Early Earth

Period in Earth's history

Early Earth also known as Proto-Earth is loosely defined as Earth in its first one billion years, or gigayear (Ga, 109 y),[1] from its initial formation in the young Solar System at about 4.55 Ga to some time in the Archean eon in approximately 3.5 Ga.[2] On the geologic time scale, this comprises all of the Hadean eon, starting with the formation of the Earth about 4.6 billion years ago,[3] and the Eoarchean, starting 4 billion years ago, and part of the Paleoarchean era, starting 3.6 billion years ago, of the Archean eon.

This period of Earth's history involved the planet's formation from the solar nebula via a process known as accretion. This time period included intense meteorite bombardment as well as giant impacts, including the Moon-forming impact, which resulted in a series of magma oceans and episodes of core formation.[4] After formation of the core, meteorites or comets may have delivered water and other volatile compounds to the Earth in a "late veneer".[5] Although little crustal material from this period survives, the oldest dated specimen is a zircon mineral of 4.404 ± 0.008 Ga enclosed in a metamorphosed sandstone conglomerate in the Jack Hills of the Narryer Gneiss terrane of Western Australia.[6] The earliest supracrustals (such as the Isua greenstone belt) date from the latter half of this period, about 3.8 Ga, around the same time as peak Late Heavy Bombardment.

## History

[edit]

According to evidence from radiometric dating and other sources, Earth formed about 4.54 billion years ago.[7][8][9] The current dominant theory of planet formation suggests that planets such as Earth form in about 50 to 100 million years but more recently proposed alternative processes and timescales have stimulated ongoing debate in the planetary science community.[10] For example, in June 2023, one team of scientists reported evidence that Earth may have formed in just three million years.[11][10] Nonetheless, within the first billion years of the formation of Earth,[12][13][14][15] life appeared in its oceans and began to affect its atmosphere and surface, promoting the proliferation of aerobic as well as anaerobic organisms. Since then, the combination of Earth's distance from the Sun, its physical properties and its geological history have allowed life to emerge, develop photosynthesis, and, later, evolve further and thrive. The earliest life on Earth arose at least 3.5 billion years ago.[16][17][18] Earlier possible evidence of life includes graphite, which may have a biogenic origin, in 3.7-billion-year-old metasedimentary rocks discovered in southwestern Greenland[19] and 4.1-billion-year-old zircon grains in Western Australia.[20][21]

In November 2020, an international team of scientists reported studies suggesting that the primeval atmosphere of the early Earth was very different from the conditions used in the Miller–Urey studies considering the origin of life on Earth.[22]

* Artist's impression of Archean Earth, showing an orange atmospheric haze, leading to the alternative description of the planet in that stage of its development as a "pale orange dot"[23][24]

## See also

[edit]

* Chronology of the universe – History and future of the universe
* History of life
* Future of Earth – Long-term extrapolated geological and biological changes of planet Earth
* Geological history of Earth
* History of Earth – Overview of Earth's history
* Timeline of the evolutionary history of life
* Timeline of natural history

## References

[edit]

