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Although the deep carbon cycle is not as well-understood as carbon movement through the atmosphere, terrestrial biosphere, ocean, and geosphere, it is nonetheless an incredibly important process. The deep carbon cycle is intimately connected to the movement of carbon in the Earth's surface and atmosphere. If the process did not exist, carbon would remain in the atmosphere, where it would accumulate to extremely high levels over long periods of time.^[1] Therefore, by allowing carbon to return to the Earth, the deep carbon cycle plays a critical role in maintaining the terrestrial conditions necessary for life to exist.

Furthermore, the process is also significant simply due to the massive quantities of carbon it transports through the planet. In fact, studying the composition of basaltic magma and measuring carbon dioxide flux out of volcanoes reveals that the amount of carbon in the mantle is actually greater than that on the Earth's surface by a factor of one thousand.^[2] Drilling down and physically observing deep Earth carbon processes is evidently extremely difficult, as the lower mantle and core extend from 660 to 2,891 km and 2,891 km to 6,371 deep into the Earth respectively. Accordingly, not much is conclusively known regarding the role of carbon in the deep Earth. Nonetheless, several pieces of evidence—many of which come from laboratory simulations of deep Earth conditions—have indicated mechanisms for the element's movement down into the lower mantle, as well as the forms that carbon takes at the extreme temperatures and pressures of said layer. Furthermore, techniques like seismology have led to greater understanding of the potential presence of carbon in the Earth's core.

Lower mantle

Carbon principally enters the mantle in the form of carbonate-rich sediments on tectonic plates of ocean crust, which pull the carbon into the mantle upon undergoing subduction. Not much is known about carbon circulation in the mantle, especially in the deep Earth, but many studies have attempted to augment our understanding of the element's movement and forms within said region. For instance, a 2011 study demonstrated that carbon cycling extends all the way to the lower mantle. The study analysed rare, super-deep diamonds at a site in Juina, Brazil, determining that the bulk composition of some of the diamonds' inclusions matched the expected result of basalt melting and crytallisation under lower mantle temperatures and pressures.^[3] Thus, the investigation's findings indicate that pieces of basaltic oceanic lithosphere act as the principle transport mechanism for carbon to Earth's deep interior. These subducted carbonates can interact with lower mantle silicates and metals, eventually forming super-deep diamonds like the one found.^[4]

However, carbonates descending to the lower mantle encounter other fates in addition to forming diamonds. In 2011, carbonates were subjected to an environment similar to that of 1800 km deep into the Earth, well within the lower mantle. Doing so resulted in the formations of magnesite, siderite, and numerous varieties of graphite.^[5] Other experiments—as well as petrologic observations—support this claim, finding that magnesite is actually the most stable carbonate phase in the majority of the mantle. This is largely a result of its higher melting temperature.^[6] Consequently, scientists have concluded that carbonates undergo reduction as they descend into the mantle before being stabilised at depth by low fugacity oxygen fugacity environments. Magnesium, iron, and other metallic compounds act as buffers throughout the process.^[7] The presence of reduced, elemental forms of carbon like graphite would indicate that carbon compounds are reduced as they descend into the mantle.

Nonetheless, it is noteworthy that polymorphism alters carbonate compounds' stability at different depths within the Earth. To illustrate, laboratory simulations and density functional theory calculations suggest that tetrahedrally-coordinated carbonates are most stable at depths approaching the Core-Mantle Boundary.^[8]^[9] A 2015 study indicates that the lower mantle's high pressures cause carbon bonds to transition from sp₂ to sp₃ hybridised orbitals, resulting in carbon tetrahedrally bonding to oxygen.^[10] CO₃ trigonal groups cannot form polymerisable networks, while tetrahedral CO₄ can, signifying an increase in carbon's coordination number, and therefore drastic changes in carbonate compounds' properties in the lower mantle. As an example, preliminary theoretical studies suggest that high pressures cause carbonate melt viscosity to increase; the melts' lower mobility as a result of the property changes described is evidence for large deposits of carbon deep into the mantle.^[11]

Accordingly, carbon can remain in the lower mantle for long periods of time, but large concentrations of carbon frequently find their way back to the lithosphere. This process, called carbon outgassing, is the result of carbonated mantle undergoing decompression melting, as well as mantle plumes carrying carbon compounds up towards the crust.^[13] Carbon is oxidised upon its ascent towards volcanic hotspots, where it is then released as CO₂. This occurs so that the carbon atom matches the oxidation state of the basalts erupting in such areas.^[14]

