In this work, we apply a soft-sphere discrete element method (SSDEM) within the PKDGRAV N -body integrator to investigate the formation of planetesimal systems through the gravitational collapse of clouds of superparticles. Previously published numerical
Jackson T. Barnes +2 more
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Carbonaceous Chondrites Provide Evidence for Late-stage Planetesimal Formation in a Pressure Bump
Carbonaceous chondrites are samples from planetesimals that formed 2–4 million years after solar system formation began. They consist of distinct dust components formed at different times and locations in the accretion disk, and whose abundances in ...
Nerea Gurrutxaga +3 more
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Chalcogen isotopes reveal limited volatile contribution from late veneer to Earth. [PDF]
Wang W +4 more
europepmc +1 more source
Phosphorus-nitrogen systematics of first-generation planetesimals constrain life-essential element delivery to Earth. [PDF]
Pathak D, Dasgupta R, Iyer N.
europepmc +1 more source
Asteroid sample return missions are critical for understanding our Solar System. [PDF]
Bates H.
europepmc +1 more source
Aqueous breakdown of aspartate and glutamate to n-ω-amino acids on the parent bodies of carbonaceous chondrites and asteroid Ryugu. [PDF]
Li Y +12 more
europepmc +1 more source
The late formation of chondrites as a consequence of Jupiter-induced gaps and rings. [PDF]
Srivastava B, Izidoro A.
europepmc +1 more source
I/Pu reveals Earth mainly accreted from volatile-poor differentiated planetesimals. [PDF]
Liu W +5 more
europepmc +1 more source
Protracted core formation and impact disruptions shaped the earliest outer Solar System planetesimals. [PDF]
Grewal DS +5 more
europepmc +1 more source
Silicon isotope constraints on terrestrial planet accretion. [PDF]
Onyett IJ +5 more
europepmc +1 more source

