214. Planets and Life Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 10. Geology and life. Part 1 (Page 99-123)

More information

Evolution of Earth Environments Bio-Geo-Chemical Cycling

Evolution of Earth Environments Bio-Geo-Chemical Cycling Evolution of Earth Environments Bio-Geo-Chemical Cycling Evolution of the Earliest Atmospheres of Mars and Earth Volcanic Outgassing Evolving to Equilibrium Atmosphere To Atmosphere Lost to space (Abundant)

More information

The Proterozoic Eon (2500 ma to 540 ma)

The Proterozoic Eon (2500 ma to 540 ma) The Proterozoic Eon (2500 ma to 540 ma) December November October September August July June May April March February January 0 Ma Phanerozoic C M P 540 Ma oldest shelly fossils Proterozoic 2500 Ma first

More information

Long-term Climate Change. We are in a period of relative warmth right now but on the time scale of the Earth s history, the planet is cold.

Long-term Climate Change. We are in a period of relative warmth right now but on the time scale of the Earth s history, the planet is cold. Long-term Climate Change We are in a period of relative warmth right now but on the time scale of the Earth s history, the planet is cold. Long-term Climate Change The Archean is thought to have been warmer,

More information

Fossils provide evidence of the change in organisms over time.

Fossils provide evidence of the change in organisms over time. Section 1: Fossils provide evidence of the change in organisms over time. K What I Know W What I Want to Find Out L What I Learned Essential Questions What are the similarities and differences between

More information

Origin of Life. What is Life? The evolutionary tree of life can be documented with evidence. The Origin of Life on Earth is another

Origin of Life. What is Life? The evolutionary tree of life can be documented with evidence. The Origin of Life on Earth is another sparked by just the right combination of physical events & chemical processes Origin of Life 500 Paleozoic 1500 2000 2500 3000 3500 ARCHEAN Millions of years ago 1000 PROTEROZOIC Cenozoic Mesozoic 4000

More information

Scholarship 2015 Earth and Space Science

Scholarship 2015 Earth and Space Science S 93104R Scholarship 2015 Earth and Space Science 2.00 p.m. Tuesday 1 December 2015 RESOURCE BOOKLET Refer to this booklet to answer the questions for Scholarship Earth and Space Science 93104. Check that

More information

1. Be able to explain how the development of a magnetosphere affected the evolution of Earth s atmosphere (3) Atmosphere 1. Be able to describe the

1. Be able to explain how the development of a magnetosphere affected the evolution of Earth s atmosphere (3) Atmosphere 1. Be able to describe the I. Evolution 1. be able to define biologic evolution. 2. be able to define and apply the principles of Natural Selection. 3. be able to describe Gregor Mendel s experiment with pea plants. a) be able to

More information

Pleistocene Glaciation (Ch.14) Geologic evidence Milankovitch cycles Glacial climate feedbacks

Pleistocene Glaciation (Ch.14) Geologic evidence Milankovitch cycles Glacial climate feedbacks Pleistocene Glaciation (Ch.14) Geologic evidence Milankovitch cycles Glacial climate feedbacks End of last ice-age rise of human civilization Modern ice-ages begin Asteroid impact end of dinosaurs Cambrian

More information

SCOPE 35 Scales and Global Change (1988)

SCOPE 35 Scales and Global Change (1988) 1. Types and origins of marine sediments 2. Distribution of sediments: controls and patterns 3. Sedimentary diagenesis: (a) Sedimentary and organic matter burial (b) Aerobic and anaerobic decomposition

More information

Guided Notes Geologic History

Guided Notes Geologic History Guided Notes Geologic History Relative Age Sequence of Events Correlation Techniques Volcanic Ash Markers Index Fossils Geologic Time Scale Evolution Radioactive Dating 9) How has Earth changed over time?

More information

A modeling case for high atmospheric oxygen concentrations during the Mesozoic and Cenozoic Mills et al.

A modeling case for high atmospheric oxygen concentrations during the Mesozoic and Cenozoic Mills et al. GSA Data Repository 2016343 A modeling case for high atmospheric oxygen concentrations during the Mesozoic and Cenozoic Mills et al. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 APPENDIX APPENDIX

More information

Evolution of the Atmosphere: The Biological Connection

Evolution of the Atmosphere: The Biological Connection Evolution of the Atmosphere: The Biological Connection The Earth s Four Spheres How It All Began Or At Least How We Think It Began O.k. it s a good guess Egg of energy The Big Bang splattered radiation

More information

Earth s History. The principle of states that geologic processes that happened in the past can be explained by current geologic processes.

