Ringwoodite

Ringwoodite is a high-pressure phase of Mg2SiO4 (magnesium silicate) formed at high temperatures and pressures of the Earth's mantle between 525 and 660 km (326 and 410 mi) depth. It may also contain iron and hydrogen. It is polymorphous with the olivine phase forsterite (a magnesium iron silicate).

Ringwoodite
Crystal (~150 micrometers across) of Fo90 composition blue ringwoodite synthesized at 20 GPa and 1200 °C.
General
CategoryNesosilicates
Spinel group
Formula
(repeating unit)		Magnesium silicate (Mg2SiO4)
IMA symbolRgd[1]
Strunz classification9.AC.15
Crystal systemCubic
Crystal classHexoctahedral (m3m)
H-M symbol: (4/m 3 2/m)
Space groupFd3m
Unit cella = 8.113 Å; Z = 8
Identification
ColourDeep blue, also red, violet, or colourless (pure Mg2SiO4)
Crystal habitMicrocrystalline aggregates
DiaphaneitySemitransparent
Specific gravity3.90 (Mg2SiO4); 4.13 ((Mg0.91,Fe0.09)2SiO4); 4.85 (Fe2SiO4)
Optical propertiesIsotropic
Refractive indexn = 1.8
Birefringencenone
Pleochroismnone
References[2][3][4]

Ringwoodite is notable for being able to contain hydroxide ions (oxygen and hydrogen atoms bound together) within its structure. In this case two hydroxide ions usually take the place of a magnesium ion and two oxide ions.[5]

Combined with evidence of its occurrence deep in the Earth's mantle, this suggests that there is from one to three times the world ocean's equivalent of water in the mantle transition zone from 410 to 660 km deep.[6][7]

This mineral was first identified in the Tenham meteorite in 1969,[8] and is inferred to be present in large quantities in the Earth's mantle.

Olivine, wadsleyite, and ringwoodite are polymorphs found in the upper mantle of the earth. At depths greater than about 660 kilometres (410 mi), other minerals, including some with the perovskite structure, are stable. The properties of these minerals determine many of the properties of the mantle.

Ringwoodite was named after the Australian earth scientist Ted Ringwood (1930–1993), who studied polymorphic phase transitions in the common mantle minerals olivine and pyroxene at pressures equivalent to depths as great as about 600 km.

Characteristics

Ringwoodite is polymorphous with forsterite, Mg2SiO4, and has a spinel structure. Spinel group minerals crystallize in the isometric system with an octahedral habit. Olivine is most abundant in the upper mantle, above about 410 km (250 mi); the olivine polymorphs wadsleyite and ringwoodite are thought to dominate the transition zone of the mantle, a zone present from about 410 to 660 km depth.

Ringwoodite is thought to be the most abundant mineral phase in the lower part of Earth's transition zone. The physical and chemical property of this mineral partly determine properties of the mantle at those depths. The pressure range for stability of ringwoodite lies in the approximate range from 18 to 23 GPa.

Natural ringwoodite has been found in many shocked chondritic meteorites, in which the ringwoodite occurs as fine-grained polycrystalline aggregates.[9]

Natural ringwoodite generally contains much more Mg than Fe but can form a gapless solid solution series from the pure Mg endmember to the pure Fe endmember. The latter has been discovered in a natural sample only recently and was named ahrensite, in honor of US mineral physicist Thomas J. Ahrens (1936–2010).

Geological occurrences

In meteorites, ringwoodite occurs in the veinlets of quenched shock-melt cutting the matrix and replacing olivine probably produced during shock metamorphism.[9]

In Earth's interior, olivine occurs in the upper mantle at depths less than about 410 km, and ringwoodite is inferred to be present within the transition zone from about 520 to 660 km depth. Seismic activity discontinuities at about 410 km, 520 km, and at 660 km depth have been attributed to phase changes involving olivine and its polymorphs.

The 520-km depth discontinuity is generally believed to be caused by the transition of the olivine polymorph wadsleyite (beta-phase) to ringwoodite (gamma-phase), while the 660-km depth discontinuity by the phase transformation of ringwoodite (gamma-phase) to a silicate perovskite plus magnesiowüstite.[10][11]

Ringwoodite in the lower half of the transition zone is inferred to play a pivotal role in mantle dynamics, and the plastic properties of ringwoodite are thought to be critical in determining flow of material in this part of the mantle. The ability of ringwoodite to incorporate hydroxide is important because of its effect on rheology.

