Snowball Earth Hoffman et al. Science 1998. Evidence.

Slides:



Advertisements
Similar presentations
Orbital-Scale Changes in Carbon Dioxide and Methane
Advertisements

Climate over the long term (Ch highlights)
GEOS 112 Lecture Topics 4/28/03 Read Chapter 12 (Glaciers) Final Exam – Monday, May 5 1:00pm 1.Types of Glaciers; 2.Glacier Formation, Mass Balance, and.
Reading: Chapter 4 Lecture 25. Snowball Earth vs. Slushball Earth..
The Early history of Earth! After the Earth formed…about 4.6 Billion years ago… …The Earth melted and differentiated into Core, Mantle, and Crust.
Climate models in (palaeo-) climatic research How can we use climate models as tools for hypothesis testing in (palaeo-) climatic research and how can.
Global Warming The Earth's climate has changed many times in the past. Subtropical forests have spread from the south into more temperate (or milder, cooler.
Climate Forcing and Physical Climate Responses Theory of Climate Climate Change (continued)
Chapter 12 Long-Term Climate Regulation Snowball Earth.
Snowball Earth Roopa Kamesh Matt Beversdorf Kathy Groome
GLACIERS AND CLIMATE Mass balance ELA Milankovic cycle Albedo feedbacks Quelcaya ice cap, Peru.
Astronomy190 - Topics in Astronomy
Future climate (Ch. 19) 1. Enhanced Greenhouse Effect 2. CO 2 sensitivity 3. Projected CO 2 emissions 4. Projected CO 2 atmosphere concentrations 5. What.
The importance of Antarctic blue ice for understanding the tropical ocean of Snowball Earth Stephen Warren University of Washington Seattle, USA.
Slushball Earth Neoproterozoic ‘snowball Earth’ simulations with a coupled climate/ice-sheet model (Hyde et al. 2000) Nick Cowan February 2006.
GREENHOUSE EFFECT Climate Change. Greenhouse Effect Is a natural process that permits the Earth to retain some of the heat from the sun. Gases in the.
Global Warming Causes and Mechanics. What is Global Warming? “The recent increase in the world's temperature that is believed to be caused by the increase.
Unit 3: Gases and the Atmosphere Atmosphere: the mass of air surrounding the earth.
Goals for this section 1.EXPLAIN the feedback mechanism believed to have maintained Earth's average temperature within the range of liquid water over 100s.
Chapter 4 Sections 3 and 4 Long Term Changes in Climate Global Changes in the Atmosphere.
Climate Change – 1: Background
Long-Term Climate Cycles &the Proterozoic Glaciations(Snowball Earth) Assigned Reading: Stanley, pp , Hoffman & Schrag (2002) Terra Nova,
The Atmosphere & Climate
Miss Nelson SCIENCE ~ CHAPTER 9 CLIMATE. Climate Change SECTION 4.
CLIMATE CHANGE THE GREAT DEBATE Session 9. BIOLOGICAL FACTORS Changes in albedo. Surfaces vary in the degree to which they absorb or reflect solar energy.
Unit 1 Lesson 1 Earth’s Spheres
Or Water, Water Everywhere. The Water Planet More than 70% of Earth’s surface is covered with water. Because of this, Earth is called ‘the Water Planet.’
Science, Society and Solutions
Evidence for Climate Change A large body of evidence from direct weather and climate observation, and from computer simulation, supports the hypothesis.
Glacial Geology of Northeast Pennsylvania. How do we know they were here? Geologic forensics…look for the evidence… …and an 800 pound gorilla leaves a.
Quaternary Environments Climate and Climatic Variation.
Feedback Loops. FEEDBACK LOOPS Change induces change What happens when you’re hot? What happens when you’re cold? These are examples of negative feedback.
Understanding the Greenhouse Effect Sara Kalinowski and Ellen Cercena.
The Greenhouse Effect Too much of a good thing?. Light from the sun is composed of many frequencies.
Greenhouse Effect Mechanisms Affecting the Greenhouse Evidence for Climate Change.
CLIMATE SYSTEM AND WEATHER. WEATHER Weather refers to: The state of the atmosphere in a particular place and time. Weather occurs over short time periods.
Extreme Climate Change: The late Neoproterozoic “Snowball Earth”
Lecture Outlines Physical Geology, 14/e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Plummer, Carlson &
Evolution of the Earth David Spergel. Evolution of Earth’s Atmosphere  Earth lost its early atmosphere in major collisions (first Myr)  Subsequent.
Ice Cores, Stable Isotopes, and Paleoclimate
UNIT 1 STUDYING EARTH. Earth Facts… The third planet from the Sun. One of the inner planets along with Mercury, Venus, and Mars; these planets are made.
By William Garner.  The part of the earth which is covered with water.  Consists of the oceans, seas, lakes, and rivers.  Divided into two categories:
Late Proterozoic Snowball Earth Brian Morgan Colby College December 3, 2012.
The Atmosphere: Structure and Temperature
Moving At A Glacial Pace How Glaciers Have Shaped Our World.
Evidence of Global Warming and Consequences
Snowball oceanography. What is Snowball Earth? Most extreme climate event in Earth history. Characteristics: Occurred at least twice between Ma.
The Faint Young Sun Problem. Systems Notation = system component = positive coupling = negative coupling.
Section 1.3 The atmosphere
Chapter 1 Vocabulary Atmosphere Altitude Density Cycle Radiation Conduction Convection Ultraviolet Radiation Infrared Radiation Ozone Greenhouse Effect.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Climate Change Ch. 12 Study Guide. 1. Identify 2 physical features and explain how they influence the climate. Latitude Elevation.
The Climate Lab Lesson 3. Signal vs. Noise Global vs. Local temperatures What’s happening in the local climate is often different from what’s happening.
Lecture 10: Ice on Earth EarthsClimate_Web_Chapter.pdfEarthsClimate_Web_Chapter.pdf, p. 8, 27-30; Ch. 2, p. 21; Ch. 10, p I.Sea Ice II.Glacial.
Radiation from the Sun
Climate L2 Greenhouse gases current interglacial Last glacial.
Schematic framework of anthropogenic climate change drivers, impacts and responses to climate change, and their linkages (IPCC, 2007).
Long-Term Climate Cycles & The Proterozoic Glaciations (‘Snowball Earth’) Assigned Reading: Hoffman & Schrag (2002) Terra Nova, Vol. 14(3): Lubick.
Snowball Earth vs. Slushball Earth..
What Causes Ice Ages?
Schematic framework of anthropogenic climate change drivers, impacts and responses to climate change, and their linkages (IPCC, 2007; 2014).
Natural Causes of Climate Change
Climate Change and Earth
Climate: Earth’s Dynamic Equilibrium, Part 2
Earth’s Materials and Processes-Part 1 The Earth’s Spheres
Composition and evolution of the atmosphere
Earth’s Materials and Processes-Part 1 The Earth’s Spheres
The global energy household
Overview of “Snowball Earth”
Human Impacts on Climate Change
Presentation transcript:

