GIG OpenIR  > 同位素地球化学国家重点实验室
Zhangzhou, J.1; Li, Yuan2; Chowdhury, Proteek3; Sen, Sayan4; Ghosh, Urmi5,6; Xu, Zheng2; Liu, Jingao7; Wang, Zaicong8; Day, James M. D.9
Predicting sulfide precipitation in magma oceans on Earth, Mars and the Moon using machine learning
Source PublicationGEOCHIMICA ET COSMOCHIMICA ACTA
ISSN0016-7037
2024-02-01
Volume366Pages:237-249
DOI10.1016/j.gca.2023.11.029
Language英语
WOS Research AreaGeochemistry & Geophysics
AbstractThe sulfur content at sulfide saturation (SCSS) of a silicate melt can regulate the stability of sulfides and, therefore, chalcophile elements' behaviors in planetary magma oceans. Many studies have reported high-pressure experiments to determine SCSS using either linear or exponential regressions to parameterize the thermodynamics of the system. Although these empirical equations describe the effects of different parameters on SCSS, they perform poorly when predicting laboratory measurements. Here, we compiled 542 published analyses of experiments performed on a range of sulfide and silicate compositions at varying P-T conditions (<24 GPa, <2673 K). Using empirical equations, linear regression, Random Forest algorithms, and a hybrid algorithm employing empirical fits to P-T conditions and the Random Forest algorithm for compositions, we developed several SCSS models and compared them to laboratory measurements. The Random Forest and hybrid models (R-2 = 0.82-0.91, mean average error [MAE] < 746 ppmw S, residual mean standard error [RMSE] < 972 ppmw S), significantly outperform previous empirical models (R-2 = 0.28-0.69, MAE = 622-1,170 ppmw S, RMSE = 1,070-1,744 ppmw S), whereas linear regression performs moderately well, i.e., between the classic and machine learning models. We applied our hybrid model to predict SCSS during magma ocean solidification on Earth, Mars, and the Moon, and we compared our model results to expected S contents in the residual magma oceans calculated by mass balance. Our results confirm that during early accretion, sulfides precipitated from magma oceans and into the outer cores of Earth and Mars, but not the Moon. Subsequently, once the respective magma oceans began precipitating minerals with increasingly FeO-rich and SiO2-, Al2O3-, and MgO-depleted compositions, the increasing S concentration in the residual magma was offset by temperature and compositional effects on SCSS, preventing sulfide precipitation during intermediate stages of crystallization. Sulfides precipitated late during magma ocean crystallization, but failed to percolate through the underlying crystalline mantle, significantly contributing to the modern bulk-silicate sulfur abundances of Earth, Mars, and the Moon. Our calculations suggest that late-stage sulfide precipitation occurred at shallow depths of 120-220 km, 40-320 km, and < 10 km in the magma oceans of Earth, Mars, and the Moon, respectively.
KeywordSCSS Machine learning Sulfide Magma ocean
WOS IDWOS:001163315800001
Indexed BySCI
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.gig.ac.cn/handle/344008/76305
Collection同位素地球化学国家重点实验室
Corresponding AuthorZhangzhou, J.
Affiliation1.Zhejiang Univ, Sch Earth Sci, Key Lab Geosci Big Data & Deep Resource Zhejiang P, Hangzhou, Peoples R China
2.Chinese Acad Sci, Guangzhou Inst Geochem, State Key Lab Isotope Geochem, Guangzhou 510640, Peoples R China
3.Rice Univ, Dept Earth Environm & Planetary Sci, Houston, TX 77005 USA
4.Bengurion Univ Negev, Zuckerberg Inst Water Res, IL-8499000 Ben Gurion, Israel
5.James Hutton Inst, Environm & Biochem Sci, Craigiebuckler, Aberdeen AB15 8QH, Scotland
6.Indian Inst Technol IIT Kharagpur, Dept Geol & Geophys, Kharagpur 721302, India
7.China Univ Geosci Beijing, State Key Lab Geol Proc & Mineral Resources, Beijing, Peoples R China
8.China Univ Geosci, Sch Earth Sci, State Key Lab Geol Proc & Mineral Resources, Wuhan 430074, Peoples R China
9.Univ Calif San Diego, Scripps Inst Oceanog, La Jolla, CA 92093 USA
Recommended Citation
GB/T 7714
Zhangzhou, J.,Li, Yuan,Chowdhury, Proteek,et al. Predicting sulfide precipitation in magma oceans on Earth, Mars and the Moon using machine learning[J]. GEOCHIMICA ET COSMOCHIMICA ACTA,2024,366:237-249.
APA Zhangzhou, J..,Li, Yuan.,Chowdhury, Proteek.,Sen, Sayan.,Ghosh, Urmi.,...&Day, James M. D..(2024).Predicting sulfide precipitation in magma oceans on Earth, Mars and the Moon using machine learning.GEOCHIMICA ET COSMOCHIMICA ACTA,366,237-249.
MLA Zhangzhou, J.,et al."Predicting sulfide precipitation in magma oceans on Earth, Mars and the Moon using machine learning".GEOCHIMICA ET COSMOCHIMICA ACTA 366(2024):237-249.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Zhangzhou, J.]'s Articles
[Li, Yuan]'s Articles
[Chowdhury, Proteek]'s Articles
Baidu academic
Similar articles in Baidu academic
[Zhangzhou, J.]'s Articles
[Li, Yuan]'s Articles
[Chowdhury, Proteek]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Zhangzhou, J.]'s Articles
[Li, Yuan]'s Articles
[Chowdhury, Proteek]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.