Evidence map›Paper›PMID 39680771›Full record

ArticleProceedings of the National Academy of Sciences of the United States of America2024

Oxygen isotope identity of the Earth and Moon with implications for the formation of the Moon and source of volatiles.

Meike Fischer, Stefan T M Peters, Daniel Herwartz, Paul Hartogh, Tommaso Di Rocco, Andreas Pack

Abstract read
In one paragraph

Article in Proceedings of the National Academy of Sciences of the United States of America, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 4 papers.

0numbers the graph read from it
0cells of the map it votes in
4citing 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

4 citing papers in PubMed.

  1. Article
  2. Constraints on the impactor flux to the Earth-Moon system from oxygen isotopes of the lunar regolith.Proceedings of the National Academy of Sciences of the United States of America · 2026
    Article
  3. Finding water on the Moon and Mars: Humanity's extraterrestrial future.Proceedings of the National Academy of Sciences of the United States of America · 2024
    Article
  4. Triple oxygen isotopes of lunar water unveil indigenous and cometary heritage.Proceedings of the National Academy of Sciences of the United States of America · 2024
    Article
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

6 authors.

Meike FischerGeowissenschaftliches Zentrum, Abteilung für Geochemie und Isotopengeologie, Georg-August-Universität Göttingen, Göttingen 37077, Germany.ORCID 0000-0003-1558-9594
Stefan T M PetersGeowissenschaftliches Zentrum, Abteilung für Geochemie und Isotopengeologie, Georg-August-Universität Göttingen, Göttingen 37077, Germany.ORCID 0000-0001-6502-8723
Daniel HerwartzInstitut für Mineralogie und Petrologie, Universität Köln, Köln 50674, Germany.ORCID 0000-0003-3604-8295
Paul HartoghMax-Planck-Institut für Sonnensystemfoschung, Abteilung Planeten und Kometen, Göttingen 37077, Germany.ORCID 0000-0002-9550-6551
Tommaso Di RoccoGeowissenschaftliches Zentrum, Abteilung für Geochemie und Isotopengeologie, Georg-August-Universität Göttingen, Göttingen 37077, Germany.
Andreas PackGeowissenschaftliches Zentrum, Abteilung für Geochemie und Isotopengeologie, Georg-August-Universität Göttingen, Göttingen 37077, Germany.ORCID 0000-0002-2618-2768

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The Moon formed 4.5 Ga ago through a collision between proto-Earth and a planetesimal known as Theia. The compositional similarity of Earth and Moon puts tight limits on the isotopic contrast between Theia and proto-Earth, or it requires intense homogenization of Theia and proto-Earth material during and in the aftermath of the Moon-forming impact, or a combination of both. We conducted precise measurements of oxygen isotope ratios of lunar and terrestrial rocks. The absence of an isotopic difference between the Moon and Earth on the sub-ppm level, as well as the absence of isotope heterogeneity in Earth's upper mantle and the Moon, is discussed in relation to published Moon formation scenarios and the collisional erosion of Theia's silicate mantles prior to colliding with proto-Earth. The data provide valuable insights into the origin of volatiles in the Earth and Moon as they suggest that the water on the Earth may not have been delivered by the late veneer. The study also highlights the scientific value of samples returned by space missions, when compared to analyses of meteorite material, which may have interacted with terrestrial water.

Indexed as

EarthMoonoxygen isotopevolatile

Identifiers

PMID39680771
PMCPMC11670184

What OpenQuestion holds

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Registered trials

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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.