A FUN-LIKE HIBONITE INCLUSION WITH A LARGE 26Mg-EXCESS

dc.contributor.authorUshikubo T.
dc.contributor.authorHiyagon H.
dc.contributor.authorSugiura N.
dc.date.accessioned2026-07-13T08:35:06Z
dc.date.issued2007
dc.description.abstractWe found a unique hibonite (CaAl 12 O 19) inclusion Kz1-2 from the Kainsaz (CO3) chondrite, which exhibits evidence for a strong link between "normal" CAIs and FUN inclusions. Kz1-2 shows strongly fractionated isotopic compositions of O, Ca, and Ti preferring heavy isotopes and a characteristic REE abundance pattern similar to those of FUN (or HAL-type hibonite) inclusions, suggesting an intensive distillation process in the formation of this inclusion. Unlike FUN inclusions, however, Kz1-2 shows large excesses in 26 Mg and possibly in 41 K most likely from the decays of now-extinct nuclides 26 Al and 41 Ca with the inferred initial ratios of (26 Al/ 27 Al) 0 ∼ 5.3 × 10 − 5 and (41 Ca/ 40 Ca) 0 ∼ 1.1 × 10 − 8 , respectively, and no detectable mass-independent isotopic anomalies in Ca and Ti, both of which are characteristic of "normal" CAIs. These observations suggest that the distillation process which produced isotopic fractionation in Kz1-2 occurred as early as the formation of "normal" CAIs. It is also inferred that the formation process of FUN inclusions is closely related to that of "normal" CAIs.
dc.identifierhttps://elibrary.ru/item.asp?id=13745428
dc.identifier.citationEarth and Planetary Science Letters, 2007, 254, 1-2, 115-126
dc.identifier.doi10.1016/j.epsl.2006.11.031
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/53437
dc.subjectCAI
dc.subjectEARLY SOLAR SYSTEM
dc.subjectFUN INCLUSION
dc.subjectHIBONITE
dc.subjectISOTOPE
dc.subjectSHORT-LIVED NUCLIDE
dc.titleA FUN-LIKE HIBONITE INCLUSION WITH A LARGE 26Mg-EXCESS
dc.typeСтатья

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