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REVIEW 4 major objections 6 minor 185 references

Earths composition: origin, evolution and energy budget

T0 review · 4 major / 6 minor · reviewed 2026-08-16 · deepseek-v4-flash

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Pith's one-line read Geoneutrino measurements place Earth's radiogenic power at about 20 terawatts and fix the bulk silicate Earth's refractory element enrichment at 2.5 to 2.7 times CI chondrite.

desk verdict Useful review with an updated BSE table, but the headline geoneutrino claim overstates what the data show and the paper's own uncertainty budget undercuts its rejection claim. read the letter →

arxiv 2505.02641 v2 pith:UMC6ZEQH submitted 2025-05-05 physics.geo-ph astro-ph.EPastro-ph.SR

William F McDonough This is my paper · ORCID
classification physics.geo-phastro-ph.EPastro-ph.SR
keywords bulksilicateEarthgeoneutrinoradiogenicheatproductionpyroliterefractorylithophileelementsCIchondriteplanetaryaccretionmantleconvection
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper sets out to show that the Earth's radiogenic power supply is now a measured quantity, not a free parameter: the combined geoneutrino signal recorded by detectors in Japan and Italy puts the total at about 20 terawatts, with roughly 13 from the mantle and 7 from the continental crust. This matters because Earth's surface heat loss is 46 terawatts, so the radioactive fraction determines how much primordial heat remains to drive mantle convection, plate tectonics, and the geodynamo. The same data fix the bulk silicate Earth's refractory lithophile elements at 2.5 to 2.7 times CI chondrite, which narrows the range of acceptable compositional models of the planet. Along the way, the paper argues that the rocky planets are not direct compositional copies of the Sun or of CI chondrites, and that Earth assembled rapidly from differentiated inner-solar-system planetesimals.

What carries the argument

The load-bearing object is the geoneutrino: an electron antineutrino produced by beta decay of uranium and thorium in the Earth's interior. Counting geoneutrinos with liquid-scintillator detectors gives the only direct, whole-planet measure of the U and Th budget, which is then converted into terawatts of radiogenic power. The conversion rests on a model of each detector's local lithosphere, which supplies about half the signal, plus a mantle contribution of about a quarter and a distant-lithosphere contribution of about a quarter; the paper shows that changing the local model (adding the U- and Th-rich Tuscan magmatic rocks near the Italian detector) moves the mantle power estimate from 30 TW down to about 20 TW. A second supporting device is the pyrolite compositional model of the bulk silicate Earth, built from peridotite residues and basalt melts, which fixes the refractory lithophile elements at 2.65 times CI and supplies the Th and U abundances (20.6 ppbw U, Th/U about 3.8) that the geoneutrino results are compared against. The paper also uses a newly precise Pb-isotope ratio (KPb = 3.90) to tie the BSE's Th/U to the chondritic value independently of the neutrino data.

What would settle it

Run the same geoneutrino inversion for a new detector with an independently characterized local crust, for example JUNO; if the total radiogenic power required to fit its observed signal falls outside the 12 to 28 TW range, the paper's 20 TW claim is wrong.

Watch

Extended reading notes

Core claim

The paper's central discovery claim is that Earth has about 20 TW of present-day radiogenic power, derived from the U and Th content of the whole planet as seen in geoneutrino flux. It reports that the mantle produces about 13±8 TW and the continental crust about 7±1 TW, leaving about 26 TW of surface heat flux to be primordial in origin. A combined analysis of the two geoneutrino experiments also places the bulk silicate Earth's refractory lithophile element enrichment at 2.5 to 2.7 times CI carbonaceous chondrite, consistent with a pyrolite mantle composition. The paper further concludes that the bulk Earth and Mars share a refractory enrichment of about 1.9 times CI, while Earth is more volatile-depleted and less oxidized than Mars. These results are presented as an update and confirmation of earlier compositional models, now tied to a direct measurement of the planet's radioactive content.

Load-bearing premise

The 20 terawatt number assumes that the uranium and thorium content of the rocks within a few hundred kilometers of each neutrino detector is known well enough to subtract; roughly half of the measured signal comes from this local crust, and the paper shows that changing one regional rock package shifts the mantle estimate by 10 terawatts.

