High precision SIMS oxygen three isotope study of chondrules in LL3 chondrites: Role of ambient gas during chondrule formation

By N. Kita, H. Nagahara, S. Tachibana, S. Tomomura, M. Spicuzza, J. Fournelle, J. Valley. 2010

192 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/935677e55ebc95eec13e27038c7b174646a359e7

How researchers see this paper

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In Astronomy and Astrophysics

1. F. Ciesla
2. T. Ushikubo
3. N. Kita
4. J. Valley
5. E. Gaidos
6. A. Krot
7. A. Mann
8. E. Scott

In Geophysics

1. T. Ushikubo
2. N. Kita
3. A. Krot

Citations in the corpus

• HETEROGENEOUS DISTRIBUTION OF 26Al AT THE BIRTH OF THE SOLAR SYSTEM (2010, background): “In contrast, most chondrules and matrix grains formed in dusty nebular regions with nonsolar composition (e.g., Alexander et al. 2008; Alexander and Cuzzi 2011) and in the presence of 16O-poor gas (D17O from approximately )5& to approximately +3&) (e.g., Kita et al. 2005, 2010; Krot et al. 2006).”
• Primordial oxygen isotope reservoirs of the solar nebula recorded in chondrules in Acfer 094 carbonaceous chondrite (2011, methodology): “Kita et al. (2010) further suggested that type II chondrules in LL3 are on the mixing line between ordinary chondritic precursors (D17O P 1.6&) and CV chondrite BO chondrule-like precursors (D17O 2&).”