Why is Mars Small? A New Terrestrial Planet Formation Model Including Planetesimal-Driven Migration

Details Why is Mars Small? A New Terrestrial Planet Formation Model Including Planetesimal-Driven Migration Why is Mars Small? A New Terrestrial Planet Formation Model Including Planetesimal-Driven Migration

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2577m&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2577

Physics

Scientific paper

The small size of Mars is a persistent problem for planet-formation
models. We present new simulations for Mars formation that include the
effect of planetesimal-driven migration, a critical mechanism that has
been left out of previous studies.

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