Chondrule formation during planetesimal accretion

By E. Asphaug, M. Jutzi, N. Movshovitz. 2011

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/b4851dee46494942c334b24f0d0177ff0fc03b8c

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Citations in the corpus

Astrophysics with Extraterrestrial Materials (2016, background): “Asphaug et al. (2011) demonstrated that low-velocity (∼1–100 m/s) collisions between molten planetesimals would liberate large amounts of melt into space.”
Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, background): “…prior to accretion (Wasson and Chou, 1974; Cassen, 1996; Bland and Ciesla, 2010), (ii) parent body hydrothermal processes (Delaney, 2009; Young et al., 2003; Fu and Elkins-Tanton, 2014, 2016), or (iii) by impact-related processes (Asphaug et al., 2006, 2011; Canup et al., 2015; Lock et al., 2016).”
Petrographic constraints on the diversity of chondrule reservoirs in the protoplanetary disk (2010, background): “…such as nebular shock waves (Ciesla and Hood 2002; Desch and Connnolly 2002; Morris and Desch 2010), and to models in which chondrules result from collisions between planetesimals (e.g., Sanders and Taylor 2005; Villeneuve et al. 2009, 2011; Asphaug et al. 2011; Libourel and Chaussidon 2011).”
Differentiated Planetesimals and the Parent Bodies of Chondrites (2013, background): “This has motivated renewed proposals that some chondrules, and therefore some chondrites, formed from the remnants of already-differentiated planetesimals (Asphaug et al. 2011, Libourel & Chaussidon 2011, Libourel & Krot 2007).”
Fossilized condensation lines in the Solar System protoplanetary disk (2015, background): “Chondrules have been proposed to have formed as debris from collisions of differentiated planetesimals (Libourel and Krot, 2007; Asphaug et al., 2011), although this is still debated (see e.g. Krot et al., 2009 for a reivew).”
The Compositional Structure of the Asteroid Belt (2015, background): “Such a scenario would be consistent with re-accretion of chondrules produced in hit and run collisions between partially molten planetesimals (Asphaug et al., 2011), for instance.”
The importance of experiments: Constraints on chondrule formation models (2010, background): “Production of chondrules as melt droplets produced during collisions of asteroids has long been suggested (Urey and Craig 1953; Urey 1967; Sanders 1996; Sanders and Taylor 2005; Asphaug et al. 2011).”