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G. Collins

4 papers hereh-index 121k citations17 works total

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

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
same name
  • G. Collins — 13 papers, h 17
  • G. Collins — 10 papers, h 49
  • G. Collins — 4 papers, h 88
  • G. Collins — 3 papers, h 2
  • G. Collins — 3 papers, h 8
  • G. Collins — 3 papers, h 7

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20122024
most citedPost-Impact Thermal Evolution of Porous Planetesimals

82 citations · 231 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2024★ 79 cited

Physical properties of asteroid Dimorphos as derived from the DART impact

S. D. Raducan, M. Jutzi, A. F. Cheng +39

On September 26, 2022, NASA's Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the binary near-Earth asteroid (65803) Didym…

astro-ph.EP2023★ 5 cited

The distribution of impactor core material during large impacts on Earth-like planets

Jonathan P. Itcovitz, Auriol S. P. Rae, Thomas M. Davison +2

Large impacts onto young rocky planets may transform their compositions, creating highly reducing conditions at their surfaces and reintroducing highly siderophile metals to their…

astro-ph.EP2013★ 65 cited

The early impact histories of meteorite parent bodies

Thomas M Davison, David P O'Brien, Fred J Ciesla +1

We have developed a statistical framework that uses collisional evolution models, shock physics modeling and scaling laws to determine the range of plausible collisional histories…

astro-ph.EP2012★ 82 cited

Post-Impact Thermal Evolution of Porous Planetesimals

T. M. Davison, F. J. Ciesla, G. S. Collins

Impacts between planetesimals have largely been ruled out as a heat source in the early Solar System, by calculations that show them to be an inefficient heat source and unlikely t…

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