Results 101 to 110 of about 1,881 (201)
Microstructure Controls Sublimation Timescales of Exposed Salt‐Rich Ices on Icy Worlds
Abstract Salt‐rich water ice at the surfaces of icy worlds, for example, Europa, Enceladus, and Ceres, is of particular interest for Solar System exploration as it can represent a record of the chemistry and potential habitability of subsurface liquid water. Endogenic salts can originate by gradual freezing of fluids within outer ice layers, or through
Hannah E. Chinnery, Mark G. Fox‐Powell
wiley +1 more source
Abstract Rock fracture surfaces in the crust are essential habitat for microorganisms. Fracture‐groundwater interfaces provide physical substrates for biofilm growth and are sources of carbon, nutrients, and electron donors and acceptors. To better understand geochemical processes impacting fracture surfaces and the subsurface microbiome, we identified
Christopher J. Schuler +5 more
wiley +1 more source
Improving Dryland Depth to Water Table Estimate Using an Integrated Model With Three Submodels
Abstract Investigating dryland phreatic water assets requires an in‐deep understanding of depth to water table (DWT). However, current DWT methods suffer from limited accuracy and demand refinement. Therefor, this study suggests one novel integrated model cascaded by twin, assimilation, and DWT submodels.
Shaohui Chen
wiley +1 more source
Survey strategies for upcoming exoplanet direct imaging missions have considered varying assumptions of prior knowledge. Precursor radial velocity surveys could have detected nearby exo-Earths and provided prior orbit and mass constraints. Alternatively,
Arnaud Salvador +3 more
doaj +1 more source
Vesteris is a large (33 × 27 km) and young (summit age: 0.65–0.010 Ma) intraplate seamount in the Greenland Sea, formed from ocean island basalt (OIB) magmatism.
L. Beloša +7 more
doaj +1 more source
Atmospheric characterization of Earth-like exoplanets through reflected light spectroscopy is a key goal for upcoming direct imaging missions. A critical challenge in this endeavor is the accurate determination of planetary mass, which may influence the ...
Mario Damiano +4 more
doaj +1 more source
Investigating the D" Reflector Beneath the Indian Ocean with Source Arrays
We used seismic P-wave reflections to search for the discontinuity at the top of the D" region beneath the Indian Ocean. Due to a lack of seismic receiver arrays to target this region, we build source arrays using earthquakes in Indonesia and taking ...
Christine Thomas +3 more
doaj +1 more source
The Vulcan Mission to Io: Lessons Learned during the 2022 JPL Planetary Science Summer School
A mission to Jupiter's moon Io, the most volcanically active body in the solar system, was suggested as a priority for the New Frontiers program in the 2013 Planetary Science Decadal Survey.
K. G. Hanley +20 more
doaj +1 more source
Planetary Albedo Is Limited by the Above-cloud Atmosphere: Implications for Sub-Neptune Climates
Energy limits that delineate the “habitable zone” for exoplanets depend on a given exoplanet’s net planetary albedo (or “Bond albedo”). We here demonstrate that the planetary albedo of an observed exoplanet is limited by the above-cloud atmosphere—the ...
Sean Jordan +2 more
doaj +1 more source
The Influence of Planetary Magnetic Fields on Atmospheric Retention and Habitability [PDF]
D. A. Brain +3 more
openalex +1 more source

