Results 231 to 240 of about 86,334 (311)
Non-geodesic timelike observers and the ultralocal limit. [PDF]
Saadati R, Valsan L, Faraoni V.
europepmc +1 more source
Differentiating Plumes and Local Torus Segments of Enceladus
Abstract Enceladus's south polar plumes and their surrounding torus segments (local plasma regions formed by plume material diffusion) are key to understanding its magnetospheric interaction; however, clear observational criteria to distinguish them remain lacking.
Shangchun Teng +6 more
wiley +1 more source
Massless and massive scalar shell dynamics from rotating BTZ black holes with nonminimally coupled scalar fields. [PDF]
Javed F +6 more
europepmc +1 more source
Impact Reactivation of a Hydrothermal System in Basalt in the Vargeão Dome Impact Structure, Brazil
Abstract As hydrous minerals have been observed in impact craters on Mars, impact‐generated hydrothermal systems (IGHSs) have been considered as potential habitats for life on that planet. The Vargeão Dome, a 12 km wide impact structure in southern Brazil, was formed in basalts with at least two hydrothermal alteration stages.
Jitse Alsemgeest +5 more
wiley +1 more source
"Sun brings all things": Sun and moon lore as biocultural knowledge on Aneityum island, Vanuatu. [PDF]
Harrison KD +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
Comparing the motion of dark matter and standard model particles on cosmological scales. [PDF]
Grimm N, Bonvin C, Tutusaus I.
europepmc +1 more source
Abstract Throughout Gale crater on Mars, the Curiosity rover has found high abundances (15–73 wt%) of X‐ray amorphous materials in the rocks and sediments. The composition of this amorphous fraction is primarily calculated by subtracting crystalline abundances measured by the Chemistry & Mineralogy X‐Ray Diffractometer (CheMin) from bulk elemental ...
R. J. Hopkins, A. D. Rogers, L. Ehm
wiley +1 more source

