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Accretional and alterational differences in a carbonaceous chondrite parent body: Evidence from the NWA 5491 CV 3 meteorite
Author(s) -
Kereszturi A.,
Gyollai I.,
Jozsa S.,
Kanuchova Z.
Publication year - 2017
Publication title -
meteoritics and planetary science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.09
H-Index - 100
eISSN - 1945-5100
pISSN - 1086-9379
DOI - 10.1111/maps.12802
Subject(s) - meteorite , parent body , chondrule , chondrite , formation and evolution of the solar system , astrobiology , geology , fragmentation (computing) , geochemistry , carbonaceous chondrite , mineralogy , physics , biology , ecology
The NWA 5491 CV 3 meteorite is a CV oxA subtype, and composed of two substantially different units (titled “upper” and “lower” units) in the cm size range with original accreted material and also subsequent alteration produced features. Based on the large chondrules in the “upper” unit and the small chondrules plus CAI s in the “lower” unit, they possibly accreted material from different parts of the solar nebula and/or at different times, whereas substantial changes happened in the nebula's composition. Differences are observed in the level of early fragmentation too, which was stronger in the upper units. During later alteration oxidizing fluids possibly circulated only in the upper unit, mechanical fragmentation and resorption were also stronger there. In the last phase of the geological history these two rock units came into physical contact, but impact‐driven shock effects were not observed. The characteristics of this meteorite provide evidence that the same parent body might accrete substantially different material and also the later processes could differ spatially in the parent body.