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Earth's Climate History
Climate is not a static set of weather conditions, constant over eons; rather it varies, sometimes in dramatic ways, over time. The hot climate of the newly formed Earth gave way to glaciers in a little more than a billion years, an immense time by human reckoning, but not nearly so long by geological standards. Earth's climate has alternated many times between hot and cold periods of varying magnitudes. Radiation from the sun, the ocean currents, rainfall, wind, continental drift, the concentration of greenhouse gases in the atmosphere, volcanic activity, radioactivity in the Earth's core, the eccentricity of Earth's orbit around the sun, the tilt of Earth's axis, and photosynthesis all affect climate. Climate has myriad causes. Disentangling these causes is not easy, but it is necessary to understanding why climate changes over time. The current climate is warming. The culprit, carbon dioxide, has been increasing in the atmosphere, driving up temperature, and prompting speculation over Earth's future climate.
The interlocking scientific theories of the 19th century—Darwinism and uniformitarianism—implied that climate changed little, and then only gradually. Uniformitarianism holds that the climactic conditions prevailing today are very similar to the conditions that prevailed centuries and even eons ago. Charles Darwin matched his theory of evolution to the dictates of uniformitarianism. Darwin posited that species evolve gradually in response to slow and small changes in the environment. Climate might change, but neither abruptly, nor by a large magnitude. In contrast, the advocates of catastrophism asserted that Earth has been racked by sudden changes. Modern geology has retained the kernel of catastrophism. The climate has changed quickly by geological standards, and by large swings in temperature and precipitation.
Earth's Early Climate
Earth is roughly 4.5 billion years old. Its early climate was the hottest in the planet's long history. Temperatures were hot enough to liquify rock, a circumstance that accounts for the absence of rock from the early geological record. The mass of radioactive elements in Earth's core was the maximum at the origin of Earth. The radioactive elements generated heat and pressure as they decayed, pushing molten rock toward Earth's surface. Volcanoes were active, bringing molten rock to the surface, where they liberated their heat. Volcanoes spewed carbon dioxide (CO2) into the atmosphere, causing the greenhouse effect. Sunlight passed through the atmosphere and struck Earth, which absorbed some sunlight as heat and radiated the rest into space as infrared radiation. Rather than disappearing into space, the infrared radiation was absorbed by CO2, heating the atmosphere. The amount of CO2 in the atmosphere of the newly formed Earth was 1,000 times higher than it is today, more than making up for the fact that the young sun burned with only 70 percent the luminosity of its mature, current phase. At its origin, Earth received only as much sunlight as Mars receives today. The young Earth was too hot for water to liquefy. Instead, the atmosphere held all of Earth's water as vapor. Like CO2, water vapor traps heat in the atmosphere, intensifying the greenhouse effect.
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