Core

Although the presence of carbon in the Earth's core is well-constrained, recent studies suggest large inventories of carbon could be stored in this region. Shear (S) waves moving through the inner core travel at about fifty percent of the velocity expected for most iron-rich alloys.^[15] Considering the core's composition is widely believed to be an alloy of crystalline iron with a small amount of nickle, this seismographic anomaly points to another substance's existence within the region. One theory postulates that such a phenomena is the result of various light elements, including carbon, in the core.^[16] In fact, studies have utilised diamond anvil cells to replicate the conditions in the Earth's core, the results of which indicate that iron carbide (Fe₇C₃) matches the inner core's sound and density velocities considering its temperature and pressure profile. Hence, the iron carbide model could serve as evidence that the core holds as much as 67% of the Earth's carbon.^[17] Furthermore, another study found that carbon dissolved in iron and formed a stable phase with the same Fe₇C₃ composition—albeit with a different structure than the one previously mentioned.^[18] Hence, although the amount of carbon potentially stored in the Earth's core is not known, recent research indicates that the presence of iron carbides could be consistent with geophysical observations.

References

^ "The Deep Carbon Cycle and our Habitable Planet | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-02-19.
^ Wilson, Mark (2003). "Where do Carbon Atoms Reside within Earth's Mantle?". Physics Today. 56 (10): 21–22. Bibcode:2003PhT....56j..21W. doi:10.1063/1.1628990.
^ "Carbon cycle reaches Earth's lower mantle: Evidence of carbon cycle found in 'superdeep' diamonds From Brazil". ScienceDaily. Retrieved 2019-02-06.
^ Stagno, V.; Frost, D. J.; McCammon, C. A.; Mohseni, H.; Fei, Y. (2015-02-05). "The oxygen fugacity at which graphite or diamond forms from carbonate-bearing melts in eclogitic rocks". Contributions to Mineralogy and Petrology. 169 (2): 16. doi:10.1007/s00410-015-1111-1. ISSN 1432-0967.
^ Fiquet, Guillaume; Guyot, François; Perrillat, Jean-Philippe; Auzende, Anne-Line; Antonangeli, Daniele; Corgne, Alexandre; Gloter, Alexandre; Boulard, Eglantine (2011-03-29). "New host for carbon in the deep Earth". Proceedings of the National Academy of Sciences. 108 (13): 5184–5187. doi:10.1073/pnas.1016934108. ISSN 0027-8424. PMID 21402927.
^ Dorfman, Susannah M.; Badro, James; Nabiei, Farhang; Prakapenka, Vitali B.; Cantoni, Marco; Gillet, Philippe (2018-05-01). "Carbonate stability in the reduced lower mantle". Earth and Planetary Science Letters. 489: 84–91. doi:10.1016/j.epsl.2018.02.035. ISSN 0012-821X.
^ Kelley, Katherine A.; Cottrell, Elizabeth (2013-06-14). "Redox Heterogeneity in Mid-Ocean Ridge Basalts as a Function of Mantle Source". Science. 340 (6138): 1314–1317. doi:10.1126/science.1233299. ISSN 0036-8075. PMID 23641060.
^ Kono, Yoshio (2018). "Magmas Under Pressure: Advances in High-Pressure Experiments on Structure and Properties of Melts" (PDF). www.sciencedirect.com. Retrieved 2019-02-07. {{cite web}}: Cite has empty unknown parameter: |dead-url= (help)
^ Fiquet, Guillaume; Guyot, François; Perrillat, Jean-Philippe; Auzende, Anne-Line; Antonangeli, Daniele; Corgne, Alexandre; Gloter, Alexandre; Boulard, Eglantine (2011-03-29). "New host for carbon in the deep Earth". Proceedings of the National Academy of Sciences. 108 (13): 5184–5187. doi:10.1073/pnas.1016934108. ISSN 0027-8424. PMID 21402927.
^ Mao, Wendy L.; Liu, Zhenxian; Galli, Giulia; Pan, Ding; Boulard, Eglantine (2015-02-18). "Tetrahedrally coordinated carbonates in Earth's lower mantle". Nature Communications. 6: 6311. doi:10.1038/ncomms7311. ISSN 2041-1723.
^ Carmody, Laura; Genge, Matthew; Jones, Adrian P. (2013-01-01). "Carbonate Melts and Carbonatites". Reviews in Mineralogy and Geochemistry. 75 (1): 289–322. doi:10.2138/rmg.2013.75.10. ISSN 1529-6466.
^ Dasgupta, Rajdeep (December 10, 2011). "From Magma Ocean to Crustal Recycling: Earth's Deep Carbon Cycle". {{cite web}}: Cite has empty unknown parameter: |dead-url= (help)
^ Dasgupta, Rajdeep; Hirschmann, Marc M. (2010-09-15). "The deep carbon cycle and melting in Earth's interior". Earth and Planetary Science Letters. 298 (1): 1–13. doi:10.1016/j.epsl.2010.06.039. ISSN 0012-821X.
^ "Shibboleth Authentication Request". login.stanford.idm.oclc.org. doi:10.1146/annurev.earth.36.031207.124322. Retrieved 2019-02-07.
^ "Does Earth's Core Host a Deep Carbon Reservoir? | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-03-09.
^ "Does Earth's Core Host a Deep Carbon Reservoir? | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-02-05.
^ Li, Jie; Chow, Paul; Xiao, Yuming; Alp, E. Ercan; Bi, Wenli; Zhao, Jiyong; Hu, Michael Y.; Liu, Jiachao; Zhang, Dongzhou (2014-12-16). "Hidden carbon in Earth's inner core revealed by shear softening in dense Fe7C3". Proceedings of the National Academy of Sciences. 111 (50): 17755–17758. doi:10.1073/pnas.1411154111. ISSN 0027-8424. PMID 25453077.
^ Hanfland, M.; Chumakov, A.; Rüffer, R.; Prakapenka, V.; Dubrovinskaia, N.; Cerantola, V.; Sinmyo, R.; Miyajima, N.; Nakajima, Y. (March 2015). "High Poisson's ratio of Earth's inner core explained by carbon alloying". Nature Geoscience. 8 (3): 220–223. doi:10.1038/ngeo2370. ISSN 1752-0908.

