Prof Lyatt Jaegle, UW, "Space-based observations of biomass-burning emissions of NOx" [a pollutant gas]

Similar documents
Ancient Climates: Readings

Temperature/Precipitation History Faint Young Sun paradox: Fig 12-2

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

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

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

Chapter 12 Long-Term Climate Regulation

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.

PTYS 214 Spring Announcements. Get exam from Kyle!

Natural Climate Variability: Longer Term

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

The Proterozoic Eon (2500 ma to 540 ma)

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

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

Today we will discuss global climate: how it has changed in the past, and how the current status and possible future look.

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

Earth History. What is the Earth s time scale? Geological time Scale. Pre-Cambrian. FOUR Eras

Chapter Introduction. Chapter Wrap-Up. Explosion

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

SCIENCE SAMPLER ~ Geology ~ Unit 4 of 5

The greenhouse effect

/ Past and Present Climate

Understanding past climate change

The Essential Cosmic Perspective Chapter 7.5: Earth as Living Planet. Dr. Regina Jorgenson

Climate and Earth Systems

IX Life on Earth.

Fossils provide evidence of the change in organisms over time.

Earth s Formation: 4.6 Billion Years ago

5 Time Marches On. TAKE A LOOK 1. Identify What kinds of organisms formed the fossils in the picture?

Mon Nov 3. Steve Warren, regional climates water cycle ocean and solid earth circulations Friday: lab on reservoirs and cycles?

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

Nebular Hypothesis (Kant, Laplace 1796) - Earth and the other bodies of our solar system (Sun, moons, etc.) formed from a vast cloud of dust and

Planetary Atmospheres (Chapter 10)

Climate Regulation. - What stabilizes the climate - Greenhouse effect

The performance expectation above was developed using the following elements from the NRC document A Framework for K-12 Science Education:

Earth & Earthlike Planets. David Spergel

Guided Notes Geologic History

ATOC OUR CHANGING ENVIRONMENT

The History of the Earth

EARTH SYSTEM SCIENCE ENVST-UA PROF. RAMPINO Fall 2015

Earth History

4 Changes in Climate. TAKE A LOOK 2. Explain Why is more land exposed during glacial periods than at other times?

Plate Tectonic Vocabulary Chapter 10 Pages

8. Climate changes Short-term regional variations

Rare Earth? See Rare Earth, by Ward and Brownlee

NATS 101 Section 13: Lecture 32. Paleoclimate

Evidence for Continental Drift and The Theory of Plate Tectonics

PTYS 214 Spring Announcements. Next midterm 3/1!

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

Geosphere Final Exam Study Guide

Radiative Balance and the Faint Young Sun Paradox

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

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

Plate Tectonics Practice Test

Development of the Global Environment

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

For the next few weeks: Terrestrial Planets, their Moons, and the Sun. Planetary Surfaces and Interiors 2/20/07

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

Mon Oct 20. Today: radiation and temperature (cont) sun-earth geometry energy balance >> conceptual model of climate change Tues:

Outline 9: Origin of the Earth: solids, liquids, and gases

Continental Drift and Plate Tectonics

GO ON. Directions: Use the diagram below to answer question 1.

Question #1: What are some ways that you think the climate may have changed in the area where you live over the past million years?

The Official CA State Science Education Standards for Earth Science K 8

3. The diagram below shows how scientists think some of Earth's continents were joined together in the geologic past.

Chapter 14: The Changing Climate

AST 105 Intro Astronomy The Solar System

Chapter 12. Thermal Energy Transfer Drives Plate tectonics

Phys 214. Planets and Life

Summary. The Ice Ages and Global Climate

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

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

What is Earth Science? Earth science is the branch of science dealing with the constitution of the earth and its atmosphere.

How the Earth was formed

UNIT 4: History Of Biological Diversity

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

Plate Tectonics. These icons indicate that teacher s notes or useful web addresses are available in the Notes Page.

The Earth. February 26, 2013

Monday, December 4, 2017 The Pleistocene Glaciations (Chapter 14) Week 14 Assessment, closes Wednesday Dec 6

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

Gopher Invitational Meteorology

Section 1: How Did Life Begin? Chapter 19: History of Life on Earth. Section 2: The Age of Earth

This Week: Biogeochemical Cycles. Hydrologic Cycle Carbon Cycle

Section 1: Continental Drift

Lecture 5: Climate Changes and Variations

Midterm 2 Scores. Class average: 40/50. # of students. Exam score

Putting Things Together. Plate Tectonics & Earth History

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Shape and Size of the Earth

Directed Reading. Section: Continental Drift. years ago? WEGENER S HYPOTHESIS

The ACTIVE EARTH!!!!!

The History of Life on Earth

Habitable Planets: Part 1 Estimating n p "

Unit 6: Interpreting Earth s History

Chapter 9. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 27: Planetary Geology [3/26/07] Announcements.

2010 Pearson Education, Inc.

FUNDING FOR THIS PROGRAM IS PROVIDED BY ANNENBERG MEDIA.

