Origin and Evolution of Condrules Based on Na/Al-Dispersion and -Convergence in Yamato-74 Ordinary Chondrites

Na/Al convergence has been observed in groundmass of chondrules and matrix from seven Yamato-74 (H, L, 4-5) chondrites. On the other hand, Na/Al dispersion has prevailed in groundmass of chondrules and matrix from Yamato-74191 (L3) chondrite. The results suggest that : (1) Primordial liquid droplets...

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Bibliographic Details
Main Authors: Naoki Onuma, Norimasa Nishida, Yoshiro Ohtsuka, Makoto Kimura, Keizo Yanai
Format: Report
Language:English
Published: Institute of Chemistry, The University of Tsukuba/Chemical Analysis Center, The University of Tsukuba/Institute of Geoscience, The University of Tsukuba/Department of Geology and Mineralogy, Faculty of Science, Hokkaido University/National Institute of Polar Research 1979
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Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=1055
http://id.nii.ac.jp/1291/00001055/
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Summary:Na/Al convergence has been observed in groundmass of chondrules and matrix from seven Yamato-74 (H, L, 4-5) chondrites. On the other hand, Na/Al dispersion has prevailed in groundmass of chondrules and matrix from Yamato-74191 (L3) chondrite. The results suggest that : (1) Primordial liquid droplets as precursors of the chondrules might be derived from a rapidly cooling solar nebula by fractional condensation. (2) The hot liquid droplets thus formed might be cooled instantaneously by radiation loss in the cooling nebula. (3) The chondrules as quenched products might be subjected to mutual collision during accumulation in the cold nebula. (4) Planetesimals accumulated by the chondrules might be transferred from the place of birth to an unknown hot region in the proto solar nebula.