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researcher

Matthew S. Clement

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
ORCID 0000-0001-8933-6878

identity via Semantic Scholar / OpenAlex

most citedThe early instability scenario: terrestrial planet formation during the giant planet instability, and the effect of collisional fragmentation

105 citations · 172 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2019★ 36 cited

A record of the final phase of giant planet migration fossilized in the asteroid belt's orbital structure

Matthew S. Clement, Alessandro Morbidelli, Sean N. Raymond +1

The asteroid belt is characterized by an extreme low total mass of material on dynamically excited orbits. The Nice Model explains many peculiar qualities of the solar system, incl…

astro-ph.EP2019★ 31 cited

Dynamical Constraints on Mercury's Collisional Origin

Matthew S. Clement, Nathan A. Kaib, John E. Chambers

Of the solar system's four terrestrial planets, the origin of Mercury is perhaps the most mysterious. Modern numerical simulations designed to model the dynamics of terrestrial pla…

astro-ph.EP2018★ 105 cited

The early instability scenario: terrestrial planet formation during the giant planet instability, and the effect of collisional fragmentation

Matthew S. Clement, Nathan A. Kaib, Sean N. Raymond +2

The solar system's dynamical state can be explained by an orbital instability among the giant planets. A recent model has proposed that the giant planet instability happened during…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.