The Earth. The Earth. Policy on absences. Processes that shape earth. Test 1 will be released on Wed afternoon.

Similar documents
Earth. Interior Crust Hydrosphere Atmosphere Magnetosphere Tides

Earth as Planet. Earth s s Magnetic Field. The Earth s s Crust. Earth s s Interior

Structure of the Earth EARTH ( ) - need a solid, will not go through a liquid

Climate Regulation. - What stabilizes the climate - Greenhouse effect

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves.

Today. Events Homework DUE next time. Terrestrial Planet Geology - Earth. Terrestrial Planet Atmospheres

ASTRO 120 Sample Exam

Astro 1010 Planetary Astronomy Sample Questions for Exam 4

Chapter 2: Physical Geography

Origin of solar system. Origin of solar system. Geology of the Hawaiian Islands. Any Questions? Class 2 15 January 2004

Any Questions? 99.9 % of mass is in the Sun; 99 % of angular momentum is in the planets. Planets in two groups:

Chapter 2 Geography. Getting to know Earth

Continental Drift. & Plate Tectonics

TEST NAME:Geology part 1 TEST ID: GRADE:06 - Sixth Grade SUBJECT:Life and Physical Sciences TEST CATEGORY: My Classroom

Astronomy 1140 Quiz 3 Review

10/11/2010. Acceleration due to gravity, a. Bulk Properties Mass = 6 x kg Diameter = 12,756 km Density = 5515 kg/m 3 (mix of rock and iron)

Summary. The Ice Ages and Global Climate

Shape and Size of the Earth

Tuesday, September 05, 2017 Planet Earth

FORCES ON EARTH UNIT 3.2. An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth.

Systems? Climate Systems. Earth Systems. Earth Interior Systems. Atmospheric/Biospheric Systems: Human Impact Hydrologic Cycle.

Important information from Chapter 1

Name Test Date Hour. the interior of the Earth to the surface. younger less dense plate.

LIGO sees binary neutron star merger on August 17, 2017

Astronomy 1140 Quiz 3 Review

Chapter 7 Earth Pearson Education, Inc.

Carbon Cycling Internal

UNIT 6 PLATE TECTONICS

The Earth Fast Facts. Outline. The Solar System is Ours! Astronomy 210. Section 1 MWF Astronomy Building

Planet Earth. Our Home APOD

Plate Tectonics. By Destiny, Jarrek, Kaidence, and Autumn

ASTR-101 Section 004 Lecture 9 Rare Earth? John T. McGraw, Professor

Today. Events. Terrestrial Planet Geology - Earth. Terrestrial Planet Atmospheres. Homework DUE next time

Chapter 20 Earth: The Standard of Comparative Planetology

Terrestrial Planets: The Earth as a Planet

Climate change: How do we know?

Can t t wait to take Exam 4!

5. Convergent boundaries produce a relatively low number of earthquakes compared to other boundaries. a. True

Introduction to Climate Change

The Sun and Planets Lecture Notes 6.

Earth. Properties of Earth. Earth's Interior. Earth is the planet that we know best

Developed in Consultation with Georgia Educators

Inner Planets (Part II)

FORCES ON EARTH. An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth.

Geology Topics. Unit 6 Notes

THE DYNAMIC EARTH NOTES. Scientists divide the Earth into 4 parts or spheres. What are these spheres?

Plate Tectonics Practice Test

EARTH TAKES SHAPE 1. Define all vocabulary words. Crust: The thin and solid outermost layer of the Earth above the mantle. Mantle: The layer of rock

Distance of Mercury to the Sun or the Orbital Radius

HOW GEOGRAPHY AND GEOLOGY AFFECT BIOLOGICAL DIVERSITY

The greenhouse effect

The Solar System. Earth as a Planet

12. The diagram below shows the collision of an oceanic plate and a continental plate.

1. The geosphere consists of three major layers: the,, and.

Social Studies. Chapter 2 Canada s Physical Landscape

Unit 4 - Water. Earth s Interior. Earth s Interior. Continental Drift. Continental Drift. Continental Drift. Crust. Mantle. Core.

