Results 41 to 50 of about 151 (127)
Abstract Martian magmas compositionally resemble those from terrestrial continental hotspot magmatic suites, characterized by low OH and high Cl and S contents. The magmatic gases exsolved from such magmas transport a variety of metal complexes and, upon cooling, precipitate vapor‐deposits into vugs and fractures within rocks and on the surfaces of ...
N. Zimmermann, M. Safari, H. Nekvasil
wiley +1 more source
Magnetic Properties of Martian Impact Basins Including the Effect of Mantle Excavation
Abstract The weak magnetism of many impact basins on Mars has historically been interpreted as evidence of the martian dynamo's cessation before ∼4.0 Ga. However, expected magnetic properties of these impact basins are poorly known because basin formation exhumes and recrystallizes mantle material, which has not been sampled by martian meteorites ...
S. C. Steele, R. R. Fu, J. M. D. Day
wiley +1 more source
Abstract Megathrust shear zones are the main fluid transport pathways during the seismic cycle and play a key role in controlling physicochemical alteration. Defining fluid‐rock interaction in wall rocks provides evidence for unraveling the hydrogeology of shear zones and their link to active fluid circulation.
Claudio Robustelli Test +7 more
wiley +1 more source
Magnetic Mineralogy in Lunar Mare Basalts and Implications for Paleointensity Retrieval
Abstract Lunar paleomagnetic studies have identified multidomain metallic Fe–Ni alloys as the dominant magnetic contributors in mare basalts. Here, we explore the low‐temperature magnetic behavior of standard samples for a suite of opaque minerals that occur within mare basalts (single‐domain and multidomain Fe, wüstite, ulvöspinel, iron chromite ...
Ji‐In Jung +6 more
wiley +1 more source
Efficiency of Thermoremanent Magnetization Acquisition in Vortex‐State Particle Assemblies
Abstract Magmatic rocks record ambient magnetic fields during cooling, preserving them for billions of years through thermoremanent magnetization (TRM). TRM accuracy depends on particle size, shape, magnetic properties, and the number of particles available to record the field.
U. D. Bellon +6 more
wiley +1 more source
Exploring the origins of magnetization within the Chicxulub crater upper peak ring
Abstract Large terrestrial impacts may produce vast subsurface hydrothermal systems, capable of generating conditions favorable to the origin of life. Modeling suggests that these systems may persist for >1 million years for basin‐sized craters; however, direct experimental constraints on hydrothermal system duration are needed.
Christina M. Verhagen +13 more
wiley +1 more source
Heterogeneous Electro-Fenton-Catalyzed Degradation of Rhodamine B by Nano-Calcined Pyrite. [PDF]
Tan Y +7 more
europepmc +1 more source
Visualization of nanoscale magnetic domain states in the asteroid Ryugu. [PDF]
Kimura Y +35 more
europepmc +1 more source
The first identification of cronstedtite in Cu-Ni-PGE ores of the Talnakh intrusion. [PDF]
Yakich TY +5 more
europepmc +1 more source
The Influence of Specific Ions and Oxyhydroxo Species in Plant Water on the Bubble-Particle Attachment of Pyrrhotite. [PDF]
October LL +4 more
europepmc +1 more source