[1] "The Deep Carbon Cycle and our Habitable Planet | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-02-19.

[:02-2] Wilson, Mark (2003). "Where do Carbon Atoms Reside within Earth's Mantle?". Physics Today. 56 (10): 21–22. Bibcode:2003PhT....56j..21W. doi:10.1063/1.1628990.

[3] "Carbon cycle reaches Earth's lower mantle: Evidence of carbon cycle found in 'superdeep' diamonds From Brazil". ScienceDaily. Retrieved 2019-02-06.

[4] Stagno, V.; Frost, D. J.; McCammon, C. A.; Mohseni, H.; Fei, Y. (2015-02-05). "The oxygen fugacity at which graphite or diamond forms from carbonate-bearing melts in eclogitic rocks". Contributions to Mineralogy and Petrology. 169 (2): 16. doi:10.1007/s00410-015-1111-1. ISSN 1432-0967.

[5] Fiquet, Guillaume; Guyot, François; Perrillat, Jean-Philippe; Auzende, Anne-Line; Antonangeli, Daniele; Corgne, Alexandre; Gloter, Alexandre; Boulard, Eglantine (2011-03-29). "New host for carbon in the deep Earth". Proceedings of the National Academy of Sciences. 108 (13): 5184–5187. doi:10.1073/pnas.1016934108. ISSN 0027-8424. PMID 21402927.

[6] Dorfman, Susannah M.; Badro, James; Nabiei, Farhang; Prakapenka, Vitali B.; Cantoni, Marco; Gillet, Philippe (2018-05-01). "Carbonate stability in the reduced lower mantle". Earth and Planetary Science Letters. 489: 84–91. doi:10.1016/j.epsl.2018.02.035. ISSN 0012-821X.

[7] Kelley, Katherine A.; Cottrell, Elizabeth (2013-06-14). "Redox Heterogeneity in Mid-Ocean Ridge Basalts as a Function of Mantle Source". Science. 340 (6138): 1314–1317. doi:10.1126/science.1233299. ISSN 0036-8075. PMID 23641060.

