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Ocean island basalt

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Figure 1. Age-progression of volcanic islands and seamounts at the Hawaiian hotspot

Ocean island basalt (OIB) is a volcanic rock, usually basaltic in composition, erupted in oceans away from tectonic plate boundaries. Although ocean island basaltic magma is mainly erupted as basalt lava, the basaltic magma is sometimes modified by igneous differentiation to produce a range of other volcanic rock types, for example, rhyolite in Iceland, and phonolite and trachyte at the intraplate volcano Fernando de Noronha.[1] Unlike mid-ocean ridge basalts (MORBs), which erupt at spreading centers (divergent plate boundaries), and volcanic arc lavas, which erupt at subduction zones (convergent plate boundaries), ocean island basalts are the result of intraplate volcanism. However, some ocean island basalt locations coincide with plate boundaries like Iceland, which sits on top of a mid-ocean ridge, and Samoa, which is located near a subduction zone.[2]

In the ocean basins, ocean island basalts form seamounts,[3] and in some cases, enough material is erupted that the rock protrudes from the ocean and forms an island, like at Hawaii, Samoa, and Iceland. Over time, however, thermal subsidence and mass loss via subaerial erosion causes islands to become completely submarine seamounts or guyots. Many ocean island basalts erupt at volcanic hotspots, which are thought to be the surface expressions of melting of thermally buoyant, rising conduits of hot rock in the mantle, called mantle plumes.[4] Mantle plume conduits may drift slowly, but Earth’s tectonic plates drift more rapidly relative to mantle plumes. As a result, the relative motion of Earth’s tectonic plates over mantle plumes produces age-progressive chains of volcanic islands and seamounts with the youngest, active volcanoes located above the axis of the mantle plume while older, inactive volcanoes are located progressively farther away from the plume conduit (see Figure 1).[2] Hotspot chains can record tens of millions of years of continuous volcanic history; for example, the oldest seamounts in the Hawaiian–Emperor seamount chain are over 80 million years old.

Not all ocean island basalts are the product of mantle plumes. There are thousands of seamounts that are not clearly associated with upwelling mantle plumes, and there are chains of seamounts that are not age progressive. Seamounts that are not clearly linked to a mantle plume indicate that regional mantle composition and tectonic activity may also play important roles in producing intraplate volcanism.

Isotope geochemistry

The geochemistry of ocean island basalts is useful for studying the chemical and physical structure of Earth’s mantle. Some mantle plumes that feed hotspot volcanism lavas are thought to originate as deep as the core–mantle boundary (~2900 km deep). The composition of the ocean island basalts at hotspots provides a window into the composition of mantle domains in the plume conduit that melted to yield the basalts, thus providing clues as to how and when different reservoirs in the mantle formed.

Early conceptual models for the geochemical structure of the mantle argued that the mantle was split into two reservoirs: the upper mantle and the lower mantle. The upper mantle was thought to be geochemically depleted due to melt extraction which formed Earth’s continents. The lower mantle was thought to be homogenous and “primitive”. (Primitive, in this case, refers to silicate material that represents the building blocks of the planet that has not been modified by melt extraction, or mixed with subducted materials, since Earth’s accretion and core formation.) Seismic tomography showed subducted slabs passing through the upper mantle and entering the lower mantle, which indicates that the lower mantle cannot be isolated.[5] Additionally, the isotopic heterogeneity observed in plume-derived ocean island basalts argues against a homogenous lower mantle. Heavy, radiogenic isotopes are a particularly useful tool for studying the composition of mantle sources because isotopic ratios are not sensitive to mantle melting. This means that the heavy radiogenic isotopic ratio of a melt, which upwells and becomes a volcanic rock on the surface of the Earth, reflects the isotopic ratio of the mantle source at the time of melting. The best studied heavy radiogenic isotope systems in ocean island basalts are 87Sr/86Sr, 143Nd/144Nd, 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb, 176Hf/177Hf and, more recently, 187Os/188Os. In each of these systems, a radioactive parent isotope with a long half-life (i.e., longer than 704 million years) decays to a “radiogenic” daughter isotope. Changes in the parent/daughter ratio by, for example, mantle melting, results in changes in the radiogenic isotopic ratios of 87Sr/86Sr, 143Nd/144Nd, 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb, 176Hf/177Hf, and 187Os/188Os. Thus, these radiogenic isotopic systems are sensitive to the timing, and degree, of parent/daughter the changed (or fractionated) parent daughter ratio, which then informs the process(es) responsible for generating observed radiogenic isotopic heterogeneity in ocean island basalts. In mantle geochemistry, any composition with relatively low 87Sr/86Sr, and high 143Nd/144Nd and 176Hf/177Hf, is a referred to as “geochemically depleted”. High 87Sr/86Sr, and low 143Nd/144Nd and 176Hf/177Hf, is referred to as “geochemically enriched”. Lead isotopic compositions (206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb) in mantle derived rocks are described as unradiogenic (for relatively low 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb) or radiogenic (for relatively high 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb).

