Primordial oxygen isotope reservoirs of the solar nebula recorded in chondrules in Acfer 094 carbonaceous chondrite

By T. Ushikubo, M. Kimura, N. Kita, J. Valley. 2011

226 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology, Geophysics

View Paper: https://www.semanticscholar.org/paper/36fc8d880fbd8e99c73db8ebeb1bf48571c77f1b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

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

In Ecology

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

In Geophysics

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

Citations in the corpus

• Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, unknown): “24) (Ushikubo et al., 2012; Tenner et al., 2015).”
• HETEROGENEOUS DISTRIBUTION OF 26Al AT THE BIRTH OF THE SOLAR SYSTEM (2010, background): “which probably formed in the disk 2–3 Ma after CAIs have (16)O-poor compositions (e.g., Krot et al. 2009; Kita et al. 2012b; Ushikubo et al. 2012).”
• Evolution of protoplanetary disk inferred from 26Al chronology of individual chondrules (2012, background): “Although new oxygen isotope data by Ushikubo et al. (2011) alone may not fully refute the planetary origin for the olivine in type I chondrules, Whattam et al. (2008) also argued against the planetary origin suggested by Libourel and Krot (2007) mainly from grain size of olivine being much smaller…”