PLATE TECTONICS. SECTION 17.1 Drifting Continents

1 Earth s Oceans. TAKE A LOOK 2. Identify What are the five main oceans?

Welcome to ATMS 111 Global Warming.

Diversity, Change and Continuity. History of Life

Transcription:

Announcements: 9.0 earthquake in Puget Sound! (in 1700) TALK TODAY: Monday 10 Nov 3:30 310 ATG Prof Lyatt Jaegle, UW, "Space-based observations of biomass-burning emissions of NOx" [a pollutant gas] Where we're going: This week: KKC Chaps 8,9 (selected) and Snowball Earth article (web) Tues: Wed: Fri: Solid Earth Circulation (wrap-up last week) Ancient Climates (or "History of Planet Earth in 3 Easy Lessons") HOLIDAY (free talk by veteran in Kane 120, 7pm) HW#4 DUE review, tutorial Mon Nov 10 but first, some first-grade wisdom...

Continental drift: Fig 6-1

Plate tectonics: Fig 6-21 the third of our three BIG pumps driven by circulations in the upper mantle; ultimately, by radioactive decay, releasing heat within the Earth's interior recycles key substances like mineralized carbon

Wilson Cycle: Fig 6-27 continents group together then spread apart timescale is ~500 million years major climatic consequences (location of continents affects atmos/ocean currents; ice-albedo feedback, etc)

Three BIG Pumps Circulation Summary Atmosphere/Surface Ocean - distributes heat poleward - cause of regional and seasonal climates - mixing timescale is ~1 week Thermo-haline circulation (THC) - mixes deep ocean - timescale of mixing is about 1000 years - may shut on and off as conditions change in N. Atlantic - possible "trigger" for global climate Solid Earth circulation: Wilson Cycle - continents group and then spread - cycle timescale is ~500 million years - major climatic effects (e.g. sets boundaries for the other two circulations) - mixes key elements like carbon and recycles them from rocks back to the atmosphere

Ancient Climates: Readings (info on website) Introduction/Overview 8:152-153, Fig 8-1 Formation of Early Atmosphere 8:158-159, Fig 8-7 Faint Young Sun paradox 8:159-161, Figs 8-8, 8-9 Long Term Climate Record 8:161-164, Fig 8-10, 8-11 Low Latitude Glaciation BOX 8:165 "Snowball Earth" article available on web Warm Mesozoic Era 8:167-169, Fig 8-15 Cooling During Cenozoic Era 8:169-170, Fig 8-17 Modern Controls on Atmos. O2 9:188-189, Fig 9-17

Ancient Climates: Stories Paleoclimate record fossils, clues and mysteries Grand Sweep of Earth History 4.6 billion years (so far) marker events (to memorize) Faint Young Sun paradox good illustration of scientific method Rise of Atmospheric Oxygen greatest global pollution event ever but made life on land possible oxygen and fire Snowball Earth >>>read from article something new in ancient history Failure of planetary life support Venus and Mars Snowball Earth asteroids

Origin of life: ~4 billion yrs ago Fig 9-5: microfossils, 3.5 billion yr old, Australia prokaryote (bacteria): single-celled organisms with no cell nucleus - only form of life for most of Earth history - still dominates eukaryote: organism whose cells have a nucleus - includes all multicellular organisms - came much later

Evidence of glaciations: tillite, 2.4 billion yrs old, Fig 8-10a

Evidence of glaciations: striations, 650 million yr old, Fig 8-10b

Evidence of glaciations: dropstone, Fig 8-10c

Wed Nov 12 Announcements: -grades on web - HW#4 due today; HW#5 due next thursday - Tad gone Tues-Thurs next week Today: - marker events in Earth history - Faint Young Sun paradox but first, tribute to a life of self-sacrifice...

end of last ice-age; begin civilization beginning of modern era of ice-ages asteroid impact; end of dinosaurs Cambrian explosion of life; beginning of fossil record Earth freezes over; life survives in pockets rise of atmospheric oxygen (greatest global pollution event; deadly to nearly all existing life) life! (prokaryotic bacteria) formation of Earth Earth is unfathomably old most of Earth history is very alien Geological Time: Fig 8-11

Geological Time: Fig 8-11 Ice-ages asteroid! Dinosaurs coal/oil Cambrian explosion

Temperature/Precipitation History

Faint Young Sun paradox: Fig 8-8 solar energy simple model of Earth's temperature model assumes: - CO2 in atmosphere same as today - Earth albedo same as today Why do we know this model is wrong?

Answer: Archeon life! Requires liquid water Fig 9-5: microfossils, 3.5 billion yr old, Australia

Faint Young Sun paradox: p159-161 paradox: despite less solar energy, Archean was warm enough to support photosynthetic life Possible explanations - sun...? - albedo... no - geothermal energy... no > greenhouse... - H2O... no - NH3... no > CO2... [see figure] less land more volcanism conceptual framework: T s = f(s o, A, T g ) plenty of carbon [see inorganic carbon cycle figure] > CH4 methane? (CH4) [recent Kasting proposal] early life would have produced it far longer atmospheric lifetime than today due to lack of oxygen Illustrates nature of scientific knowledge/progress (draw figure)

CO2 over Earth History: Fig 8-9

Thurs Nov 13 Announcements:? Today: - marker events in Earth history - Mesozoic Warmth - Cenozoic Cooling -Sister planets - Snowball science history (and some pretty pictures) but first, a few late-breaking headlines...

