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Earth's crust
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<h2 id="composition">Composition</h2> <p class="note">Main articles: <a href="/facts/Abundance_of_elements_in_Earth%2527s_crust/UDSVHH56">Abundance of elements in Earth's crust</a> and <a href="/facts/Goldschmidt_classification/8p9CWrpe">Goldschmidt classification</a></p> <p>The crust of Earth is of two distinct types: </p> <ol><li><a href="/facts/Continental_crust/cGnK3oEr">Continental</a>: 25–70km ( about 15–44 mi) thick and mostly composed of less dense, more <a href="/facts/Felsic/0jpm1eSA">felsic</a> rocks, such as <a href="/facts/Granite/G2evuVKo">granite</a>. In a few places, such as the <a href="/facts/Tibetan_Plateau/6qkLjmCg">Tibetan Plateau</a>, the <a href="/facts/Altiplano/Eq1pASWK">Altiplano</a>, and the eastern <a href="/facts/Baltic_Shield/Um1CVxsI">Baltic Shield</a>, the continental crust is thicker (50 – 80 km (30 – 50 mi)).</li> <li><a href="/facts/Oceanic_crust/0lGjI7jN">Oceanic</a>: 5 – 10 km (3 – 6 mi) thick<a class="footnote-ref" id="fnref:4" href="#fn:4"><sup>4</sup></a> and composed primarily of denser, more <a href="/facts/Mafic/mVL7Ahuw">mafic</a> rocks, such as <a href="/facts/Basalt/uhbwGPTb">basalt</a>, <a href="/facts/Diabase/7XK2Sf8g">diabase</a>, and <a href="/facts/Gabbro/79gTqpyg">gabbro</a>.</li></ol> <p>The average thickness of the crust is about 15 – 20 km (9 – 12 mi).<a class="footnote-ref" id="fnref:5" href="#fn:5"><sup>5</sup></a> </p><p>Because both the continental and oceanic crust are less dense than the mantle below, both types of crust "float" on the mantle. The surface of the continental crust is significantly higher than the surface of the oceanic crust, due to the greater buoyancy of the thicker, less dense continental crust (an example of <a href="/facts/Isostasy/GaRMFQNP">isostasy</a>). As a result, the continents form high ground surrounded by deep ocean basins.<a class="footnote-ref" id="fnref:6" href="#fn:6"><sup>6</sup></a> </p><p>The continental crust has an average composition similar to that of <a href="/facts/Andesite/AMVbAGJ0">andesite</a>,<a class="footnote-ref" id="fnref:7" href="#fn:7"><sup>7</sup></a> though the composition is not uniform, with the upper crust averaging a more felsic composition similar to that of <a href="/facts/Dacite/Cd4vGJlI">dacite</a>, while the lower crust averages a more mafic composition resembling basalt.<a class="footnote-ref" id="fnref:8" href="#fn:8"><sup>8</sup></a> The most abundant <a href="/facts/Mineral/LkUFbNmv">minerals</a> in <a href="/facts/Earth/HLLmDfj0">Earth</a>'s <a href="/facts/Continental_crust/cGnK3oEr">continental crust</a> are <a href="/facts/Feldspar/DVvFnfA9">feldspars</a>, which make up about 41% of the crust by weight, followed by <a href="/facts/Quartz/4n86tE2G">quartz</a> at 12%, and <a href="/facts/Pyroxene/hWMTLF9o">pyroxenes</a> at 11%.<a class="footnote-ref" id="fnref:9" href="#fn:9"><sup>9</sup></a> </p> <table><tbody><tr><th scope="col" rowspan="1.5">Most Abundant Elements of Earth's Crust</th><th scope="col" colspan="1.5">Approximate % by weight<a class="footnote-ref" id="fnref:10" href="#fn:10"><sup>10</sup></a></th><th>Oxide</th><th>Approximate % oxide by weight</th></tr><tr><td>O</td><td>46.1</td><td></td><td></td></tr><tr><td>Si</td><td>28.2</td><td><a href="/facts/Quartz/4n86tE2G">SiO2</a></td><td>60.6</td></tr><tr><td>Al</td><td>8.23</td><td><a href="/facts/Corundum/B7RRbcaE">Al2O3</a></td><td>15.9</td></tr><tr><td>Fe</td><td>5.63</td><td><a href="/facts/Iron_(element)/QK1JYy8E">Fe</a> as <a href="/facts/FeO/H9V7S3MG">FeO</a></td><td>6.7</td></tr><tr><td>Ca</td><td>4.15</td><td><a