Earth s History. The principle of states that geologic processes that happened in the past can be explained by current geologic processes. Earth s History Date: Been There, Done That What is the principle of uniformitarianism? The principle of states that geologic processes that happened in the past can be explained by current geologic processes.

More information

X The evolution of life on Earth.

X The evolution of life on Earth. X The evolution of life on Earth http://sgoodwin.staff.shef.ac.uk/phy229.html 10.0 Introduction A combination of the fossil record, biology and genetics allows us to examine the evolution of life on Earth.

More information

ATOC OUR CHANGING ENVIRONMENT Lecture 21 (Chp 12) Objectives of Today s Class The long-term climate record

ATOC OUR CHANGING ENVIRONMENT Lecture 21 (Chp 12) Objectives of Today s Class The long-term climate record ATOC 1060-002 OUR CHANGING ENVIRONMENT Lecture 21 (Chp 12) Objectives of Today s Class The long-term climate record Announcements: 1. The Project; HW3; 2. Review session for the final exam: Dec 7 th. Sean

More information

Chapter 11. The Archean Era of Precambrian Time

Chapter 11. The Archean Era of Precambrian Time Chapter 11 The Archean Era of Precambrian Time 1 Guiding Questions When and how did Earth and its moon come into being? How did the core, mantle, crust form? Where did Archean rocks form, and what is their

More information

Answer ALL questions in Section A, and TWO questions from Section B.

Answer ALL questions in Section A, and TWO questions from Section B. UNIVERSITY OF EAST ANGLIA School of Environmental Sciences Main Series Undergraduate Examination 2012-2013 Candidate s no.: GEODYNAMICS: EARTH S ENGINE ENV-2A43 Time allowed: 2 hours. Answer ALL questions

More information

Formation of the Earth and Solar System

Formation of the Earth and Solar System Formation of the Earth and Solar System a. Supernova and formation of primordial dust cloud. NEBULAR HYPOTHESIS b. Condensation of primordial dust. Forms disk-shaped nubular cloud rotating counterclockwise.

More information

The Role of Biology in the Climate System: Long Term Climate Regulation. Earth History, Gaia and Human Perturbations of Biological Systems

The Role of Biology in the Climate System: Long Term Climate Regulation. Earth History, Gaia and Human Perturbations of Biological Systems The Role of Biology in the Climate System: Long Term Climate Regulation Earth History, Gaia and Human Perturbations of Biological Systems How would the Earth differ if Life had not evolved or expanded?

More information

CHAPTER 19 THE HISTORY OF LIFE. Dr. Bertolotti

CHAPTER 19 THE HISTORY OF LIFE. Dr. Bertolotti CHAPTER 19 THE HISTORY OF LIFE Dr. Bertolotti Essential Question: HOW DO FOSSILS HELP BIOLOGISTS UNDERSTAND THE HISTORY OF LIFE ON EARTH? WHAT DO FOSSILS REVEAL ABOUT ANCIENT LIFE? FOSSILS AND ANCIENT

More information

EVOLUTION OF PLANTS THROUGH AGES

EVOLUTION OF PLANTS THROUGH AGES EVOLUTION OF PLANTS THROUGH AGES B. Sc. III Botany Dr. (Miss) Kalpana R. Datar Assistant Professor DEPARTMENTOF BOTANY WILLINGDON COLLEGE, SANGLI. kalpana_datar@yahoo.com The origin of Earth 1.Ultra dense,

More information

Visualizing Earth Science. Chapter Overview. The Ever-Changing Earth. Early Life. Evolution and the Fossil Record. Life in the Phanerozoic Eon

Visualizing Earth Science. Chapter Overview. The Ever-Changing Earth. Early Life. Evolution and the Fossil Record. Life in the Phanerozoic Eon Visualizing Earth Science By Z. Merali and B. F. Skinner Chapter 11 A Brief History of Life on Earth Chapter Overview The Ever-Changing Earth Early Life Evolution and the Fossil Record Life in the Phanerozoic