Earth History: Marker Events 1. Origin of Earth 2. Origin of Life 3. Rise of Oxygen to ~ modern levels 4. Snowball Earth events 5. Beginning of fossil record (Cambrian explosion) 6. Extinction of Dinosaurs by asteroid 7. Beginning of modern glaciations 8. End of last ice-age 4.6 billion ybp (years before present) ~4 billion ybp ~2 billion ybp 600-900 million ybp 540 million ybp 65 million ybp 3 million ybp 10 thousand ybp

Mesozoic Warmth (250-65 million ybp) What: - Warmer global-mean temperature. -Muchwarmer Polar Regions; no ice-caps. - Much warmer deep ocean. Evidence: - Lush ferns and alligators in Siberia. - Carbon isotopes in ocean sediments Cause: - Higher CO2 is leading suspect. - sea-floor spreading rate was greater - higher sea level (no ice caps) Remaining mysteries: - Ocean/atmos heat transport must have been much more efficient. - latitudinal and vertical - this is not understood

Cenozoic cooling, 65 million ybp to present What: - Earth cools, beginning ~60 million ybp. - Life retreats from Poles. - Polar ice caps form. - Eventually, ice-ages begin. Cause (one leading theory): - India collides with Asia. - Himalayas form. - Silicate weathering increases. - Atmospheric CO2 goes down.

Venus (runaway greenhouse) Sister planets Earth ("just right") Mars (virtually no greenhouse) - Oceans boiled away - No more weathering - Carbon partitions to atmosphere - CO2 is ~100,000 times that on Earth -T s = 427 C; T g = 466C - has oceans - farther from Sun; too - hydrological cycle cold for liquid water - weathering returns - no water vapor greenhouse CO2 to lithosphere - too small for plate tectonics - plate tectonics (volcanoes) - no carbon cycle return carbon to atmos. - CO2 is ~10 times Earth - negative feedback -T s = -53C; T g = ~3C

Mars, CO2 and Greenhouse Mars (virtually no greenhouse) - CO2 is ~10 times Earth - T g = ~3C Do you notice something strange about these facts??? What can we conclude about the cause of the greenhouse effect on Earth???

Hoffmann, Schrag, and Dropstone http://www-eps.harvard.edu/people/faculty/hoffman/snowball_paper.html

Snowball Science History -1 1960's: Mikhail Budyko (theoretical climate modeling) "run-away" ice-albedo feedback if Earth freezes below 30-degree latitude this must never have happened for two reasons... 1. continuous life 2. Earth could never recover 1964: Brian Harland (geologist) Late proterozoic glacial deposits on almost every continent magnetic alignment of grains indicate continents were near Equator

ice-albedo feedback Positive feedback loop: - amplifies an initial perturbation - potentially causes current equilibrium state to be unstable

Earth's Magnetic Field

Possible continental positions during Late Proterozoic Glaciations: Fig 8-12 Critical latitude for "runaway" ice-albedo (~30 degrees): Why would ice-albedo feedback get stronger as the ice-line got to lower and lower latitudes??? Answer: - more sunlight to reflect at lower latitudes - the amount of area per degree latitude gets much larger (major factor)

Snowball Science History -2 1960's: Martin Rudwick (biologist) with Brian Harland Recovery from global glaciation may have spurred Cambrian explosion "all 11 animal phyla ever to inhabit the earth emerged within a narrow window of time" after the end of the last glaciation 1970's: more biology discovery of life in extreme environments organisms near geothermal vents at ocean bottom have no need of sunlight bacteria and algea living in snow, ice, and rock pores under extreme cold, heat, and pressure overcomes argument (1), above 1992: Joseph Kirschvink (geophysicist) Atmospheric CO2 would build up during a global glaciation CO2 removal by silicate weathering would cease, but CO2 input from volcanoes would continue unabated overcomes argument (2), above

Snowball Science History -3 1992: Kenneth Caldeira and James Kasting Calculate that CO2 would have to be 350 times current levels to melt a global glaciation This would take about 10 million years 1992: Kirschvink Iron deposits mixed with glacial debris indicate ocean lacked oxygen This implies ice-covered oceans 1990's: Hoffman and Schrag Carbon isotopes in rocks surrounding glacial deposits indicate a virtual shut-down of biological activity Massive carbonate deposits on top of the glacial deposits ("cap carbonates") indicate very warm water and sudden deposition of huge amounts of carbon Apparently, the glaciation events were immediately followed by a global hothouse period This is consistent with huge buildup of atmospheric CO2.

Idealized carbon isotope record through a Snowball event

Measured carbon isotope record through a Snowball event Ghaub Glaciation, Otavi Group, NW Namibia

Iron Solubility and Deposition in Relation to a Snowball Event http://www-eps.harvard.edu/people/faculty/hoffman/snowball_paper.html

Namibia cliffs, snowball record