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A metamorphic rock dominated by amphibole and plagioclase, commonly derived from a mafic precursor.

An igneous rock composed predominantly of plagioclase. Lunar anorthositic rocks are central to the flotation interpretation of the lunar magma ocean. Their mineral and chemical composition does not alone date the formation of the complete crustal layer; sample context and radiometric dating are needed.

A coarse-grained intrusive rock with intermediate composition, commonly containing plagioclase and amphibole or pyroxene.

High-pressure metamorphic rock with a major assemblage of garnet and omphacitic clinopyroxene, generally lacking plagioclase. It can derive from mafic crust by several burial mechanisms.

A coarse-grained intrusive rock containing quartz and feldspar, with more plagioclase relative to alkali feldspar than typical granite.

An early extensively molten silicate reservoir in the Moon. The flotation model forms an anorthosite-rich crust by accumulation of buoyant plagioclase, leaving differentiated cumulates and incompatible-element-rich residual liquid beneath. The distribution of late KREEP-rich material and the survival of hemispheric chemical gradients are important constraints on proposed explanations of the lunar crustal dichotomy.

The lunar crustal dichotomy combines several observables: the far side of the Moon has generally thicker, higher, feldspathic lunar highlands, whereas most visible lunar maria and the Procellarum KREEP Terrane occupy the near side of the Moon. These need not all have been produced by a single event. The old anorthosite crust formed mainly before the younger basaltic mare infill. Gravity-based crustal models combined with sample and seismic constraints demonstrate that crustal thickness and porosity must be considered alongside surface color.^[ref]

An early thermal and chemical asymmetry is one physically motivated option. In a lunar magma ocean, crystallizing, relatively buoyant plagioclase can accumulate to form feldspathic crust. On a young Moon that rapidly attained synchronous rotation, radiation from a still-hot nearby Earth would preferentially warm the nearside. The primordial Earthshine hypothesis proposes that this imposed a thermal gradient in the atmosphere and accreting material: crust-forming refractory constituents condensed preferentially toward the cooler farside, favoring thicker farside crust. This is more specific than simply saying that the farside cooled faster; it requires a persistent hemispheric chemical contrast.^[ref]

Subsequent concentration of incompatible elements in KREEP-rich late liquids can help preserve a thermal asymmetry: potassium, uranium and thorium provide radiogenic heating, supporting later melting in the nearside source region. Lower surface elevation and a thinner crust also facilitate some magma transport and pooling, although crustal thickness alone cannot specify eruption rates. The origin of the crustal contrast and the later production and emplacement of mare basalt are separate parts of the explanation.

The thermal option is consistent with a thick feldspathic farside crust, a hemispheric chemical contrast and the existence of an early hot Earth. It is not uniquely demonstrated by those observations. Vigorous magma-ocean mixing could erase the proposed gradient; the required irradiation must persist during the relevant condensation and crust-building interval, not merely occur at some early time. A failure to find the predicted bulk compositional contrast in demonstrably ancient deep crust, or a chronology placing the asymmetry after complete crystallization, would challenge this particular mechanism. The existence of farside mare deposits and large thin-crust basins also warns against treating thickness as an on/off volcanic switch.

Accretion of a smaller companion is a contrasting option. A low-speed collision of a smaller co-orbiting moon with the lunar farside could add a broad layer of relatively cold silicate material rather than excavate an ordinary deep crater. Numerical impact models demonstrate that such a depositional event can build thick highlands and displace underlying residual liquid toward the opposite hemisphere.^[ref] Broad crustal excess and asymmetric evolved material are compatible with that mechanism, but are not unique evidence for it. The necessary companion, collision timing and impact geometry must be dynamically feasible. A predicted buried depositional interface, age discontinuity or lateral fabric should survive somewhere; their systematic absence in well-resolved, unmodified ancient crust would count against the model. Closely related bodies could have similar isotopes, so failure to find a large isotopic difference alone would not disprove accretion.

Both scenarios allow later basin impacts, partial melting of the lunar mantle and mare emplacement to modify the original contrast. A useful explanation must reproduce crustal mass, chemistry, chronology and volcanic distribution together, and state which observations would distinguish its initial cause.

A useful idealization is a thin sedimentary cover over a felsic upper continental crust, an intermediate middle continental crust, and a more mafic lower continental crust, ending at the Mohorovičić discontinuity at about 35–40 km. The boundaries within the continental crust are approximate compositional divisions, not three universal sharp interfaces.

The important trend is increasing average mafic character with depth, rather than a change from granite directly to peridotite. Granulite describes a metamorphic facies, not a unique chemical composition. The synthesis in Nature and composition of the continental crust: A lower crustal perspective by Roberta L. Rudnick and David M. Fountain combines seismic and petrological evidence for these distinctions.

Today the usual first melt is basaltic melt from the mantle wedge; in a hotter Archean subduction zone, melting of hydrated basaltic crust itself could generate sodic felsic melt of tonalite-trondhjemite-granodiorite composition. Distinguish a primary melt from the evolved melt ultimately added to the upper continental crust.

On the modern Phanerozoic Earth:

This adds juvenile material derived from the mantle; simply remelting old continental crust is reworking, not net juvenile addition. The amount and depth of slab water release depend on its thermal history, as quantified in Subduction factory: 4. Depth-dependent flux of H2O from subducting slabs worldwide by Peter E. van Keken and others.

For the hotter Archean endmember posited in the question, a hotter mantle and a warm descending plate make it easier for hydrated basaltic crust to reach its solidus. Its partial melting can directly make silica-rich, sodium-rich tonalite-trondhjemite-granodiorite liquids, leaving a more mafic residue. Residual garnet and amphibole, and the presence or absence of residual plagioclase, help determine the rare-earth element and strontium signatures. These are not ultramafic liquids merely because the surrounding mantle was hotter.

The contrast is therefore commonly fluid-fluxed mantle melting followed by differentiation today, versus a greater potential contribution from direct melting of hydrated mafic crust in the hotter case. Tonalite-trondhjemite-granodiorite is not unique evidence for subduction: melting of thickened mafic crust can produce similar liquids. Nor are all modern arcs devoid of slab melting. These qualifications are central to The composite Archaean grey gneisses: Petrological significance, and evidence for a non-unique tectonic setting for Archaean crustal growth by Jean-François Moyen.

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.

An intrusive rock containing quartz and predominantly plagioclase rather than alkali feldspar; it is one member of tonalite-trondhjemite-granodiorite.