Results 211 to 220 of about 458,695 (311)
Recent Advances in Gels for Water Treatment. [PDF]
Chiriac AL, Sarbu A, Zaharia A.
europepmc +1 more source
Impact‐Generated Mixing, Melting and Vaporization of the Early Earth's Crust
Abstract Earth's primary accretion was followed by a protracted flux of interplanetary collisions by leftover planetesimals. The effects of the largest collisions—with bodies possibly exceeding 1,000 km diameter—would have been devastating for terrestrial near‐surface environments.
S. Marchi +3 more
wiley +1 more source
Planetary health and non-communicable diseases-A converging global crisis. [PDF]
Kakaraparthi VN +5 more
europepmc +1 more source
Abstract Hyper‐velocity impacts on planetary surfaces lead to impact craters whose morphology evolves due to exogenous factors such as atmospheric processes, as well as endogenous factors including tectonic and metamorphism. On Earth, erosion processes driven by climate (fluvial, aeolian, glacial processes) progressively erase these structures, or even
Lounis Ait Oufella +3 more
wiley +1 more source
BepiColombo cruise science: overview of the mission contribution to heliophysics. [PDF]
Sánchez-Cano B +82 more
europepmc +1 more source
Assessing Pb Isotopic Equilibrium Between Apatite and K‐Feldspar
Abstract Quantifying common Pb, the non‐radiogenic Pb present in a mineral independent of in situ U decay, is essential for obtaining accurate U–Pb ages in common Pb‐bearing minerals such as apatite. However, constraining the amount and composition of common Pb, as well as the timing of its entrapment, remains a persistent challenge.
Priyanjan Datta +3 more
wiley +1 more source
Warm, water-depleted rocky exoplanets with surface ionic liquids: A proposed class for planetary habitability. [PDF]
Agrawal R +8 more
europepmc +1 more source
Origin of the Bulge Topography Within Caloris Basin, Mercury
Abstract Caloris basin on Mercury has a massive circular bulge topography imprinted with unique fault sets. A variety of deformational processes have been proposed to have influenced their formation, including both global contraction and basin evolution, as well as the deposition and weight of the volcanic infill.
G. Schmidt +6 more
wiley +1 more source

