Title: Earth
1Earths Environment, Climate Change, and Human
Impacts
2The Earths Energy Budget
3Return 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
5Electromagnetic 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!
7Spectrum 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.
9Absorption
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)
10Albedo
- Albedo the ratio of reflected radiation to
incident radiation. - Surface albedo varies
- Spatially
- Temporally
- Earths average albedo is 31.
11With Greenhouse Effect
Fig. 23.6
12The Greenhouse Effect
13The 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.
14Composition of the Atmosphere
- Atmosphere
- Nitrogen (78)
- Oxygen (21)
- Minor constituents Argon, carbon dioxide, water
vapor, ozone - Major greenhouse gases
- Water vapor
- Carbon dioxide
15The future of climate change is difficult to
predict.
16What do we know?
- Temperature and carbon dioxide are highly
correlated.
Fig. 23.7
17What do we know?
- Temperature and carbon dioxide have been
increasing since the Industrial Revolution.
Fig. 23.8
18What do we know?
- Compared to the last 1000 years, temperatures and
carbon dioxide levels have been higher in the
last century.
Fig. 23.8
19What do we think we know?
- We think we know how carbon is cycled through
various Earth reservoirs.
Fig. 23.11
20How 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
21Why 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.
22Feedbacks
- 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.
23Feedbacks
- Albedo feedback Positive.
- Increasing temperature decreases snow and ice,
which decreases albedo. Decreased albedo means
more absorbed energy, which means increasing
temperature.
24Feedbacks
- 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.
25Feedbacks
- Plant growth feedback Negative.
- More carbon dioxide means more plant growth,
which means more use of carbon dioxide in
photosynthesis.
26So, 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
27Why else do we have trouble predicting climate
change?
28So 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