Tandem planet formation for solar system-like planetary systems
Sign Up to like & getrecommendations! Published in 2017 at "Geoscience frontiers"
DOI: 10.1016/j.gsf.2016.06.011
Abstract: Abstract We present a new united theory of planet formation, which includes magneto-rotational instability (MRI) and porous aggregation of solid particles in a consistent way. We show that the “tandem planet formation” regime is likely… read more here.
Keywords: system like; solar system; formation; tandem planet ... See more keywords
United theory of planet formation (i): Tandem regime
Sign Up to like & getrecommendations! Published in 2017 at "New Astronomy"
DOI: 10.1016/j.newast.2016.11.001
Abstract: Abstract The present paper is the first one of a series of papers that present the new united theory of planet formation, which includes magneto-rotational instability and porous aggregation of solid particles in an consistent… read more here.
Keywords: disk; planet; formation; regime ... See more keywords
Silicate Melting and Vaporization During Rocky Planet Formation
Sign Up to like & getrecommendations! Published in 2020 at "Journal of Geophysical Research"
DOI: 10.1029/2019je006227
Abstract: Author(s): Davies, E. J; Carter, P. J; Root, S.; Kraus, R. G; Spaulding, D. K; Stewart, S. T; Jacobsen, S. B read more here.
Keywords: rocky planet; vaporization rocky; melting vaporization; silicate melting ... See more keywords
Evidence for the start of planet formation in a young circumstellar disk
Sign Up to like & getrecommendations! Published in 2018 at "Nature Astronomy"
DOI: 10.1038/s41550-018-0497-x
Abstract: The growth of dust grains in protoplanetary disks is a necessary first step towards planet formation1. This growth has been inferred from observations of thermal dust emission2 towards mature protoplanetary systems (age >2 million years)… read more here.
Keywords: planet; evidence; dust; growth ... See more keywords
Terrestrial planet formation in a circumbinary disc around a coplanar binary
Sign Up to like & getrecommendations! Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2419
Abstract: With N-body simulations, we model terrestrial circumbinary planet (CBP) formation with an initial surface density profile motivated by hydrodynamic circumbinary gas disc simulations. The binary plays an important role in shaping the initial distribution of… read more here.
Keywords: disc; planet; formation; giant planets ... See more keywords
Filling in the gaps: Can gravitationally unstable discs form the seeds of gas giant planets?
Sign Up to like & getrecommendations! Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1564
Abstract: Circumstellar discs likely have a short window when they are self-gravitating and prone to the effects of disc instability, but during this time the seeds of planet formation can be sown. It has long been… read more here.
Keywords: gas; form; gas giant; planet formation ... See more keywords