CONTINENTAL DRIFT THEORY

4 Layers of the earth 7 main plates of the earth 3 main plate boundaries 2 types of crust 3 main features of plate tectonics 3 main theorists and

Q1. Scientists study the atmosphere on planets and moons in the Solar System to understand how the Earth s atmosphere has changed.

The Earth - Surface and Interior

The Earth. Overall Structure of Earth

Plate Tectonics CHAPTER 17

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Chapter 5 Review. 1) Our Earth is about four times larger than the Moon in diameter. 1)

Chapter 2 Planet Earth

TAKE HOME EXAM 8R - Geology

Plate Tectonics. Earth has distinctive layers - Like an onion

Chapter 4: Plate Tectonics

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings

The Theory of Continental Drift. Continental Drift Discovery

The Planet Earth. Life and Civilization Dennis Silverman UCI OLLI

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red

Outcome C&D Study Guide

Chapter 7 Plate Tectonics. Plate tectonics accounts for important features of Earth s surface and major geologic events.

The Structure of the Earth and Plate Tectonics

25-Nov-14. The Structure of Earth s Interior. What unique features of Earth are important for life as we know it?

Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds

Section 1: Earth s Interior and Plate Tectonics Section 2: Earthquakes and Volcanoes Section 3: Minerals and Rocks Section 4: Weathering and Erosion

Name Date Class. How have geologists learned about Earth s inner structure? What are the characteristics of Earth s crust, mantle, and core?

A Living Planet. The Earth Inside and Out

The Dynamic Earth Section 1. Chapter 3 The Dynamic Earth Section 1: The Geosphere DAY 1

Chapter. Graphics by Tasa Graphic Arts. Inc.

Section 1: The Geosphere

AST 105 Intro Astronomy The Solar System

The Four Layers The Earth is composed of four different layers. The crust is the layer that you live on, and it is the most widely studied and

Topic 5: The Dynamic Crust (workbook p ) Evidence that Earth s crust has shifted and changed in both the past and the present is shown by:

Use models to describe the sun s place in space in relation to the Milky Way Galaxy and the distribution of galaxy clusters in the universe.

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

12.2 Plate Tectonics

2010 Pearson Education, Inc.

Chapter 1 Section 2. Land, Water, and Climate

Chapter 7 Plate Tectonics. Plate tectonics accounts for important features of Earth s surface and major geologic events.

Heat Transfer. Heat Transfer. Convection Heat transfer due to the actual motion of a fluid. Conduction Heat transfer by successive atomic collisions

SCIENCE IN THE NEWS Plate Tectonics

1.4 Notes: Plates Converge or Scrape Past Each Other Think About Tectonic Plates Push Together at Convergent Boundaries

Plate Tectonics: A Scientific Revolution Unfolds

EARTH S INTERIOR, EVIDENCE FOR PLATE TECTONICS AND PLATE BOUNDARIES

Global climate change

Plate Tectonics Tutoiral. Questions. Teacher: Mrs. Zimmerman. Plate Tectonics and Mountains Practice Test

Transcription:

The Earth Processes that shape earth Plate tectonics Volcanism Energy trapping: Greenhouse effect Carbon dioxide cycle Effects of increased CO 2 Erosion (you already know this) Loss of gases (Thurs) Policy on absences You may miss classes for a university sanctioned event if you bring me a letter from your sponsor or coach. You may miss class if you are really sick if you bring me a note from your doctor. If you miss class for either of these two reasons, you will not be penalized for missing clicker questions. Of course you will need to learn the material that you missed. Test 1 will be released on Wed afternoon. The Earth Planets in the solar system are very different. Q1: Besides Earth, is rocky. A Venus, B Jupiter, C Saturn, D Uranus. Q2: Besides Earth, may have life near it. Same foils. Big questions What determines planets size, temperature, composition? What makes a planet support life? Earth, Venus, and Mars formed in similar ways. What processes caused them to become so different? Processes that shape earth Plate tectonics Volcanism Energy trapping: Greenhouse effect Carbon dioxide cycle Erosion Loss of gases 1

