Evidence map›Paper›PMID 42120414›Full record

ArticleNature communications2026

Manganese (Hydr)oxides record the dynamic evolution of a million-year Hesperian Ocean in Utopia Planitia, Mars.

Bingxu Hou, Heng Sun, Zhaoyang Hu, Chunjiang Li, Dingquan Xue, Yanzhang Li, Yong Lai, Yuxuan Hu, Ziyu Wang, Honglei Lin and 5 more

Abstract read
In one paragraph

Article in Nature communications, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 3 papers.

0numbers the graph read from it
0cells of the map it votes in
3citing 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

3 citing papers in PubMed.

  1. Review
  2. Review
  3. 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.

Bingxu Hou *SKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.ORCID http://orcid.org/0000-0001-8136-1083
Heng Sun *School of Astronautics, Beihang University, Beijing, China.
Zhaoyang HuSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.ORCID http://orcid.org/0009-0006-9748-6570
Chunjiang LiSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.
Dingquan XueSchool of Astronautics, Beihang University, Beijing, China.
Yanzhang LiSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.ORCID http://orcid.org/0000-0002-3312-3256
Yong LaiSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.
Yuxuan HuSchool of Astronautics, Beihang University, Beijing, China.ORCID http://orcid.org/0009-0002-9009-0312
Ziyu WangKey Laboratory of Planetary Science and Frontier Technology, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
Honglei LinKey Laboratory of Planetary Science and Frontier Technology, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.ORCID http://orcid.org/0000-0002-9945-5050
Jiaqi ZhuSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.
Tianci HuaSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.
Anhuai LuSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China.ORCID http://orcid.org/0000-0002-8521-482X
Xiangzhi BaiSchool of Astronautics, Beihang University, Beijing, China. jackybxz@buaa.edu.cn.ORCID http://orcid.org/0000-0002-6115-8237
Yan LiSKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China. liyan-pku@pku.edu.cn.ORCID http://orcid.org/0000-0002-0347-7774

Funding

National Natural Science Foundation of China (National Science Foundation of China) 42372049, 42192502, 42550210, 62271016Natural Science Foundation of Beijing Municipality (Beijing Natural Science Foundation) 4222007
6 · The paper itself

Abstract

The duration and dynamic evolution of surface water on Mars are key to understanding its past habitability. Utopia Planitia, Mars' largest northern basin, preserves mineralogical signatures of ancient aqueous activity that remains chronologically unconstrained. Here, we present the quantitative reconstruction of the Hesperian Ocean's lifecycle using spectral analysis of manganese (Mn) (hydr)oxides as paleohydrological markers. Our innovative Spectral Contrastive-Aware Network, a deep learning framework trained on 13,742 infrared spectra of Martian soil simulants, decodes short-wave infrared data from China's Zhurong rover and orbiters operated by ESA and NASA. We identify altitude-dependent Mn (hydr)oxides enrichment that forms a distinctive mineralogical "bathtub ring", indicating an ancient ocean with defined boundaries. By quantitative mapping the spatiotemporal distribution of these minerals, we reconstruct the ocean's origin, expansion, regression, and extinction. Depositional modeling constrains its lifespan to 0.8-1.5 million years, providing the chronometrically constrained evidence for sustained surface water stability during the Hesperian.

Identifiers

PMID42120414
PMCPMC13377089

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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.