Editorial extensions

If this is right

  • About 26 TW of Earth's 46 TW surface heat flux would be non-radiogenic, implying substantial primordial power from core cooling and mantle secular cooling rather than radioactive decay.
  • BSE models with roughly 30 ppb U and 30 TW of radiogenic power, the high end of the published range, would be rejected at the 1-sigma level by geoneutrino data.
  • The continental crust would hold 30 to 40 percent of the planet's potassium, thorium, and uranium, which requires mantle processing beyond the upper 660 km and supports whole-mantle convection.
  • The bulk Earth's refractory element enrichment would be about 1.9±0.2 times CI, a tighter anchor for planetary accretion models than the earlier factor-of-three spread among BSE models.
  • New detectors with longer exposure or larger target mass will provide a direct, independent check of the 20 TW budget within a few years.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • The sensitivity of the result to local geology suggests that every future geoneutrino site should be paired with a pre-registered, high-resolution crustal model; otherwise the mantle component remains hostage to the same 10 TW swings seen at Borexino.
  • If the 20 TW budget is correct, then any geochemical model invoking a large hidden reservoir of heat-producing elements in the deep mantle or core would need to store those elements without contributing to the geoneutrino flux, which is physically difficult; the paper's Th/U constraint already hints at this tension.
  • Extending the method to a mobile ocean-bottom detector, which the paper mentions as a future goal, would test whether the mantle's U and Th are as homogeneous as the pyrolite model assumes; strong lateral variation in geoneutrino flux would challenge the single-value BSE budget.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

4 major / 6 minor

Summary. The paper is a broad review and reinterpretation of Earth's bulk composition, origin, and energy budget. It updates the McDonough and Sun (1995) bulk silicate Earth (BSE) model, argues that the terrestrial planets are neither solar-photosphere nor CI-chondrite analogs, and uses the NC/CC meteorite dichotomy to frame early solar system accretion. The central quantitative claims are that KamLAND and Borexino geoneutrino data affirm a present-day radiogenic power of about 20 TW (abstract: "≤20 TW"; text: "20±8 TW"), that the BSE has refractory lithophile elements at 2.5–2.7 times CI chondrite, and that bulk Earth and Mars are enriched in refractory elements by about 1.9 times CI. The paper also discusses mantle convection, volatile and noble gas budgets, core composition, and future neutrino geoscience experiments.

Significance. If the 20 TW geoneutrino result were robust, it would be a landmark global-scale constraint on Earth's radioactive heat budget and would help discriminate among competing BSE compositional models. The paper's most useful contributions are the updated BSE table (Table 3), the side-by-side comparison of published BSE models and their heat production (Table 4), the clear separation of the geochemical BSE derivation from the geoneutrino measurement, and the careful discussion of biases in the meteorite record. The paper is transparent about the subjective nature of many abundance uncertainties and explicitly states that a full error propagation is not possible, which is an honest and important caveat. However, several of the headline statements, especially the abstract's "≤20 TW" and the 1σ rejection of >2.5× CI models, go beyond what the paper's own uncertainty budget supports. The future SNO+ and JUNO measurements are correctly identified as tests that could sharpen or overturn the present inference.

major comments (4)
  1. [Section 8, abstract] The claim that "at the 1σ level, the geoneutrino data reject bulk Earth compositional models that propose high concentrations of refractory lithophile elements (>2.5× CI)" is not supported by the paper's own quoted uncertainty. The text gives a total radiogenic power of 20±8 TW, i.e., a 1σ interval of 12–28 TW. Table 4 lists Palme and O'Neill (2014) at 21.6 TW with U = 22.9 ppbw (about 2.9× CI) and Jagoutz et al. (1979) at 23.8 TW with U = 26 ppbw (about 3.3× CI); both models exceed 2.5× CI and both fall inside the 12–28 TW interval. Only the Turcotte and Schubert (2002) model at 29.3 TW lies outside. The data therefore favor, but do not reject at 1σ, the >2.5× CI class of models. This statement should be softened or the uncertainty must be reduced.
  2. [Abstract / Section 8] The abstract states that geoneutrino data "affirm that the Earth has ≤20 TW of radiogenic power," while Section 8 reports "a total of 20±8 TW." These are materially different statements: a symmetric 1σ interval of 12–28 TW cannot be summarized as one-sided upper bound of 20 TW without an explicit prior or a one-sided statistical treatment. The abstract either must be revised to "20±8 TW" or the paper must justify the change to a one-sided claim. As written, the two statements are internally inconsistent and the stronger abstract claim is not derived from the quoted uncertainty.
  3. [Section 8] The quoted uncertainty of 20±8 TW appears to omit the dominant geological-model uncertainty. The text correctly states that the local lithosphere contributes about 50% of the geoneutrino signal and then describes how including the Tuscan magmatic rocks in the Borexino near-field model changed the mantle estimate from 30 TW to 20 TW, a 10 TW shift. That model-driven shift is comparable to or larger than the quoted mantle uncertainty of ±8 TW. Unless the quoted uncertainties already propagate the full covariance of the crustal models around KamLAND and Borexino, the total uncertainty is understated and the "20 TW affirmation" is not a robust experimental result but a model-dependent estimate. The paper should either include this term in the uncertainty budget or explicitly state that the 20 TW value is conditional on the adopted crustal models.
  4. [Section 6.4 / Table 3] Section 6.4 states that "one cannot conduct a full and rigorous error propagation of all of the uncertainties as is carried out in physics experiments" and describes the Table 3 uncertainties as "a subjective judgment." Given that admitted limitation, the abstract's wording that the data "set the proportions of refractory lithophile elements in the bulk silicate Earth at 2.5 to 2.7 times that in CI chondrites" overstates the certainty of the BSE model. The EFRLE value of 2.65 and its range are not derived through a formal statistical procedure, and the same subjective uncertainties feed into the heat-production comparison in Table 4. The paper should either supply a more rigorous uncertainty for EFRLE or qualify the abstract's claim as an estimate rather than a determination.
minor comments (6)
  1. [Section 8] The word "terrawatts" should be "terawatts."
  2. [Section 3] The sentence "a PPD is a rotating gas and dust cloud with a composition comparable to that of the its star" contains a duplicated article; it should read "that of its star."
  3. [Section 9] The text refers to a "T50 accretion age" for Mars, but the same section uses "τaccretion"; the notation should be made consistent and the typo corrected.
  4. [Section 9] The specific heat capacity is given as "1,000 J kg−1 s−1"; the correct unit for specific heat capacity is J kg−1 K−1.
  5. [Abstract] The abstract contains "the Suns O/Fe," which should be "the Sun's O/Fe" with an apostrophe.
  6. [Section 8] The phrase "the closet 250 km" appears to be a typo for "the closest 250 km" or "the nearest 250 km"; please clarify.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the BSE composition and geoneutrino interpretation rest on independent data sources, despite heavy self-citation.

