Article
Geochemistry & Geophysics
A. J. P. Guelcher, G. J. Golabek, M. Thielmann, M. D. Ballmer, P. J. Tackley
Summary: The rheological properties of Earth's lower mantle play a crucial role in mantle dynamics and planetary evolution. This study presents a new strain-dependent rheology formulation for lower mantle materials, which has several direct and indirect effects on mantle convection. The results suggest that the new rheology formulation leads to changing dynamics of weakened plume channels, formation of larger thermochemical piles, and increased convective vigor. Furthermore, it may explain the discrepancy between expected and observed thermal anomalies of deep-seated mantle plumes on Earth.
GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS
(2022)
Article
Materials Science, Multidisciplinary
Kaishuai Yang, Xianlong Wang, Jie Zhang, Ya Cheng, Chuanguo Zhang, Zhi Zeng, Haiqing Lin
Summary: The distribution of Fe in MgO plays a critical role in broadening the spin crossover pressure zone, with varied SCPZ depending on Fe concentration. Below a critical temperature, Fe segregation occurs, while above this temperature, entropy-driven randomized Fe distribution leads to broadening of SCPZ, consistent with the high-temperature state of the lower mantle.
Article
Mechanics
Yadan Mao
Summary: This study provides a detailed analysis of continent motion and thermal-mechanic feedback by using a simplified model. The results reveal that plate motion characteristics and frequencies change with plate size, and these changes have significant implications for continent motion and geological evolution.
JOURNAL OF FLUID MECHANICS
(2022)
Article
Geochemistry & Geophysics
A. S. J. Mendez, S. Stackhouse, V Trautner, B. Wang, N. Satta, A. Kurnosov, R. J. Husband, K. Glazyrin, H-P Liermann, H. Marquardt
Summary: The study reveals the elastic bulk modulus softening of (Mg,Fe)O ferropericlase across the iron spin crossover and its significant impact on the physical properties. Experimental and computational results show that the softening effect is sensitive to the distribution of iron in the ferropericlase structure. Mixed-spin (Mg,Fe)O dominates the lower mantle at depths below 1,000 km.
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH
(2022)
Article
Multidisciplinary Sciences
Grace E. Shephard, Christine Houser, John W. Hernlund, Juan J. Valencia-Cardona, Reidar G. Tronnes, Renata M. Wentzcovitch
Summary: This study identifies the predicted seismic expression of the high-to-low iron spin crossover in the deep Earth mineral ferropericlase. The research shows that the iron spin crossover affects seismic wave velocity and indicates the presence of thermochemical heterogeneities in the lower mantle. Results suggest that the global signature of the Fp spin crossover is dampened by non-uniformly distributed heterogeneities in the lower mantle.
NATURE COMMUNICATIONS
(2021)
Article
Multidisciplinary Sciences
Han Hsu, Koichiro Umemoto
Summary: It is found that Fe-bearing MgO undergoes structural and spin transitions under high pressure, which can affect the physical properties of planetary interiors.
NATURE COMMUNICATIONS
(2022)
Article
Geochemistry & Geophysics
Viktoria E. Trautner, Stephen Stackhouse, Alice R. Turner, Paula Koelemeijer, D. Rhodri Davies, Alba San Jose Mendez, Niccolo Satta, Alexander Kurnosov, Hanns-Peter Liermann, Hauke Marquardt
Summary: This study presents the first experimental results on the spin crossover-induced bulk modulus softening at high temperatures in ferropericlase. The existence of spin crossover in the mantle is validated through theoretical calculations and synthetic seismic tomography models. The S-C correlation is found to be a suitable measure for detecting the presence of spin crossover in tomographic models and provides evidence for the presence of ferropericlase in the lower mantle.
EARTH AND PLANETARY SCIENCE LETTERS
(2023)
Article
Geochemistry & Geophysics
Derek Neuharth, Eric Mittelstaedt
Summary: Research suggests that the rate of volcanic eruptions varies over time. Time-series analysis reveals that these rates change periodically over periods of tens of millions of years, indicating fluctuations in the production of molten material in underlying mantle plumes. Many hotspot volcano chains exhibit cycles of approximately 2 to 10 million years, which align with proposed mechanisms for changing near-surface plume flux and melting rate.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2023)
Article
Geochemistry & Geophysics
Mingming Li
Summary: Mantle plumes are deflected by surrounding mantle flow, which carries information of deep mantle dynamics and is used to reconstruct absolute plate motions. This study compares two models for computing deep mantle flow and plume lateral motions and finds that backward models have certain inaccuracies that can be improved with better understanding of the deep mantle structure and dynamics.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2023)
Article
Geochemistry & Geophysics
Erik van der Wiel, Douwe J. J. van Hinsbergen, Cedric Thieulot, Wim Spakman
Summary: Numerical models of Earth's mantle dynamics can predict the vigour and mixing of mantle flow, and the average slab sinking rates are an unexplored parameter that can provide intrinsic information on these characteristics. Through numerical experiments, it has been found that slab sinking rates are strongly correlated with mantle convection and mixing, and may explain geochemical observations from hotspot volcanoes.