More information

The History of the Earth

The History of the Earth The History of the Earth Origin of the Universe The universe began about 13.9 billion years ago According to Big Bang theory almost all matter was in the form of energy E = MC 2 E = energy, M = mass and

More information

The Hadean Earth Gya Impacts melt the surface. Volatiles escape to space

The Hadean Earth Gya Impacts melt the surface. Volatiles escape to space Life on Earth. II 4.5-3.9 Gya Impacts melt the surface. Volatiles escape to space The Hadean Earth Source of atmosphere, oceans: outgassing and impacts Early atmosphere: CO 2, H 2 O, N 2, H 2 S, SO 2,

More information

Chapter 5. The Biogeochemical Cycles. Botkin & Keller Environmental Science 5e

Chapter 5. The Biogeochemical Cycles. Botkin & Keller Environmental Science 5e Chapter 5 The Biogeochemical Cycles How Chemicals Cycle Biogeochemical Cycle The complete path a chemical takes through the four major components or reservoirs of Earth s systems 1. Atmosphere 2. Hydrosphere

More information

Life on Earth Topic Test

Life on Earth Topic Test Life on Earth Topic Test Multiple Choice Questions Select the best alternative and indicate your response on the answer sheet. (1 mark each) 1. The list below contains common substances that exist in Earth

More information

The History of Life. Before You Read. Read to Learn

The History of Life. Before You Read. Read to Learn 14 The History of Life section 1 Fossil Evidence of Change Before You Read Throughout Earth s history, many species have become extinct. On the lines below, name some organisms that have become extinct.

More information

Origins of Life and Extinction

Origins of Life and Extinction Origins of Life and Extinction What is evolution? What is evolution? The change in the genetic makeup of a population over time Evolution accounts for the diversity of life on Earth Natural selection is

More information

N = R * f p n e f l f i f c L

N = R * f p n e f l f i f c L Astronomy 230 Section 1 MWF 1400-1450 106 B6 Eng Hall This Class (Lecture 10): Nature of Life Next Class: Nucleic Acids Some Oral Presentation on Feb 16 th and 18 th! Mike Somers Chris Kramer Sarah Goldrich

More information

COMPUTER METHODS AND MODELING IN GEOLOGY THE GLOBAL PHOSPHORUS CYCLE

COMPUTER METHODS AND MODELING IN GEOLOGY THE GLOBAL PHOSPHORUS CYCLE COMPUTER METHODS AND MODELING IN GEOLOGY THE GLOBAL PHOSPHORUS CYCLE Phosphorous (P) is an essential nutrient for life. It is found in the RNA and DNA of all organisms, as well as in the adenosine triphosphate

More information

Lecture 4 What Controls the Composition of Seawater

Lecture 4 What Controls the Composition of Seawater Lecture 4 What Controls the Composition of Seawater Seawater is salty! Why? What controls the composition of seawater? Do Chemical Equilibrium reactions control the composition of the Ocean? What is meant

More information

Figure 65: Reservoir in a steady state condition where the input flux is equal to the output flux and the reservoir size remains constant.

Figure 65: Reservoir in a steady state condition where the input flux is equal to the output flux and the reservoir size remains constant. 7. The carbon cycle 7.1. Box model of the carbon cycle Without the greenhouse effect, our planet would experience a permanent ice age and life as we know it would not be possible. The main contributors

More information

4) Outline the major developments that allowed life to exist on Earth.

4) Outline the major developments that allowed life to exist on Earth. Objectives 4) Outline the major developments that allowed life to exist on Earth. 5) Describe the types of organisms that arose during the four major divisions of the geologic time scale. Each layer of

More information

IX Life on Earth.

IX Life on Earth. IX Life on Earth http://sgoodwin.staff.shef.ac.uk/phy229.html 9.0 Introduction Life exists on the surface layers of the Earth. We cannot consider life and the planet separately: they interact with one

More information

The Earth System Connections among the great spheres

The Earth System Connections among the great spheres Why should we discuss the Earth System? The Earth System Connections among the great spheres Before we delve into the connection between geology, health, and forensics, we must gain an appreciation of

More information

The greenhouse effect

The greenhouse effect The greenhouse effect Visible light arrives About half reflected, half is absorbed by the ground. This absorbed energy is then reradiated, but NOT in the visible (would just go out again anyway); in the

More information

First, an supershort History of the Earth by Eon

First, an supershort History of the Earth by Eon HISTORY OF LIFE WRITTEN IN THE ROCKS (geological record): notice how at first no life, very simple if for billions of years, complex life only recently 600 mya In these chapters, two primary themes: History

More information

The Biogeochemical Carbon Cycle: CO 2,the greenhouse effect, & climate feedbacks. Assigned Reading: Kump et al. (1999) The Earth System, Chap. 7.

