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Geography 1001: Climate & Vegetation Instructor: Andrés Holz Teaching Assistant: Eungul Lee

Geography 1001: Climate & Vegetation

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Geography 1001: Climate & Vegetation. Instructor: Andr é s Holz Teaching Assistant: Eungul Lee. Agenda for Lecture 13: Thursday June 29. Announcements Yesterday’s lecture is online First reading for guest lecture is also online FIELD TRIP TO ISABELLE LAKE, INDIAN PEAKS Objective - PowerPoint PPT Presentation

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Page 1: Geography 1001: Climate & Vegetation

Geography 1001:Climate & Vegetation

Instructor: Andrés HolzTeaching Assistant:

Eungul Lee

Page 2: Geography 1001: Climate & Vegetation

• Announcements– Yesterday’s lecture is online– First reading for guest lecture is

also online

– FIELD TRIP TO ISABELLE LAKE, INDIAN PEAKS

• Objective

– MEET AT THE REC CENTER TURN AROUND AT 9 AM. WE WILL DEPART PROMPTLY.

Agenda for Lecture 13: Thursday June 29

Page 3: Geography 1001: Climate & Vegetation

Agenda for Lecture 13: Thursday June 29

• Gear Requirements: – hiking boots (the trail is

muddy in places and there is still some snow on the ground)

– raingear– sun block & chap stick– Sunglasses hat, gloves– warm layers (fleece)– notebook and pen to take

notes

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FIELD TRIP TO ISABELLE LAKE, INDIAN PEAKS

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Access and Trail Description:• Lake Isabelle is one of the more

beautiful trails in the Front Range.

• The lake lies near timberline in a dramatic valley, offering views of high peaks such as Shoshone, Apache and Navajo Peaks

• Distance: 2.0 miles one-wayLake elevation: 10,868 feetTrailhead elevation: 10,480 feetNet elevation gain: 388 feet

Page 6: Geography 1001: Climate & Vegetation

• Today’s lecture:– Historical development of

the ecosphere• Biological processes that

changed the atmosphere– Anaerobic respiration– Photosynthesis– Aerobic respiration

• Atmospheric changes– Increase O & N– Stabilization of CO2– O3 layer

Agenda for Lecture 13: Thursday June 29

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• Today’s lecture:– A bit of ourselves

• DNA• Earth colonization

– Changes on earth• Milanković

Agenda for Lecture 13: Thursday June 29

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Be aware of..

• How the Ecosphere have developed over time: Timeline and processes occurring

• How Climate & Life on earth have co-evolved

• The fact that regardless of co-evolution, we still have large scale climate changes Milanković Theory

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A bit of history here…

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500 million years ago..

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400 million years ago..

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300 million years ago..

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200 million years ago..

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100 million years ago..

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50 million years ago..

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1 million year ago..

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Less than a million year ago..•So far, we know that the Earth has experienced at least 8 ice ages•Last one?

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Today•If we think of the earth life being a calendar year (i.e. from Jan 1 to Dec 31), when do you think we appeared?

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But how have the conditions for life changed over these 4 billion years?

The solar system form 4.6 billion years ago.

4 billion years ago, the atmosphere was made of from volcanic emissions

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• TIME– 4 billion yrs ago

• PROCESS– Water vapor– Ammonia (NH3)– Methane (CH4)– Hydrogen sulfide (H2S)

– Hydrogen gas (H2)– Carbon monoxide

(CO)– **Very little O2 & N2

All water was held in the atmosphere as vapor because of high temperatures (water vapor greenhouse effect).

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• TIME– 4 billion yrs ago

– 3.1-3.5 billion yrs ago

• PROCESS– H2O, CO2, (N) dominant.

– CO2, H2O, N2 dominant O2 begins to accumulate.

– Cooling of the atmosphere causes precipitation and the development of the oceans.

– Break of H2O by ultraviolet rays H2O O2 + H

– Water vapor clouds common in the lower atmosphere.