href="/facts/Calcium_oxide/Wh9C8l7j">CaO</a></td><td>6.4</td></tr><tr><td>Na</td><td>2.36</td><td><a href="/facts/Sodium_oxide/QbdIGb8u">Na2O</a></td><td>3.1</td></tr><tr><td>Mg</td><td>2.33</td><td><a href="/facts/Magnesium_oxide/0GfLn47t">MgO</a></td><td>1.8</td></tr><tr><td>K</td><td>2.09</td><td><a href="/facts/Potassium_oxide/mmUVvPef">K2O</a></td><td>4.7</td></tr><tr><td>Ti</td><td>0.565</td><td><a href="/facts/Titanium_dioxide/T0KWmKcz">TiO2</a></td><td>0.7</td></tr><tr><td>H</td><td>0.14</td><td></td><td></td></tr><tr><td>P</td><td>0.105</td><td><a href="/facts/Phosphorus_pentoxide/GKTSUNqS">P2O5</a></td><td>0.1</td></tr></tbody></table> <p>All the other constituents except water occur only in very small quantities and total less than 1%.<a class="footnote-ref" id="fnref:11" href="#fn:11"><sup>11</sup></a> </p><p>Continental crust is enriched in <a href="/facts/Incompatible_element/RqEMlFUu">incompatible elements</a> compared to the <a href="/facts/Basalt/uhbwGPTb">basaltic</a> ocean crust and much enriched compared to the underlying mantle. The most incompatible elements are enriched by a factor of 50 to 100 in the continental crust relative to primitive mantle rock, while oceanic crust is enriched with incompatible elements by a factor of about 10.<a class="footnote-ref" id="fnref:12" href="#fn:12"><sup>12</sup></a> </p><p>The estimated average density of the continental crust is 2.835 g/cm3, with density increasing with depth from an average of 2.66 g/cm3 in the uppermost crust to 3.1 g/cm3 at the base of the crust.<a class="footnote-ref" id="fnref:13" href="#fn:13"><sup>13</sup></a> </p><p>In contrast to the continental crust, the oceanic crust is composed predominantly of pillow lava and sheeted dikes with the composition of <a href="/facts/Mid-ocean_ridge/wYdgdSW3">mid-ocean ridge</a> basalt, with a thin upper layer of sediments and a lower layer of <a href="/facts/Gabbro/79gTqpyg">gabbro</a>.<a class="footnote-ref" id="fnref:14" href="#fn:14"><sup>14</sup></a> </p> <h2 id="formation-and-evolution">Formation and evolution</h2> <p class="note">Main article: <a href="/facts/Earth%2527s_crustal_evolution/zy8RAujn">Earth's crustal evolution</a></p> <p class="note">Further information: <a href="/facts/Earth/HLLmDfj0">Earth § Formation</a></p> <p>Earth formed approximately 4.6 billion years ago from a disk of dust and gas orbiting the newly formed Sun. It formed via accretion, where <a href="/facts/Planetesimal/PK60dofs">planetesimals</a> and other smaller rocky bodies collided and stuck, gradually growing into a planet. This process generated an enormous amount of heat, which caused early Earth to melt completely. As planetary accretion slowed, Earth began to cool, forming its first crust, called a primary or primordial crust.<a class="footnote-ref" id="fnref:15" href="#fn:15"><sup>15</sup></a> This crust was likely repeatedly destroyed by large impacts, then reformed from the <a href="/facts/Magma/hRotHju9">magma</a> ocean left by the impact. None of Earth's primary crust has survived to today; all was destroyed by <a href="/facts/Erosion/gaGJXy0W">erosion</a>, impacts, and <a href="/facts/Plate_tectonics/RtRG5lY4">plate tectonics</a> over the past several billion years.