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The Greenland sediments include [[banded iron formation|banded iron]] beds. They contain possibly [[organic compound|organic]] [[carbon]] and imply some possibility that [[photosynthesis|photosynthetic]] [[life]] had already emerged at that time. The oldest known [[fossil]]s (from Australia) date from a few hundred million years later.
The Greenland sediments include [[banded iron formation|banded iron]] beds. They contain possibly [[organic compound|organic]] [[carbon]] and imply some possibility that [[photosynthesis|photosynthetic]] [[life]] had already emerged at that time. The oldest known [[fossil]]s (from Australia) date from a few hundred million years later.

No rocks found are from this age, only meteorites and asteroids.


==Atmosphere and oceans==
==Atmosphere and oceans==

Revision as of 21:48, 3 April 2013

Template:Geological eon The Hadean (/[invalid input: 'icon']ˈhdiən/) is the first geologic eon of Earth and lies before the Archean. It began with the formation of the Earth about 4600 million years ago and ended as defined by the ICS 4,031 million years ago.[1] The name "Hadean" derives from Hades, the Greek name for the god of the underworld. The name is in reference to the "hellish" conditions on Earth at the time: the planet had just formed and was still very hot due to high volcanism, a partially molten surface and frequent collisions with other Solar System bodies. The geologist Preston Cloud coined the term in 1972, originally to label the period before the earliest-known rocks on Earth. W. Brian Harland later coined an almost synonymous term: the "Priscoan period". Other, older texts simply refer to the eon as the Pre-Archean.

Subdivisions

Since few geological traces of this period remain on Earth there is no official subdivision. However, the Lunar geologic timescale embraces several major divisions relating to the Hadean and so these are sometimes used in a somewhat informal sense to refer to the same periods of time on Earth.

The Lunar divisions are:

There is a recently proposed alternative scale published in 2010 by Solid Earth, a new open access journal. The article proposes the addition of the Chaotian and Prenephelean Eons preceding it and divides the Hadean into three eras with two periods each. The Paleohadean era consists of the Hephaestean (4.5–4.4 Ga) and the Jacobian periods (4.4–4.3 Ga). The Mesohadean is divided into the Canadian (4.3–4.2 Ga) and the Procrustean periods (4.2–4.1 Ga). The Neohadean is divided into the Acastan (4.1–4.0 Ga) and the Promethean periods (4.0–3.9 Ga).[2]

Hadean rocks

In the last decades of the 20th century geologists identified a few Hadean rocks from Western Greenland, Northwestern Canada, and Western Australia. Rock formations in Greenland comprise sediments dated around 3,800 million years ago and are somewhat altered by a volcanic dike that penetrated the rocks after they were deposited. Individual zircon crystals redeposited in sediments in Western Canada and the Jack Hills region of Western Australia are much older. The oldest dated zircons date from about 4,000 million years ago[3]—very close to the hypothesized time of the Earth's formation.

The Greenland sediments include banded iron beds. They contain possibly organic carbon and imply some possibility that photosynthetic life had already emerged at that time. The oldest known fossils (from Australia) date from a few hundred million years later.

No rocks found are from this age, only meteorites and asteroids.

Atmosphere and oceans

The newly formed Hadean Earth experienced very high temperatures due to extreme volcanism and frequent collisions with other bodies, but eventually began to cool.

A sizeable quantity of water would have been in the material which formed the Earth.[4] Water molecules would have escaped Earth's gravity more easily when it was less massive during its formation. Hydrogen and helium are expected to continually leak from the atmosphere[clarification needed].

