The importance of experiments: Constraints on chondrule formation models
By S. Desch, M. Morris, H. C. Connolly, A. Boss. 2010
142 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/67d1bd1cb1da50b1b669f2ecdcba8e4b3f05816c
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In Astronomy and Astrophysics
Citations in the corpus
- The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, background): “Among the most successful models for chondrule formation (because of their adherence 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…”
- Astrophysics with Extraterrestrial Materials (2016, methodology): “Peak temperatures of 1,700–2,400 K are needed to melt chondrules (Connolly & Desch 2004, Desch et al. 2012), a temperature range that again exceeds the temperatures typically expected or observationally inferred within protoplanetary disks.”