Learners develop skills for thoroughly exploring STS issues as they apply those skills in investigating the focusing STS question. These include the study of science and social studies concepts or aspects of technology that are foundational to understanding the STS issue, through library research using primary and secondary sources, securing data and information from outside agencies, hands-on inquiry activities, collecting natural science data on site, and using social science research techniques such as questionnaires and interviews to collect data within the community. The information and data from the investigations are consolidated by learners to answer the STS focusing question.
Title: The Atmosphere
In the last lesson, Foundations/Awareness Lesson 11, students identified three STS issues that fall under the umbrella of global atmospheric change (GAC) and requested information from outside agencies. In the next 15 lessons included in this the second or Investigations Section of the unit, student will carry out investigations on the STS question, "Is global atmospheric change a threat?" in order to develop an in-depth and multifaceted understanding of GAC in preparation for making informed decisions and taking appropriate actions in the last section of the unit. Students will begin their study of the atmosphere in this lesson by examining the composition and structure of the atmosphere. This information will serve as a base for all future discussions of GAC. Investigations Lesson 2 introduces students to the electromagnetic spectrum (EMS), which is another big idea basic to understanding GAC.
This lesson helps learners:
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).
Content. We can think of the earth as being composed of four interacting systems: atmosphere, hydrosphere, lithosphere and the biosphere. The first three are abiotic or non-living, which the biosphere is comprised of living matter.
The Atmosphere is comprised of gases: nitrogen (N), oxygen (O), argon (Ar), carbon dioxide (CO2), , water vapor (H2O) and trace gases. ( More detailed information is given later in this section.) The hydrosphere is composed of water in its solid, liquid and gas forms. These may exist in the atmosphere, on the earth's surface, and in the earth's crust.
The ware may exist as salt or fresh water. The lithosphere is earth's crust and a portion of the upper mantle, it is brittle and it moves (plate tectonics). The biosphere contains all living organisms and the environment in which they live. The biosphere overlaps with the abiotic spheres, as it covers from the sea floor to about 8 Km (5 miles) into the atmosphere. When thinking in terms of these four spheres, it is important to understand that there boundaries are not distinct, and they may overlap.
The atmosphere is not only a very essential component of the biosphere, but a very dynamic part as well. The dynamic, multifaceted nature of the atmosphere is often not completely understood by students. This lesson is intended to provide an information base for several future lessons. Students will not only study the composition and structure of the atmosphere, but also come to "appreciate" the many functions of the atmosphere as well as its constancy through time.
Function of the atmosphere-The atmosphere is often difficult to appreciate given the fact that on a clear, calm day, its presence is almost undetectable as are the essential gases it is composed of. The following is a brief list of atmosphere functions, most of which are necessary to support life:
Composition of the atmosphere-Many of the physical and chemical processes that occur in the atmosphere are directly related to its composition. The atmosphere is now composed almost entirely of oxygen and nitrogen in their diatomic forms (two atoms bound together by chemical forces). However, it was not always this way. When the earth formed about 4.5 billion years ago it probably did not even have an atmosphere. While the evolution of the atmosphere is not included in this lesson, it is interesting to note that once photosynthetic organisms evolved (beginning approximately 3.5 billion years ago), the atmosphere changed significantly. As oxygen (O2) was produced by these organisms, it built up in the atmosphere, as did ozone (O3). By about 400 million years ago, the atmosphere contained as much oxygen as it does today and overall, the proportion of gases in the atmosphere has remained about the same. This is an important feature of the atmosphere. It is vital that students understand that the relatively stable composition of the atmosphere is essential to its stable function.
The following table and pie graph provide basic information about the composition of the atmosphere:
| GAS | PERCENTAGE IN ATMOSPHERE |
|---|---|
| Nitrogen | 78% |
| Oxygen | 21% |
| Argon | 0.9% |
| Carbon Dioxide | 0.03% |
| Water Vapor | <0.01% |
| Nitrous Oxide | |
| Ozone | |
| Methane | |
| Neon | |
| Helium |
The concentration of the "trace" gases (those occurring in amounts less than 0.1%) can also be given in parts per million rather than in parts per 100 (per cent). The most abundant of these is carbon dioxide at 340 parts per million (ppm). Interestingly, ozone concentration varies with altitude, reaching a maximum of 12 ppm at approximately 30 kilometers. It is important to note that even though there are only "traces" of certain gases, their concentrations are very important to living things and to the function of the atmosphere. For example carbon dioxide, water vapor, ozone and methane are "greenhouse gases-they absorb heat from sunlight at an average temperature of 53oF is a greenhouse gas-and ozone protects us cancer causing from UV light. In identifying the gases that make up the atmosphere, many sources refer to the composition of "dry air." This is due to the fact that the composition of dry air is remarkably constant over the globe, while the amount of water vapor varies widely, ranging from 4% by volume to less than 1%.
