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Thermal evolution of planetesimals during accretion
Icarus, 2017 cited By 2International audienceAlthough the mass distribution of planetesimals during the early stages of planetary formation has been discussed in various studies, this is not the case for their temperature distribution.
Yanick Ricard +2 more
exaly +2 more sources
Thermal evolution and differentiation of planetesimals and planetary embryos
Icarus, 2012 International audienceIn early Solar System during the runaway growth stage of planetary formation, the distribution of planetary bodies progressively evolved from a large number of planetesimals to a smaller number of objects with a few dominant embryos.
Ondřej Sramek +2 more
exaly +2 more sources
Some of the next articles are maybe not open access.
Structure of differentiated planetesimals: A chondritic fridge on top of a magma ocean
Icarus, 2022Cyril Sturtz +2 more
exaly
Accretion rates of planetesimals by protoplanets embedded in nebular gas
Icarus, 2010Takayuki Tanigawa, Keiji Ohtsuki
exaly
Planetesimal Population Synthesis: are Planetesimals formed in Pressure Bumps?
2019Planetesimals, the smallest building blocks of planets that are gravitationally bound, are believed to be needed in order to form planets. The spacial distribution of these objects that are typically 100 km in diameter is important for the outcome of planet formation.
openaire +1 more source
Radial diffusion rate of planetesimals due to gravitational encounters
Icarus, 2003Keiji Ohtsuki
exaly