Ringwoodite has been synthesized at conditions appropriate to the transition zone, containing up to 2.6 weight percent water.[12][13]

Because the transition zone between the Earth's upper and lower mantle helps govern the scale of mass and heat transport throughout the Earth, the presence of water within this region, whether global or localized, may have a significant effect on mantle rheology and therefore mantle circulation.[14] In subduction zones, the ringwoodite stability field hosts high levels of seismicity.[15]

An "ultradeep" diamond (one that has risen from a great depth) found in Juína in western Brazil contained an inclusion of ringwoodite — at the time the only known sample of natural terrestrial origin — thus providing evidence of significant amounts of water as hydroxide in the Earth's mantle.[6][16][17][18] The gemstone, about 5mm long,[18] was brought up by a diatreme eruption.[19] The ringwoodite inclusion is too small to see with the naked eye.[18] A second such diamond was later found.[20]

The mantle reservoir could contain about three times more water, in the form of hydroxide contained within the wadsleyite and ringwoodite crystal structure, than the Earth's oceans combined.[7]

Synthetic

For experiments, hydrous ringwoodite has been synthesized by mixing powders of forsterite (Mg
2SiO
4), brucite (Mg(OH)
2), and silica (SiO
2) so as to give the desired final elemental composition. Putting this under 20 gigapascals of pressure at 1,523 K (1,250 °C; 2,282 °F) for three or four hours turns this into ringwoodite, which can then be cooled and depressurized.[5]

Crystal structure

Ringwoodite has the spinel structure, in the isometric crystal system with space group Fd3m (or F43m[21]). On an atomic scale, magnesium and silicon are in octahedral and tetrahedral coordination with oxygen, respectively. The Si-O and Mg-O bonds have mixed ionic and covalent character.[22] The cubic unit cell parameter is 8.063 Å for pure Mg2SiO4 and 8.234 Å for pure Fe2SiO4.[23]

Chemical composition

Ringwoodite compositions range from pure Mg2SiO4 to Fe2SiO4 in synthesis experiments. Ringwoodite can incorporate up to 2.6 percent by weight H2O.[5]

Physical properties
Molar volume vs. pressure at room temperature for ringwoodite γ-Mg2SiO4
Molar volume vs. pressure at room temperature for ahrensite γ-Fe2SiO4

The physical properties of ringwoodite are affected by pressure and temperature. At the pressure and temperature condition of the Mantle Transition Zone, the calculated density value of ringwoodite is 3.90 g/cm3 for pure Mg2SiO4;[24] 4.13 g/cm3 for (Mg0.91,Fe0.09)2SiO4[25] of pyrolitic mantle; and 4.85 g/cm3 for Fe2SiO4.[26] It is an isotropic mineral with an index of refraction n = 1.768.

The colour of ringwoodite varies between the meteorites, between different ringwoodite bearing aggregates, and even in one single aggregate. The ringwoodite aggregates can show every shade of blue, purple, grey and green, or have no colour at all.

A closer look at coloured aggregates shows that the colour is not homogeneous, but seems to originate from something with a size similar to the ringwoodite crystallites.[27] In synthetic samples, pure Mg ringwoodite is colourless, whereas samples containing more than one mole percent Fe2SiO4 are deep blue in colour. The colour is thought to be due to Fe2+–Fe3+ charge transfer.[28]