full rationale

The paper's central compositional claim for the bulk silicate Earth is built from peridotite and basalt chemical correlations normalized to CI chondrites (Sections 6.3 and 6.5), not from geoneutrinos. The geoneutrino section (Section 8) interprets measured KamLAND and Borexino fluxes using local lithosphere models and attributes the resulting 20 +/- 8 TW to Abe et al. (2022), Agostini et al. (2020), and the author's own re-analysis, Sammon and McDonough (2022). The measured flux is an external experimental quantity, so the inference of radiogenic power is not a restatement of the BSE model. The paper does contain a statistical overclaim: at 1 sigma, 20 +/- 8 TW does not reject models with 21.6 TW (Palme and O'Neill) or 23.8 TW (Jagoutz) listed in Table 4, and the abstract's '<= 20 TW' conflicts with the text's '20 +/- 8 TW'. That is an internal consistency or correctness issue, not circularity. Self-citations are numerous and some are load-bearing in the sense that the 20 TW estimate comes from the author's own group, but the underlying data are external and the analysis is not shown to use the target BSE model as an input. No equation or fitted parameter is exhibited that reduces a prediction to the paper's own definitions.

Assumptions & free parameters 4 free parameters · 6 assumptions · 0 invented entities

The central claims rest on a chain of domain assumptions about chondrite reference values, mantle homogeneity, and the accuracy of local crustal models around neutrino detectors. The peridotite selection criteria and the EFRLE are effectively fitted choices; the local crustal model is a recognized source of systematic uncertainty.

free parameters (4)
  • EFRLE (BSE enrichment factor for refractory lithophile elements) = 2.65
    Fitted to peridotite sample data in McDonough and Sun (1995); used to set all RLE concentrations in Table 3 (Section 6.5).
  • Mg number of the mantle = 0.89
    Assumed value used to derive FeO and MgO contents of BSE (Section 6.4).
  • DSi and DFe (bulk partition coefficients) = DSi=1, DFe~0.95
    Assumed distribution coefficients for mantle melting (Section 6.4).
  • Borexino near-field crustal model (Tuscan magmatic rocks) = Included high-K, Th, U rocks
    Choice affects mantle radiogenic power estimate from 30 TW to 20 TW (Section 8).
assumptions (6)
  • domain assumption CI chondrite is a reference for solar system non-volatile element composition
    Used as baseline for enrichment factors throughout (Section 6.5).
  • domain assumption Refractory lithophile elements occur in chondritic relative proportions in the BSE
    Underpins use of one enrichment factor for all RLE (Section 6.5).
  • domain assumption The mantle is pyrolitic and largely homogeneous in major elements
    Enters the interpretation of seismic tomography and the BSE model (Section 6.2 and 6.6).
  • ad hoc to paper Peridotite samples with MgO <= 40.5 wt% and [La/Yb]N <2 are representative of BSE
    Selection criteria from McDonough and Sun (1995) used to derive EFRLE (Section 6.3).
  • domain assumption Local geological models around KamLAND and Borexino accurately represent crustal U and Th
    Needed to subtract crustal geoneutrino signal and obtain mantle power (Section 8).
  • domain assumption Core composition is as given in Fischer and McDonough (2025)
    Used to compute bulk Earth composition and heat sources (Section 7).