Part of the ancient planet is theorized to have been disrupted by the impact that created the Moon, which should have caused melting of one or two large areas. Present composition does not match complete melting and it is hard to completely melt and mix huge rock masses.[5] However, a fair fraction of material should have been vaporized by this impact, creating a rock vapor atmosphere around the young planet. The rock vapor would have condensed within two thousand years, leaving behind hot volatiles which probably resulted in a heavy CO
2
atmosphere with hydrogen and water vapor. Liquid water oceans existed despite the surface temperature of 230 °C (446 °F) because of the atmospheric pressure of the heavy CO
2
atmosphere. As cooling continued, subduction and dissolving in ocean water removed most CO
2
from the atmosphere but levels oscillated wildly as new surface and mantle cycles appeared.[6]

Study of zircons has found that liquid water must have existed as long ago as 4,400 million years ago, very soon after the formation of the Earth.[7][8][9] This requires the presence of an atmosphere. The Cool Early Earth theory covers a range from about 4,400 to 4,000 million years ago.

A September 2008 study of zircons found that Australian Hadean rock holds minerals that point to the existence of plate tectonics as early as 4,000 million years ago.[10][11] If this is true, the time when Earth finished its transition from having a hot, molten surface and atmosphere full of carbon dioxide, to being very much like it is today, can be roughly dated to about 4.0 billion years ago. The action of plate tectonics and the oceans traps vast amounts of carbon dioxide, thereby eliminating the greenhouse effect and leading to a much cooler surface temperature and the formation of solid rock, and possibly even life.[10][11]

See also

References

  1. ^ "International Chronostratigraphic Chart 2012". ICS. Retrieved 6 December 2012.
  2. ^ "The Eons of Chaos and Hades last=Goldblatt" (PDF). Solid Earth. January 26, 2010. {{cite news}}: Missing pipe in: |title= (help)
  3. ^ Wilde et al. (2001).
  4. ^ Drake, Michael J. (2005), "Origin of water in the terrestrial planets" (PDF), Meteoritics & Planetary Science, 40 (4): 515–656, Bibcode:2005M&PS...40..515J, doi:10.1111/j.1945-5100.2005.tb00958.x.
  5. ^ Solar System Exploration: Science & Technology: Science Features: View Feature
  6. ^ Sleep, N. H.; Zahnle, K.; Neuhoff, P. S. (2001), "Initiation of clement surface conditions on the earliest Earth", PNAS, 98 (7): 3666–3672, Bibcode:2001PNAS...98.3666S, doi:10.1073/pnas.071045698, PMC 31109, PMID 11259665.
  7. ^ ANU - Research School of Earth Sciences - ANU College of Science - Harrison
  8. ^ ANU - OVC - MEDIA - MEDIA RELEASES - 2005 - NOVEMBER - 181105HARRISONCONTINENTS
  9. ^ A Cool Early Earth
  10. ^ a b Chang, Kenneth (December 2, 2008). "A New Picture of the Early Earth". The New York Times.
  11. ^ a b Thermal State of the Lithosphere During Late Heavy Bombardment: Implications for Early Life, by Abramov, O. and Mojzsis, S. J.

Further reading

  • Hopkins, Michelle; Harrison, T. Mark; Manning, Craig E. (2008), "Low heat flow inferred from >4 Gyr zircons suggests Hadean plate boundary interactions", Nature, 456 (7221): 493–496, Bibcode:2008Natur.456..493H, doi:10.1038/nature07465, PMID 19037314.
  • Valley, John W.; Peck, William H.; King, Elizabeth M. (1999), "Zircons Are Forever", The Outcrop for 1999, University of Wisconsin-Madison, retrieved January 10, 2006Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago.
  • Wilde, S. A.; Valley, J. W.; Peck, W. H.; Graham, C. M. (2001), "Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago", Nature, 409 (6817): 175–178, doi:10.1038/35051550, PMID 11196637 {{citation}}: Unknown parameter |lastauthoramp= ignored (|name-list-style= suggested) (help).
  • Wyche, S.; Nelson, D. R.; Riganti, A. (2004), "4350–3130 Ma detrital zircons in the Southern Cross Granite–Greenstone Terrane, Western Australia: implications for the early evolution of the Yilgarn Craton", Australian Journal of Earth Sciences, 51 (1): 31–45, doi:10.1046/j.1400-0952.2003.01042.x {{citation}}: Unknown parameter |lastauthoramp= ignored (|name-list-style= suggested) (help).

External links