1. ^ Rankama, Kalervo (May 1967). "Megayear and Gigayear: Two Units of Geological Time". Nature. 214 (5088): 634. Bibcode:1967Natur.214..634R. doi:10.1038/214634a0. ISSN 1476-4687.
2. ^ Vaclav Cilek, ed. (2009). "Early Earth". Earth System: History and Natural Variability Volume I. Eolss Publishers. p. 98\. ISBN 978-1-84826-104-4.
3. ^ "International Chronostratigraphic Chart 2015" (PDF). ICS. Retrieved 23 January 2016.
4. ^ Carlson, Richard W.; Garnero, Edward; Harrison, T. Mark; Li, Jie; Manga, Michael; McDonough, William F.; Mukhopadhyay, Sujoy; Romanowicz, Barbara; Rubie, David (2014-01-01). "How Did Early Earth Become Our Modern World?". Annual Review of Earth and Planetary Sciences. 42 (1): 151–178\. Bibcode:2014AREPS..42..151C. doi:10.1146/annurev-earth-060313-055016.
5. ^ Drake, Michael J.; Righter, Kevin (2002-03-07). "Determining the composition of the Earth". Nature. 416 (6876): 39–44\. Bibcode:2002Natur.416...39D. doi:10.1038/416039a. ISSN 0028-0836. PMID 11882886. S2CID 4380038.
6. ^ Wilde, Simon A.; Valley, John W.; Peck, William H.; Graham, Colin M. (2001-01-11). "Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 Gyr ago : Abstract : Nature". Nature. 409 (6817): 175–178\. Bibcode:2001Natur.409..175W. doi:10.1038/35051550. ISSN 0028-0836. PMID 11196637. S2CID 4319774.
7. ^ "Age of the Earth". U.S. Geological Survey. 1997. Archived from the original on 23 December 2005. Retrieved 2006-01-10.
8. ^ Dalrymple, G. Brent (2001). "The age of the Earth in the twentieth century: a problem (mostly) solved". Special Publications, Geological Society of London. 190 (1): 205–221\. Bibcode:2001GSLSP.190..205D. doi:10.1144/GSL.SP.2001.190.01.14. S2CID 130092094.
9. ^ Manhesa, Gérard; Allègre, Claude J.; Dupréa, Bernard & Hamelin, Bruno (1980). "Lead isotope study of basic-ultrabasic layered complexes: Speculations about the age of the earth and primitive mantle characteristics". Earth and Planetary Science Letters. 47 (3): 370–382\. Bibcode:1980E&PSL..47..370M. doi:10.1016/0012-821X(80)90024-2.
10. ^ a b Onyett, Isaac J.; et al. (14 June 2023). "Silicon isotope constraints on terrestrial planet accretion". Nature. 619 (7970): 539–544\. Bibcode:2023Natur.619..539O. doi:10.1038/s41586-023-06135-z. PMC 10356600. PMID 37316662. S2CID 259161680.
11. ^ Patel, Kasha (16 June 2023). "Scientists have a controversial theory for how — and how fast — Earth formed". The Washington Post. Archived from the original on 17 June 2023. Retrieved 17 June 2023.
12. ^ Dalrymple, G.B. (1991). The Age of the Earth. California: Stanford University Press. ISBN 978-0-8047-1569-0.
13. ^ Newman, William L. (2007-07-09). "Age of the Earth". Publications Services, USGS. Retrieved 2007-09-20.
14. ^ Dalrymple, G. Brent (2001). "The age of the Earth in the twentieth century: a problem (mostly) solved". Geological Society, London, Special Publications. 190 (1): 205–21\. Bibcode:2001GSLSP.190..205D. doi:10.1144/GSL.SP.2001.190.01.14. S2CID 130092094. Retrieved 2007-09-20.
15. ^ Stassen, Chris (2005-09-10). "The Age of the Earth". TalkOrigins Archive. Retrieved 2008-12-30.
16. ^ Schopf, JW, Kudryavtsev, AB, Czaja, AD, and Tripathi, AB. (2007). Evidence of Archean life: Stromatolites and microfossils. Precambrian Research 158:141–155.
17. ^ Schopf, JW (2006). Fossil evidence of Archaean life. Philos Trans R Soc Lond B Biol Sci 29;361(1470) 869-85.
18. ^ Hamilton Raven, Peter; Brooks Johnson, George (2002). Biology. McGraw-Hill Education. p. 68. ISBN 978-0-07-112261-0. Retrieved 7 July 2013.
19. ^ Ohtomo, Yoko; Kakegawa, Takeshi; Ishida, Akizumi; et al. (January 2014). "Evidence for biogenic graphite in early Archaean Isua metasedimentary rocks". Nature Geoscience. 7 (1): 25–28\. Bibcode:2014NatGe...7...25O. doi:10.1038/ngeo2025. ISSN 1752-0894.
20. ^ Borenstein, Seth (19 October 2015). "Hints of life on what was thought to be desolate early Earth". Excite. Yonkers, NY: Mindspark Interactive Network. Associated Press. Archived from the original on 2015-10-23. Retrieved 2015-10-20.
21. ^ Bell, Elizabeth A.; Boehnike, Patrick; Harrison, T. Mark; et al. (19 October 2015). "Potentially biogenic carbon preserved in a 4.1 billion-year-old zircon" (PDF). Proc. Natl. Acad. Sci. U.S.A. 112 (47): 14518–21\. Bibcode:2015PNAS..11214518B. doi:10.1073/pnas.1517557112. ISSN 1091-6490. PMC 4664351. PMID 26483481. Retrieved 2015-10-20. Early edition, published online before print.
22. ^ Zurich, Eth (29 November 2020). "Uncovering Mysteries of Earth's Primeval Atmosphere 4.5 Billion Years Ago and the Emergence of Life". Retrieved 30 November 2020.
23. ^ Arney, G. N.; Meadows, V. S.; Domagal-Goldman, S. D.; Claire, M.; Schwieterman, E. (2014). "The Pale Orange Dot: Spectral Effects of a Hazy Early Earth". AGU Fall Meeting Abstracts. 2014. Bibcode:2014AGUFMPP53A1202A.
24. ^ "NASA Team Looks to Ancient Earth First to Study Hazy Exoplanets - NASA". 8 February 2017.

## External links

[edit]

Listen to this article (4 minutes)

This audio file was created from a revision of this article dated 29 December 2024 (2024-12-29), and does not reflect subsequent edits.

(Audio help · More spoken articles)

* Earth – Speed through space – about 1 million miles an hour – NASA and (WP discussion)

* v
* t
* e

Earth science

* Outline
* Index

* Atmospheric science
* Environmental science
* Geodesy
* Geology
* Geophysics
* Glaciology
* Hydrology
* Meteorology
* Oceanography
* Paleogeoscience
* Physical geography
* Soil science
* Volcanology

* Category
* Portal
* Commons

Portals:

* Biology
* Earth sciences

*[v]: View this template
*[t]: Discuss this template
*[e]: Edit this template