Amoeboid olivine aggregates and related objects in carbonaceous chondrites: records of nebular and asteroid processes

By A. Krot, M. Petaev, S. Russell, S. Itoh, T. Fagan, H. Yurimoto, L. Chizmadia, M. Weisberg, M. Komatsu, A. A. Ul'yanov and 1 more. 2004

148 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Geophysics

View Paper: https://www.semanticscholar.org/paper/4f51f1c2cd7689926ac481a92cd87b9ed7e4d530

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. E. Scott
2. F. Ciesla
3. C. Alexander
4. A. Kalyaan
5. S. Desch
6. L. Grossman
7. S. Simon
8. J. Beckett

In Geophysics

1. E. Scott
2. C. Alexander

Citations in the corpus

• Redox Conditions in the Solar Nebula: Observational, Experimental, and Theoretical Constraints (2008, background): “The lowest XFa reported in AOAs in Acfer 094 is ~0.002 (Krot et al. 2004a).”
• The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “Explaining these CAIs and explaining the distribution of mass is why we choose a single CAI radius of 2.5 mm. AOAs: Chondrites also contain varying portions of another type of refractory inclusion, amoeboid olivine aggregates, or AOAs (Grossman & Steel 1976; Krot et al. 2004).”
• Chondrules and the Protoplanetary Disk (2011, background): “…1999); oxygen isotopic analysis of secondary fayalite, magnetite, and Ca-rich pyroxene (e.g., Choi et al. 2000); and thermodynamic analysis (Krot et al. 2004a, Fedkin & Grossman 2006) all indicate that asteroidal fluid-assisted metamorphism at temperatures above ∼200◦C was the cause of…”