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NAME: DATE: Use the space on each page to take notes on what is discussed verbally in class, any board notes, and all diagrams. 1. The processes of the atmosphere are responsible for most of the erosion of the land that works against the uplift actions of the Earth's internal processes. TEXT PAGE: 2. The atmosphere is the layer of gases that covers the surface of the planet. TEXT PAGE: 3. The atmosphere of the planet is made of a variety of gases that cycle through the atmosphere in a variety of ways. TEXT PAGE: 4. Understanding the evolution of the atmosphere helps to understand the importance and cycles of these gases. TEXT PAGE: 5. If Earth's first atmosphere (before 4 billion years before present) was similar to that of the outer planets of the solar system, it was probably mostly methane CH2, and ammonia CH4. TEXT PAGE:References:6. This early atmosphere was probably too thin to provide any protection from the heavy meteorite bombardment of the time. TEXT PAGE: 7. Earth's first atmosphere was replaced by nitrogen N2, water vapor H2O, and carbon dioxide CO2 from the widespread volcanic activity that occurred from around 4 billion to 3.5 billion ybp. TEXT PAGE: 8. The thicker, heavier N2/CO2/H2O air shielded the surface of the planet from meteorites, most of which were already cleared from Earth's orbit. TEXT PAGE: 9. N2, CO2, H2O vapor do not provide any protection from ultraviolet radiation (UV) that disrupts complex molecules such as those of living organisms. TEXT PAGE: 10. The atmosphere of Venus is a good model for Earth's second atmosphere, where high levels of CO2 keep surface temperatures extremely high. TEXT PAGE: 11. As the meteorite bombardment lessened, the surface of the planet and the early atmosphere was able to cool enough for the H2O to condense, and rain began to fill the low areas to form the first oceans. TEXT PAGE: 12. Those hot, early oceans must have contained a vast variety of dissolved chemicals from the land, ocean bottoms, volcanic activity, continuous lightning from the storms, and contributions from meteorite impacts. TEXT PAGE:
13. Lab experiments have imitated these conditions, and have produced very complex molecules similar to some of the simpler molecules found in living organisms. TEXT PAGE: 14. Lab experiments have demonstrated that after hundreds of millions of years, increasingly complex molecules could have begun to replicate themselves, used other molecules for sustenance, and react to stimulus, all of which are properties of life. TEXT PAGE: 15. Fossil evidence of the earliest form of living organisms indicates that organisms similar to today's cyanobacteria (blue-green algae) were living in the oceans around 3.5 to 3 billion ybp. TEXT PAGE: 16. These primitive organisms are photosynthetic, using the energy of the Sun to take in CO2 and H2O to form their tissues, and releasing oxygen gas O2 as a waste product. TEXT PAGE: 17. The primitive cyanobacteria must have lived deep enough in the oceans to be shielded from UV, but close enough to the surface to get sunlight. TEXT PAGE: 18. As the primitive cyanobacteria flourished, the levels of CO2 dissolved in the water went down, and CO2 from the air would have dissolved into the water. TEXT PAGE: 19. As O2 entered the water, its high reactivity would have caused it to combine with many of the elements dissolved in the water, such as metals, especially iron. TEXT PAGE: 20. Over time, the oxygen from photosynthetic organisms would combine with most of the abundant iron in the water, forming iron oxides or rust. TEXT PAGE: 21. Solid rust particles precipitate from water, and form dense formations around present day cyanobacteria. TEXT PAGE: 22. As the oceans were cleared of iron by the oxygen from cyanobacteria, vast deposits of iron ore were formed which are now being mined by people in many areas of the world, including the Great Lakes Region of the US. TEXT PAGE: 23. These iron ore deposits are nonrenewable resources because the conditions that formed them took millions of years and were hopefully unique in the history of the planet. TEXT PAGE: 24. After the easily oxidized elements such as iron were removed from ocean waters, the oxygen levels would increase in the water and then in the air as oxygen dissolved into the air from the surface of the water. TEXT PAGE:
http://www.geo.cornell.edu/geology/classes/SES302/00notes/00SES302Lect09.pdf
http://www.sprl.umich.edu/GCL/paper_to_html/evolut_clim.html
and
http://www.uta.edu/geology/geol1425earth_system/images/gaia_chapter_3/earth_differentiation.htm
http://www.livescience.com/othernews/060823_oxygen_world.html
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