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Earth

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Earth's Environment, Climate Change, and Human Impacts. The ... Faster molecules bump into slower molecules. Heating a skillet on the stove. Convection. ... – PowerPoint PPT presentation

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Title: Earth


1
Earths Environment, Climate Change, and Human
Impacts
2
The Earths Energy Budget
3
Return to Physics
  • Energy is transferred by
  • Conduction. Faster molecules bump into slower
    molecules. Heating a skillet on the stove.
  • Convection. Energy is transferred with the
    material. Boiling pot of soup.
  • Latent heat. Energy is lost or absorbed when
    changing states (e.g., energy required to
    evaporate water).
  • Radiation. Heat from Sun reaching Earth.

4
  • Radiation Basic Concepts
  • All matter radiates energy.
  • Radiant energy travels in the form of
    electromagnetic waves.
  • These waves do not require molecules to
    propagate.
  • Different types of radiation are characterized
    by different wavelengths
  • AM radio waves 100 meters
  • Microwaves 1 mm
  • Infrared 10-6 meters (1 micrometer (µm) 10-6
    meters)
  • Visible light 5 x 10-7 meters
  • UV 1 x 10-7 meters

5
Electromagnetic Spectrum of the Sun
6
  • Radiation Basic Law
  • Stefan Boltzman law
  • E ? T4
  • E is energy in Watts/m2
  • T is temperature.
  • ? is a constant.
  • As T increases, E increases by a power of 4.
  • If T doubles, E increases by 16 times!

7
Spectrum of the Sun vs. Spectrum of the Earth
8
  • If the Earth always radiates energy, why doesnt
    it cool?
  • It is in a state of radiative equilibrium.
    Incoming radiation is balanced by outgoing
    radiation.
  • Radiative equilibrium predicts surface
    temperature of approximately 255 K (approximately
    -18C).
  • But, the Earths observed average surface
    temperature is 288 K (approximately 15C).
  • Why the difference? The answer lies in an
    understanding of absorption, reflection,
    transmission of radiation.

9
Absorption
Day
  • Objects that are good absorbers are also good
    emitters.
  • Consider an asphalt road.
  • During the day the asphalt absorbs solar
    radiation and warms.
  • At night the asphalt emits infrared radiation and
    cools relative to its surroundings.

Warm
Asphalt Road (warms due to solar radiation)
Night
Cool
Asphalt Road (cools by IR radiation)
10
Albedo
  • Albedo the ratio of reflected radiation to
    incident radiation.
  • Surface albedo varies
  • Spatially
  • Temporally
  • Earths average albedo is 31.

11
With Greenhouse Effect
Fig. 23.6
12
The Greenhouse Effect
13
The Greenhouse Effect
  • A global warming effect in which the atmosphere
    of a planet traps heat and maintains the surface
    of the planet at a higher temperature than if
    there were no atmosphere.
  • Has existed throughout Earths history.
  • TMJ.

14
Composition of the Atmosphere
  • Atmosphere
  • Nitrogen (78)
  • Oxygen (21)
  • Minor constituents Argon, carbon dioxide, water
    vapor, ozone
  • Major greenhouse gases
  • Water vapor
  • Carbon dioxide

15
The future of climate change is difficult to
predict.
  • What do we know?

16
What do we know?
  • Temperature and carbon dioxide are highly
    correlated.

Fig. 23.7
17
What do we know?
  • Temperature and carbon dioxide have been
    increasing since the Industrial Revolution.

Fig. 23.8
18
What do we know?
  • Compared to the last 1000 years, temperatures and
    carbon dioxide levels have been higher in the
    last century.

Fig. 23.8
19
What do we think we know?
  • We think we know how carbon is cycled through
    various Earth reservoirs.

Fig. 23.11
20
How do we figure out whats going to happen?
  • Computer models.
  • Supercomputers.
  • General Circulation Models (GCMs) encompass
    various parts of the Earth system (atmosphere,
    oceans, etc.).
  • Very complex.

Fig. 23.2
21
Why do we have difficulties with predictions?
  • Positive and negative feedbacks complicate
    climate change predictions.
  • Positive feedback A change in one component is
    enhanced by changes in another component.
  • Negative feedback Change in one component
    counteracts a change in another component.

22
Feedbacks
  • Water vapor feedback Positive.
  • Increasing temperature increases amount of water
    vapor in atmosphere. Water is a greenhouse gas,
    so this increases surface temperature, which in
    turn increases evaporation, etc.

23
Feedbacks
  • Albedo feedback Positive.
  • Increasing temperature decreases snow and ice,
    which decreases albedo. Decreased albedo means
    more absorbed energy, which means increasing
    temperature.

24
Feedbacks
  • Radiation feedback Negative.
  • An increase in energy reaching the Earths
    surface causes an increase in the temperature of
    the Earth, and therefore the amount of heat the
    Earth reradiates back out.

25
Feedbacks
  • Plant growth feedback Negative.
  • More carbon dioxide means more plant growth,
    which means more use of carbon dioxide in
    photosynthesis.

26
So, could we add Fe to fertilize ocean thus
ameliorate greenhouse CO2 build-up? 1. Will it
work? 2. What are the ecological consequences?
 Just Add Iron ABCnews.com, Amanda Onion
10/11/00   How algae may slow warming By Gareth
Cook, Boston Globe Staff, 10/12/2000   Helping
ocean algae could beat greenhouse effect
LONDON (Reuters), WIRE10/11/2000 Global
Warming NPR Morning Edition- John Nielsen,
10/11/00 Iron-Fed Plankton Absorbs Greenhouse
Gases By ANDREW C. REVKIN, NY Times,
0/12/00   Iron May Increase Gas - Eating
Algae By THE ASSOCIATED PRESS, 10/11/00
Oct. 2000
27
Why else do we have trouble predicting climate
change?
  • Systems are
  • COMPLEX!

28
So what do you do if you want to learn more about
this?
29
 Department Course Number Course Name Semester Units
 MAC  2311 Calculus with Analytics Geometry I  4
 MAC  2312 Calculus with Analytic Geometry II    4
 CHM  1045 General Chemistry I    3
 CHM  1045L General Chemistry I Laboratory  1 
 CHM  1046 General Chemistry II  3
 CHM  1046L General Chemistry II Laboratory  2
PHY  2048C General Physics A and Laboratory    5
PHY  2049C General Physics B and Laboratory  5
 GLY  2010C Physical Geology  4
 GLY  2100 Historical Geology  3
 GLY  2100L Historical Geology Laboratory  1
 GLY  3200C Mineralogy and Crystallography  3
 GLY  3220C Optical Mineralogy 2
 GLY  3310C Igneous and Metamorphic Petrology  3
 GLY  3340C Sedimentary Petrography  2
 GLY  3400C Structural Geology  4
 GLY  3600C Paleontology  4
 GLY  4511 Principles of Stratigraphy  3
 GLY  4750 Geological Field Methods  1
 GLY   4751 Field Course  6
 GLY  4XXX Geological Elective  2
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