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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Instantaneous formation of interstellar minerals and mineral quantum dots. [PDF]
Roy A +13 more
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Erratum: “Compound Chondrule Formation in Optically Thin Shock Waves” (2019, ApJ, 877, 84)
Sota Arakawa, T. Nakamoto
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Petrologic evidence for core sulfur degassing in partially differentiated planetesimals. [PDF]
Wang SZ +5 more
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Experimental chondrules by melting samples of olivine, clays and carbon with a CO2 laser
K. E. Cervantes-de la Cruz +7 more
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Secondary Ion Mass Spectrometry for Mg Isotope Ratio Measurements: Application to Meteoritic Chondrules and Cometary Particles [PDF]
N. T. Kita +2 more
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Impact-induced sublimation drives volatile depletion in carbonaceous meteorites. [PDF]
Long ZY +11 more
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Experiments to understand crystallization of levitated high temperature silicate melt droplets under low vacuum conditions. [PDF]
Mishra B +4 more
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Chondrule age distribution and rate of heating events for chondrule formation
Chondrules are considered to be formed by flash heating events in the protoplanetary disk. In order to evaluate some basic factors in the heating mechanism, we examined the rate of heating events that explains the abundance and the observed age distribution of chondrules in unequilibrated ordinary chondrites. First, we compiled the literature data of ^(
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