Carbon and sulfur budget of the silicate Earth explained by accretion of differentiated planetary embryos-Reference-Cited by-同舟云学术

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Carbon and sulfur budget of the silicate Earth explained by accretion of differentiated planetary embryos

Published:2016-09-05 Issue:10 Volume:9 Page:781-785
ISSN:1752-0894
Container-title:Nature Geoscience
language:en
Short-container-title:Nature Geosci

Author:

Li Yuan,Dasgupta Rajdeep,Tsuno Kyusei,Monteleone Brian,Shimizu Nobumichi

Publisher

Springer Science and Business Media LLC

Subject

General Earth and Planetary Sciences

Link

http://www.nature.com/articles/ngeo2801.pdf

Reference38 articles.

1. Wang, Z. & Becker, H. Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer. Nature 499, 328–331 (2013).

2. Albarede, F. Volatile accretion history of the terrestrial planets and dynamic implications. Nature 461, 1227–1233 (2009).

3. Rose-Weston, L., Brenan, J. M., Fei, Y., Secco, R. A. & Frost, D. J. Effect of pressure, temperature, and oxygen fugacity on the metal-silicate partitioning of Te, Se, and S: implications for Earth differentiation. Geochim. Cosmochim. Acta 73, 4598–4615 (2009).

4. Bergin, E. A., Blake, G. A., Ciesla, F., Hirschmann, M. M. & Li, J. Tracing the ingredients for a habitable Earth from interstellar space through planet formation. Proc. Natl Acad. Sci. USA 112, 8965–8970 (2015).

5. Li, Y., Dasgupta, R. & Tsuno, K. The effects of sulfur, silicon, water, and oxygen fugacity on carbon solubility and partitioning in Fe-rich alloy and silicate melt systems at 3 GPa and 1600 °C: implications for core–mantle differentiation and degassing of magma oceans and reduced planetary mantles. Earth Planet. Sci. Lett. 415, 54–66 (2015).

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