References
  1. Warr, L.N. (2021). "IMA–CNMNC approved mineral symbols". Mineralogical Magazine. 85 (3): 291–320. Bibcode:2021MinM...85..291W. doi:10.1180/mgm.2021.43. S2CID 235729616.
  2. Handbook of Mineralogy
  3. Ringwoodite on Mindat.org
  4. Ringwoodite on Webmineral
  5. Ye, Y.; Brown, D.A.; Smyth, J. R.; Panero, W.R.; Jacobsen, S.D.; Chang, Y.-Y.; Townsend, J.P.; Thomas, S.M.; Hauri, E.; Dera, P.; Frost, D.J. (2012). "Compressibility and thermal expansion study of hydrous Fo100 ringwoodite with 2.5(3) wt% H2O" (PDF). American Mineralogist. 97: 573–582. doi:10.2138/am.2012.4010. S2CID 29350628. Archived from the original (PDF) on 2014-06-29.
  6. "Rare Diamond confirms that Earth's mantle holds an ocean's worth of water". Scientific American. March 12, 2014. Retrieved March 13, 2014.
  7. Schmandt, Brandon; Jacobsen, Steven D.; Becker, Thorsten W.; Liu, Zhenxian; Dueker, Kenneth G. (13 June 2014). "Dehydration melting at the top of the lower mantle". Science. 344 (6189): 1265–1268. Bibcode:2014Sci...344.1265S. doi:10.1126/science.1253358. PMID 24926016. S2CID 206556921.
  8. Binns, R A.; Davis, R. J.; Reed, No S. J. B (1969). "Ringwoodite, natural (Mg,Fe)2SiO4 Spinel group in the Tenham meteorite". Nature. 221: 943–944. doi:10.1038/221943a0. S2CID 4207095.
  9. Chen. M, El Goresy A., and Gillet P. (2004). "Ringwoodite lamellae in olivine: Clues to olivine–ringwoodite phase transition mechanisms in shocked meteorites and subducting slabs". PNAS.
  10. A. Deuss; J. Woodhouse (12 October 2001). "Seismic Observations of Splitting of the Mid-Transition Zone Discontinuity in Earth's Mantle". Science. New Series. 294 (5541): 354–357. Bibcode:2001Sci...294..354D. doi:10.1126/science.1063524. PMID 11598296. S2CID 28563140.
  11. G. R. Helffrich; B. J. Wood (2001). "The Earth's mantle". Nature. 412 (6846): 501–507. doi:10.1038/35087500. PMID 11484043. S2CID 4304379.
  12. David L. Kohlstedt; Hans Keppler; David C. Rubie (1996). "Solubility of water in the alpha, beta, and gamma phases of (Mg,Fe)2SiO4". Contributions to Mineralogy and Petrology. 123 (4): 345–357. Bibcode:1996CoMP..123..345K. doi:10.1007/s004100050161. S2CID 96574743.
  13. J. R. Smyth; C. M. Holl; D. J. Frost; S. D. Jacobsen; F. Langenhorst; C. A. McCammon (2003). "Structural systematics of hydrous ringwoodite and water in Earth's interior". American Mineralogist. 88 (10): 1402–1407. Bibcode:2003AmMin..88.1402S. doi:10.2138/am-2003-1001. S2CID 41414643.
  14. A. Kavner (2003). "Elasticity and strength of hydrous ringwoodite at high pressure". Earth and Planetary Science Letters. 214 (3–4): 645–654. Bibcode:2003E&PSL.214..645K. doi:10.1016/s0012-821x(03)00402-3.
  15. Y. Xu; D.J. Weider; J.Chen; M.T. Vaughan; Y. Wang; T. Uchida (2003). "Flow-law for ringwoodite at subduction zone conditions". Physics of the Earth and Planetary Interiors. 136 (1–2): 3–9. Bibcode:2003PEPI..136....3X. doi:10.1016/s0031-9201(03)00026-8.
  16. Richard A. Lovett (12 March 2014). "Tiny diamond impurity reveals water riches of deep Earth". Nature. doi:10.1038/nature.2014.14862. S2CID 138212710.
  17. D. G. Pearson; F. E. Brenker; F. Nestola; J. McNeill; L. Nasdala; M. T. Hutchison; S. Matveev; K. Mather; G. Silversmit; S. Schmitz; B. Vekemans; L. Vincze (13 March 2014). "Hydrous mantle transition zone indicated by ringwoodite included within diamond" (PDF). Nature. 507 (7491): 221–224. Bibcode:2014Natur.507..221P. doi:10.1038/nature13080. PMID 24622201. S2CID 205237822.
  18. Sample, Ian (March 12, 2014). "Rough diamond hints at vast quantities of water inside Earth". The Guardian. Retrieved December 6, 2014.
  19. "sample of the week: ringwoodite". super/collider. Retrieved December 6, 2014.
  20. Andy Coghlan (Jun 21, 2014). "Massive 'ocean' discovered towards Earth's core". New Scientist.
  21. The structure of spinel structure is more accurately described as F43m, according to N. W. Grimes; et al. (Apr 8, 1983). "New Symmetry and Structure for Spinel". Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences. 386 (1791): 333–345. Bibcode:1983RSPSA.386..333G. doi:10.1098/rspa.1983.0039. JSTOR 2397417. S2CID 96560029.
  22. Price, Geoffrey D.; Parker, Stephen C. (April 1984). "Computer simulations of the structural and physical properties of the olivine and spinel polymorphs of Mg2SiO4". Physics and Chemistry of Minerals. 10 (5): 209–216. Bibcode:1984PCM....10..209P. doi:10.1007/BF00309313. S2CID 96165079.
  23. Smyth, J.R. and T.C. McCormick (1995). "Crystallographic data for minerals". in (T.J. Ahrens, ed.) Mineral Physics and Crystallography: A Handbook of Physical Constants, AGU Washington DC, 1-17.
  24. Katsura, T., Yokoshi, S., Song, M., Kawabe, K., Tsujimura, T., Kubo, A., Ito, E., Tange, Y., Tomioka, N., Saito, K. and Nozawa, A. (2004). "Thermal expansion of Mg2SiO4 ringwoodite at high pressures". Journal of Geophysical Research: Solid Earth. 109 (B12): B12. Bibcode:2004JGRB..10912209K. doi:10.1029/2004JB003094.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  25. Nishihara, Y., Takahashi, E., Matsukage, K. N., Iguchi, T., Nakayama, K., & Funakoshi, K. I. (2004). "Thermal equation of state of (Mg0. 91Fe0. 09) 2SiO4 ringwoodite". Physics of the Earth and Planetary Interiors. 143: 33–46. Bibcode:2004PEPI..143...33N. doi:10.1016/j.pepi.2003.02.001.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  26. Armentrout, M., & Kavner, A. (2011). "High pressure, high temperature equation of state for Fe2SiO4 ringwoodite and implications for the Earth's transition zone". Geophysical Research Letters. 38 (8): n/a. Bibcode:2011GeoRL..38.8309A. doi:10.1029/2011GL046949.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  27. Lingemann C. M. and D. Stöffler 1994. "New Evidence for the Colouration and Formation of Ringwoodite in Severely Shocked Chondrites". Lunar and Planetary Science XXIX, p. 1308.
  28. Keppler, H.; Smyth, J.R. (2005). "Optical and near infrared spectra of ringwoodite to 21.5 GPa". American Mineralogist. 90: 1209–1214. doi:10.2138/am.2005.1908. S2CID 32069655.
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