Evidence map›Paper›PMID 38976765›Full record

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

Sediment subduction in Hadean revealed by machine learning.

Jilian Jiang, Xinyu Zou, Ross N Mitchell, Yigang Zhang, Yong Zhao, Qing-Zhu Yin, Wei Yang, Xiqiang Zhou, Hao Wang, Christopher J Spencer and 5 more

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 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Review
  2. Review
  3. Interstep compatibility of a model for the prebiotic synthesis of RNA consistent with Hadean natural history.Proceedings of the National Academy of Sciences of the United States of America · 2025
    Article
  4. Article
  5. 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

15 authors.

Jilian Jiang *State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.ORCID 0000-0002-1170-8982
Xinyu Zou *Key Laboratory of Mineral Resources, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.
Ross N MitchellState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.ORCID 0000-0002-5349-7909
Yigang ZhangKey Laboratory of Computational Geodynamics, College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China.ORCID 0000-0002-8632-297X
Yong ZhaoState Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, People's Republic of China.
Qing-Zhu YinDepartment of Earth and Planetary Sciences, University of California, Davis, CA 95616.ORCID 0000-0002-4445-5096
Wei YangCollege of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China.ORCID 0000-0001-6267-4981
Xiqiang ZhouCollege of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China.ORCID 0009-0007-6662-8692
Hao WangState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.ORCID 0000-0002-0021-7563
Christopher J SpencerDepartment of Geological Sciences and Geological Engineering, Queen's University, Kingston, ON K7L 3N6, Canada.ORCID 0000-0003-4264-3701
Xiaocai ShanState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.
Shitou WuState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.
Guangming LiCollege of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China.
Kezhang QinCollege of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China.
Xian-Hua LiState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, People's Republic of China.ORCID 0000-0001-5512-7736

Funding

Kezhang Qin 2019QZKK0806Ross N. Mitchell 41888101Ross N. Mitchell XDB0710000Wei Yang D020203Xinyu Zou 42003021Xiqiang Zhou 41890833Yigang Zhang XDB18000000
6 · The paper itself

Abstract

Due to the scarcity of rock samples, the Hadean Era predating 4 billion years ago (Ga) poses challenges in understanding geological processes like subaerial weathering and plate tectonics that are critical for the evolution of life. The Jack Hills zircon from Western Australia, the primary Hadean samples available, offer valuable insights into magma sources and tectonic genesis through trace element signatures. However, a consensus on these signatures has not been reached. To address this, we developed a machine learning classifier capable of deciphering the geochemical fingerprints of zircon. This allowed us to identify the oldest detrital zircon originating from sedimentary-derived "S-type" granites. Our results indicate the presence of S-type granites as early as 4.24 Ga, persisting throughout the Hadean into the Archean. Examining global detrital zircon across Earth's history reveals consistent supercontinent-like cycles from the present back to the Hadean. These findings suggest that a significant amount of Hadean continental crust was exposed, weathered into sediments, and incorporated into the magma sources of Jack Hills zircon. Only the early operation of both subaerial weathering and plate subduction can account for the prevalence of S-type granites we observe. Additionally, the periodic evolution of S-type granite proportions implies that subduction-driven tectonic cycles were active during the Hadean, at least around 4.2 Ga. The evidence thus points toward an early Earth resembling the modern Earth in terms of active tectonics and habitable surface conditions. This suggests the potential for life to originate in environments like warm ponds rather than extreme hydrothermal settings.

Indexed as

Hadeanmachine learningS-type granitesubductionzircon

Identifiers

PMID38976765
PMCPMC11287277

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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.