The Biogeochemical Carbon Cycle: CO 2,the greenhouse effect, & climate feedbacks. Assigned Reading: Kump et al. (1999) The Earth System, Chap. 7. The Biogeochemical Carbon Cycle: CO 2,the greenhouse effect, & climate feedbacks Assigned Reading: Kump et al. (1999) The Earth System, Chap. 7. Overhead Transparencies Faint Faint Young Sun Paradox Young

More information

Atmospheric Evolution: Earth s s Oxidation

Atmospheric Evolution: Earth s s Oxidation Earth s s Atmosphere Thematic Questions about the Atmosphere Observations of the Modern Atmosphere What is its structure and composition? What controls atmospheric dynamics? Information from the Rock Record

More information

sparked by just the right combination of physical events & chemical processes Life s Origin & Early Evolution (Ch. 20)

sparked by just the right combination of physical events & chemical processes Life s Origin & Early Evolution (Ch. 20) sparked by just the right combination of physical events & chemical processes Life s Origin & Early Evolution (Ch. 20) 2007-2008 ARCHEAN Millions of years ago PRECAMBRIAN PROTEROZOIC 0 500 1000 Cenozoic

More information

A climatic thermostat making Earth habitable

A climatic thermostat making Earth habitable A climatic thermostat making Earth habitable Peter D. Ditlevsen, arxiv:astro-ph/0505245v1 12 May 2005 The Niels Bohr Institute, Department of Geophysics, University of Copenhagen, Juliane Maries Vej 30,

More information

Complexity of the climate system: the problem of the time scales. Climate models and planetary habitability

Complexity of the climate system: the problem of the time scales. Climate models and planetary habitability Complexity of the climate system: the problem of the time scales Climate models and planetary habitability Time scales of different components of the climate system Planets and Astrobiology (2016-2017)

More information

Welcome to Class 13: Is (or was) Life on Mars? Remember: sit only in the first 10 rows of the room

Welcome to Class 13: Is (or was) Life on Mars? Remember: sit only in the first 10 rows of the room Welcome to Class 13: Is (or was) Life on Mars? Remember: sit only in the first 10 rows of the room What are we going to discuss today? Why didn t Mars maintain a warm, wet climate? If life could exist

More information

ESA's Rosetta spacecraft What are habitable exoplanets? Is there an Earth 2.0?

ESA's Rosetta spacecraft What are habitable exoplanets? Is there an Earth 2.0? ESA's Rosetta spacecraft - 2009 What are habitable exoplanets? Is there an Earth 2.0? Christina Hedges (Institute of Astronomy) For the past 20 years, since the discovery of planets outside our solar system,

More information

Earth s history can be broken up into 4 time periods: Precambrian Paleozoic Era Mesozoic Era Cenozoic Era

Earth s history can be broken up into 4 time periods: Precambrian Paleozoic Era Mesozoic Era Cenozoic Era Earth s History Video Clip Earth s History Earth s history can be broken up into 4 time periods: Precambrian Paleozoic Era Mesozoic Era Cenozoic Era Scientists have put together a timeline of Earth s history

More information

CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1)

CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1) Student Sheet 1 CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1) The Goldilocks Effect is derived from a children's story "The Three Bears" in which a little girl named Goldilocks finds

More information

Earth s Atmosphere. Atmospheric Composition 78% Nitrogen 21% Oxygen 1 % Argon, 0.03% Carbon dioxide, Water. Recall the Electro-Magnetic (EM) Spectrum

Earth s Atmosphere. Atmospheric Composition 78% Nitrogen 21% Oxygen 1 % Argon, 0.03% Carbon dioxide, Water. Recall the Electro-Magnetic (EM) Spectrum Key Concepts: Lecture 11 Earth s Atmosphere and Greenhouse Effect Blackbody Radiation and Temperature Earth s Oceans Earth s Magnetic Field and Aurora The Green House Effect Temperature set by balancing