– First single cell algae & bacteria

Page 26: Geography 1001: Climate & Vegetation

• TIME– 3.1-3.5 billion yrs ago

• PROCESS– Anaerobic respiration

• Single cells algae were able to – produce Energy without O2

– Take C-H20 (simple organic molecules food) & break down into CO2 + alcohols

energy

For ~800 millions of years, CO2 was released (as by-products of respiration) & built up in the atmosphere and oceans

There was enough CO2 in the atmosphere to sustain life….

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• TIME

– 2.3 billion yrs ago….

• PROCESS

– Photosynthesis Single-cells (blue-green algae have chlorophyll)

CO2 + H2O CH2O + O2 built up

–Initially, the released O2 was lethal to the living organisms

energy

sunlight

food

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• TIME

– 1.9 billion yrs ago….

• PROCESS

– Ozone (O3) layer is being built in the stratosphere

Filters out the UV radiation make life possible on land development of O2 tolerant organisms

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Aerobic life on the land took longer to start because it could only occurred after the ozone layer was formed

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• TIME

– 1.3 billion yrs ago….

• PROCESS

– Aerobic respiration

CH2O + O2 CO2 + H2O

energy

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• TIME

– 600 mill yrs ago….

• PROCESS

– Life is widespread in the oceans• Single cells• Early fishes• Large algae

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• TIME

– 420 mill yrs ago….

• PROCESS

– Life is widespread on lands

• Earliest plants• Invertebrates• Vertebrates

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• TIME

– 350 mill yrs ago….

• PROCESS

– Development of tropical rainforest

• fossil fuel today’s oil

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• TIME

– 200 mill yrs ago….

• PROCESS

– Colonization of larger vertebrates

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A bit of ourselves..

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Date of Separation according to Mitochondrial DNA

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Early Human Phylogeny

southern Africa

eastern Africa

eastern Africa

Asia

Africa Asia

Europe

Africa?

Europe & W Asia

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Expansion of Human Habitat(old theory)

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At 18,000 years ago, the Earth looked like this map from Earth and Life Through Time

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Food Chain of Land Animals

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World Population Trend from 10,000 B.C. to 200 A.D.

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First civilization collapse..

• Eastern Island• Mayas Empire

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UN, World Population Prospects:1992

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Why has climate change?

• Meteorite impacts (very infrequent & random)

• Hugh Volcanic eruptions (more frequent, but still random)

• Enough evidence of glacial and interglacial periods for the last 2-3 mill yrs– Hypotheses, Theories, & Laws…the same?

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Milanković cycles (Theory)

Performed detailed calculations concerning the periodicity of the earth’s orbital parameters

• Precession• Axial tilt• Eccentricity

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Eccentricity

• During periods of high eccentricity higher differences between max & min distance from sun to earth more potential for extreme (cold & warm) climate

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Orbit eccentricity

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Tilt angle (or obliquity)

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Tilt angle (or obliquity)

• The greater the angle of the tilt the greater the potential for extremes in seasonal climate (especially for polar regions)

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Precession (or wobble)

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Precession (or wobble)

• It’s a ‘slowing down’ of the rotation of the earth tilt of the earth point to various directions (like the axe of a spinning top)

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Evidence of glaciations?

• Swiss hunter in the Alps (1815) associated scratch marks on rocks with the P of ice

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Yosemite

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How do scientists track glaciation?

• Stable-isotopes from zooplankton (tiny shells of calcite)

• Come from seawater• Once dead built up

on the ocean bottom as layers (~2.5 cm or 1” = 1,000 yrs)

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Comparison between O2 isotope record & Milanković theory

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How do scientists track glaciation?

Lighter Oxigen (16O) evaporates with water vapor (due to insolation) andthen precipitates as either:

a) rain and returns with rivers and groundwater to oceans seawater remains the ~same (interglacial) [e.g. now]

Or b) snow and accumulates and does NOT return to oceans seawaterchange rate between 16O & 18O