The CR chondrite clan: Implications for early solar system processes

By A. Krot, A. Meibom, M. Weisberg, K. Keil. 2002

229 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1838028c7f9fe0603d7157b27f3130e038959b57

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In Astronomy and Astrophysics

1. E. Scott
2. L. Elkins‐Tanton
3. B. Weiss
4. F. Ciesla
5. A. Krot
6. E. Gaidos
7. Sara Seager
8. Leslie A. Rogers

Citations in the corpus

• Differentiated Planetesimals and the Parent Bodies of Chondrites (2013, background): “An interesting possible example of partial differentiation is provided by the CR carbonaceous chondrites, a metal-rich group with heavily hydrated matrices once thought to contain only type 2 members (Krot et al. 2002, Weisberg et al. 2006).”
• Chondrules and the Protoplanetary Disk (2011, background): “However, the CB and CH chondrites are very poor in carbon and matrix material and rich in metallic Fe,Ni, although they share isotopic characteristics with the matrix-rich CR chondrites (Weisberg et al. 1990, Krot et al. 2002).”
• HETEROGENEOUS DISTRIBUTION OF 26Al AT THE BIRTH OF THE SOLAR SYSTEM (2010, background): “…(CBa, CBb, CH, and Isheyevo) are mineralogically and petrographically diverse, but genetically related meteorites (e.g., Weisberg et al. 1995, 2001; Krot et al. 2002b) characterized by a number of unique features, including mineralogy, oxygen- and magnesium-isotope compositions of CAIs (Kimura et…”