<a class="footnote-ref" id="fnref:16" href="#fn:16"><sup>16</sup></a> </p><p>Since then, Earth has been forming a secondary and tertiary crust, which correspond to oceanic and continental crust, respectively. Secondary crust forms at mid-ocean <a href="/facts/Spreading_centers/wYdgdSW3">spreading centers</a>, where partial-melting of the underlying <a href="/facts/Mantle_(geology)/RpDdtjCr">mantle</a> yields <a href="/facts/Basalt/uhbwGPTb">basaltic</a> magmas and new ocean crust forms. This "ridge push" is one of the driving forces of plate tectonics, and it is constantly creating new ocean crust. Consequently, old crust must be destroyed, so opposite a spreading center, there is usually a subduction zone: a trench where an ocean plate is sinking back into the mantle. This constant process of creating a new ocean crust and destroying the old ocean crust means that the oldest ocean crust on Earth today is only about 200 million years old.<a class="footnote-ref" id="fnref:17" href="#fn:17"><sup>17</sup></a> </p><p>In contrast, the bulk of the continental crust is much older. The oldest continental crustal rocks on Earth have ages in the range from about 3.7 to 4.28 billion years <a class="footnote-ref" id="fnref:18" href="#fn:18"><sup>18</sup></a><a class="footnote-ref" id="fnref:19" href="#fn:19"><sup>19</sup></a> and have been found in the <a href="/facts/Narryer_Gneiss_terrane/eNCgCpND">Narryer Gneiss terrane</a> in <a href="/facts/Western_Australia/1ouCbwNh">Western Australia</a>, in the <a href="/facts/Acasta_Gneiss/oAcze9EC">Acasta Gneiss</a> in the <a href="/facts/Northwest_Territories/au0ajf7T">Northwest Territories</a> on the <a href="/facts/Canadian_Shield/TklzY7Ln">Canadian Shield</a>, and on other <a href="/facts/Craton/fSuY37IC">cratonic</a> regions such as those on the <a href="/facts/Fennoscandian_Shield/Um1CVxsI">Fennoscandian Shield</a>. Some <a href="/facts/Zircon/84APfbLt">zircon</a> with age as great as 4.3 billion years has been found in the <a href="/facts/Narryer_Gneiss_terrane/eNCgCpND">Narryer Gneiss terrane</a>. Continental crust is a tertiary crust, formed at subduction zones through recycling of subducted secondary (oceanic) crust.<a class="footnote-ref" id="fnref:20" href="#fn:20"><sup>20</sup></a> </p><p>The average age of Earth's current continental crust has been estimated to be about 2.0 billion years.<a class="footnote-ref" id="fnref:21" href="#fn:21"><sup>21</sup></a> Most crustal rocks formed before 2.5 billion years ago are located in <a href="/facts/Craton/fSuY37IC">cratons</a>. Such an old continental crust and the underlying mantle <a href="/facts/Asthenosphere/lXpE97oP">asthenosphere</a> are less dense than elsewhere on Earth and so are not readily destroyed by subduction. Formation of new continental crust is linked to periods of intense <a href="/facts/Orogeny/XrvRMpsw">orogeny</a>, which coincide with the formation of the <a href="/facts/Supercontinent/amID2KQp">supercontinents</a> such as <a href="/facts/Rodinia/oBjuSeet">Rodinia</a>, <a href="/facts/Pangaea/VGruHKJj">Pangaea</a> and <a href="/facts/Gondwana/zqbAvsnY">Gondwana</a>. The crust forms in part by aggregation of <a href="/facts/Island_arc/J7FIJPmy">island arcs</a> including granite and metamorphic fold belts, and it is preserved in part by depletion of the underlying mantle to form buoyant <a href="/facts/Lithosphere/1mqaxASd">lithospheric</a> mantle. Crustal movement on continents may result in earthquakes, while movement under the seabed can lead to tidal waves. </p> <h2 id="see-also">See also</h2> <ul> <li>Earth sciences portal</li><li>World portal</li></ul> <ul><li><a href="/facts/Brittle%25E2%2580%2593ductile_transition_zone/JKPVP0J4">Brittle–ductile transition zone</a></li> <li><a href="/facts/Internal_structure_of_Earth/678dYXU7">Internal structure of Earth</a></li></ul> <h2 id="external-links">External links</h2> The Wikibook <i>Historical Geology</i> has a page on the topic of: <i>Structure of the Earth</i> <ul><li><a href="https://en.wikisource.org/wiki/The_Encyclopedia_Americana_(1920)/Crust_of_the_Earth">"Crust of the Earth" </a>. <i><a href="/facts/Encyclopedia_Americana/rsmEnQT5">Encyclopedia Americana</a></i>. 