Investigations
Lesson 6
Title: The Greenhouse Effect
Overview & Outcomes:
An understanding of the ultraviolet, visible and infrared portions
of the electromagnetic spectrum and of reflection, absorption,
transmission and emission of electromagnetic energy, and albedo
are essential elements needed for comprehension of the "greenhouse
effect." In that manner, Investigations Lesson 5 served
as a bridge between Investigations Lesson 2 and this lessons.
This lesson is in many respects a continuation of ideas presented
in those Investigations Lessons, as well as Investigations Lesson
1. However, it is written as a separate lesson in order to focus
students' attention on the phenomena known as the "greenhouse
effect" and to explain why the term "greenhouse effect"
is actually a misnomer. This lesson also is an important precursor
to Lesson 8, the topic of which is human-produced greenhouse gases
and the "enhanced greenhouse effect." In Investigations
Lesson 7 students will determine the role that the atmosphere
plays in temperature regulation.
This lesson helps learners:
- define the greenhouse effect.
- identify naturally occurring greenhouse gases.
- identify other common examples of the greenhouse effect.
- explain the limitations of the term greenhouse effect as an
explanation of the phenomena responsible for keeping the planet
warm.
The concept map shows model relationships
among concepts this lesson seeks to develop. Concepts introduced
in this lesson are bolded on that concept map and concepts from
other lessons are in plain text (not bolded).
Background Notes for the Teacher:
Content. In Investigations Lesson 5 we learned that the
Earth's Energy Budget is an equilibrium; that is, the amount of
incoming short wave radiation (UV, visible light, and near infrared
wavelengths) is balanced by the same amount of outgoing longer
wave radiation. This is a result of reflection (albedo), absorption
and transmission, and re-radiation of the incoming radiation.
In order to make the link between electromagnetic radiation,
the Earth's atmosphere and the greenhouse effect, a bit more knowledge
is needed about Earth's Energy Budget that was provided in Investigations
Lesson 5.
To begin with Earth's equilibrium temperature can be calculated
using a series of equations generated from important physical
laws, including Plank's Law, the Stefan-Boltzmann Law, and Wen's
Law. The equilibrium temperature is the temperature of the Earth
resulting from the balance of incoming short wave and outgoing
long wave radiation, and is a function of the distance the earth
is from the sun (which affect the intensity of the solar radiation
reaching the Earth) and the Earth's albedo. Earth's equilibrium
temperature, as solved by the equations is 0oF. That is, 32 degrees below freezing.
However, we know from measurements that the actual temperature
of the Earth is 60oF! When you think about it, we know the calculated
equilibrium temperature can't be "right" because if
it were, then most of the surface of the earth would be frozen.
The question then is, Why is there a discrepancy between the calculated
and observed temperatures? The answer is: the Greenhouse Effect.
Remember from Investigations Lesson 5 that some of the incoming
short wave radiation is absorbed by the Earth's surface and re-radiated
as long wave radiation. The atmosphere is not very transparent
to these long waves. Atmospheric gases such as CO2, water vapor,
methane, ozone and N2O are known as greenhouse gases because
they absorb and re-emit long-wavelength energy, causing much of
it to go back to the earth's surface. Thus this long-wavelength
energy that cannot escape the earth's atmosphere warms the earth.
This is the greenhouse effect, which is very important
in that if this phenomena did not occur, the Earth would be a
frigid 0oF (or -18° C), otherwise. The intensity of this
effect depends on the concentration of absorbing gases in the
atmosphere. Although CO2 makes up only about .03% (pre-industrial
concentration - years 1750 to 1800 - was about 280 parts per million
by volume) of the atmosphere, it is vital in maintaining the temperature
balance because it strongly absorbs infrared energy. Water vapor
(ranging in quantities from 0-4% by volume) also absorbs considerable
infrared energy. The other naturally occurring greenhouse gases,
methane, ozone and N20, play a part in this as well. Another
example of the greenhouse effect-We have all had the experience
of getting into our car on a sunny day only to find that the temperature
of the air is warmer inside the car than outside. This is especially
notable if the car has a dark interior. This common experience
provides a good example of the greenhouse effect.
The greenhouse effect...a misnomer-While this discussion may seem
unnecessary, we must be careful not to promote any alternative
conceptions to students. The term "greenhouse effect"
came to be used as an analogy to describe the atmosphere's role
in the warming of the planet because of the similarities between
the glass of a greenhouse and the atmosphere. They are both "clear"
and allow many wavelengths of electromagnetic energy to pass through.
They then both seem to prevent heat (long-wavelength infrared
energy) from escaping. Here is where the analogy breaks down.
A greenhouse stays warm because the glass acts as a solid barrier
that effectively prevents air inside the greenhouse from mixing
with air on the outside. The greenhouse gases do not function
similarly. First of all, these gases are not a solid boundary.
Secondly, as previously described in Investigations Lesson 5,
these gases absorb and re-emit long-wavelength energy and do
so in all directions, not just back to the earth. This is
why it is the concentration of greenhouse gases that determines
the degree of warming.
Additional Teacher References. Both earth science and
physics (physical science books) are useful references.
Materials:
For class.
- Materials to represent greenhouse gases so that they may
be added to the bulletin/storyboard.
Preparation:
Prior to day of lesson.
Assemble materials for or prepare
representations of the greenhouse gases.
Instructional Procedures: (1 Day, 40 minutes)
- Using information from Lessons 1, 2 and 5 and this lesson's
Background Notes for Teacher, organize the lesson in such a way
as to most effectively present the information. It is suggested
that the bulletin/storyboard continue to be used, depending on
how it was originally set up. For example, if the gases discussed
in this lesson (CO2, methane, ozone and N20) have already been
represented on the bulletin/storyboard, perhaps they could now
be distinguished from the other atmospheric gases using color
or a border. It is important that students understand that not
all gases in the atmosphere are greenhouse gases. It is also
important that the gases be seen as separate molecules, not as
a solid layer or boundary.
- Ask students if they have ever been to a greenhouse. Explore
what distinguishes a greenhouse from other buildings and why it
is particularly well suited for growing plants. Ask students
if they can think of another situation that they personally have
experienced that is similar to a greenhouse (i.e., a car interior
on a sunny day). Relate this discussion not only to the greenhouse,
but also to the previous discussion of albedo (do darker car interiors
produce warmer temperatures?) and reflection of incoming radiation
by clouds (why do people put sun shields in the windshield? what
color are the sun shields?).
- Expand on this discussion by defining the greenhouse effect
and discussing how certain gases in the atmosphere are both similar
and different from the glass of a greenhouse or a car. (Refer
to Background Notes.) Explain to students that a car with the
windows down slightly is a better analogy of our atmosphere.
The car interior typically remains warmer than the outside temperature,
but some infra-red wavelengths do "escape."
Assessment/Portfolio Items:
Journal Entry.
Explain why the greenhouse effect is not
entirely correct in describing the role the atmosphere plays in
warming the planet.
Project.
Ask students to think of other examples of the
greenhouse effect.
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This unit was produced by the editors listed on the masthead.