These isotopic systems have provided evidence for a heterogenous lower mantle. There are several distinct “mantle domains” or endmembers that appear in the ocean island basalt record. When plotted in multi-isotope space, ocean island basalts tend to form arrays trending from a central composition out to an endmember with an extreme composition. The depleted mantle, or DM, is one endmember, and is defined by low 87Sr/86Sr, 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb, and high 143Nd/144Nd and 176Hf/177Hf. The DM is therefore geochemically depleted (as the name states), and relatively unradiogenic. Mid-ocean ridge passively sample the upper mantle and MORBs are typically geochemically depleted, and therefore it is widely accepted that the upper mantle is composed mostly of depleted mantle. Thus, the term depleted MORB mantle (DMM) is often used to describe the upper mantle that sources mid-ocean ridge volcanism. Ocean island basalts also sample geochemically depleted mantle domains. In fact, most ocean island basalts are geochemically depleted, and <10% of ocean island basalts have lavas that extend to geochemically enriched (i.e., 143Nd/144Nd lower than the Earth’s building blocks) compositions.

There are two geochemically enriched domains, named enriched mantle 1 (EM1), and enriched mantle 2 (EM2). Though broadly similar, there are some important distinctions between EM1 and EM2. EM1 has unradiogenic 206Pb/204Pb, moderately high 87Sr/86Sr, and extends to lower 143Nd/144Nd and 176Hf/177Hf than EM2.[6] Pitcairn, Kerguelen-Heard, and Tristan-Gough are the type localities of EM1.  EM2 is defined by higher 87Sr/86Sr than EM1, and higher 143Nd/144Nd and 176Hf/177Hf at a given 87Sr/86Sr value, and intermediate 206Pb/204Pb.[6] Samoa and Society are the archetypal EM2 localities.

Another distinct mantle domain is the HIMU mantle. In isotope geochemistry, the Greek letter µ (or mu) is used to describe the 238U/204Pb, such that ‘high µ’ (abbreviated HIMU) describes a high 238U/204Pb ratio. Over time, as 238U decays to 206Pb, HIMU Earth materials develop particularly radiogenic (high) 206Pb/204Pb. If an Earth material has elevated 238U/204Pb (HIMU), then it will also have elevated 235U/204Pb, and therefore will produce radiogenic Pb compositions for both the 206Pb/204Pb and 207Pb/204Pb isotopic systems (238U decays 206Pb, 235U decays to 207Pb). Similarly, Earth materials with high U/Pb also tend to have high Th/Pb, and thus evolve to have high 208Pb/204Pb (232Th decays to 208Pb). Ocean island basalts with highly radiogenic 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb are the products of HIMU mantle domains. St. Helena, and several islands in the Cook-Austral volcanic lineament (e.g., Mangaia) are the type localities for HIMU ocean island basalts.

The final mantle domain discussed here is the common composition that ocean island basalts trend toward in radiogenic isotopic multi-space. This is also most prevalent mantle source in ocean island basalts, and has intermediate to geochemically depleted 87Sr/86Sr, 143Nd/144Nd, and 176Hf/177Hf, as well as intermediate 206Pb/204Pb, 207Pb/204Pb, 208Pb/204Pb.  This central mantle domain has several names, each with slightly different implications. PREMA, or “Prevalent Mantle” was the first term coined by Zindler and Hart (1986) to describe the most common composition sampled by ocean island basalts.[7] Hart et al. (1992) later named the location of the intersection of ocean island basalt compositions in radiogenic isotopic multi-space as the “Focus Zone”, or FOZO.[8] Farley et al. (1992) in the same year described a high 3He/4He (a primitive geochemical signature) component in plumes as the “Primitive Helium Mantle”, or PHEM.[9] Finally, Hanan and Graham (1996) used the term “C” (for common component) to describe a common mixing component in mantle derived rocks.[10]

The presence of a particular mantle domain in ocean island basalts from two hotspots, signaled by a particular radiogenic isotopic composition, does not necessarily indicate that mantle plumes with similar isotopic compositions are sourced from the same physical reservoir in the deep mantle. Instead, mantle domains with similar radiogenic isotopic compositions sampled at different hotspot localities are thought to share similar geologic histories.[11] For example, the EM2 hotspots of Samoa and Society are both thought to have a mantle source that contains recycled upper continental crust,[12] an idea that is supported by stable isotope observations, including δ18O and δ7Li. The isotopic similarities do not imply that Samoa and Society have the same physical mantle source, as evidenced by their slightly distinct arrays in radiogenic isotopic multi-space. Thus, hotspots that are categorized as “EM1”, “EM2”, “HIMU”, or “FOZO”, may each sample physically distinct, but compositionally similar, portions of the mantle. Furthermore, some hotspot chains host lavas with wide range of isotopic compositions so that the plume source seems to either sample multiple domains which can be sampled at different times in the volcanic evolution of a hotspot.