Interior of the Earth [see Fig 7.2] 12,800 km Crust ~6 km thick under oceans. 20-70 km thick under continents. Rocks composed of silicon, oxygen, etc. 0.3% of mass. Mantle Slowly flowing semi-solid rock. Core 7000 km diameter. Metallic (iron, nickel, sulfur) Outer core is liquid. Inner core probably solid. Plate Tectonics Crust split into huge plates drifting around on top of the mantle. Driven by convection (same as bubbles in boiling water). Convection time is 200Myears. Plates pushed apart in rift zones Mid-Atlantic Ridge Plates bash together in subduction zones. e.g. Rim of Fire around Pacific Ocean. Plates can slide at the boundaries San Andreas Fault in California 2

Geological Activity on Earth Plate collisions mountain building Light continental plate collides with light continental plate; eg, Himalayas. Heavy oceanic plate collides with light continental plate; eg, Andes. Volcanoes Magma (molten rock) forced upwards from mantle. Along mid-ocean ridges. Around subduction zones (Rim of Fire) Plate drifts over a hot spot Hawaiian Island chain Hot Spot older volcanoes The Earth s Atmosphere [7.5] Weighs 13.6 pounds per square inch 78% nitrogen, 21% oxygen, + argon, H 2 O, CO 2, etc. Unusual mixture Oxygen should not be present because it reacts easily. Hydrogen & helium should be dominant because they are the most abundant elements in the universe. Ozone (O 3 ) is critical for life blocks Sun s ultraviolet radiation Ozone hole: over Antarctica, where ozone destroyed by manmade pollutants. 3

Greenhouse Effect [Fig 7.14] Incoming sunlight passes through atmosphere. Absorbed by ground. Re-emitted as infrared radiation. Water & CO 2 gas absorbs infrared light. Reradiated. Infrared light is trapped, so heats surface. Carbon Dioxide Cycle Removal of CO2 from atmosphere Rain dissolves CO2 Rivers carry CO2 into the oceans Carbonate rocks lock up carbon Introduction of CO2 into the atmosphere Subduction of oceanic plate carries carbonate rocks underneath continent Volcanoes release CO2 4

Faint-sun Problem Removal of CO2 from atmosphere Rain dissolves CO2 Rivers carry CO2 into the oceans Carbonate rocks lock up carbon Introduction of CO2 into the atmosphere Subduction of oceanic plate carries carbonate rocks underneath continent Volcanoes release CO2 The sun was fainter when it was younger. The earth should have been frozen. Fossils show earth was warm, instead. Carbon dioxide is a feedback that maintains temperature. Less solar radiation cooler less rain more CO2 more effective greenhouse warmer Carbon Dioxide Cycle Removal of CO2 from atmosphere Rain dissolves CO2 Rivers carry CO2 into the oceans Carbonate rocks lock up carbon Introduction of CO2 into the atmosphere Subduction of oceanic plate carries carbonate rocks underneath continent Volcanoes release CO2 Assignment for Thurs: Which is the main reason Venus so hot? a. CO2 traps heat b. It is close to the sun c. Its atmosphere has so much CO2 d. Its atmosphere has so much water. Assignment for Thurs: Venus and Earth are nearly twins. What went wrong on Venus? 5

The Science of Climate Change: Part 1--1 --Overview Presented at Michigan State University 22 March 2006 Dr. Michael MacCracken Climate Institute Washington DC Photo taken from first Apollo flight to the Moon, December, 1968 Emissions from human activities alter the natural carbon cycle, increasing the amount of carbon in the air, the oceans, and the living biosphere Source: EIA, Greenhouse Gas brochure 6

CO 2 Emissions are Significantly Increasing its Atmospheric Concentration The current value is about 380 ppmv, over 35% above the preindustrial value, which had not varied significantly since the end of the last glacial (i.e., roughly 8000 years). ppm=parts per million (by volume) Observations by C. David Keeling That the magnitude of the seasonal cycle has increased suggests that, even with a reduced amount of vegetation, the higher CO 2 concentration is enhancing the seasonal growth of global vegetation tion The CO 2 concentration is now about 35% higher than its preindustrial level Year 7

