Results 151 to 160 of about 259 (174)
Anchored Oxygen‐Release‐Suppression Phase Stabilizing High‐Voltage Ni‐Rich Cathode Materials
Angewandte Chemie, EarlyView.A one‐step dual‐structure strategy was proposed to synthesize LiNi0.9Co0.05Mn0.05O2 (DA‐NCM) material, which is rich in oxygen vacancies and coated with a perovskite‐type La4LiNiO8 layer stabilized by La─O anchoring provided by La2Mo2O9. This strategy effectively suppressed structural degradation and oxygen release, thereby achieving stable high ...
Ziqi Liu +8 more
wiley +1 more source
The Composition and Chemistry of Titan's Atmosphere. [PDF]
ACS Earth Space ChemNixon CA.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
A common mass scaling for satellite systems of gaseous planets
Nature, 2006The Solar System's outer planets that contain hydrogen gas all host systems of multiple moons, which notably each contain a similar fraction of their respective planet's mass (approximately 10(-4)). This mass fraction is two to three orders of magnitude smaller than that of the largest satellites of the solid planets (such as the Earth's Moon), and its
Robin Canup, William R Ward
exaly +3 more sources
Icarus, 2003
For a satellite to survive in the disk the time scale of satellite migration must be longer than the time scale for gas dissipation. For large satellites (∼1000 km) migration is dominated by the gas tidal torque. We consider the possibility that the redistribution of gas in the disk due to the tidal torque of a satellite with mass larger than the ...
Ignacio Mosqueira, Paul R. Estrada
openaire +1 more source
For a satellite to survive in the disk the time scale of satellite migration must be longer than the time scale for gas dissipation. For large satellites (∼1000 km) migration is dominated by the gas tidal torque. We consider the possibility that the redistribution of gas in the disk due to the tidal torque of a satellite with mass larger than the ...
Ignacio Mosqueira, Paul R. Estrada
openaire +1 more source
2020
The purpose of this chapter is to demonstrate pathways to make Mars more habitable. Mars as it exists today is not habitable but it probably had habitable conditions for a brief era in the history of the planet. Prograde gravitational capture of a 0.1 moon-mass (~0.01 mars-mass) planetoid would cause high tidal amplitudes and ranges in both the ocean ...
openaire +1 more source
The purpose of this chapter is to demonstrate pathways to make Mars more habitable. Mars as it exists today is not habitable but it probably had habitable conditions for a brief era in the history of the planet. Prograde gravitational capture of a 0.1 moon-mass (~0.01 mars-mass) planetoid would cause high tidal amplitudes and ranges in both the ocean ...
openaire +1 more source
Compositional turbulence and layering in the gaseous envelopes of forming planets
Monthly Notices of the Royal Astronomical Society, 2022Kristen Menou
exaly
The growth and migration of massive planets under the influence of external photoevaporation
Monthly Notices of the Royal Astronomical Society, 2022Gavin Coleman +2 more
exaly
Composition of giant planets: The roles of pebbles and planetesimals
Astronomy and Astrophysics, 2023Jingyi Mah +2 more
exaly
Forming Planets via Pebble Accretion
Annual Review of Earth and Planetary Sciences, 2017Anders Johansen, Michiel Lambrechts
exaly