Meteorites and the early solar system II

By Dante S. Lauretta, H. McSween. 2006

966 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/7773d34dfd85152d5391fb41b9dab84b32110fb3

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Citations in the corpus

Chelyabinsk Airburst, Damage Assessment, Meteorite Recovery, and Characterization (2013, background): “The meteorite is composed of a breccia (17) of mildly-shocked lighter clasts and moderately-shocked darker clasts with abundant thin to cm-wide shock melt veins (Fig.”
NEUTRON-RICH CHROMIUM ISOTOPE ANOMALIES IN SUPERNOVA NANOPARTICLES (2010, background): “…effect as the nanospinels identified here do not contain appreciable amounts of Ca. FUN and hibonite-bearing inclusions in meteorites contain correlated excess in 48Ca and other neutron-rich isotopes that are consistent with a SNIa origin (Völkening & Papanastassiou 1989; Meyer & Zinner 2006).”
Toward Planetesimals: Dense Chondrule Clumps in the Protoplanetary Nebula (2008, background): “The more common, less dense of these regions may provide typical chondrule melting environments (Cuzzi and Alexander 2006).”
Chondrites as samples of differentiated planetesimals (2009, background): “These early-accreting bodies would have melted from the interior outward, resulting in an interiormagma ocean under a solid, conductive, undifferentiated shell (Ghosh and McSween Jr., 1998; Hevey and Sanders, 2006; McCoy et al., 2006; Merk et al., 2002; Sahijpal et al., 2007; Schölling and Breuer, 2”
Differentiated Planetesimals and the Parent Bodies of Chondrites (2013, background): “See Lauretta & McSween 2006, pp. 19–52 Weiss BP, Berdahl S, Elkins-Tanton LT, Stanley S, Lima EA, Carporzen L. 2008.”
Asteroids Were Born Big (2009, result): “Accordingly, these results suggest that planet formation followed a path different from what is usually assumed and the classical model, despite its simplicity and appeal, should be reconsidered.”