Eons

  • The Hadean eon (4,540 – 4,000 mya) represents the time before a reliable (fossil) record of life.
  • Temperatures were extremely high, and much of the Earth was molten because of frequent collisionswith other bodies, extreme volcanism  and the abundance of short-lived radioactive elements.
  • A giant impact collision with a planet-sized body named Theia (approximately 4.5 billion years ago) is thought to have formed the Moon.
  • The moon was subjected to Late Heavy Bombardment(LHB – lunar cataclysm – 4 billion years ago).
  • During the LHB phase, a disproportionately large number of asteroids are theorised to have collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars.
  • Volcanic outgassingprobably created the primordial atmosphere and then the ocean.
  • The early atmosphere contained almost no oxygen.
  • Over time, the Earth cooled, causing the formation of a solid crust, leaving behind hot volatiles which probably resulted in a heavy CO2atmosphere with hydrogen and water vapour.
  • Liquid water oceans existed despite the surface temperature of 230° C because, at an atmospheric pressure of above 27 atmospheres, caused by the heavy CO2 atmosphere, water is still liquid.
  • The beginning of lifeon Earth and evidence of cyanobacteria date to 3500 mya.
  • Life was limited to simple single-celled organisms lacking nuclei, called Prokaryota.
  • The atmosphere was without oxygen,and the atmospheric pressure was around 10 to 100 atmospheres.
  • The Earth’s crust had cooled enough to allow the formation of continents.
  • The oldest rock formations exposed on the surface of the Earth are Archean.
  • Volcanic activity was considerably higher than today, with numerous lava eruptions.
  • The oceans were more acidicdue to dissolved carbon dioxide than during the Proterozoic.
  • By the end of the Archaean, plate tectonicsmay have been similar to that of the modern Earth.
  • Liquid water was prevalent, and deep oceanic basins are known to have existed.
  • The earliest stromatolites are found in 3.48 billion-year-old sandstone discovered in Western Australia.
  • The earliest identifiable fossilsconsist of stromatolites, which are microbial mats formed in shallow water by cyanobacteria.
  • It is the last eon of the Precambrian “supereon”.
  • It spans for the time of appearance of oxygenin Earth’s atmosphere to just before the proliferation of complex life (such as corals) on the Earth.
  • Bacteriabegin producing oxygen, leading to the sudden rise of life forms.
  • Eukaryotes (have a nucleus), emerge, including some forms of soft-bodied multicellular 
  • Earlier forms of fungi formed around this time.
  • The early and late phases of this eon may have undergone Snowball Earthperiods (the planet suffered below-zero temperatures, extensive glaciation and as a result drop in sea levels).
  • It was a very tectonically activeperiod in the Earth’s history.
  • It featured the first definitive supercontinent cycles and modern orogeny (mountain building).
  • It is believed that 43% of modern continental crust was formed in the Proterozoic, 39% formed in the Archean, and only 18% in the Phanerozoic.
  • In the late Proterozoic (most recent), the dominant supercontinent was Rodinia (~1000–750 Ma).

The Timescale Division

  • Started about 541 million years ago and continues to the present is known as the Phanerozoic Eon.
  • This eon can be divided into 3 Eras.
  • These 3 eras are the Paleozoic, Mesozoic, and Cenozoic.
  • Each of these Eras can be subdivided even further into Periods.

    Phanerozoic Eon

 

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