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Cite this review

Pith. "Pith review of Earths composition: origin, evolution and energy budget." pith.science (2026). https://pith.science/paper/UMC6ZEQH

@misc{pith2026250502641,
  author       = {Pith},
  title        = {Pith review of: Earths composition: origin, evolution and energy budget},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/UMC6ZEQH}},
  note         = {Machine review of arXiv:2505.02641}
}
read the original abstract

One in every two atoms in the Earth, Mars, and the Moon is oxygen; it is the third most abundant element in the solar system. The oxygen isotopic compositions of the terrestrial planets are different from those of the Sun and demonstrate that these planets are not direct compositional analogs of the solar photosphere. Likewise, the Suns O/Fe, Fe/Mg and Mg/Si values are distinct from those of inner solar system chondrites and terrestrial planets. These four elements (O, Fe, Mg, Si) make up about 94% by mass of the rocky planets and their abundances are determined uniquely using geophysical, geochemical and cosmochemical constraints. The rocky planets grew rapidly from planetesimals, most of which were differentiated, having a core and a mantle, before being accreted. Planetary growth in the early stages of protoplanetary disk evolution was rapid and was only partially recorded by the meteoritic record. The noncarbonaceous meteorites (NC) provide insights into the early history of the inner solar system and are used to construct a framework for how the rocky planets were assembled. NC chondrites have chondrule ages that are two to three million years younger than t_zero (the age of calcium-aluminum inclusions, CAI), documenting that chondrites are middle- to late-stage products of solar system evolution. The composition of the Earth, its current form of mantle convection, and the amount of radiogenic power that drives its engine remain controversial topics. Earths dynamics are driven by primordial and radiogenic heat sources. Measurement of the Earths geoneutrino flux defines its radiogenic power and restricts its bulk composition. Using the latest data from the KamLAND and Borexino geoneutrino experiments affirms that the Earth has 20 TW of radiogenic power and sets the proportions of refractory lithophile elements in the bulk silicate Earth at 2.5 to 2.7 times that in CI chondrites.

Figures

Figures reproduced from arXiv: 2505.02641 by the authors.

Figure 1
Figure 1. The weight and atomic proportions of the 8 [PITH_FULL_IMAGE:figures/full_fig_p006_1.png] view at source ↗
Figure 2
Figure 2. The solar chemical abundance curve, with element abundance expressed as A [PITH_FULL_IMAGE:figures/full_fig_p007_2.png] view at source ↗
Figure 3
Figure 3. Comparison of the CI normalized patterns of elements in carbonaceous (circle data points) and [PITH_FULL_IMAGE:figures/full_fig_p009_3.png] view at source ↗
Figures from the paper (6 more)
Figure 4
Figure 4. Figure 4: Log abundances of CI chondrite versus the solar [PITH_FULL_IMAGE:figures/full_fig_p010_4.png]
Figure 5
Figure 5. Figure 5: Mg/Si variation in NC (red) and CC (blue) [PITH_FULL_IMAGE:figures/full_fig_p012_5.png]
Figure 6
Figure 6. Figure 6: Violin plot for µ 142N dcorr. in chondrites and Earth (see text for details). Data for NC (Enstatite and Ordinary chon￾drites; inner solar system) and CC (Carbonaceous chondrites; outer solar system) meteorites are from Frossard et al. (2022). Alternative models (Boyet…
Figure 7
Figure 7. Figure 7: An idealized mantle-normalized diagram illustrating [PITH_FULL_IMAGE:figures/full_fig_p016_7.png]
Figure 8
Figure 8. Figure 8: The abundances of elements in the bulk silicate Earth normalized to Mg and Cl chondrites versus [PITH_FULL_IMAGE:figures/full_fig_p020_8.png]
Figure 9
Figure 9. Figure 9: The radiogenic heat contributions over the first 50 million years of Earth’s history, including that [PITH_FULL_IMAGE:figures/full_fig_p031_9.png]

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    write newline

    " write newline "" before.all 'output.state := FUNCTION n.dashify 't := "" t empty not t #1 #1 substring "-" = t #1 #2 substring "--" = not "--" * t #2 global.max substring 't := t #1 #1 substring "-" = "-" * t #2 global.max substring 't := while if t #1 #1 substring * t #2 gl...

Pith tools

Reviewed August 16, 2026 · model on record in the stance chip above.