{"id":919,"date":"2021-09-16T19:30:55","date_gmt":"2021-09-16T19:30:55","guid":{"rendered":"https:\/\/pressbooks.ccconline.org\/accphysicalgeography\/chapter\/22-4-earths-first-2-billion-years-physical-geology-2nd-edition\/"},"modified":"2022-01-06T02:08:22","modified_gmt":"2022-01-06T02:08:22","slug":"22-4-earths-first-2-billion-years-physical-geology-2nd-edition","status":"publish","type":"chapter","link":"https:\/\/pressbooks.ccconline.org\/accphysicalgeology\/chapter\/22-4-earths-first-2-billion-years-physical-geology-2nd-edition\/","title":{"raw":"22.4 Earth\u2019s First 2 Billion Years — Physical Geology – 2nd Edition","rendered":"22.4 Earth\u2019s First 2 Billion Years — Physical Geology – 2nd Edition"},"content":{"raw":"
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Figure 22.4.1 Artist\u2019s impression of a collision between planets. A similar collision between Earth and the planet Theia might have given us our Moon. Fortunately for us, the collision that gave us the moon was a glancing blow rather than the direct hit shown here. Earth might not have survived a direct hit.<\/div>\n <\/div>\n

One thing we can say for sure about Earth\u2019s second experiment is that there was effectively no free oxygen (O2<\/sub>, the form of oxygen that we breathe) in the atmosphere. We know this in part because prior to 2 billion years ago, there were no sedimentary beds stained red from oxidized iron minerals. Iron minerals were present, but not in oxidized form. At that time, O2<\/sub> was produced in the atmosphere when the Sun\u2019s ultraviolet rays split water molecules apart; however, chemical reactions removed the oxygen as quickly as it was produced.<\/p>\n

It wasn\u2019t until well into Earth\u2019s third experiment\u2014life\u2014that the atmosphere began to become oxygenated. Photosynthetic organisms used the abundant CO2<\/sub> in the atmosphere to manufacture their food, and released O2<\/sub> as a by-product. At first all of the oxygen was consumed by chemical reactions, but eventually the organisms released so much O2<\/sub> that it overwhelmed the chemical reactions and oxygen began to accumulate in the atmosphere, although present levels of 21% oxygen didn\u2019t occur until about 350 Ma. Today the part of our atmosphere that isn\u2019t oxygen consists largely of nitrogen (78%).<\/p>\n

The oxygen-rich atmosphere on our planet is life\u2019s signature. If geologic process were the only processes controlling our atmosphere, it would consist mostly of carbon dioxide, like the atmosphere of Venus. It is an interesting notion (or a disconcerting one, depending on your point of view) that for the last 2 billion years the light reflected from our planet has been beaming a bar code out to the universe, similar to the ones in Figure 22.1.4, except ours says \u201coxygen.\u201d For 2 billion years, our planet has been sending out a signal that could cause an observer from another world to say, \u201cThat\u2019s odd\u2026 I wonder what\u2019s going on over there.\u201d<\/p>\n

Media Attributions<\/h3>\n