Isotopic systems help to deconvolve the geologic processes that contributed to, and in some cases the timing of, the formation of these mantle domains. Some important examples include the presence of crustal fingerprints in enriched mantle sources that indicate that material from Earth’s continents and oceans can be subducted into the mantle and brought back up to the surface in buoyantly rising mantle plumes. Sulfur isotopic analyses have shown mass-independent-fractionation (MIF) in the sulfur isotopes in some plume-derived lavas.[13] MIF of sulfur isotopes is a phenomenon that occurred in Earth’s atmosphere only before the Great Oxidation Event ~2.3 Ga. The presence of recycled material with MIF signatures indicates that some of the recycled material brought is older than 2.3 Ga, formed prior to the Great Oxidation Event and has resurfaced via mantle plume volcanism. Noble gas isotopic systems, such as 3He/4He, 20Ne/22Ne, and 129Xe/130Xe, have been used to demonstrate that parts of the lower mantle are relatively less degassed and have not been homogenized despite billions of years of mantle convective mixing.[14] Some large, hot mantle plumes have anomalously high 3He/4He. Since 4He is being constantly produced within the Earth via alpha decay (of 235,238U, 232Th, and 147Sm), but 3He is not being generated in appreciable quantities in the deep Earth, the ratio of 3He to 4He is decreasing in the interior of the Earth over time. The early Solar System began with high 3He/4He and therefore the Earth first accreted with high 3He/4He. Thus, in plume-derived lavas, high 3He/4He is an “ancient” geochemical signature that indicates the existence of a well-preserved helium reservoir in the deep mantle. The timing of the formation of this reservoir is constrained by observed anomalies of 129Xe/130Xe in ocean islands basalts, because 129Xe was only produced by decay of 129I during the first ~100 My of Earth’s history.[15] Together, high 3He/4He and 129Xe/130Xe indicate a relatively less degassed, primitive noble gas domain that has been relatively well preserved since the early Hadean.

Mantle sources

There are various sources identified for ocean island basalt magma in Earth's mantle. These mantle sources are inferred from differences in radiogenic isotope ratios that magmas inherit from their source rock. Sources have been defined from a combined analysis of strontium (Sr), neodymium (Nd) and lead (Pb) isotopes. The sources as defined by radiogenic isotopes are:

Enriched sources
EMI Enriched Mantle I[16] Probably mantle contaminated with material derived from subducted pelagic sediments. An alternative explanation is that this source derives from the sub-continental lithosphere which could also be contaminated by subducted pelagic sediments.[17]
EMII Enriched Mantle II Likely mantle contaminated with material derived from the recycling[A] of terrigenous sediments from the continental crust into the mantle.[17]
HIMU High U/Pb ratio Likely derived from subducted oceanic crust that has not been homogenized with the rest of the mantle. The lack of homogenization could be indebted to the accumulation of subducted oceanic crust in large-scale “megaliths” at the 670 km seismic discontinuity or near the core–mantle boundary.[18]
Depleted sources
PREMA Prevalent Mantle Possible formed by mixing of all the other mantle sources or a source formed early in Earth's history.[16]
DMM Depleted Mantle
FOZO Focus Zone A source associated with mantle plumes. It is of intermediate composition between DMM and HIMU. The name Focus Zone derives from the apparent fanning out of compositions from this zone when displaying isotope composition data on tetrahedron chart. FOZO contains high contents of Helium-3. The FOZO source is associated with deep mantle plumes. FOZO has been proposed to be either the plume material that rises from the core–mantle boundary or material that becomes attached to the plume as a sheet as the plume it rises from the core–mantle boundary.[19]

Footnotes

  1. ^ Subduction, subduction erosion etc.

