Historical geology

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To be distinguished from History of geology.


Historical geology is a discipline that uses the principles and techniques of geology to reconstruct and understand the geological history of Earth.[1] It focuses on geologic processes that change the Earth's surface and subsurface; and the use of stratigraphy, structural geology and paleontology to tell the sequence of these events. It also focuses on the evolution of plants and animals during different time periods in the geological timescale. The discovery of radioactivity and the development of a variety of radiometric dating techniques in the first half of the 20th century provided a means of deriving absolute versus relative ages of geologic history.

Economic geology, the search for and extraction of energy and raw materials, is heavily dependent on an understanding of the geological history of an area. Environmental geology, including most importantly the geologic hazards of earthquakes and volcanism, must also include a detailed knowledge of geologic history.

Historical development[edit]

Nicolaus Steno, also known as Niels Stensen, was the first to observe and propose some of the basic concepts of historical geology. One of these concepts was that fossils originally came from living organisms. The other, more famous, observations are often grouped together to form the laws of stratigraphy.

James Hutton and Charles Lyell also contributed to early understanding of the Earth's history with their observations at Edinburgh in Scotland concerning angular unconformity in a rock face and it was in fact Lyell that influenced Charles Darwin greatly in his theory of evolution by speculating that the present is the key to the past. Hutton first proposed the theory of uniformitarianism, which is now a basic principle in all branches of geology. Hutton also supported the idea that the Earth was very old as opposed to the prevailing concept of the time which said the Earth had only been around a few millennia. Uniformitarianism describes an Earth created by the same natural phenomena that are at work today.

The prevailing concept of the 18th century in the West was that of a very short Earth history dominated by catastrophic events. This view was strongly supported by adherents of Abrahamic religions based on a largely literal interpretation of their religious scriptural passages. The concept of uniformitarianism met with considerable resistance and the catastrophism vs. gradualism debate of the 19th century resulted. A variety of discoveries in the 20th century provided ample evidence that Earth history is a product of both gradual incremental processes and sudden cataclysmic events. Violent events such as meteorite impacts and large volcanic explosions do shape the Earth's surface along with gradual processes such as weathering, erosion and deposition much as they have throughout Earth history. The present is the key to the past - includes catastrophic as well as gradual processes.

Brief geological history[edit]

Main article: Geologic time scale
Eon Era Period Epochs Start
Phanerozoic Cenozoic Quaternary Holocene 0.0117
Pleistocene 2.558
Neogene Pliocene 5.333*
Miocene 23.030*
Paleogene Oligocene 33.9*
Eocene 56.0*
Paleocene 66.0*
Mesozoic Cretaceous Late Cretaceous 100.5*
Early Cretaceous c. 145.0
Jurassic Late Jurassic 163.5 ± 1.0
Middle Jurassic 174.1 ± 1.0*
Early Jurassic 201.3 ± 0.2*
Triassic Late Triassic c. 235*
Middle Triassic 247.2
Early Triassic 252.2 ± 0.5*
Paleozoic Permian 298.9 ± 0.2*
Carboniferous Pennsylvanian 323.2 ± 0.4*
Mississippian 358.9 ± 0.4*
Devonian 419.2 ± 3.2*
Silurian 443.4 ± 1.5*
Ordovician 485.4 ± 1.9*
Cambrian 541.0 ± 1.0*
Proterozoic Neoproterozoic Ediacaran Precambrian c. 635*
Cryogenian 850
Tonian 1000
Mesoproterozoic Stenian 1200
Ectasian 1400
Calymmian 1600
Paleoproterozoic Statherian 1800
Orosirian 2050
Rhyacian 2300
Siderian 2500
Archean Neoarchean 2800
Mesoarchean 3200
Paleoarchean 3600
Eoarchean 4000
Hadean 4567

See also[edit]


Notes[edit]

  1. ^ Levin, Harold. The Earth through Time, Hoboken, New Jersey: John Wiley & Sons, 2003, p.2