[8] Kono, Yoshio (2018). "Magmas Under Pressure: Advances in High-Pressure Experiments on Structure and Properties of Melts" (PDF). www.sciencedirect.com. Retrieved 2019-02-07. {{cite web}}: Cite has empty unknown parameter: |dead-url= (help)

[9] Fiquet, Guillaume; Guyot, François; Perrillat, Jean-Philippe; Auzende, Anne-Line; Antonangeli, Daniele; Corgne, Alexandre; Gloter, Alexandre; Boulard, Eglantine (2011-03-29). "New host for carbon in the deep Earth". Proceedings of the National Academy of Sciences. 108 (13): 5184–5187. doi:10.1073/pnas.1016934108. ISSN 0027-8424. PMID 21402927.

[10] Mao, Wendy L.; Liu, Zhenxian; Galli, Giulia; Pan, Ding; Boulard, Eglantine (2015-02-18). "Tetrahedrally coordinated carbonates in Earth's lower mantle". Nature Communications. 6: 6311. doi:10.1038/ncomms7311. ISSN 2041-1723.

[11] Carmody, Laura; Genge, Matthew; Jones, Adrian P. (2013-01-01). "Carbonate Melts and Carbonatites". Reviews in Mineralogy and Geochemistry. 75 (1): 289–322. doi:10.2138/rmg.2013.75.10. ISSN 1529-6466.

[12] Dasgupta, Rajdeep (December 10, 2011). "From Magma Ocean to Crustal Recycling: Earth's Deep Carbon Cycle". {{cite web}}: Cite has empty unknown parameter: |dead-url= (help)

[13] Dasgupta, Rajdeep; Hirschmann, Marc M. (2010-09-15). "The deep carbon cycle and melting in Earth's interior". Earth and Planetary Science Letters. 298 (1): 1–13. doi:10.1016/j.epsl.2010.06.039. ISSN 0012-821X.

[14] "Shibboleth Authentication Request". login.stanford.idm.oclc.org. doi:10.1146/annurev.earth.36.031207.124322. Retrieved 2019-02-07.

[15] "Does Earth's Core Host a Deep Carbon Reservoir? | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-03-09.

[16] "Does Earth's Core Host a Deep Carbon Reservoir? | Deep Carbon Observatory". deepcarbon.net. Retrieved 2019-02-05.

[17] Li, Jie; Chow, Paul; Xiao, Yuming; Alp, E. Ercan; Bi, Wenli; Zhao, Jiyong; Hu, Michael Y.; Liu, Jiachao; Zhang, Dongzhou (2014-12-16). "Hidden carbon in Earth's inner core revealed by shear softening in dense Fe7C3". Proceedings of the National Academy of Sciences. 111 (50): 17755–17758. doi:10.1073/pnas.1411154111. ISSN 0027-8424. PMID 25453077.

[18] Hanfland, M.; Chumakov, A.; Rüffer, R.; Prakapenka, V.; Dubrovinskaia, N.; Cerantola, V.; Sinmyo, R.; Miyajima, N.; Nakajima, Y. (March 2015). "High Poisson's ratio of Earth's inner core explained by carbon alloying". Nature Geoscience. 8 (3): 220–223. doi:10.1038/ngeo2370. ISSN 1752-0908.