EARTH AND PLANETARY SCIENCE LETTERS
(2024)
Article
Geochemistry & Geophysics
Juliane Dannberg, Rene Gassmoller, Ranpeng Li, Carolina Lithgow-Bertelloni, Lars Stixrude
Summary: Phase transitions play a crucial role in mantle convection, affecting the style and evolution of the mantle. Developing new numerical methods can more accurately model the influence of phase transitions on mantle convection, with the thickness of the phase transitions having a significant impact on the style of convection.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2022)
Article
Geochemistry & Geophysics
S. Ghelichkhan, H-P Bunge, J. Oeser
Summary: The text discusses multiple first-order geological events during the Cenozoic that are likely related to mantle flow, and explores their correlation through high-resolution mantle flow retrodictions. The research shows that the mantle flow history is sensitive to present-day mantle state estimates and rheological properties of dynamic Earth models.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2021)
Article
Geochemistry & Geophysics
Ziqiang Yang, Hongsheng Yuan, Lu Liu, Nico Giordano, Yongjin Chen, Li Zhang
Summary: The presence of water may cause compositional heterogeneities in the deep lower mantle. Experiments on the chemical reaction between (Mg,Fe)O and H2O confirmed the formation of FeO2Hx (x ≤ 1, Py-phase) in the deepest lower mantle, serving as a water storage.
AMERICAN MINERALOGIST
(2023)
Article
Geochemistry & Geophysics
Yongming Wang, Mingming Li
Summary: The interaction between mantle plumes and lithosphere leads to various surface expressions, which are influenced by the properties of the plume and lithosphere. Different surface features have different sensitivities to these properties, with melt production being most affected by plume properties.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2021)
Article
Geochemistry & Geophysics
A. G. Semple, A. Lenardic
Summary: The study suggests that the viscosity and flow wavelengths of the mantle are influenced by the non-Newtonian rheology of the upper mantle, resulting in different upper and lower mantle flow dynamics. Through coupled feedback loops, mantle viscosity, flow wavelengths, and the extent to which mantle drives plate motions are interconnected and impact each other.
GEOPHYSICAL JOURNAL INTERNATIONAL
(2021)
Article
Astronomy & Astrophysics
Irene Bonati, Tim Lichtenberg, Dan J. Bower, Miles L. Timpe, Sascha P. Quanz
ASTRONOMY & ASTROPHYSICS
(2019)
Article
Geochemistry & Geophysics
R. Reali, J. M. Jackson, J. Van Orma, D. J. Bower, P. Carrez, P. Cordier
PHYSICS OF THE EARTH AND PLANETARY INTERIORS
(2019)
Article
Geochemistry & Geophysics
R. Dietmar Muller, Sabin Zahirovic, Simon E. Williams, John Cannon, Maria Seton, Dan J. Bower, Michael G. Tetley, Christian Heine, Eline Le Breton, Shaofeng Liu, Samuel H. J. Russell, Ting Yang, Jonathon Leonard, Michael Gurnis
Article
Astronomy & Astrophysics
Dan J. Bower, Daniel Kitzmann, Aaron S. Wolf, Patrick Sanan, Caroline Dorn, Apurva Oza
ASTRONOMY & ASTROPHYSICS
(2019)
Article
Astronomy & Astrophysics
Rob J. Spaargaren, Maxim D. Ballmer, Dan J. Bower, Caroline Dorn, Paul J. Tackley
ASTRONOMY & ASTROPHYSICS
(2020)
Article
Geochemistry & Geophysics
Tim Lichtenberg, Dan J. Bower, Mark Hammond, Ryan Boukrouche, Patrick Sanan, Shang-Min Tsai, Raymond T. Pierrehumbert
Summary: This study presents a coupled numerical framework to investigate the early evolution of Earth-sized rocky planets with idealized clear-sky atmospheres dominated by different volatile elements. The results show that the central metrics of early planetary evolution are controlled by the dominant volatile and outgassing history of the planet, with thermal sequences falling into three general classes based on cooling timescale. The numerical experiments demonstrate the capabilities of the modeling framework to link the interior and atmospheric evolution of rocky exoplanets with multiwavelength astronomical observations.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2021)
Article
Multidisciplinary Sciences
Jiewen Li, Daoyuan Sun, Dan J. Bower
Summary: A mega-sized ULVZ has been discovered at the northern edge of the Pacific LLVP, almost double the size of a previously imaged ULVZ in the region, with half of the shear velocity reduction. It is formed by stable mantle flow converging at the LLVP edge driven by slab-debris in the lower mantle.
