Evidence map›Paper›PMID 42789695›Full record

ArticleScience advances2026

Core formation resolves Earth's siderophile excess without a late veneer.

Ingrid Blanchard, Julien Siebert, Lucas Calvo, Sergey S Lobanov, Coline Pinchon, Edith Kubik, Max Wilke, Anja Schreiber, Valentina Bonino, François Guyot and 3 more

Abstract read
In one paragraph

Article in Science advances, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

13 authors.

Ingrid BlanchardSorbonne Université, Muséum National d'Histoire Naturelle, UMR CNRS 7590, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), Paris, France.ORCID 0000-0002-8041-5702
Julien SiebertInstitut de Physique du Globe de Paris, Université Paris Cité, Paris, France.
Lucas CalvoInstitut de Physique du Globe de Paris, Université Paris Cité, Paris, France.ORCID 0000-0001-8304-0769
Sergey S LobanovGFZ Helmholtz Centre for Geosciences, Potsdam, Germany.ORCID 0000-0001-9728-2363
Coline PinchonInstitut de Physique du Globe de Paris, Université Paris Cité, Paris, France.
Edith KubikInstitut de Physique du Globe de Paris, Université Paris Cité, Paris, France.ORCID 0000-0003-2226-8502
Max WilkeInstitut für Geowissenschaften, Universität Potsdam, Potsdam, Germany.ORCID 0000-0002-1890-3940
Anja SchreiberGFZ Helmholtz Centre for Geosciences, Potsdam, Germany.
Valentina BoninoESRF-The European Synchrotron, Grenoble, France.ORCID 0000-0002-3616-5494
François GuyotMuséum National d'Histoire Naturelle, Sorbonne Université, UMR CNRS 7590, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), Paris, France.ORCID 0000-0003-4622-2218
Sylvain PetitgirardDepartment of Earth Sciences, ETH Zürich, Zürich 8025, Switzerland.ORCID 0000-0001-9838-1742
Paraskevas ParisiadesSorbonne Université, Muséum National d'Histoire Naturelle, UMR CNRS 7590, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), Paris, France.ORCID 0000-0001-6962-264X
Nicolas GuignotSynchrotron SOLEIL, Gif-sur-Yvette, France.ORCID 0000-0003-1105-6985

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Highly siderophile elements (HSEs) are expected to be extensively depleted in the mantle due to their affinity for metal during core formation. Yet, their abundances in the mantle far exceed the predictions based on low pressure and low temperature partitioning experiments. In addition, all HSEs are present in similar chondritic relative proportion in the mantle. This has traditionally been attributed to the late accretion of chondritic material, the late veneer. We present laser-heated diamond anvil cell experiments that quantify the partitioning behavior of five HSEs (rhenium, osmium, iridium, palladium, and gold) under pressure-temperature conditions directly relevant to early Earth's magma ocean. Our results demonstrate a substantial decrease in metal-silicate partition coefficients with increasing temperature. Multistage accretion models reproduce the observed HSE abundances and ratios in the mantle without invoking a late veneer. This resolves the longstanding paradox of HSEs excess' in the mantle and suggests that the delivery of volatile compounds to the young Earth is primarily explained by early accretion and differentiation processes.

Identifiers

PMID42789695
PMCPMC13614371

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.