courses:ast100:5.2
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| + | The initial formation of Earth’s atmosphere and oceans was a direct consequence of the planet’s violent birth and subsequent planetary differentiation during the Hadean Eon. While the surface was once thought to be a hellish landscape of molten rock, the discovery of Hadean zircons—tiny, | ||
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| + | The second stage of evolution was characterized by a planet-wide biological phenomenon where the primordial oceans became a vast, interconnected **laboratory for life**. During this era, much of the global ocean was likely covered by a continuous, slimy film of microorganisms, | ||
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| + | The transition to the third stage began approximately 3.2 billion years ago, marked by the appearance of **stromatolites**—layered sedimentary structures formed by the trapping and binding of mineral grains within the biofilms of cyanobacteria. As indicated by the initial small rise in the dashed line of the geological record, these organisms began performing oxygenic photosynthesis. However, this biological innovation was essentially a suicide mission; the byproduct of their survival was oxygen, a highly reactive and toxic gas to the anaerobic organisms of the time. Like a mirror to modern industrial society’s impact on the global climate, these early cyanobacteria were inadvertently polluting their world with a " | ||
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| + | The fourth stage, occurring approximately 2.3 billion years ago, represents the **Great Oxidation** Event, where oxygen levels rose sharply as the planet’s natural " | ||
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| + | In the final stage, the atmospheric and oceanic systems reached a state of relative equilibrium that permitted the explosion of complex, multicellular biological diversity. Oxygen concentrations eventually stabilized near the modern level of twenty-one percent, fueling the high-energy demands of animals and the eventual conquest of land. The interaction between the biosphere, the hydrosphere, | ||
courses/ast100/5.2.1774166210.txt.gz · Last modified: by asad