More information

Evolution of the Atmosphere

Evolution of the Atmosphere Evolution of the Atmosphere Anticipation Guide Oxygen is the main gas found in the atmosphere The current atmosphere is the same atmosphere that the Earth had when it formed Water vapor is a gas found

More information

Radiogenic Isotopes as Tracers of Sources and Mixing in the Solid Earth, Hydrosphere, Biosphere

Radiogenic Isotopes as Tracers of Sources and Mixing in the Solid Earth, Hydrosphere, Biosphere Radiogenic Isotopes as Tracers of Sources and Mixing in the Solid Earth, Hydrosphere, Biosphere Reading: White, Lecture 22, part on the mathematics of binary mixing. Also: Faure, 1986, Chs. 9, 11 OR...

More information

Module Contact: Dr Xiaoming Zhai, ENV Copyright of the University of East Anglia Version 2

Module Contact: Dr Xiaoming Zhai, ENV Copyright of the University of East Anglia Version 2 UNIVERSITY OF EAST ANGLIA School of Environmental Sciences Main Series UG Examination 2017-2018 OCEAN CIRCULATION ENV-5016A Time allowed: 2 hours Answer THREE questions Write each answer in a SEPARATE

More information

Earth Science COURSE DESCRIPTION: PREREQUISITES: COURSE LENGTH: REQUIRED TEXT: MATERIALS LIST:

Earth Science COURSE DESCRIPTION: PREREQUISITES: COURSE LENGTH: REQUIRED TEXT: MATERIALS LIST: Earth Science COURSE DESCRIPTION: This course provides students with a solid earth science curriculum, focusing on geology, oceanography, astronomy, weather, and climate. The program consists of online

More information

Natural Climate Variability: Longer Term

Natural Climate Variability: Longer Term Natural Climate Variability: Longer Term Natural Climate Change Today: Natural Climate Change-2: Ice Ages, and Deep Time Geologic Time Scale background: Need a system for talking about unimaginable lengths

More information

UNIT 4: History Of Biological Diversity

UNIT 4: History Of Biological Diversity UNIT 4: History Of Biological Diversity CHAPTER 14: The History of Life PAST NOW FUTURE? What is this? Earth s Early history Approximately 4.6 billion years ago, the Earth was formed when many pieces of

More information

Biogeochemical cycles

Biogeochemical cycles Lecture -2: Biogeochemical cycles ENV 107: Introduction to Environmental Science Dr. A.K.M. Saiful Islam Case Study: Lake Washington The city of Seattle, USA lies between two major bodies of water- saltwater

More information

Earth s Formation: 4.6 Billion Years ago

Earth s Formation: 4.6 Billion Years ago Earth s Formation: 4.6 Billion Years ago Formed from interstellar gas & dust into molten planet Earth s early atmosphere was hostile, made of carbon monoxide, methane, ammonia, nitrogen, nitrogen, sulfur,

More information

sparked by just the right combination of physical events & chemical processes Origin of Life

sparked by just the right combination of physical events & chemical processes Origin of Life sparked by just the right combination of physical events & chemical processes Origin of Life 2010-2011 ARCHEAN Millions of years ago PRECAMBRIAN PROTEROZOIC 0 500 1000 Cenozoic Mesozoic Paleozoic Colonization

More information

THIS IS A NEW SPECIFICATION

THIS IS A NEW SPECIFICATION THIS IS A NEW SPECIFICATION ADVANCED SUBSIDIARY GCE CHEMISTRY B (SALTERS Chemistry of Natural Resources: Advance Notice article F332/ADVANCE NOTICE *OCE/T68972* For issue on or after: 13 MARCH 2009 Wednesday

More information

Summary The Fossil Record Earth s Early History. Name Class Date

Summary The Fossil Record Earth s Early History. Name Class Date Name Class Date Chapter 17 Summary The History of Life 17 1 The Fossil Record Fossils are preserved traces and remains of ancient life. Scientists who study fossils are called paleontologists. They use

More information

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) NCEA Level 3 Earth and Space Science (91414) 2017 page 1 of 6 Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) Evidence Statement

