Jihua Hao

Dr. Jihua Hao

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Research Focus & Metrics

Academic Career Length

10Years (2017-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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12 February 2021 in Science
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MTMing Tang
Ming Tang
XCXu Chu
Xu Chu
JHJihua Hao
Jihua Hao
BSBing Shen
Bing Shen
A boring billion for mountains: Earth's crust has changed over time as supercontinents formed and broke apart. Tied into this cycle are the building and erosion of high mountains, which are tied to collisions between tectonic plates. Tang et al. use europium anomalies in zircons to estimate the mean thickness of crust over Earth's history. This proxy shows that mountain building has not always been as active as it is today or as it was very early in Earth's history. Mountain building, and the subsequent erosion, was less intense for about a billion years, roughly correlated with a so-called “boring billion” period of biological evolution. Science , this issue p. 728

17 April 2023 in Nature Geoscience
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CWCraig R. Walton
Craig R. Walton
SESophia Ewens
Sophia Ewens
JCJohn Coates
John Coates
RBRuth E. Blake
Ruth E. Blake
NPNoah J. Planavsky
Noah J. Planavsky
Matthew PasekMatthew Pasek
Matthew Pasek

1 July 2020 in Geochimica et Cosmochimica Acta
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Journal Article
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JHJihua Hao
Jihua Hao
AKAndrew H. Knoll
Andrew H. Knoll
FHFang Huang
Fang Huang
JSJuergen Schieber
Juergen Schieber
RHRobert M. Hazen
Robert M. Hazen
IDIsabelle Daniel
Isabelle Daniel

1 March 2020 in Geochimica et Cosmochimica Acta
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Journal Article
Closed access
JHJihua Hao
Jihua Hao
AKAndrew H. Knoll
Andrew H. Knoll
FHFang Huang
Fang Huang
RHRobert M. Hazen
Robert M. Hazen
IDIsabelle Daniel
Isabelle Daniel

1 January 2017 in Earth and Planetary Science Letters
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Journal Article
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JHJihua Hao
Jihua Hao
DSDimitri A. Sverjensky
Dimitri A. Sverjensky
RHRobert M. Hazen
Robert M. Hazen

19 September 2022 in Proceedings of the National Academy of Sciences
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JHJihua Hao
Jihua Hao
CGChristopher R. Glein
Christopher R. Glein
FHFang Huang
Fang Huang
NYNathan Yee
Nathan Yee
DCDavid C. Catling
David C. Catling
RHRobert Hazen
Robert Hazen
Saturn’s moon Enceladus has a potentially habitable subsurface water ocean that contains canonical building blocks of life (organic and inorganic carbon, ammonia, possibly hydrogen sulfide) and chemical energy (disequilibria for methanogenesis). However, its habitability could be strongly affected by the unknown availability of phosphorus (P). Here, we perform thermodynamic and kinetic modeling that simulates P geochemistry based on recent insights into the geochemistry of the ocean–seafloor system on Enceladus. We find that aqueous P should predominantly exist as orthophosphate (e.g., HPO42−), and total dissolved inorganic P could reach 10−7to 10−2mol/kg H2O, generally increasing with lower pH and higher dissolved CO2, but also depending upon dissolved ammonia and silica. Levels are much higher than <10−10mol/kg H2O from previous estimates and close to or higher than ∼10−6mol/kg H2O in modern Earth seawater. The high P concentration is primarily ascribed to a high (bi)carbonate concentration, which decreases the concentrations of multivalent cations via carbonate mineral formation, allowing phosphate to accumulate. Kinetic modeling of phosphate mineral dissolution suggests that geologically rapid release of P from seafloor weathering of a chondritic rocky core could supply millimoles of total dissolved P per kilogram of H2O within 105y, much less than the likely age of Enceladus’s ocean (108to 109y). These results provide further evidence of habitable ocean conditions and show that any oceanic life would not be inhibited by low P availability.