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 Furthermore, the process is also significant simply due to the massive quantities of carbon it transports through the planet. In fact, studying the composition of basaltic [[magma]] and measuring carbon dioxide flux out of volcanoes reveals that the amount of carbon in the [[Mantle (geology)|mantle]] is actually greater than that on the Earth's surface by a factor of one thousand.<ref name=":02">{{cite journal|last1=Wilson|first1=Mark|year=2003|title=Where do Carbon Atoms Reside within Earth's Mantle?|journal=Physics Today|volume=56|issue=10|pages=21–22|bibcode=2003PhT....56j..21W|doi=10.1063/1.1628990}}</ref> Drilling down and physically observing deep Earth carbon processes is evidently extremely difficult, as the lower mantle and [[Earth's Core|core]] extend from 660 to 2,891&nbsp;km and 2,891&nbsp;km to 6,371 deep into the Earth respectively. Accordingly, not much is conclusively known regarding the role of carbon in the deep Earth. Nonetheless, several pieces of evidence—many of which come from laboratory simulations of deep Earth conditions—have indicated mechanisms for the element's movement down into the lower mantle, as well as the forms that carbon takes at the extreme temperatures and pressures of said layer. Furthermore, techniques like [[seismology]] have led to greater understanding of the potential presence of carbon in the Earth's core.
-== Carbon in the Lower Mantle ==
+== Lower mantle ==
 Carbon principally enters the mantle in the form of [[carbonate]]-rich sediments on [[Plate tectonics|tectonic plates]] of ocean crust, which pull the carbon into the mantle upon undergoing [[subduction]]. Not much is known about carbon circulation in the mantle, especially in the deep Earth, but many studies have attempted to augment our understanding of the element's movement and forms within said region. For instance, a 2011 study demonstrated that carbon cycling extends all the way to the lower mantle. The study analysed rare, super-deep [[diamond]]s at a site in [[Juína|Juina, Brazil]], determining that the bulk composition of some of the diamonds' inclusions matched the expected result of basalt melting and [[Crystallization|crytallisation]] under lower mantle temperatures and pressures.<ref>{{Cite web|url=https://www.sciencedaily.com/releases/2011/09/110915141227.htm|title=Carbon cycle reaches Earth's lower mantle: Evidence of carbon cycle found in 'superdeep' diamonds From Brazil|website=ScienceDaily|access-date=2019-02-06}}</ref> Thus, the investigation's findings indicate that pieces of basaltic oceanic lithosphere act as the principle transport mechanism for carbon to Earth's deep interior. These subducted carbonates can interact with lower mantle [[silicate]]s and metals, eventually forming super-deep diamonds like the one found.<ref>{{Cite journal|last=Stagno|first=V.|last2=Frost|first2=D. J.|last3=McCammon|first3=C. A.|last4=Mohseni|first4=H.|last5=Fei|first5=Y.|date=2015-02-05|title=The oxygen fugacity at which graphite or diamond forms from carbonate-bearing melts in eclogitic rocks|url=https://doi.org/10.1007/s00410-015-1111-1|journal=Contributions to Mineralogy and Petrology|volume=169|issue=2|pages=16|doi=10.1007/s00410-015-1111-1|issn=1432-0967}}</ref>[[File:Carbon tetrehedral oxygen.png|thumb|Diagram of carbon tetrahedrally bonded to oxygen]]However, carbonates descending to the lower mantle encounter other fates in addition to forming diamonds. In 2011, carbonates were subjected to an environment similar to that of 1800&nbsp;km deep into the Earth, well within the lower mantle. Doing so resulted in the formations of [[magnesite]], [[siderite]], and numerous varieties of [[graphite]].<ref>{{Cite journal|last=Fiquet|first=Guillaume|last2=Guyot|first2=François|last3=Perrillat|first3=Jean-Philippe|last4=Auzende|first4=Anne-Line|last5=Antonangeli|first5=Daniele|last6=Corgne|first6=Alexandre|last7=Gloter|first7=Alexandre|last8=Boulard|first8=Eglantine|date=2011-03-29|title=New host for carbon in the deep Earth|url=https://www.pnas.org/content/108/13/5184|journal=Proceedings of the National Academy of Sciences|volume=108|issue=13|pages=5184–5187|doi=10.1073/pnas.1016934108|issn=0027-8424|pmid=21402927}}</ref> Other experiments—as well as [[Petrology|petrologic]] observations—support this claim, finding that magnesite is actually the most stable carbonate phase in the majority of the mantle. This is largely a result of its higher melting temperature.