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By A. H. Ali.

Radiochemistry 59, 579–586. The abstract reports extraction of Ce(IV) and Th(IV) from nitric acid into TBP/kerosene, followed by selective cerium stripping with peroxide and subsequent thorium stripping with water. The publisher identifies the author by initials; no unverified expansion of that name is supplied.

Built by André Baranne, Michel Mayor, Didier Queloz and colleagues, the ELODIE fiber-fed spectrograph carried light from Haute-Provence's 1.93-metre telescope through optical fibers. Its echelle grating dispersed light in high diffraction orders; an optical prism and grism cross-disperser separated them perpendicularly on a charge-coupled device. This cross-dispersed echelle spectrograph achieved spectral resolving power $R=42000$. A simultaneous thorium reference tracked instrumental drift. Wavelength calibration mapped detector positions to wavelengths; spectral cross-correlation combined many spectral lines into a fitted profile. A barycentric velocity correction removed the observer's motion.^[ref]

Why can a spectrograph measure a Doppler shift much smaller than one spectral resolution element? Resolution concerns separating neighbouring features, whereas locating the centre of a known profile uses information across that profile and across many spectral lines. For a chosen example, at $\lambda =500\mathrm{nm}$ a recession velocity of $60\mathrm{m}{\mathrm{s}}^{-1}$ givesAt $R=42000$, one spectral resolution element corresponds to $c/R\simeq 7.14\mathrm{km}{\mathrm{s}}^{-1}$, about $119$ times larger. A well measured centre can move by a small fraction of that width. More photons and more useful spectral lines improve the estimate, but do not remove wavelength calibration errors or stellar activity.

A simple mathematical picture of spectral cross-correlation makes the readout concrete. Define $x=c\log (\lambda /{\lambda }_0)$, with fixed reference wavelength ${\lambda }_0$, and let $d(x)$ be continuum-normalized line absorption. For small velocities, a common Doppler shift approximately translates $d(x)$. A positive absorption mask $m(x)$ then givesIf $d(x)=m(x-v_r)$, the maximum occurs at $u=v_r$; a convention correlating the received observed radiative flux instead produces a dip. A fitted correlation centre is an effective collective line position, not a claim that each individual spectral line has been resolved into a narrower feature. The lamp tracks instrumental drift, while the barycentric velocity correction removes the observer's changing line-of-sight velocity; neither removes changes in the star itself.

A natural feed can contain thorium and uranium, as well as other lanthanides. Th(IV) hydrolyses readily and can accompany the cerium precipitate; uranium speciation depends on its oxidation state and the ligands present. Raising pH too far also precipitates other rare-earth hydroxides. Even before their bulk precipitation thresholds, adsorption and coprecipitation on a high-area hydrated cerium oxide can contaminate the solid. Local high-pH zones during base addition and incomplete Ce(III) oxidation make the separation less reproducible.

Thus a cerium-rich precipitate need not be pure cerium. A sensible test measures the Ce oxidation state, analyses both filtrate and washed solid, and includes thorium-containing and thorium-free mixtures; otherwise low dissolved cerium could be mistaken for selective purification.

A better controlled route is selective solvent extraction in acid, followed by selective stripping, rather than precipitating everything near overlapping hydrolysis thresholds. Oxidize Ce(III) to Ce(IV) in a controlled acidic nitrate medium, extract its nitrate complexes into an organic donor phase, and separate the phases. Then reduce the extracted Ce(IV) to Ce(III) and back-extract it into an aqueous phase. Trivalent rare earths are less strongly extracted under suitable conditions.

This still needs a thorium separation: tributyl phosphate can coextract Th(IV). One demonstrated strategy deliberately coextracts Ce(IV) and Th(IV), then uses reducing peroxide solution to strip Ce as Ce(III), followed by a separate thorium strip. The appropriate controls are distribution measurements for each ion at the chosen acid concentration, a cerium oxidation-state check, and a complete mass balance over extraction and stripping. Selectivity comes from combining oxidation state and complexation, not from assuming that one extraction removes every contaminant.^[ref]

At a convergent margin, the incoming oceanic lithosphere is a chemically and mechanically layered package: sediments, oceanic crust and lithospheric mantle. Subduction does not deliver this whole package unchanged to one destination. Solids can be accreted, underplated, exhumed or recycled deeply, while released fluids and melts carry selected components to the overriding plate. The outcome depends on incoming composition and hydration, slab age, convergence rate, thermal structure, interface coupling and subsequent tectonic history.