1920.</li></ul> <h2 id="references">References</h2> <ol> <li id="fn:1"><p>Robinson, Eugene C. (January 14, 2011). "The Interior of the Earth". U.S. Geological Survey. Retrieved August 30, 2013. <a href="https://pubs.usgs.gov/gip/interior/" target="_blank">https://pubs.usgs.gov/gip/interior/</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></p></li> <li id="fn:2"><p>Peele, Robert (1911). "Boring" . In Chisholm, Hugh (ed.). Encyclopædia Britannica. Vol. 4 (11th ed.). Cambridge University Press. p. 251. <a href="https://en.wikisource.org/wiki/1911_Encyclop%C3%A6dia_Britannica/Boring" target="_blank">https://en.wikisource.org/wiki/1911_Encyclop%C3%A6dia_Britannica/Boring</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></p></li> <li id="fn:3"><p>Philpotts, Anthony R.; Ague, Jay J. (2009). Principles of igneous and metamorphic petrology (2nd ed.). Cambridge, UK: Cambridge University Press. p. 14. ISBN 978-0-521-88006-0. <a href="978-0-521-88006-0" target="_blank">978-0-521-88006-0</a> <a href="#fnref:3" class="footnote-back-ref">↩</a></p></li> <li id="fn:4"><p>Structure of the Earth. The Encyclopedia of Earth. March 3, 2010 <a href="http://www.eoearth.org/article/Structure_of_the_Earth" target="_blank">http://www.eoearth.org/article/Structure_of_the_Earth</a> <a href="#fnref:4" class="footnote-back-ref">↩</a></p></li> <li id="fn:5"><p>US Geological Survey (5 May 1999) Earth's Crust <a href="https://pubs.usgs.gov/gip/dynamic/inside.html" target="_blank">https://pubs.usgs.gov/gip/dynamic/inside.html</a> <a href="#fnref:5" class="footnote-back-ref">↩</a></p></li> <li id="fn:6"><p>Levin, Harold L. (2010). The Earth through time (9th ed.). Hoboken, N.J.: J. Wiley. pp. 173–174. ISBN 978-0-470-38774-0. <a href="978-0-470-38774-0" target="_blank">978-0-470-38774-0</a> <a href="#fnref:6" class="footnote-back-ref">↩</a></p></li> <li id="fn:7"><p>R. L. Rudnick and S. Gao, 2003, Composition of the Continental Crust. In The Crust (ed. R. L. Rudnick) volume 3, pp. 1–64 of Treatise on Geochemistry (eds. H. D. Holland and K. K. Turekian), Elsevier-Pergamon, Oxford ISBN 0-08-043751-6 <a href="/wiki/ISBN_(identifier)" target="_blank">/wiki/ISBN_(identifier)</a> <a href="#fnref:7" class="footnote-back-ref">↩</a></p></li> <li id="fn:8"><p>Philpotts & Ague 2009, p. 2. - Philpotts, Anthony R.; Ague, Jay J. (2009). Principles of igneous and metamorphic petrology (2nd ed.). Cambridge, UK: Cambridge University Press. p. 14. ISBN 978-0-521-88006-0. <a href="#fnref:8" class="footnote-back-ref">↩</a></p></li> <li id="fn:9"><p>Anderson, Robert S.; Anderson, Suzanne P. (2010). Geomorphology: The Mechanics and Chemistry of Landscapes. Cambridge University Press. p. 187. ISBN 978-1-139-78870-0. <a href="978-1-139-78870-0" target="_blank">978-1-139-78870-0</a> <a href="#fnref:9" class="footnote-back-ref">↩</a></p></li> <li id="fn:10"><p>ABUNDANCE OF ELEMENTS IN THE EARTH’S CRUST AND IN THE SEA, CRC Handbook of Chemistry and Physics, 97th edition (2016–2017), p. 14–17 <a href="#fnref:10" class="footnote-back-ref">↩</a></p></li> <li id="fn:11"><p>Klein, Cornelis; Hurlbut, Cornelius S. Jr. (1993). Manual of mineralogy : (after James D. Dana) (21st ed.). New York: Wiley. pp. 221–224. ISBN 0-471-57452-X. <a href="0-471-57452-X" target="_blank">0-471-57452-X</a> <a href="#fnref:11" class="footnote-back-ref">↩</a></p></li> <li id="fn:12"><p>Hofmann, Albrecht W. (November 1988). "Chemical differentiation of the Earth: the relationship between mantle, continental crust, and oceanic crust". Earth and Planetary Science Letters. 