The Origin of Chondrules and Refractory Inclusions in Chondritic Meteorites

By F. Shu, H. Shang, M. Gounelle, A. Glassgold, Typhoon Lee. 2001

316 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/761867aac27956d5e37eaa91818695aeebaf4d24

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In Astronomy and Astrophysics

Citations in the corpus

The importance of experiments: Constraints on chondrule formation models (2010, methodology): “Some models invoke melting by virtue of being near the Sun, either due to sunlight and solar flares (the X-wind model of Shu et al. 1996, 1997, 2001) or by ablation in the bipolar outflow that accompanies the proto-Sun (Skinner 1990; Liffman and Brown 1996; Liffman 2009).”
A Perspective from Extinct Radionuclides on a Young Stellar Object: The Sun and Its Accretion Disk (2011, methodology): “Different calculations have been performed assuming various irradiation scenarios, either at asteroidal distances assuming no shielding by nebular gas (Goswami et al. 2001, Marhas et al. 2002) or at distances close to the Sun (Gounelle et al. 2001, 2006; Leya et al. 2003) in the framework of the X-w”
Stellar Activity on the Young Suns of Orion: COUP Observations of K5-7 Pre-Main-Sequence Stars (2005, background): “…ergs s 1 flares seen in T Tauri stars surrounded by protoplanetary disks, the inferred X-ray or shock wave heating may flash melt chondrules (Shu et al. 2001; Nakamoto et al. 2005) and the inferredMeV particle fluence may produce anomalous abundances of short-lived radionuclides seen in…”
CRYSTALLINE SILICATES AND DUST PROCESSING IN THE PROTOPLANETARY DISKS OF THE TAURUS YOUNG CLUSTER (2007, background): “Leading candidates for the radial grain-transport method include turbulent diffusion within the disk, with (Boss 2004) or without (Gail 2001; Bockelée-Morvan et al. 2002; Wehrstedt & Gail 2002; Ciesla 2007) convection, large-scale meridional flows in an α-disk (Keller & Gail 2004), and reflux of ma”
Chronology of the Solar System’s Oldest Solids (2008, methodology): “Taking advantage of improved methods for isotopic analysis of small quantities of Pb by thermal ionization mass spectrometry (Table 1) and relatively large sizes of CAIs (∼5– 10 mm) and chondrules (∼1 mm) in CV chondrites, we have investigated the absolute chronology of chondrules and CAIs from this”
Generation of nonclassical photon pairs for scalable quantum communication with atomic ensembles (2003, background): “More extensive investigations of the timing characteristics of the emitted ﬁelds (1, 2) will be part of our subsequent investigations, including the relationship to elec-tromagnetically induced transparency (EIT) 23,24 .”
26 Al- 26 Mg and 207 Pb- 206 Pb systematics of Allende CAIs: Canonical solar initial 26 Al/ 27 Al ratio reinstated (2008, background): “The tight spread in (26)Al/(27)Al ratio in both whole-rock and mineral separate of Allende CAIs from our work limits the X-wind model (Shu et al., 2001) as the origin of (26)Al due to early solar irradiation, unless the impulsive solar flare events were operational only for b±20 Ka.”
Grain growth in the inner regions of Herbig Ae/Be star disks (2003, background): “The X-wind mechanism (Shu et al. 2001) may also be capable of adding some (processed) material on the surface of the disk.”
Chondrules and the Protoplanetary Disk (2011, background): “Shu et al. (1996, 2001) infer that proto-CAIs were manufactured between the inner edge of the disk and the protosun in the reconnection ring where magnetic reconnection events and impulsive flares analogous to those observed in the modern Sun heated and irradiated refractory particles.”
Magnetic Flaring in the Pre-Main-Sequence Sun and Implications for the Early Solar System (2002, methodology): “This is the geometry assumed in the meteoritic spallation calculations of Lee et al. (1998) and Gounelle et al. (2001) and in the chondrule melting model of Shu et al. (2001).”