References

Notes
  1. ^ Weaver, Barry L. (October 1990). "Geochemistry of highly-undersaturated ocean island basalt suites from the South Atlantic Ocean: Fernando de Noronha and Trindade islands". Contributions to Mineralogy and Petrology. 105 (5): 502–515. Bibcode:1990CoMP..105..502W. doi:10.1007/BF00302491.
  2. ^ a b Jackson, Matthew Gerard (2016). "Oceanic Island Basalts". Encyclopedia of Engineering Geology. Encyclopedia of Earth Sciences Series. pp. 1–5. doi:10.1007/978-3-319-39193-9_248-1. ISBN 978-3-319-12127-7.
  3. ^ Staudigel, Hubert; Koppers, Anthony A.P. (2015). "Seamounts and Island Building". The Encyclopedia of Volcanoes. pp. 405–421. doi:10.1016/b978-0-12-385938-9.00022-5. ISBN 9780123859389.
  4. ^ French, Scott W.; Romanowicz, Barbara (2 September 2015). "Broad plumes rooted at the base of the Earth's mantle beneath major hotspots". Nature. 525 (7567): 95–99. Bibcode:2015Natur.525...95F. doi:10.1038/nature14876. PMID 26333468.
  5. ^ Grand, Stephen P.; Van Der Hilst, Rob D.; Widiyantoro, Sri (1997). "Global seismic tomography: A snapshot of convection in the earth" (PDF). GSA Today. 7 (4): 1–7.
  6. ^ a b Jackson, Matthew G.; Dasgupta, Rajdeep (November 2008). "Compositions of HIMU, EM1, and EM2 from global trends between radiogenic isotopes and major elements in ocean island basalts". Earth and Planetary Science Letters. 276 (1–2): 175–186. Bibcode:2008E&PSL.276..175J. doi:10.1016/j.epsl.2008.09.023.
  7. ^ Zindler, A (1 January 1986). "Chemical Geodynamics". Annual Review of Earth and Planetary Sciences. 14 (1): 493–571. doi:10.1146/annurev.earth.14.1.493.
  8. ^ Hart, S. R.; Hauri, E. H.; Oschmann, L. A.; Whitehead, J. A. (24 April 1992). "Mantle Plumes and Entrainment: Isotopic Evidence". Science. 256 (5056): 517–520. Bibcode:1992Sci...256..517H. doi:10.1126/science.256.5056.517.
  9. ^ Farley, K.A.; Natland, J.H.; Craig, H. (June 1992). "Binary mixing of enriched and undegassed (primitive?) mantle components (He, Sr, Nd, Pb) in Samoan lavas". Earth and Planetary Science Letters. 111 (1): 183–199. Bibcode:1992E&PSL.111..183F. doi:10.1016/0012-821X(92)90178-X.
  10. ^ Hanan, B. B.; Graham, D. W. (17 May 1996). "Lead and Helium Isotope Evidence from Oceanic Basalts for a Common Deep Source of Mantle Plumes". Science. 272 (5264): 991–995. Bibcode:1996Sci...272..991H. doi:10.1126/science.272.5264.991.
  11. ^ White, William M. (December 2015). "Isotopes, DUPAL, LLSVPs, and Anekantavada". Chemical Geology. 419: 10–28. Bibcode:2015ChGeo.419...10W. doi:10.1016/j.chemgeo.2015.09.026.
  12. ^ Jackson, Matthew G.; Hart, Stanley R.; Koppers, Anthony A. P.; Staudigel, Hubert; Konter, Jasper; Blusztajn, Jerzy; Kurz, Mark; Russell, Jamie A. (August 2007). "The return of subducted continental crust in Samoan lavas". Nature. 448 (7154): 684–687. Bibcode:2007Natur.448..684J. doi:10.1038/nature06048. hdl:1912/2075.
  13. ^ Cabral, Rita A.; Jackson, Matthew G.; Rose-Koga, Estelle F.; Koga, Kenneth T.; Whitehouse, Martin J.; Antonelli, Michael A.; Farquhar, James; Day, James M. D.; Hauri, Erik H. (24 April 2013). "Anomalous sulphur isotopes in plume lavas reveal deep mantle storage of Archaean crust". Nature. 496 (7446): 490–493. Bibcode:2013Natur.496..490C. doi:10.1038/nature12020. PMID 23619695.
  14. ^ Graham, David W. (2002). "Noble Gas Isotope Geochemistry of Mid-Ocean Ridge and Ocean Island Basalts: Characterization of Mantle Source Reservoirs". Noble Gases. pp. 247–318. doi:10.1515/9781501509056-010. ISBN 978-1-5015-0905-6.
  15. ^ Mukhopadhyay, Sujoy (6 June 2012). "Early differentiation and volatile accretion recorded in deep-mantle neon and xenon". Nature. 486 (7401): 101–104. Bibcode:2012Natur.486..101M. doi:10.1038/nature11141. PMID 22678288.
  16. ^ a b Dickin 2005, p. 157
  17. ^ a b Dickin 2005, pp. 161–162
  18. ^ Dickin 2005, p. 151
  19. ^ Dickin 2005, p. 164
Sources
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