More information

Website Lecture 3 The Physical Environment Part 1

Website   Lecture 3 The Physical Environment Part 1 Website http://websites.rcc.edu/halama Lecture 3 The Physical Environment Part 1 1 Lectures 3 & 4 1. Biogeochemical Cycling 2. Solar Radiation 3. The Atmosphere 4. The Global Ocean 5. Weather and Climate

More information

SCI112: Earth Science

SCI112: Earth Science SCI112: Earth Science In this course, students focus on geology, oceanography, astronomy, weather, and climate. Students follow a program of online study days that alternate with review-and-assessment

More information

The Sun and Planets Lecture Notes 6.

The Sun and Planets Lecture Notes 6. The Sun and Planets Lecture Notes 6. Lecture 6 Venus 1 Spring Semester 2017 Prof Dr Ravit Helled Cover photo: Venus in true color (Courtesy of NASA) Venus Properties Venus is the second brightest natural

More information

4.0 Billion Years of Earth Environmental Change

4.0 Billion Years of Earth Environmental Change 4.0 Billion Years of Earth Environmental Change We have already explored the various ways the Earth has evolved over the past 4 billion years. 1. Volcanic arcs, to proto-continents, to microcontinents,

More information

EARTH S HISTORY. What is Geology? logy: science. Geology is the scientific study of the Earth, including its:

EARTH S HISTORY. What is Geology? logy: science. Geology is the scientific study of the Earth, including its: EARTH S HISTORY 1 What is Geology? Geo: earth logy: science Geology is the scientific study of the Earth, including its: composition, structure, and physical properties. 2 1 Geologists study: the origin

More information

You are advised to spend an equal amount of time on each question. All questions carry an equal number of marks.

You are advised to spend an equal amount of time on each question. All questions carry an equal number of marks. UNIVERSITY OF EAST ANGLIA School of Chemistry Main Series UG Examination 2014-15 INORGANIC CHEMISTRY CHE-2C32/5301B Time allowed: 2 hours Answer THREE questions. You are advised to spend an equal amount

More information

Chapter 12 - Long term climate regulation. Chapter 10-11* -Brief History of the Atmosphere. What is p really about? New and improved!

Chapter 12 - Long term climate regulation. Chapter 10-11* -Brief History of the Atmosphere. What is p really about? New and improved! What is p16164 really about? New and improved! 1) When CO 2 dissolves in water, some reacts with water to produce acid and ions, making gas exchange NOT just CO 2 (g in atm) CO 2 (aq in ocn) 2) If

More information

(4) Give an example of important reactions that are responsible for the composition of river water.

(4) Give an example of important reactions that are responsible for the composition of river water. Lecture 12 Global Biogeochemical Cycles (1) If rivers are the chief source of the dissolved salts in seawater, why is seawater not simply a concentrated version of average composition of all rivers? The

More information

Geologic Time on a Strip of Paper

Geologic Time on a Strip of Paper Geologic Time on a Strip of Paper Introduction The Earth is 4,600,000,000 years old. That s 4.6 billion years! But what does this mean? This activity is designed to help you get a feel for the age of the

More information

Ast 281 Review for Exam 1 Tuesday, February 25, 2014 in class

Ast 281 Review for Exam 1 Tuesday, February 25, 2014 in class Ast 281 Review for Exam 1 Tuesday, February 25, 2014 in class The Exam will be a CLOSED BOOK exam, lasting the whole period. You will be allowed to have calculators and the sheet of planetary data, but

More information

Earth & Earthlike Planets. David Spergel

Earth & Earthlike Planets. David Spergel Earth & Earthlike Planets David Spergel Course Logistics Life Everywhere and Rare Earths are now in the U-Store Each precept will be divided into two teams (at this week s s precept). Debate topic: Are

More information

Study Guide. Section 1: Fossil Evidence of Change CHAPTER 14

Study Guide. Section 1: Fossil Evidence of Change CHAPTER 14 Name Date Class Study Guide CHAPTER 14 Section 1: Fossil Evidence of Change In your textbook, read about Earth s early history. For each statement below, write true or false. 1. Solid Earth formed about

