P(論文) Textures of chondrules in the unequilibrated ordinary chondrites have been summarized on the basis of the processes of their formation inferred from the results of previous experiments. The chondrules studied are classified by their textures into the following four groups : (1) those formed by complete melting of the precursor materials, (2 ...
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Constraining the cooling rates of chondrules
Chondrules are up to mm-sized spherical melt droplets that are the main component in chondritic meteorites, constituting up to 80 vol %. They are products of widespread but poorly understood heating events in the early Solar System. Most chondrules have experienced complete or extensive melting, destroying much of what could be learned from the melting
Stockdale, Shannon +4 more
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Oxygen isotopes of anhydrous primary minerals show kinship between asteroid Ryugu and comet 81P/Wild2. [PDF]
Kawasaki N +93 more
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Paleomagnetic evidence for a disk substructure in the early solar system. [PDF]
Borlina CS +6 more
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Chondrite parent bodies as escaped satellites of proto-planetary embryos. [PDF]
Levison HF +6 more
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Paleomagnetic evidence for a nebular magnetic field from calcium-aluminum-rich inclusions. [PDF]
Borlina CS +8 more
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A novel method for extracting metals from asteroids using non-aqueous deep eutectic solvents. [PDF]
Rivera RM +3 more
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All-Laser Suite Analytical Platform (Microsampling, Catapulting, Trapping, and LIBS) for the Characterization of Discrete Domains in Samples of Astrochemical Interest. [PDF]
Burgos-Palop C +4 more
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Imprint of chondrule formation on the K and Rb isotopic compositions of carbonaceous meteorites. [PDF]
Nie NX +7 more
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