The formation of Jupiter by hybrid pebble–planetesimal accretion

Author:

Alibert YannORCID,Venturini Julia,Helled Ravit,Ataiee Sareh,Burn RemoORCID,Senecal Luc,Benz Willy,Mayer Lucio,Mordasini Christoph,Quanz Sascha P.ORCID,Schönbächler Maria

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Reference41 articles.

1. Helled, R. et al. in Protostars and Planets VI (eds Beuther, H. et al.) 643–666 (Univ. Arizona Press, Tucson, AZ, 2014).

2. Johansen, A. et al. in Protostars and Planets VI (eds Beuther, H. et al.) 547–570 (Univ. Arizona Press, Tucson, AZ, 2014).

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. Pollack et al. Formation of the giant planets by concurrent accretion of solids and gas. Icarus 124, 62–85 (1996).

5. Alibert, Y., Mordasini, C., Benz, W. & Winisdoerffer, C. Models of giant planet formation with migration and disc evolution. Astron. Astrophys. 434, 343–353 (2005).

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