Planet formation by coagulation: A focus on Uranus and Neptune
P Goldreich, Y Lithwick, R Sari - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Planets form in the circumstellar disks of young stars. We review the basic physical
processes by which solid bodies accrete each other and alter each others' random …
processes by which solid bodies accrete each other and alter each others' random …
Planet formation—Observational constraints, physical processes, and compositional patterns
A general theory of planet formation has been a topic of intense study over many years. The
interest in such a theory emerges naturally from asking the question of where our planet …
interest in such a theory emerges naturally from asking the question of where our planet …
The New Generation Planetary Population Synthesis (NGPPS)-IV. Planetary systems around low-mass stars
Context. Previous theoretical works on planet formation around low-mass stars have often
been limited to large planets and individual systems. As current surveys routinely detect …
been limited to large planets and individual systems. As current surveys routinely detect …
Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion
Chondrules are millimeter-sized spherules that dominate primitive meteorites (chondrites)
originating from the asteroid belt. The incorporation of chondrules into asteroidal bodies …
originating from the asteroid belt. The incorporation of chondrules into asteroidal bodies …
[BOOK][B] Astrophysics of planet formation
PJ Armitage - 2020 - books.google.com
" The study of planet formation has a long history. The idea that the Solar System formed
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …
The effect of gas drag on the growth of protoplanets-analytical expressions for the accretion of small bodies in laminar disks
CW Ormel, HH Klahr - Astronomy & Astrophysics, 2010 - aanda.org
Planetary bodies form by accretion of smaller bodies. It has been suggested that a very
efficient way to grow protoplanets is by accreting particles of size≪ km (eg, chondrules …
efficient way to grow protoplanets is by accreting particles of size≪ km (eg, chondrules …
The New Generation Planetary Population Synthesis (NGPPS)-I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems
Context. The explosion of observational data on exoplanets gives many constraints on
theoretical models of planet formation and evolution. Observational data probe very large …
theoretical models of planet formation and evolution. Observational data probe very large …
RV-detected planets around M dwarfs: Challenges for core accretion models
Context. Planet formation is sensitive to the conditions in protoplanetary disks, for which
scaling laws as a function of stellar mass are known. Aims. We aim to test whether the …
scaling laws as a function of stellar mass are known. Aims. We aim to test whether the …
The New Generation Planetary Population Synthesis (NGPPS)-II. Planetary population of solar-like stars and overview of statistical results
Context. Planetary formation and evolution is a combination of multiple interlinked
processes. Constraining the mechanisms observationally requires statistical comparison to …
processes. Constraining the mechanisms observationally requires statistical comparison to …
Predicted diversity in water content of terrestrial exoplanets orbiting M dwarfs
Exoplanet surveys around M dwarfs have detected a growing number of exoplanets with
Earth-like insolation. It is expected that some of those planets are rocky planets with the …
Earth-like insolation. It is expected that some of those planets are rocky planets with the …