Results 161 to 170 of about 679 (199)

An Advanced High‐Performance Ultrafast Ammonium‐Ion Aqueous Battery Based on Dual‐Metal Redox Open Framework Molecular Magnet

open access: yesAdvanced Science, EarlyView.
The Prussian Blue Analogue molecular magnet KMnFeHCF is demonstrated as a high‐performance cathode for ultra‐fast aqueous ammonium‐ion batteries. A full cell using KMnFeHCF and graphite delivers ~71 mAh g−1 at 1.25 A g−1 and ~51 mAh g−1 at 2.2 A g−1, retaining 50% capacity after 1850 cycles. Its scalability, cycling stability, and low cost offer strong
Nilasha Maiti   +5 more
wiley   +1 more source

Astronomical Observations in Support of Planetary Entry-Probes to the Outer Planets. [PDF]

open access: yesSpace Sci Rev
Buratti BJ   +4 more
europepmc   +1 more source

BepiColombo cruise science: overview of the mission contribution to heliophysics. [PDF]

open access: yesEarth Planets Space
Sánchez-Cano B   +82 more
europepmc   +1 more source

Multiple Probe Measurements at Uranus Motivated by Spatial Variability. [PDF]

open access: yesSpace Sci Rev
Wong MH   +3 more
europepmc   +1 more source

Metastable Dihydrate of Sodium Chloride at Ambient Pressure. [PDF]

open access: yesJ Phys Chem Lett
Hamp RE   +10 more
europepmc   +1 more source

The origin of complex crater formation during high-speed impacts. [PDF]

open access: yesSci Adv
Celebi HF   +6 more
europepmc   +1 more source

The Formation of Nitriles in Hydrocarbon-Rich Atmospheres of Planets and Their Satellites:  Laboratory Investigations by the Crossed Molecular Beam Technique

open access: closedAccounts of Chemical Research, 2001
Crossed molecular beam experiments of cyano radicals, CN(X(2)Sigma(+)), reacting with unsaturated hydrocarbons have been performed to investigate synthetic routes to nitriles formation in hydrocarbon-rich atmospheres of planets and their moons. We have verified that all cyano radical reactions with acetylene, ethylene, methylacetylene, allene, benzene,
Kaiser R. I., BALUCANI, Nadia
openaire   +4 more sources

Formation of the regular satellites of giant planets in an extended gaseous nebula II: satellite migration and survival

open access: closedIcarus, 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   +2 more sources

Formation of the regular satellite systems and rings of the major planets

open access: closedThe Moon and the Planets, 1979
In this paper, we apply the ideas presented by one of us (Prentice, 1978a, b) for the development of the proto-solar cloud into a system of Laplacian rings to the development of the protoplanetary clouds which ultimately led to Jupiter, Saturn and Uranus.
A. J. R. Prentice, D. Ter Haar
openaire   +2 more sources

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