Results 41 to 50 of about 26,344 (179)
NIRCam and MIRI coronagraphy has successfully demonstrated the ability to directly image young sub-Jupiter-mass and mature gas giant exoplanets. However, these modes struggle to reach the sensitivities needed to find the population of cold giant planets ...
Rachel Bowens-Rubin +11 more
doaj +1 more source
During the late stage of planet formation when Mars-size cores appear, interactions among planetary cores can excite their orbital eccentricities, speed their merges and thus sculpture the final architecture of planet systems.
Andrews +38 more
core +1 more source
Field‐Directed Growth of Hematite for Advanced Solar Hydrogen Production
Magnetic field‐assisted chemical vapor deposition enables controlled anisotropic growth of hematite nanostructures, boosting photoelectrochemical performance and ensuring 100 h stability for solar water oxidation reaction. This study employs photoelectrochemistry not only as a performance metric but also as a probing tool to reveal how magnetic field ...
Fabio A. Pires +5 more
wiley +1 more source
Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths
Recent studies have found an observational correlation between the presence of outer giant planets and inner super-Earths, which implies that outer giants do not suppress the formation of super-Earths.
Phoebe Sandhaus +4 more
doaj +1 more source
It has been proposed recently that the first step in the formation of both rocky and gas giant planets is dust sedimentation into a solid core inside a gas clump (giant planet embryo). The clumps are then assumed to migrate closer to the star where their
Binder +21 more
core +1 more source
Impacts of the renewable energy transition on global plant diversity: A review
People and nature need a renewable energy transition to help address the growing, and catastrophic, effects of climate change. A sustainable energy transition involves rigorously examining the potential impacts on nature – including plant life – and creating pathways for impact mitigation that strike a clear balance between energy production and ...
Rachael V. Gallagher +7 more
wiley +1 more source
The Evolution of Jupiter and Saturn as a Function of the Rρ Parameter
Computed using the APPLE planetary evolution code, we present updated evolutionary models for Jupiter and Saturn that incorporate helium rain, nonadiabatic thermal structures, and “fuzzy” extended heavy-element cores.
Ankan Sur +3 more
doaj +1 more source
The formation and habitability of terrestrial planets in the presence of hot jupiters
`Hot jupiters,' giant planets with orbits very close to their parent stars, are thought to form farther away and migrate inward via interactions with a massive gas disk.
Alibert +43 more
core +1 more source
Structure of Jupiter's High‐Latitude Storms: Folded Filamentary Regions Revealed by Juno
Abstract Sprawling, turbulent cloud formations dominate the meteorology of Jupiter's mid‐to‐high latitudes, known as Folded Filamentary Regions (FFRs). A multi‐wavelength characterization by Juno reveals the spatial distribution, vertical structure, and energetics of the FFRs.
L. N. Fletcher +19 more
wiley +1 more source
Formation of Asteroid (16) Psyche by a Giant Impact
Abstract Asteroid (16) Psyche is the largest likely metal‐rich asteroid in the Solar System and the target of the NASA Psyche mission. The mission aims to determine whether the asteroid is the core of a differentiated planetesimal that lost its mantle via a giant impact.
Saverio Cambioni +14 more
wiley +1 more source