<ref>{{Cite journal|last=Dorfman|first=Susannah M.|last2=Badro|first2=James|last3=Nabiei|first3=Farhang|last4=Prakapenka|first4=Vitali B.|last5=Cantoni|first5=Marco|last6=Gillet|first6=Philippe|date=2018-05-01|title=Carbonate stability in the reduced lower mantle|url=http://www.sciencedirect.com/science/article/pii/S0012821X18300979|journal=Earth and Planetary Science Letters|volume=489|pages=84–91|doi=10.1016/j.epsl.2018.02.035|issn=0012-821X}}</ref> Consequently, scientists have concluded that carbonates undergo [[Reduction (chemistry)|reduction]] as they descend into the mantle before being stabilised at depth by low [https://link.springer.com/content/pdf/10.1007/978-3-642-27833-4_4021-3.pdfOxgyen fugacity oxygen fugacity] environments. Magnesium, iron, and other metallic compounds act as buffers throughout the process.<ref>{{Cite journal|last=Kelley|first=Katherine A.|last2=Cottrell|first2=Elizabeth|date=2013-06-14|title=Redox Heterogeneity in Mid-Ocean Ridge Basalts as a Function of Mantle Source|url=http://science.sciencemag.org/content/340/6138/1314|journal=Science|volume=340|issue=6138|pages=1314–1317|doi=10.1126/science.1233299|issn=0036-8075|pmid=23641060}}</ref> The presence of reduced, elemental forms of carbon like graphite would indicate that carbon compounds are reduced as they descend into the mantle.
 Nonetheless, it is noteworthy that [[Polymorphism (materials science)|polymorphism]] alters carbonate compounds' stability at different depths within the Earth. To illustrate, laboratory simulations and [[density functional theory]] calculations suggest that [[Tetrahedral molecular geometry|tetrahedrally-coordinated]] carbonates are most stable at depths approaching the [[Core–mantle boundary|Core-Mantle Boundary]].<ref>{{Cite web|url=https://ac.els-cdn.com/B9780128113011180025/3-s2.0-B9780128113011180025-main.pdf?_tid=0dec16ed-576a-4f5a-8e2f-1ddfa3af52c1&acdnat=1552485356_8a36591db2e70a9d990eb4271ac45a79|title=Magmas Under Pressure: Advances in High-Pressure Experiments on Structure and Properties of Melts|last=Kono|first=Yoshio|date=2018|website=www.sciencedirect.com|archive-url=|archive-date=|dead-url=|access-date=2019-02-07}}</ref><ref>{{Cite journal|last=Fiquet|first=Guillaume|last2=Guyot|first2=François|last3=Perrillat|first3=Jean-Philippe|last4=Auzende|first4=Anne-Line|last5=Antonangeli|first5=Daniele|last6=Corgne|first6=Alexandre|last7=Gloter|first7=Alexandre|last8=Boulard|first8=Eglantine|date=2011-03-29|title=New host for carbon in the deep Earth|url=https://www.pnas.org/content/108/13/5184|journal=Proceedings of the National Academy of Sciences|volume=108|issue=13|pages=5184–5187|doi=10.1073/pnas.1016934108|issn=0027-8424|pmid=21402927}}</ref> A 2015 study indicates that the lower mantle's high pressures cause carbon bonds to transition from sp<sub>2</sub> to sp<sub>3</sub> [[Orbital hybridisation|hybridised orbitals]], resulting in carbon tetrahedrally bonding to oxygen.<ref>{{Cite journal|last=Mao|first=Wendy L.|last2=Liu|first2=Zhenxian|last3=Galli|first3=Giulia|last4=Pan|first4=Ding|last5=Boulard|first5=Eglantine|date=2015-02-18|title=Tetrahedrally coordinated carbonates in Earth’s lower mantle|url=https://www.nature.com/articles/ncomms7311|journal=Nature Communications|volume=6|pages=6311|doi=10.1038/ncomms7311|issn=2041-1723}}</ref> CO<sub>3</sub> trigonal groups cannot form polymerisable networks, while tetrahedral CO<sub>4</sub> can, signifying an increase in carbon's [[coordination number]], and therefore drastic changes in carbonate compounds' properties in the lower mantle. As an example, preliminary theoretical studies suggest that high pressures cause carbonate melt viscosity to increase; the melts' lower mobility as a result of the property changes described is evidence for large deposits of carbon deep into the mantle.<ref>{{Cite journal|last=Carmody|first=Laura|last2=Genge|first2=Matthew|last3=Jones|first3=Adrian P.|date=2013-01-01|title=Carbonate Melts and Carbonatites|url=https://pubs.geoscienceworld.org/msa/rimg/article-abstract/75/1/289/140948/carbonate-melts-and-carbonatites|journal=Reviews in Mineralogy and Geochemistry|volume=75|issue=1|pages=289–322|doi=10.2138/rmg.2013.75.10|issn=1529-6466}}</ref>
