2021
DOI: 10.48550/arxiv.2104.11252
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Dynamical avenues for Mercury's origin II: in-situ formation in the inner terrestrial disk

Matthew S. Clement,
John E. Chambers

Abstract: Modern terrestrial planet formation models are highly successful at consistently generating planets with masses and orbits analogous to those of Earth and Venus. In stark contrast to classic theoretical predictions and inferred demographics of multi-planet systems of rocky exoplanets, the mass ( 10) and orbital period ( 2) ratios between Venus and Earth and the neighboring Mercury and Mars are not common outcomes in numerically generated systems. While viable solutions to the small-Mars problem are abundant in… Show more

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