The incoming material already contains a history. Sediments include terrigenous debris, biogenic carbonates, siliceous deposits, clay minerals, pore water and organic matter. Oceanic crust consists mainly of basalt, sheeted dikes and gabbro; hydrothermal alteration can add water, carbonates and mobile elements before subduction. Beneath it, residual peridotite forms the lithospheric mantle. Faulting at a spreading environment, a transform boundary or an outer-rise bending region can let seawater enter and cause serpentinization. The lithospheric mantle is not uniformly hydrated to its full thickness. Consequently, sediment thickness alone does not measure the incoming volatile inventory.

Sediments: separation starts near the trench. Compaction and increasing effective pressure expel pore fluids, which can escape through the forearc, transport dissolved constituents and influence pore pressure on the plate interface. Some sediments are scraped off into an accretionary prism, shortened by thrusts and retained in the upper plate. Others pass beneath the leading edge, then detach and undergo tectonic underplating beneath the forearc. Deeper underplated material may return to the surface during tectonic exhumation, preserving a record of burial and deformation. At a sediment-starved erosive margin, little prism may form, and tectonic erosion can entrain material from the overriding plate as well. Thus net continental gain and net continental loss are both possible; they can even alternate at one margin.

Sediments that remain attached to the slab undergo metamorphism, dehydration, and potentially decarbonation or carbonate dissolution. The released fluids can transport boron, barium, strontium, lead and other soluble constituents. Carbon can leave as dissolved species, remain in carbonate, or occur as reduced carbon depending on redox conditions and reaction history. Along sufficiently hot paths, sediment-derived melts or mixtures of sediment and altered rock can transfer material into the mantle wedge; buoyant mixed material may rise as a mélange diapir. Cold paths can instead retain more solid material and some volatile-bearing phases to greater depths. These are alternative reaction and transport pathways, not a single compulsory sequence. A carbon-budget study explicitly includes fluid dissolution, sediment diapirism and storage in the upper plate, showing why volcanic carbon dioxide alone cannot close the whole subduction carbon budget.^[ref]

Oceanic crust: metamorphic transformation and chemical filtration. Altered basalt and gabbro are progressively buried. Depending on their pressure-temperature paths and reaction kinetics, they can pass through blueschist facies or warmer assemblages and eventually form eclogite, dominated by garnet and omphacite. Eclogitization increases density and can strengthen negative slab buoyancy, but a kinetic delay can leave metastable rock. It is incorrect to assign every slab the same sequence or the same fixed depths for these changes.

During burial, breakdown of hydrous phases releases water-rich fluids; different mineral assemblages retain different quantities of water. The fluids migrate through or along the interface and into the mantle wedge, where they cause metasomatism and lower the solidus of peridotite. Flux melting of the mantle wedge generates much of the primary magma feeding a volcanic arc. This is different from saying that the entire descending oceanic crust melts beneath the arc. Most of its refractory mass can remain solid. Partial melting of oceanic crust is more plausible for unusually hot or young slabs, or other favorable thermal conditions, and produces a distinct crustal contribution.

The depth of dehydration is controlled by thermal structure and composition. Global thermal-petrological calculations, for example, predict more efficient deep water transport in old, fast, cold slabs than in hot ones, with substantial differences between volcanic crust, gabbro and hydrated peridotite. Such a calculation supports conditional deep retention; its modeled proportions should not be imposed on every margin.^[ref]

Mechanical detachment adds more branches. Upper-crustal slices, seamounts or oceanic plateaus may be accreted or underplated instead of continuing down the slab. A complete or partial ophiolite can be emplaced onto another plate by obduction in suitable convergence histories. Most intact oceanic crust is not saved this way. High-pressure fragments may be entrained in an interface channel or mélange and exhumed; their small preserved volume should not be mistaken for the dominant global mass flux. Magma generated after slab-derived transfer may also pond and crystallize beneath the upper crust by magmatic underplating, which is a different process from mechanical tectonic underplating of solid slices.

Lithospheric mantle: residual rock and a variable water carrier. Most incoming lithospheric mantle is depleted peridotite left after extraction of ridge melts. Its cold, dense, mechanically coherent portion contributes to slab pull and generally sinks with the plate. Hydrated portions contain serpentine and possibly other hydrous minerals. Breakdown of these phases releases water at conditions that depend on the thermal path, feeding further metasomatism of the mantle wedge and sometimes dehydration embrittlement. The latter is a proposed contributor to intermediate-depth earthquakes, not an exclusive explanation for all such events. Very cold paths may transfer some water onward in high-pressure hydrous phases or as hydrogen incorporated in nominally anhydrous minerals.

