Accretion of the earliest inner Solar System planetesimals beyond the water snowline
Author:
Funder
Barr Foundation
National Aeronautics and Space Administration
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-023-02172-w.pdf
Reference82 articles.
1. Kruijer, T. S. et al. Protracted core formation and rapid accretion of protoplanets. Science (1979) 344, 1150–1154 (2014).
2. Goldstein, J. I., Scott, E. R. D. & Chabot, N. L. Iron meteorites: crystallization, thermal history, parent bodies, and origin. Chem. der Erde 69, 293–325 (2009).
3. Kruijer, T. S., Burkhardt, C., Budde, G. & Kleine, T. Age of Jupiter inferred from the distinct genetics and formation times of meteorites. Proc. Natl Acad. Sci. USA 114, 6712–6716 (2017).
4. Spitzer, F., Burkhardt, C., Nimmo, F. & Kleine, T. Nucleosynthetic Pt isotope anomalies and the Hf-W chronology of core formation in inner and outer solar system planetesimals. Earth Planet. Sci. Lett. 576, 117211 (2021).
5. Youdin, A. N. & Goodman, J. Streaming instabilities in protoplanetary disks. Astrophys. J. 620, 459–469 (2005).
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