The thermal conductivity of meteorites: New measurements and analysis

By C. Opeil, G. Consolmagno, D. Britt. 2010

162 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/3f6e9c422b67259b278e6471ba27d5e0df596b4f

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1. B. Gundlach
2. J. Blum
3. T. Birnstiel
4. Anders Johansen
5. C. Guttler
6. C. Ormel
7. C. Dullemond
8. R. Weidling

Citations in the corpus

• Chondrites as samples of differentiated planetesimals (2009, unknown): “Density of planetesimal magma ocean ρ_MO 3000 kg m−3 Density of iron core ρ_CORE 8000 kg m−3 Thermal diffusivity of crust κ 8×10−7 m2s−1 Opeil et al. (2010)”
• A new method to determine the grain size of planetary regolith (2012, methodology): “(6) Here, ψ = 1 − φ is the porosity of the respective meteorite (ψ = 0.167 for Cronstad (S), ψ = 0.191 for Lumpkin (S), ψ = 0.373 for Cold Bokkeveld (C), ψ = 0.251 for NWA 5515 (C) and ψ = 0.012 for Campo del Cielo (M), Opeil et al., 2010).”