More information

Origins of Life & the Cambrian Explosion

Origins of Life & the Cambrian Explosion Origins of Life & the Cambrian Explosion Impact Frustration period forces origins of life into a narrow time period to have gotten started! Hydrothermal vents may have served as zones of refuge. Origin

More information

Origins of Life & the Cambrian Explosion

Origins of Life & the Cambrian Explosion Origins of Life & the Cambrian Explosion Impact Frustration period forces origins of life into a narrow time period to have gotten started! Hydrothermal vents may have served as zones of refuge. 1 Origin

More information

The Chemistry of Global Warming

The Chemistry of Global Warming The Chemistry of Global Warming Venus Atmospheric pressure is 90x that of Earth 96% CO 2 and sulfuric acid clouds Average temperature = 450 C Expected temperature based on solar radiation and distance

More information

9.1- Earth Forms and Life Begins

9.1- Earth Forms and Life Begins 9.1- Earth Forms and Life Begins About Earth: Earth was formed about 4.6 billion years ago! The first life on earth appeared about 4 billion years ago Life started out as small, single-celled organisms

More information

Climate Regulation. - What stabilizes the climate - Greenhouse effect

Climate Regulation. - What stabilizes the climate - Greenhouse effect Climate Regulation - What stabilizes the climate - Greenhouse effect Last time! Processes that shaped Earth: Volcanism, tectonics! How we retain atmospheric molecules ( escape speed )! A magnetic field

More information

17-1 The Fossil Record Slide 2 of 40

17-1 The Fossil Record Slide 2 of 40 2 of 40 Fossils and Ancient Life What is the fossil record? 3 of 40 Fossils and Ancient Life Fossils and Ancient Life Paleontologists are scientists who collect and study fossils. All information about

More information

The History of Life. Before You Read. Science Journal

The History of Life. Before You Read. Science Journal The History of Life Before You Read Use the What I Know column to list the things you know about the history of life. Then list the questions you have about the history of life in the What I Want to Find

More information

Module 9: Earth's History Topic 3 Content: A Tour of Geologic Time Notes

Module 9: Earth's History Topic 3 Content: A Tour of Geologic Time Notes The geologic time scale holds secrets to the life that has existed on Earth since the beginning of time. It is time for you to take a journey through the history of Earth. 1 Click on each of the segments

More information

Long-Term Climate Regulation (Ch.12) The Faint Young Sun Paradox Revisited (P )

Long-Term Climate Regulation (Ch.12) The Faint Young Sun Paradox Revisited (P ) Long-Term Climate Regulation (Ch.12) The Faint Young Sun Paradox Revisited (P. 230-236) Dating with radioactive elements Carbon 14 (read Ch.5, P97-98) Natural radioactivity Atomic nuclei are composed of

More information

Outline. Origin and History of Life

Outline. Origin and History of Life Origin and History of Life Chapter 19 Primitive Earth Origin of First Cells Fossils The Precambrian The Paleozoic The Mesozoic The Cenozoic Continental Drift Mass Extinctions Outline 1 2 The Primitive

More information

This Week: Biogeochemical Cycles. Hydrologic Cycle Carbon Cycle

This Week: Biogeochemical Cycles. Hydrologic Cycle Carbon Cycle This Week: Biogeochemical Cycles Hydrologic Cycle Carbon Cycle Announcements Reading: Chapters 4 (p. 74 81) and 8 Another Problem Set (Due next Tuesday) Exam 2: Friday Feb 29 My office hours today and

More information

Daisy World Assignment

Daisy World Assignment Daisy World Assignment Learning Objectives: Explore homeostasis on Daisy World, i.e. how it self regulates it global temperature; Understand the faint-young sun paradox; Make graphs and discuss their meaning;

More information

How do we learn about ancient life? Fossil- a trace or imprint of a living thing that is preserved by geological processes.

How do we learn about ancient life? Fossil- a trace or imprint of a living thing that is preserved by geological processes. Unit 1B Lesson 4 History of Life on Earth How do we learn about ancient life? Paleontologists scientists that studies fossils Fossil- a trace or imprint of a living thing that is preserved by geological

More information

key to long-term sustainability is recycling..

key to long-term sustainability is recycling.. .. to support life over ~ 4 billion years, Earth must be sustainable system.. key to long-term sustainability is recycling.. Earth System how are key elements needed for life (C, N, P) recycled on the

More information