Structure of the Atmosphere-Meteorologists divide the atmosphere into four layers: the troposphere (where 90% of the total mass of the atmosphere and where almost all of the earth's weather occurs), stratosphere, mesosphere and thermosphere. The exact height of the atmosphere has no real meaning, for the air gets thinner and thinner the higher one goes and eventually thins out to outer space. Air is more compressed at sea level than at higher altitudes similar to feathers in a huge pile. What's at the bottom is more "squashed" than what's near the top. The division into layers is based on temperature and each layer has a different temperature range and profile. Temperatures decrease with altitude in the troposphere and mesosphere and increase with altitude in the stratosphere and thermosphere. These temperature layers are created primarily by the selective absorption of electromagnetic energy (which is discussed in Investigations Lesson 5). The following chart and graphic provides basic information about each of the layers:
| Layer | Location | Temperature | Other Significant Characteristics |
|---|---|---|---|
| Troposphere | Over North/South Poles: 0-6 miles (10km) Over equator: 0-10 miles (16km) | Varies from ground level air temperatures to -75F (-57C) | -the layer in which we live -90% of total mass of atmosphere is found here -where almost all the earth's weather occurs -jet stream found in upper troposphere |
| Stratosphere | 6-10 miles - 30 miles (48km) | Varies from -67F (-55C) at lower layer to 28F (-2C) at upper layer | -very little moisture, clouds are rare -pilots fly here to avoid weather distrubances -where most of ozone is found -"WARMER temperatures are due to ozone's reaction with UV light |
| Thermosphere | 50 miles - outer space | Temperature of molecules can climb to 1100F (600C) at 120 miles above the earth | -the extremely thin air is completely exposed to the sun's radiation, accounting for the high temperatures that molecules can reach when they are bombarded by the radiation. Otherwise it is VERY COLD |
Location of the Ozone Layer-Ozone (O3) is a molecule composed of three atoms of oxygen-a tri-atomic form of oxygen. Ozone is highly reactive with other atoms and molecules, and it acts as a filter for cancer causing UV light. Ozone absorbs the UV (shorter) wavelengths of sunlight and re-radiates the energy in the form of infrared (longer) wavelengths of light. In the process, the more common di-atomic form of oxygen (O2) is broken down forming non-atomic oxygen (O), which combines with other diatomic molecules of oxygen to form ozone (O3).
While the function of the ozone layer will be discussed in Investigations Lesson 4, the location of the ozone "layer" is an important idea to address in this lesson. Many sources describe the ozone layer as a band found in the stratosphere at a height of approximately 15 miles (25 km). However, in actuality, ozone molecules are found throughout the atmosphere but are "concentrated" in a broad band beginning at approximately 10 miles (16 km) and extending into the mesosphere to about 50 miles (80 km). While it is true that the ozone layer, if compressed, would be approximately 3 cm thick, it is inappropriate to refer to it as a thin band in the stratosphere. Tropospheric and stratospheric ozone will be distinguished and discussed at length in future lessons.
Additional Teacher References. Earth science texts and encyclopedias are good sources of additional information, diagrams, tables, charts and explanations about the atmosphere. If you do not have one, check with an earth science teacher in your district.
Prior to day of lesson. Assemble bulletin or storyboard materials (see Appendix D). Duplicate worksheet (if desired). Assemble other appropriate student materials.
Student constructed or completed Pie Charts or Graphs representing the composition of the atmosphere.
Concept map (individual and/or class)
| Layer | Location | Temperature | Other Significant Characteristics |
|---|---|---|---|
| Troposphere | . | . | . |
| Stratosphere | . | . | . |
| Mesosphere | . | . | . |
| Thermosphere | . | . | . |
Click Here to go to Investigations Lesson 2: EMS: Visible and Invisible Light