The CO 2 concentration had been roughly steady over the centuries (and millennia) preceding the Industrial Revolution Results from observations at Mauna Loa CO 2 in ppmv Results from measuring CO 2 in the air bubbles in ice cores Year The Concentrations of Carbon Dioxide (CO 2 ), Methane (CH 4 ), and Nitrous Oxide (N 2 O) all Show Sharp Increases Concentrations of three well- mixed greenhouse gases. Measurements before about 1960 are mostly from bubbles trapped in glacial ice Atmospheric methane has increased by over 150% since 1750. About half of current emissions are anthropogenic. Carbon Dioxide Methane Atmospheric nitrous oxide has increased by over 17% since 1750. About a third of current emissions are anthropogenic. Nitrous Oxide Source, IPCC, 2001 8

The Earth s natural Greenhouse Effect occurs because the atmosphere recycles most of the infrared (heat) energy that is emitted by the surface, providing energy that significantly augments incoming solar radiation The timing of glacial advances and retreats over the past 400,000 years seems to be driven by changes in the shape, tilt, and timing of the Earth s orbit-- --with associated changes in CO 2 and CH 4 concentrations providing an important amplifying effect 9

Warming has occurred in all four seasons over the past 50 years Extensive Additional Evidence Confirms that Climate Change is Occurring Ground (subsurface) temperatures,, which respond to long-term average conditions at the surface, are rising Ocean temperatures are rising, at the surface and through the upper kilometer of ocean depth Sea ice cover is decreasing, particularly in the Arctic Mountain glaciers and the Greenland Ice Sheet are melting, snow cover extent is reduced, and the snow line is rising Sea level is rising due to added meltwater from glaciers and expansion caused by warming Atmospheric water vapor concentrations are rising (in the lower and upper troposphere) and rainfall events are becoming more intense Distributions of a large fraction of studied species are shifting poleward (except where they run out of habitat) 10

Minimum Extent of Arctic Ocean Sea Ice Cover September 1979 September 2003 Global sea level rose by about 10 to 20 cm (4 to 8 inches) during the 20 th century U.S. Sea Level Trends 1900-2000 Scale (cm) 40 20 0 Galveston, TX New York, NY Baltimore, MD Key West, FL Contributions to increases in global sea level occur as a result of thermal expansion of warming ocean waters, melting of mountain glaciers, and net losses from the Greenland and Antarctica Ice Sheets. Changes in land stored on land in reservoirs and aquifers can also be important. San Francisco, CA 1900 1920 1940 1960 1980 2000 Year Sitka, AK Changes in local sea level (relative sea level) are also determined by coastal subsidence or emergence due to long-term (e.g., glacial rebound) and short-term term (e.g. aquifer pumping) factors. 11

Although other approaches provide supporting results, only climate models can be used to project the likely changes from this global geophysical experiment 1. Laboratory and field experiments are too limited 2. Mathematical analyses must greatly simplify the Earth system 3. Analogs from the past are suggestive, but insufficiently similar to the current situation 4. Trend extrapolation is difficult due to natural variability and the uniquely changing conditions 5. Numerical models are theoretical constructs, but can treat the expected types of changes Climate model simulations used in the US National Assessment project a 21 st century warming of about 5-10ºF Canadian model scenario for increase by 2100 Hadley (UK)model scenario for increase by 2100 Find the Hadley and Canadian model estimates of change in temp Plots show the projected change in annual average temperature (ºF) over the 21 st century 12

Global sea level is projected to rise by about 9 to 88 cm (4 to 35 inches) during the 21 st century, with a mid-range value or higher increasingly likely Contributions to global sea level rise are projected to come mainly from thermal expansion of ocean waters and melting of mountain glaciers. These IPCC (2001) 01) estimates suggested that melting of the Greenland and Antarctica Ice Sheets s would be small, but more recent indications are that there will be more significant contributions. 13