NATURE COMMUNICATIONS
(2022)
Article
Astronomy & Astrophysics
Kaustubh Hakim, Meng Tian, Dan J. Bower, Kevin Heng
Summary: Carbonate precipitation in oceans is crucial for maintaining the inorganic carbon cycle and temperate climates. The ocean pH decreases by approximately 0.5 for every tenfold increase in atmospheric carbon dioxide. The upper limit of ocean pH, buffered by carbonate precipitation, defines the pH when the carbon cycle operates, while if the carbonate compensation depth (CCD) resides above the ocean floor, the carbon cycle ceases to operate.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
Alexander Grayver, Dan J. Bower, Joachim Saur, Caroline Dorn, Brett M. Morris
Summary: This article investigates the impact of stellar flares and associated CMEs on the interiors and atmospheres of planets. Using a physical model applied to the TRAPPIST-1 star, the study shows that magnetic flux carried by flare-associated CMEs results in planetary interior heating and leads to geological processes and volcanic activity. These findings are important for maintaining consistency in planetary atmospheric and geological models.
ASTROPHYSICAL JOURNAL LETTERS
(2022)
Article
Geochemistry & Geophysics
Paolo A. Sossi, Peter M. E. Tollan, James Badro, Dan J. Bower
Summary: In this study, the solubility of water in peridotite liquids was determined, providing insights into the nature of early atmospheres on Earth and other rocky planets. The research findings contribute to our understanding of the formation of steam- and carbon-rich atmospheres during magma ocean events.
EARTH AND PLANETARY SCIENCE LETTERS
(2023)
Article
Astronomy & Astrophysics
Aaron S. Wolf, Noah Jaggi, Paolo A. Sossi, Dan J. Bower
Summary: Silicate vapors are crucial for planetary evolution, especially during the early stages of rocky planet formation. Our open-source thermodynamic modeling software VapoRock combines the MELTS liquid model with gas-species properties to calculate the partial pressures of 34 gaseous species in equilibrium with magmatic liquid. The model's accuracy has been validated through experiments and benchmarked against various igneous rock compositions.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Dan J. Bower, Kaustubh Hakim, Paolo A. Sossi, Patrick Sanan
Summary: This study investigates the evolution of magma ocean-atmosphere systems and finds that small initial hydrogen budgets, high C/H ratios, and oxidizing conditions suppress the outgassing of hydrogen, resulting in mainly carbon-rich atmospheres in equilibrium with magma oceans. The high solubility of water limits its outgassing, while processes such as crystal settling and dissolution in crystallizing minerals further constrain the outgassing of hydrogen. This suggests that a significant amount of water can be stored in the interiors of planets during the magma ocean stage.
PLANETARY SCIENCE JOURNAL
(2022)
Article
Astronomy & Astrophysics
Noah Jaeggi, Diana Gamborino, Dan J. Bower, Paolo A. Sossi, Aaron S. Wolf, Apurva V. Oza, Audrey Vorburger, Andre Galli, Peter Wurz
Summary: Messenger observations indicate that a magma ocean may have formed on proto-Mercury, leading to the early atmosphere through evaporation of metals and outgassing of volatiles. Atmospheric escape processes include plasma heating, photoevaporation, Jeans escape, and photoionization, which result in relatively small mass loss rates but do not significantly alter the mantle composition of Mercury.
PLANETARY SCIENCE JOURNAL
(2021)
Article
Astronomy & Astrophysics
Kaustubh Hakim, Dan J. Bower, Meng Tian, Russell Deitrick, Pierre Auclair-Desrotour, Daniel Kitzmann, Caroline Dorn, Klaus Mezger, Kevin Heng
Summary: Weathering of silicate rocks on planetary surfaces plays a crucial role in regulating climate by drawing down CO2 from the atmosphere. The rates of weathering are influenced by surface lithology, with thermodynamics and kinetics exerting control on the process. The temperature sensitivity of thermodynamically limited silicate weathering may lead to a positive feedback to the carbon cycle as surface temperature increases.
PLANETARY SCIENCE JOURNAL
(2021)
Article
Astronomy & Astrophysics
Tobias G. Meier, Dan J. Bower, Tim Lichtenberg, Paul J. Tackley, Brice-Olivier Demory
Summary: The study utilizes observations from the thermal phase curve of LHS 3844b to analyze the planet's interior dynamics and tectonic regimes through numerical models. Three viable convective regimes are identified, with the observation of hemispheric tectonics in certain scenarios.
ASTROPHYSICAL JOURNAL LETTERS
(2021)