Abstract
It is not widely recognized that a significant fraction of the chondrules from ordinary chondrites contain silicate grains that survived the chondrule formation process without melting. In the most typical case these grains consist of coarse olivine, rarely orthopyroxene, crystals located in the core of chondrules and displaying a zoning that is inconsistent with crystallization from a silicate melt. The surrounding groundmass contains abundant glass and fine grained euhedral olivines that appear to be of igneous origin. The relict grains still preserve the imprint of processes that occurred in the solar nebula and, in some cases, may include the isotopic record of interstellar grains. The original properties of these chondrules are best preserved in the most unequilibrated ordinary chondrites1–3. I present here important information with regard to the chondrule precursor materials and the process of chondrule formation which was acquired by a compositional and textural study of three of the most unequilibrated type 3 ordinary chondrites.
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Rambaldi, E. Relict grains in chondrules. Nature 293, 558–561 (1981). https://doi.org/10.1038/293558a0
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DOI: https://doi.org/10.1038/293558a0
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