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To tackle low electrocatalytic nitrate reduction to ammonia efficiency in neutral media, this work designs chain‐like dinuclear/trinuclear polyoxometalate‐based metal‐organic complexes. Metal clusters provide nitrate adsorption/activation sites, while polyoxometalates (POMs) drive water dissociation to generate active hydrogen (*H) that migrates to ...
Qiushuang Jiang +5 more
wiley +1 more source
Inspired by the regulation mechanism of window blinds, this study designs an electromagnetic wave‐absorbing metamaterial. By introducing the magneto‐electric coupling concept and integrating it with an artificial intelligence‐based data‐driven collaborative optimization strategy, the material optimizes impedance matching performance and enhances loss ...
Zhe Wang +9 more
wiley +1 more source
The spectral evolution of white dwarfs: where do we stand? [PDF]
Bédard A.
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Free-Floating Planets and Stellar Clusters
American Scientist, 2002The existence of planets outside our solar system has been a licate matter in astronomy ever since the 16th-century philosopher Giordano Bruno was burned at the stake for (among other things) proposing that the universe holds an infinite number of other worlds.
Hurley, Jarrod, Shara, Michael
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Free-floating Planets in Orion
Science, 2000ASTRONOMY Extrasolar planets and brown dwarfs have been discovered with increasing frequency around young stars, yet still more discoveries will be needed to understand conditions under which a star or a planet will form from the collapse of a molecular cloud or other processes.
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Simulation of Images of Protoplanetary Disks after Collision with Free-Floating Planets
Astronomy lettersObservational manifestations of disturbances in a protoplanetary disk caused by a collision with a massive planet are studied. It is assumed that the planet moves along a parabolic trajectory that intersects the disk plane near the star.
T. Demidova, V. Grigoryev
semanticscholar +1 more source
On the capture of free floating planets
2015Diese Masterarbeit bearbeitet die Interaktion zwischen einem free-floating planet und einem gebundenen Stern-Planeten System. Besonders wird dabei auf den Fall einge- gangen, in dem der free-floating planet vom System eingefangen wird und auf einer Bahn gravitativ gebunden bleibt. Sogenannte free-floating planets werden laufend entdeckt.
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Constraints on the free-floating planets supporting aqueous life
Acta Astronautica, 2011Abstract Optically thick atmospheres provide conditions for life on free-floating planets (FFPs). These atmospheres may ensure conservation of energy released by radio-nuclides and the long-term thermal stability of a necessary life-supporting liquid solvent (e.g. water) on the surface.
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