Do not confuse the incoming hydrated lithospheric mantle with newly serpentinized forearc mantle in the overriding plate. The latter receives slab-derived fluids and can temporarily store their water. Hydrated, relatively buoyant interface material can facilitate return flow and tectonic exhumation, while the colder deeper bulk of the lithospheric mantle continues down. Some peridotite may also be accreted or obducted with an ophiolite. These exchanges mean that even an exposed serpentinite requires structural and chemical context before it can be assigned to its original plate.

Deep recycling and eventual return. The residual eclogite, remaining sediments and lithospheric mantle can enter the deeper mantle. A slab can temporarily stagnate around the mantle transition zone or penetrate into the lower mantle, depending on buoyancy, phase transformations, geometry and mantle viscosity. Crustal material can remain as compositionally distinct domains, mix, or react with surrounding peridotite; it need not retain the near-surface eclogite assemblage indefinitely as pressure rises. Subsequent mantle convection can return recycled components toward spreading regions or mantle plumes, where partial melting incorporates them into new basalt. A primary study of Hawaiian basalt illustrates a specific model in which melts derived from recycled crust react with peridotite to form a pyroxenite source. It is an interpretation of combined chemical evidence, not a unique label attached to every enriched basalt.^[ref]

How the pathways can be observed. Seismic reflection profiles, drilling, wedge geometry and balanced structural sections constrain accretion, fluid escape and tectonic erosion. High-pressure metamorphism, mineral zoning, radiometric dating and pressure-temperature-time paths in exhumed rocks reveal burial, reaction and return. Their reconstructable histories are especially useful when deformation and fluid inclusions are linked to the dated mineral growth. Earthquake distributions, seismic tomography, seismic attenuation and electrical conductivity constrain the geometry and physical state of the slab and mantle wedge, although fluids, melts and temperature can produce nonunique signals.

Arc magmas carry complementary chemical evidence: relatively mobile barium, boron, lead or strontium can trace fluid-mediated transfer, whereas sediment-sensitive thorium and isotope ratios can help identify other contributions. Element mobility changes with fluid composition and pressure-temperature conditions, so no one element is an infallible tracer. Boron isotope ratios, radiogenic strontium isotope ratios and lead isotope ratios should be interpreted with measured incoming sediments and altered oceanic crust. Arc gases and forearc fluid discharge constrain volatile return; ocean-island basalts, mantle xenoliths and diamond inclusions provide possible evidence of deeper recycling. Each observation samples only part of the system.

For any element $X$, a useful control-volume statement isHere permanent accretion is counted outside the chosen reactive control volume, return includes fluid, melt and exhumed-solid exports, and transient underplating or reservoir growth contributes to storage until exported. For a different boundary choice, the terms must be regrouped consistently. The three incoming layers can have very different transfer efficiencies for bulk rock, water, carbon and a particular trace element. A small mass of escaping fluid can dominate an element's return while most of the solid slab continues into the deep mantle.

Use chemical signatures to reconstruct processes, then test tectonic context. Geochemistry can establish melting conditions, surface alteration and recycling, but plate tectonics is a kinematic system. I would sample dated suites across a mapped geological succession and compare competing origins, rather than declare an isolated “arc-like” analysis proof of a global regime. Radiometric dating must identify whether the measured age records crystallization, later metamorphism, alteration or inheritance.

Hydrous magmatism and selective element transfer. Analyze fresh basalt, associated intrusive rocks and differentiated volcanic suites for major elements, trace elements and isotope ratios. Relative enrichment of fluid-mobile elements such as barium, strontium and lead, together with relative depletion of niobium and tantalum, can support addition of slab-derived components to a depleted mantle wedge. Test coherent variations in barium/niobium, thorium/niobium and rare-earth element patterns against modeled fluid addition, sediment melting, source depletion and fractional crystallization. Do not treat these ratios as fixed universal cutoffs. Crustal contamination, remelting of previously arc-modified crust, residual rutile or other source effects can create some similar patterns. Altered rocks can also gain mobile elements long after their formation.

The case becomes stronger if the chemical evolution occurs in a plausible succession of oceanic, early forearc and mature arc magmas, with supporting structure and geochronology. The key evidence would be correlated process changes in an independently reconstructed margin, not resemblance to one modern basalt plot. A geochemical discrimination diagram is a comparison tool; its modern training associations are not a proof that only those settings could exist on a hotter Earth.