Snowball Earth Hoffman et al. Science 1998

Evidence

Hypothesis Ice buildup due to lower carbon dioxide in the atmosphere (Qo: 6% lower) Biological productivity is at normal level prior to ice buildup Earth becomes ice covered, ocean become anoxic, and rich in ferrous iron Volcanic eruption raises the level of CO2 in the atmosphere (CO2 stays in atm due to ice cover – reaches 350 x today’s level) Sudden collapse of the ice sheet  leads to extreme greenhouse earth CO2 dissolves in ocean, precipitates  cap carbonates

Method Studies rocks in Namibia (Ottavi group), measured delta 13C, thickness of carbonate layers, etc

Mechanism Simple life would have survived in places where the ice sheet was thin and water (lakes was present) It would take 4 Myr at present day CO2 emission from volcano to bring CO2 level to 0.12 bar to get out of snow ball earth If 0.12 bar of CO2 precipitate to present day level (0.001bar)  5m layer thick of cap carbonate

Snowball Earth Hyde et al. Nature 1998

Hypothesis Climate ice sheet models / GCM –EBM can reproduce this fast transition from glacial to interglacial BUT is this scenario coherent with more complex climate model? Delays in melting, lag in ice growth  filters high frequency changes in Qo Bedrock depression, lower sea level  different land-ocean configuration  albedo GCM: Ice cover over ocean  less cloud  more SW

Method Glacial model: 4000 year depression time scale Temperature and pressure independent rheology Qo = 6% lower than today CO2 half of present day climate

Results Model gives realistic present and LGM climate With reduced Qo and CO2 level  Ice covered earth Use the ice configuration as boundary condition for a GCM  equatorial band of open water  allows life to survive

Snowball Earth Bruce Runegar, Comments Nature 1998 If the equatorial ocean is open: how can the CO2 in the atmosphere to extremely high level and end the snow ball earth? – It would simply dissolve in the ocean.

Snowball Earth Schrag and Hoffman, Comments Nature 1998 If the equatorial ocean is ice free, then the level of CO2 required to end the snow ball earth are lower  not consistent with cap carbonate thickness Also it implies a slow/gradual termination of snow ball earth  again not consistent with cap carbonate

Snowball Earth Hyde et al, Reply Nature 1998 CO2 increase gradually, but the response of the ice Sheet is still a rapid melt back at come critical CO2 level Life needs open ocean to survive. Multicellular cant live on Ridge along with chemosynthethic life (still needs oxygen) And ocean are anoxic.

Snowball Earth MacKay, GRL 2000

Results/Hypothesis Yes ice would be km thick if the only heat balance is geothermal heat flux BUT if you include light transmissivity, then it could be as thin as a few meters. Then you can have both ice covered ocean and large buildup of CO2 in the atm, and light for live.