Results 171 to 180 of about 382,361 (336)
ABSTRACT Atmospheric deposition of organic pollutants plays a crucial role in the transport and fate of contaminants in the environment, with implications for ecosystem health and human exposure. Persistent organic pollutants (POPs), polycyclic aromatic hydrocarbons (PAHs) and microplastics are increasingly recognized as transboundary threats due to ...
Iva Smoljo +2 more
wiley +1 more source
Icy worlds: Moons and Dwarf Planets
invited review paper, accepted for publication in Oxford Research Encyclopedia of Planetary ...
openaire +2 more sources
Fluid-rock interactions on icy moons
Les missions Cassini-Huygens et Dawn ont révélé des preuves surprenantes de l'altération active des roches d'eau NH3 sur plusieurs mondes glacés du système solaire externe. En particulier, les observations de la petite lune de Saturne Encelade suggèrent qu'elle pourrait même dissimuler une activité hydrothermale active dans un océan d'eau NH3 enrichie ...
openaire +1 more source
Minor epic: Notes toward a different “Anthropoetry”
Abstract Anthropologists have often turned to poetry as a means of accessing emotional registers of which conventional academic prose is unable to avail. In doing so, they have tacitly conflated poetry with lyric poetry, today probably the most widely practiced poetic genre, associated in particular with the expression of inner feelings and subjectival
Stuart McLean
wiley +1 more source
RIME-REASON synergistic opportunities for surface and near-surface investigations of icy moons
Kristian Chan +3 more
openalex +1 more source
A Youthful Titan Implied by Improved Impact Simulations
Abstract The small number of impact craters found on Titan suggests that its surface is relatively young. Previous work estimated its surface age to be between 200 and 1000 Myr. This estimate, however, is based on crater scaling laws for water and sand, which are not representative of the composition of Titan's icy surface.
S. Wakita +3 more
wiley +1 more source
Slantwise Convection and Heat Transport in Icy Moon Oceans
Abstract Ocean heat transport on icy moons shapes the ice shell topography, a primary observable of these moons. Two key processes control the heat transport: baroclinic instability driven by surface buoyancy contrasts and convective instability driven by heating from the core.
Yaoxuan Zeng, Malte F. Jansen
wiley +1 more source
Science of omics: a molecular space odyssey
Experimental Physiology, EarlyView.
Salomé Coppens +3 more
wiley +1 more source

