Planetesimal Impact Vapor Plumes and Nebular Shocks Form Chondritic Mixtures
The origin of chondrules and the chondritic sedimentary rocks that dominate the meteoritic record is a long-standing problem in planetary science. Here, we develop a physical model for the formation of chondritic mixtures as an outcome of vaporizing ...
Sarah T. Stewart +5 more
doaj +1 more source
On the Formation of Planetesimals [PDF]
Kerry Hourigan, A. J. R. Prentice
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Detailed Calculations of the Efficiency of Planetesimal Accretion in the Core-accretion Model [PDF]
Morris Podolak +9 more
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Primitive noble gases sampled from ocean island basalts cannot be from the Earth's core. [PDF]
Li Y +3 more
europepmc +1 more source
Dust Evolution and the Formation of Planetesimals [PDF]
T. Birnstiel, Min Fang, Anders Johansen
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Insights into the formation and evolution of extraterrestrial amino acids from the asteroid Ryugu. [PDF]
Potiszil C +23 more
europepmc +1 more source
Early volatile depletion on planetesimals inferred from C-S systematics of iron meteorite parent bodies. [PDF]
Hirschmann MM +4 more
europepmc +1 more source
Numerous chondritic impactors and oxidized magma ocean set Earth's volatile depletion. [PDF]
Sakuraba H, Kurokawa H, Genda H, Ohta K.
europepmc +1 more source
VARIATIONS ON DEBRIS DISKS. II. ICY PLANET FORMATION AS A FUNCTION OF THE BULK PROPERTIES AND INITIAL SIZES OF PLANETESIMALS [PDF]
Scott J. Kenyon, Benjamin C. Bromley
openalex +1 more source
Silicon isotope constraints on terrestrial planet accretion. [PDF]
Onyett IJ +5 more
europepmc +1 more source