90 (3): 297–314. Bibcode:1988E&PSL..90..297H. CiteSeerX 10.1.1.464.5698. doi:10.1016/0012-821X(88)90132-X. S2CID 3211879. <a href="/wiki/Bibcode_(identifier)" target="_blank">/wiki/Bibcode_(identifier)</a> <a href="#fnref:12" class="footnote-back-ref">↩</a></p></li> <li id="fn:13"><p>Christensen, Nikolas I.; Mooney, Walter D. (June 10, 1995). "Seismic velocity structure and composition of the continental crust: A global view". Journal of Geophysical Research: Solid Earth. 100 (B6): 9761–9788. Bibcode:1995JGR...100.9761C. doi:10.1029/95JB00259. <a href="/wiki/Bibcode_(identifier)" target="_blank">/wiki/Bibcode_(identifier)</a> <a href="#fnref:13" class="footnote-back-ref">↩</a></p></li> <li id="fn:14"><p>Philpotts & Ague 2009, pp. 370–371. - Philpotts, Anthony R.; Ague, Jay J. (2009). Principles of igneous and metamorphic petrology (2nd ed.). Cambridge, UK: Cambridge University Press. p. 14. ISBN 978-0-521-88006-0. <a href="#fnref:14" class="footnote-back-ref">↩</a></p></li> <li id="fn:15"><p>Erickson, Jon (2014). Historical Geology: Understanding Our Planet's Past. Infobase Publishing. p. 8. ISBN 978-1-4381-0964-0. Retrieved September 28, 2017. <a href="978-1-4381-0964-0" target="_blank">978-1-4381-0964-0</a> <a href="#fnref:15" class="footnote-back-ref">↩</a></p></li> <li id="fn:16"><p>Taylor, S. Ross; McLennan, Scott M. (1996). "The Evolution of Continental Crust". Scientific American. 274 (1): 76–81. Bibcode:1996SciAm.274a..76T. doi:10.1038/scientificamerican0196-76. JSTOR 24989358. <a href="/wiki/Bibcode_(identifier)" target="_blank">/wiki/Bibcode_(identifier)</a> <a href="#fnref:16" class="footnote-back-ref">↩</a></p></li> <li id="fn:17"><p>Taylor & McLennan 1996. - Taylor, S. Ross; McLennan, Scott M. (1996). "The Evolution of Continental Crust". Scientific American. 274 (1): 76–81. Bibcode:1996SciAm.274a..76T. doi:10.1038/scientificamerican0196-76. JSTOR 24989358. <a href="https://ui.adsabs.harvard.edu/abs/1996SciAm.274a..76T" target="_blank">https://ui.adsabs.harvard.edu/abs/1996SciAm.274a..76T</a> <a href="#fnref:17" class="footnote-back-ref">↩</a></p></li> <li id="fn:18"><p>"Team finds Earth's 'oldest rocks'". BBC News. September 26, 2008. Retrieved March 27, 2010. <a href="http://news.bbc.co.uk/1/hi/sci/tech/7639024.stm" target="_blank">http://news.bbc.co.uk/1/hi/sci/tech/7639024.stm</a> <a href="#fnref:18" class="footnote-back-ref">↩</a></p></li> <li id="fn:19"><p>P. J. Patchett and S. D. Samson, 2003, Ages and Growth of the Continental Crust from Radiogenic Isotopes. In The Crust (ed. R. L. Rudnick) volume 3, pp. 321–348 of Treatise on Geochemistry (eds. H. D. Holland and K. K. Turekian), Elsevier-Pergamon, Oxford ISBN 0-08-043751-6 <a href="/wiki/ISBN_(identifier)" target="_blank">/wiki/ISBN_(identifier)</a> <a href="#fnref:19" class="footnote-back-ref">↩</a></p></li> <li id="fn:20"><p>Taylor & McLennan 1996. - Taylor, S. Ross; McLennan, Scott M. (1996). "The Evolution of Continental Crust". Scientific American. 274 (1): 76–81. Bibcode:1996SciAm.274a..76T. doi:10.1038/scientificamerican0196-76. JSTOR 24989358. <a href="https://ui.adsabs.harvard.edu/abs/1996SciAm.274a..76T" target="_blank">https://ui.adsabs.harvard.edu/abs/1996SciAm.274a..76T</a> <a href="#fnref:20" class="footnote-back-ref">↩</a></p></li> <li id="fn:21"><p>A. I. S. Kemp and C. J. Hawkesworth, 2003, Granitic Perspectives on the Generation and Secular Evolution of the Continental Crust. In The Crust (ed. R. L. Rudnick) volume 3, pp. 349–410 of Treatise on Geochemistry (eds. H. D. Holland and K. K. Turekian), Elsevier-Pergamon, Oxford ISBN 0-08-043751-6 <a href="/wiki/ISBN_(identifier)" target="_blank">/wiki/ISBN_(identifier)</a> <a href="#fnref:21" class="footnote-back-ref">↩</a></p></li> </ol>