Bifurcation of planetary building blocks during Solar System formation [PDF]
Science, 2021 Two-part formation of the Solar System Measurements of meteorites have shown that the inner and outer Solar System formed from two distinct reservoirs of material.
Tim Lichtenberg +2 more
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Theoretical models of planetary system formation. II. Post-formation evolution [PDF]
Astronomy & Astrophysics, 2015 We extend the results of planetary formation synthesis by computing the long-term evolution of synthetic systems from the clearing of the gas disk into the dynamical evolution phase.
S. Pfyffer +3 more
semanticscholar +5 more sources
Post-main-sequence planetary system evolution [PDF]
Royal Society Open Science, 2016 The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical
Dimitri Veras
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The contribution of the ARIEL space mission to the study of planetary formation [PDF]
Experimental Astronomy, 2018 The study of extrasolar planets and of the Solar System provides complementary pieces of the mosaic represented by the process of planetary formation. Exoplanets are essential to fully grasp the huge diversity of outcomes that planetary formation and the
Yamila MIGUEL +2 more
exaly +2 more sources
On the formation of the Kepler-10 planetary system [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 12 pages, accepted for publication in ...
Caroline Terquem, Terquem Caroline
exaly +5 more sources
Planetary population synthesis and the emergence of four classes of planetary system architectures [PDF]
The European Physical Journal Plus, 2023 Planetary population synthesis is a helpful tool to understand the physics of planetary system formation. It builds on a global model, meaning that the model has to include a multitude of physical processes. The outcome can be statistically compared with
A. Emsenhuber, C. Mordasini, R. Burn
semanticscholar +1 more source
Particle–particle particle–tree code for planetary system formation with individual cut-off method: GPLUM [PDF]
, 2020 In the standard theory of the formation of planets in our Solar System, terrestrial planets and the cores of gas giant planets are formed through accretion of km size objects (planetesimals) in the protoplanetary disk.
Yota Ishigaki +4 more
semanticscholar +1 more source
Searching For the t=0 of Planetary System Formation [PDF]
EPJ Web of Conferences, 2022 The composition of bodies in the solar system points to strong gradients in the volatile content within solid bodies hinting at the presence of gas-ice transitions across sublimation fronts in the young formative stages when the gas-rich disk was present.
Bergin Edwin +2 more
doaj +1 more source
The formation of planetary systems with SPICA [PDF]
Publications of the Astronomical Society of Australia, 2021 Abstract In this era of spatially resolved observations of planet-forming disks with Atacama Large Millimeter Array (ALMA) and large ground-based telescopes such as the Very Large Telescope (VLT), Keck, and Subaru, we still lack statistically relevant information on the quantity and composition of the material that is building the planets, such as ...
Kamp, I. +40 more
openaire +6 more sources
An Analytical Theory for the Growth from Planetesimals to Planets by Polydisperse Pebble Accretion
The Astrophysical Journal, 2023 Pebble accretion is recognized as a significant accelerator of planet formation. Yet only formulae for single-sized (monodisperse) distribution have been derived in the literature.
Wladimir Lyra +3 more
doaj +1 more source