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Archean

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The Archean is the second of Earth's four geologic eons. Its name comes from the Greek word meaning "beginning" or "origin." This eon began approximately 4,031 million years ago. This starting point is defined by the age of the oldest intact rock formations on our planet. The Archean followed the Hadean Eon and preceded the Proterozoic Eon. It represents a fundamental era when the Earth began to form its lasting features.

NASA-EarlyEarth-PaleOrangeDot-20190802
NASA-EarlyEarth-PaleOrangeDot-20190802

During this time, Earth was mostly a water world. There was some continental crust, but much of it sat under oceans deeper than those we have today. The atmosphere was also very different from the air we breathe now. It was a reducing atmosphere, which means it was rich in methane. It lacked free oxygen, which is the gas necessary for most modern life. Because of the methane, the Earth may have appeared as a pale orange dot.

NASA-EarlyEarth-PaleOrangeDot-20190802
NASA-EarlyEarth-PaleOrangeDot-20190802

This hazy atmosphere likely helped keep the planet warm even though the Sun was much dimmer than it is today.

Earth's internal heat was much higher during the Archean. The heat flow was nearly three times as high as it is today. This heat came from several sources. It was partly remnant heat from the formation of the planet. It also came from the formation of the metallic core. Finally, it arose from the decay of radioactive elements.

Evolution of Earth's radiogenic heat
Evolution of Earth's radiogenic heat

This extra heat made the mantle, the layer beneath the crust, much hotter than it is now. This resulted in very high volcanic activity. Some volcanoes erupted unusual types of lava, such as komatiite.

Geology in the Archean was shaped by moving plates. Plate tectonics likely started in the Hadean but slowed down during the Archean. This slowdown may have happened because the mantle became more viscous, or thick, as water moved out of it. These moving plates helped create large amounts of continental crust. However, the deep oceans likely covered most of the continents. It was only toward the end of the Archean that continents began to emerge from the sea. This emergence caused weathering that changed the chemistry of the seawater.

Scientists have found Archean rocks in many places around the world. These include Greenland, Siberia, Canada, Brazil, and Australia. Many of these rocks are granitic, meaning they are made of granite. Other rocks include metamorphosed sediments like mudstones and volcanic rocks. One common formation is called a greenstone belt. These belts consist of alternating layers of different types of rock. They often represent the places where early continents joined together. Archean rocks make up only about 8% of the continental crust we see today. Most of the original Archean crust has been recycled by the Earth's processes.

Life began to emerge during this eon. The earliest evidence of life includes graphite found in 3.7 billion-year-old rocks in Greenland. The most famous fossils from this time are stromatolites.

Lake Thetis-Stromatolites-LaRuth
Lake Thetis-Stromatolites-LaRuth

Stromatolites are microbial mats formed by tiny organisms in shallow water. These organisms were prokaryotes, which are simple, single-celled life forms like bacteria and archaea. They lacked a nucleus, which is a central part of more complex cells. The oldest identifiable stromatolite fossils were found in 3.48 billion-year-old sandstone in Western Australia.

Lake Thetis-Stromatolites-LaRuth
Lake Thetis-Stromatolites-LaRuth

As the Archean progressed, a major change occurred through photosynthesis. Early cyanobacteria began using sunlight to make food. This process released oxygen as a byproduct. While oxygen levels remained very low for most of the eon, these tiny organisms changed the chemistry of the oceans and the atmosphere. This set the stage for the Great Oxygenation Event that followed. Even though asteroid impacts were frequent, life continued to establish itself. These tiny biological processes eventually transformed the entire planet.

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🖼️ Images & Media (3)
File:Evolution of Earth's radiogenic heat.svg
Evolution of Earth's radiogenic heat.svg
File:NASA-EarlyEarth-PaleOrangeDot-20190802.jpg
NASA-EarlyEarth-PaleOrangeDot-20190802.jpg
File:Lake Thetis-Stromatolites-LaRuth.jpg
Lake Thetis-Stromatolites-LaRuth.jpg
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