High-pressure melting and the fate of mafic crust. Tonalite-trondhjemite-granodiorite suites with high strontium/yttrium or lanthanum/ytterbium and low heavy rare-earth element abundances can indicate melting with residual garnet and little plagioclase. Model the combined major element composition, residual phases and melt fraction to estimate the pressure, hydration and source of melting. This could support melting of buried hydrous oceanic crust. However, basal melting of thickened crust, delamination and nonplate vertical burial can produce related conditions. High strontium/yttrium alone neither proves a descending slab nor dates the first subduction. Conversely, hotter ancient subduction might not produce exactly the same magmatic products as modern cold slabs.^[ref]

Radiogenic isotopes distinguish new extraction from reworking. Couple zircon uranium-lead dating with hafnium isotope ratios, and whole-rock samarium-neodymium isotope ratios with strontium isotope ratios or lead isotope ratios. These systems can constrain contributions from depleted mantle, older continental crust and altered surface reservoirs. For a closed parent-daughter system,where $P(t)$ is the present parent abundance, $D^{\ast }$ the radiogenic daughter accumulated since closure, and $\lambda$ the radioactive decay constant. Initial daughter composition, closure and mixing must be constrained before interpreting an age. A crustal extraction model age depends on a reference mantle evolution and subsequent history; it is not automatically a rock's crystallization age or the date of a tectonic transition.

Juvenile signatures can indicate addition from the mantle, while evolved signatures can indicate reworking of older crust; neither is exclusive to a particular tectonic regime. Spatially organized juvenile additions at a reconstructed margin, followed by collision and reworking, are more diagnostic than an undifferentiated global age histogram. Work combining zircon hafnium isotope ratios, oxygen isotope ratios and age distributions illustrates how crustal generation, reworking and preservation can be separated conceptually, while remaining dependent on sampling and model assumptions.^[ref]

Stable isotopes can identify a visit to the surface. Zircon oxygen isotope ratios substantially different from an appropriate mantle reference may record melting of material that previously underwent low-temperature water-rock interaction. This would support surface alteration followed by burial or remelting. It would not, by itself, distinguish subduction from burial under a thick volcanic pile or another form of recycling. Alteration, metamorphic exchange, inherited cores and analytical domains need checking. Multiple stable isotope systems, including boron isotope ratios in appropriate rocks, can strengthen a fluid-transfer interpretation if their fractionation and later resetting are modeled.

Deep samples provide an independent archive. If dated diamond inclusions or mantle xenoliths preserve eclogite compositions together with a surface-alteration chemical signature, they could demonstrate transfer of crustal material into deep lithospheric mantle. Dating the relevant mineral assemblage and distinguishing inclusion growth from later host transport are essential. A primary diamond-inclusion study used coupled chemical and isotopic observations to infer changes in deep recycling; the general lesson is to test a transport history, not to make the first preserved sample an infallible onset clock.^[ref] Delamination or other sinking processes remain alternatives unless structure and regional history establish plate convergence.

For each candidate signal, I would seek an older comparison population, quantify alteration and analytical uncertainty, reproduce the pattern in several independent regions, and combine chemistry with the tests in the other parts. A securely dated demonstration of subduction shows that it operated by that time in that region; it does not demonstrate that it began then everywhere. A secular shift toward more frequent, spatially coherent signatures can support expansion of the regime, but only after correcting for the survival of its archive.

Roberta Rudnick is a geologist who investigates the composition and origin of continental crust. Much of the lower continental crust is inaccessible to direct sampling, so its composition must be inferred by combining geochemistry, petrology and seismology. Her 1995 synthesis with David M. Fountain linked laboratory measurements of elastic wave speeds in rocks to seismic refraction surveys, using granulites to constrain the composition of the deep continental crust.^[ref]

Their reconstruction distinguished a compositionally heterogeneous, on average mafic lower continental crust from an intermediate-composition middle continental crust. The distinction matters for Earth's heat budget: the abundance of potassium, thorium and uranium, and hence heat production from radioactive decay, varies between rock types and with depth. Seismic wave speeds alone are not a unique chemical analysis; different rocks can have overlapping elastic properties, making independent constraints from geochemistry essential.^[ref]

Research author of Nature and composition of the continental crust: A lower crustal perspective by Roberta L. Rudnick and David M. Fountain.

Thorium is the chemical element with atomic number 90 and symbol $\mathrm{Th}$. It is a actinide. It has no stable isotopes, but thorium-232 is sufficiently long-lived to occur naturally. The $+4$ oxidation state is characteristic of its chemistry, distinguishing it from the more usual $+3$ chemistry of many neighboring f-block elements.^[ref]