Results 131 to 140 of about 3,596 (289)
Atmospheric Dynamics of Terrestrial Planets [PDF]
The solar system presents us with a number of planetary bodies with shallow atmospheres that are sufficiently earthlike in their form and structure to be termed “terrestrial.” These atmospheres have much in common, in having circulations that are driven ...
Vallis, Geoffrey K. +2 more
core +1 more source
An overview of grain boundary engineering in the field of electrocatalysis. ABSTRACT Key electrocatalytic reactions such as HER, OER, ORR, CO2RR, and NRR offer promising routes for storing renewable energy as chemical fuels. However, their widespread application is constrained due to the lack of highly active and stable catalysts. Grain boundaries (GBs)
Jingyu Gao +8 more
wiley +1 more source
Extreme Shock Pressures: Recovery and Detection of Microfossils. [PDF]
In this thesis an experimental method is utilised to test the viability and suitability of algal microfossils in the context of simulating the shock phase of lithopanspermia.
Yolland, Lawrence
core
Forming Mercury from Excited Initial Conditions
Mercury is notoriously difficult to form in Solar System simulations, due to its small mass and iron-rich composition. Smooth particle hydrodynamics simulations of collisions have found that a Mercury-like body could be formed by one or multiple giant ...
Jennifer Scora +3 more
doaj +1 more source
This review focuses on multielectron redox regulation across molecular and hybrid architectures for photocatalytic CO2 reduction, covering intrinsic POM photocatalysts, photosensitizer‐assisted assemblies, POM–metal–organic complexes, and POM‐integrated semiconductors and MOF/COF heterostructures to link structural motifs with charge transport, product
Bonan Li, Xiaowen Ruan, Sai Kishore Ravi
wiley +1 more source
Size–Frequency Distribution of Terrestrial Leftover Planetesimals and S-complex Implanted Asteroids
The isotopic composition of meteorites linked to S-complex asteroids has been used to suggest that these asteroids originated in the terrestrial planet’s region, i.e., within 1.5 au, and later got implanted into the main asteroid belt (MAB).
Rogerio Deienno +5 more
doaj +1 more source
Abstract – We compare the ion foreshocks of the solar system’s four terrestrial planets by applying the numerical three-dimensional (3D) global hybrid-particle model RHybrid (paRallel Hybrid). The RHybrid model is a high-performance computing framework that describes space plasma in an ion-kinetic, collisionless particle formulation with self ...
Honkonen Ilja +4 more
openaire +1 more source
Effect of Sequential and Combined Space‐Based Stressors on Perovskite Solar Cell Stability
A correlation between loss in performance and mobile ion concentration has been established by sequential stressing of perovskite solar cells under Low Earth Orbit conditions with exposure to protons, light, and thermal cycling. It is shown that the loss in performance increases when ion concentration increases and vice versa.
Saivineeth Penukula +9 more
wiley +1 more source
Comparison Charts of Geological Processes: Terrestrial Planets [PDF]
This chart presents information on the geological processes (volcanism, impact cratering, tectonics, and gradation) that have affected the Earth, Moon, and the terrestrial planets.
core
Two-source Terrestrial Planet Formation with a Sweeping Secular Resonance
The models that most successfully reproduce the orbital architecture of the solar system terrestrial planets start from a narrow annulus of material that grows into embryos and then planets.
Max Goldberg +2 more
doaj +1 more source

