A model of the thermal processing of particles in solar nebula shocks: Application to the cooling rates of chondrules

By S. Desch, H. C. Connolly. 2002

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View Paper: https://www.semanticscholar.org/paper/bcf4ee046a6d794687aef6f01612eb9033945c14

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In Astronomy and Astrophysics

Citations in the corpus

Paleomagnetic Records of Meteorites and Early Planetesimal Differentiation (2010, background): “…also been intimately involved in the formation and/or magnetization of the earliest solar system macroscopic solids, inclusions and chondrules in chondrites (Levy and Araki 1989; Shu et al. 1996, 1997; Crawford and Schultz 1999; Desch and Cuzzi 2000; Desch and Connolly 2002; Joung et al. 2004).”
The physics of star formation (2003, background): “Shock waves in protostellar disks with speeds of several km/sec could produce temperatures of the required order for the required short times, and thus could provide a viable heating mechanism (Connolly and Love 1998; Jones et al 2000; Desch and Connolly 2002; Susa and Nakamoto 2002).”
Planetary accretion in the inner Solar System (2004, background): “Models in which dust is melted by shock waves in the nebula are currently in vogue [10,11], although the source of these shock waves is unclear.”
Chondrule formation during planetesimal accretion (2011, background): “…popular idea that low density mechanical aggregates of solar-composition dust, or pre-chondrules of some sort, were melted when the nebula was heated by powerful shocks (e.g. Boss and Durisen 2005; Ciesla and Hood, 2002; Desch and Connolly, 2002; Morris and Desch, 2010) whose cause is much debated.”
The Nebular Shock Wave Model for Chondrule Formation: Shock Processing in a Particle–Gas Suspension (2002, methodology): “2001, Desch and Connolly 2002), but they should be reexamined for the case of a particle–gas suspension. As stated above, the gas temperature and density are affected by interactions with the chondrules. This has important effects on the kinetics of the dissociation reaction, for example. Finally, w”
Chondrules and the Protoplanetary Disk (2011, background): “Several groups have shown that millimetersized silicate grains in the nebula could have been heated during passage of a shock wave and cooled at the rates inferred from laboratory experiments (Iida et al. 2001, Desch & Connolly 2002, Ciesla & Hood 2002, Desch et al. 2005).”
The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “…to meteoritic constraints; Desch et al. 2012) are passage through large-scale nebular shocks (Wood 1963; Connolly & Love 1998; Iida et al. 2001; Desch & Connolly 2002; Ciesla & Hood 2002; Morris & Desch 2010) and passage through bow shocks around large planetary embryos (Morris et al. 2012;…”