ArticleScience advances2021
Late accretionary history of Earth and Moon preserved in lunar impactites.
Article in Science advances, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.
What it found
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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.
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.
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Who cites it
7 citing papers in PubMed.
- 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 · 2026Article
- Differentiated planetesimals record differing sources of sulfur in inner and outer solar system materials.Proceedings of the National Academy of Sciences of the United States of America · 2025Article
- Review
- Terrestrial atmospheric ion implantation occurred in the nearside lunar regolith during the history of Earth's dynamo.Communications earth & environment · 2025Article
- Automated Mineralogy Analysis of the Apollo 17 73002 Continuous Core Thin Sections Using QEMSCAN Mapping Techniques.Journal of geophysical research. Planets · 2024Article
- Long-term reduced lunar mantle revealed by Chang'e-5 basalt.Nature communications · 2024Article
- Origin of water in the Moon.National science review · 2024Article
Corrections and comments
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Authors and funding
2 authors.
Funding
No grant is acknowledged in the PubMed record.
Abstract
Late accretion describes the final addition of Earth’s mass following Moon formation and includes a period of Late Heavy Bombardment (LHB), which occurred either as a short-lived cataclysm triggered by a late giant planet orbital instability or a declining bombardment during late accretion. Using genetically characteristic ruthenium and molybdenum isotope compositions of lunar impact–derived rocks, we show that the impactors during the LHB and the entire period of late accretion were the same type of bodies and that they originated in the terrestrial planet region. Because a cataclysmic LHB would have, in part, resulted in compositionally distinct projectiles, we conclude that the LHB reflects the tail end of accretion. This implies that the giant planet orbital instability occurred during the main phase of planet formation. Last, because of their inner solar system origin, late-accreted bodies cannot be the primary source of Earth’s water.
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Registered trials
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