Porosity models for pre-planetesimals: modified P-α like models and the effect of dissipated energy [PDF]
, 2010 S. E. Arena, R. Speith
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Mini-Oort clouds: compact isotropic planetesimal clouds from planet–planet scattering [PDF]
, 2012 Sean N. Raymond, Philip J. Armitage
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Shock-generating Planetesimals Perturbed by a Giant Planet in a Gas Disk [PDF]
, 2019 Makiko Nagasawa +5 more
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Chondrule Survivability in the Solar Nebula
The Astrophysical JournalThe lifetime of millimeter-sized dust grains, such as chondrules, in the nominal solar nebula model is limited to ∼10 ^5 yr, due to an inward drift driven by gas drag.
Tetsuo Taki, Shigeru Wakita
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Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Sci Adv, 2023 Wang W +4 more
europepmc +1 more source
Planetesimal Scattering Efficiency of Cold Giant Planet Architectures
The Astronomical JournalThe discovery of many exoplanets has revealed an incredible diversity of orbital architectures. These orbital configurations are intrinsically linked to the potential for habitable environments within the system, since the gravitational influence of the ...
Stephen R. Kane, Emma L. Miles
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The effect of an early planetesimal-driven migration of the giant planets on terrestrial planet formation [PDF]
, 2010 K. J. Walsh, A. Morbidelli
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Conditions of core melt segregation in planetesimals [PDF]
, 2022 Hidenori Terasaki +3 more
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Collisional disruption of planetesimals in the gravity regime with iSALE code: Comparison with SPH code for purely hydrodynamic bodies [PDF]
, 2018 Ryo Suetsugu +3 more
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Turbulent Dust-trapping Rings as Efficient Sites for Planetesimal Formation [PDF]
, 2022 Ziyan Xu, Xue‐Ning Bai
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