Nebular thermal evolution and the properties of primitive planetary materials
By P. Cassen. 2001
135 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/602567cede8aa99ac3b2cdf1201d1635414a001c
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In Astronomy and Astrophysics
Citations in the corpus
- Condensation of Rocky Material in Astrophysical Environments (2023, background): “Parameterizations of chemical equilibrium calculations can be integrated into large-scale nebula models (e.g., Cassen, 2001).”
- Turbulent Radial Mixing in the Solar Nebula as the Source of Crystalline Silicates in Comets (2000, background): “In the solar nebula models investigated here, the vaporization distance of silicates is ∼1 AU, a value less than the value rsub ∼ 2 AU required to explain the relative abundances of moderately volatile elements of carbonaceous meteorites (Cassen 1996, 2001).”
- Chondrules and the Protoplanetary Disk (2011, background): “…volatile elements in chondrites, to produce a small fraction of zoned metallic Fe,Ni grains in CH chondrites (Meibom et al. 2000), and to form CAIs (Cassen 2001), It is plausible that fine-grained CAIs may have formed early in the innermost region of the nebula disk, as condensation of REE, for…”
- Redox Conditions in the Solar Nebula: Observational, Experimental, and Theoretical Constraints (2008, methodology): “It should be noted that Cassen (2001) reported that enrichment factors in excess of 100 are rare in his models, and that factors of ~10 are more likely.”
- Planetary accretion in the inner Solar System (2004, background): “The depletion pattern may represent a distant memory of an early hot phase in the history of the nebula [32], rather as the cosmic microwave background radiation provides a glimpse of the early history of the universe.”