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N-body simulations of planet formation via pebble accretion I: First Results
Soko Matsumura, Ramon Brasser, Shigeru Ida
Context. Planet formation with pebbles has been proposed to solve a couple of long-standing issues in the classical formation model. Some sophisticated simulations have been done t…
Saving super-Earths: Interplay between pebble accretion and type I migration
R. Brasser, B. Bitsch, S. Matsumura
Overcoming type I migration and preventing low-mass planets from spiralling into the central star is a long-studied topic. It is well known that outward migration is possible in vi…
The cool and distant formation of Mars
R. Brasser, S. J. Mojzsis, S. Matsumura +1
With approximately one ninth of Earth's mass, Mars is widely considered to be a stranded planetary embryo that never became a fully-grown planet. A currently popular planet formati…