@@ Line 9: / Line 9: @@
 Accordingly, carbon can remain in the lower mantle for long periods of time, but large concentrations of carbon frequently find their way back to the lithosphere. This process, called carbon outgassing, is the result of carbonated mantle undergoing decompression melting, as well as [[mantle plume]]s carrying carbon compounds up towards the crust.<ref>{{Cite journal|last=Dasgupta|first=Rajdeep|last2=Hirschmann|first2=Marc M.|date=2010-09-15|title=The deep carbon cycle and melting in Earth's interior|url=http://www.sciencedirect.com/science/article/pii/S0012821X10004140|journal=Earth and Planetary Science Letters|volume=298|issue=1|pages=1–13|doi=10.1016/j.epsl.2010.06.039|issn=0012-821X}}</ref> Carbon is oxidised upon its ascent towards volcanic hotspots, where it is then released as CO<sub>2</sub>. This occurs so that the carbon atom matches the oxidation state of the basalts erupting in such areas.<ref>{{Cite web|url=https://login.stanford.idm.oclc.org/login?url=https://www.annualreviews.org/doi/full/10.1146/annurev.earth.36.031207.124322|title=Shibboleth Authentication Request|website=login.stanford.idm.oclc.org|doi=10.1146/annurev.earth.36.031207.124322|access-date=2019-02-07}}</ref>
-== Carbon in the Core ==
+== Core ==
 [[File:Speeds of seismic waves.PNG|thumb|Analysis of shear wave velocities has played an integral role in the development of knowledge about carbon's existence in the core]]Although the presence of carbon in the Earth's core is well-constrained, recent studies suggest large inventories of carbon could be stored in this region. S[[S-wave|hear (S) waves]] moving through the inner core travel at about fifty percent of the velocity expected for most iron-rich alloys.<ref>{{Cite web|url=https://deepcarbon.net/feature/does-earths-core-host-deep-carbon-reservoir|title=Does Earth's Core Host a Deep Carbon Reservoir? {{!}} Deep Carbon Observatory|website=deepcarbon.net|access-date=2019-03-09}}</ref> Considering the core's composition is widely believed to be an alloy of crystalline iron with a small amount of nickle, this seismographic anomaly points to another substance's existence within the region. One theory postulates that such a phenomena is the result of various light elements, including carbon, in the core.<ref>{{Cite web|url=https://deepcarbon.net/feature/does-earths-core-host-deep-carbon-reservoir|title=Does Earth's Core Host a Deep Carbon Reservoir? {{!}} Deep Carbon Observatory|website=deepcarbon.net|access-date=2019-02-05}}</ref> In fact, studies have utilised [[diamond anvil cell]]s to replicate the conditions in the Earth's core, the results of which indicate that [[Cementite|iron carbide]] (Fe<sub>7</sub>C<sub>3</sub>) matches the inner core's sound and density velocities considering its temperature and pressure profile. Hence, the iron carbide model could serve as evidence that the core holds as much as 67% of the Earth's carbon.<ref>{{Cite journal|last=Li|first=Jie|last2=Chow|first2=Paul|last3=Xiao|first3=Yuming|last4=Alp|first4=E. Ercan|last5=Bi|first5=Wenli|last6=Zhao|first6=Jiyong|last7=Hu|first7=Michael Y.|last8=Liu|first8=Jiachao|last9=Zhang|first9=Dongzhou|date=2014-12-16|title=Hidden carbon in Earth’s inner core revealed by shear softening in dense Fe7C3|url=https://www.pnas.org/content/111/50/17755|journal=Proceedings of the National Academy of Sciences|volume=111|issue=50|pages=17755–17758|doi=10.1073/pnas.1411154111|issn=0027-8424|pmid=25453077}}</ref> Furthermore, another study found that carbon dissolved in iron and formed a stable phase with the same Fe<sub>7</sub>C<sub>3</sub> composition—albeit with a different structure than the one previously mentioned.<ref>{{Cite journal|last=Hanfland|first=M.|last2=Chumakov|first2=A.|last3=Rüffer|first3=R.|last4=Prakapenka|first4=V.|last5=Dubrovinskaia|first5=N.|last6=Cerantola|first6=V.|last7=Sinmyo|first7=R.|last8=Miyajima|first8=N.|last9=Nakajima|first9=Y.|date=March 2015|title=High Poisson's ratio of Earth's inner core explained by carbon alloying|url=https://www.nature.com/articles/ngeo2370|journal=Nature Geoscience|volume=8|issue=3|pages=220–223|doi=10.1038/ngeo2370|issn=1752-0908}}</ref> Hence, although the amount of carbon potentially stored in the Earth's core is not known, recent research indicates that the presence of iron carbides could be consistent with geophysical observations.