Results 21 to 30 of about 90,567 (226)
FORMATION OF PLANETARY CORES AT TYPE I MIGRATION TRAPS [PDF]
The Astrophysical Journal, 2011 Accepted for publication in ApJ ...
Zs. Sándor +2 more
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Connecting planetary health, climate change, and migration [PDF]
The Lancet Planetary Health, 2018 Stefanie Schütte +4 more
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Vertical instability and inclination excitation during planetary migration [PDF]
, 2014 We consider a two-planet system, which migrates under the influence of dissipative forces that mimic the effects of gas-driven (Type II) migration. It has been shown that, in the planar case, migration leads to resonant capture after an evolution that ...
G. Voyatzis +2 more
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Effect of Wind-Driven Accretion on Planetary Migration
, 2020 Can wind-driven accretion modify planetary migration? Planetary migration plays an important role in planet formation models and statistics of observed exoplanets. So far, the theory of planetary migration has focused on the interaction of one or more planets with an inviscid or viscously evolving gaseous disk.
C. N. Kimmig
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Planetary formation and early phases
Comptes Rendus. Physique, 2023 Planets form in proto-planetary disks. In this review, we describe the structure and properties of such disks, and the various phenomenons that lead to the final product: a planetary system. First, micrometre dust settles and coagulates.
Crida, Aurélien
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Dissipative Capture of Planets into First-order Mean-motion Resonances
The Astrophysical Journal Letters, 2023 The emergence of orbital resonances among planets is a natural consequence of the early dynamical evolution of planetary systems. While it is well established that convergent migration is necessary for mean-motion commensurabilities to emerge, recent ...
Konstantin Batygin, Antoine C. Petit
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Photoevaporation-Triggered Runaway Migration: Sculpting Inner Planetary Systems
The formation and evolution of planetary systems are intimately linked to the dynamics of protoplanetary disks. Planetary migration, driven by gravitational interactions between forming planets and their natal gas disks, is a critical process for shaping planetary architectures, especially for inner systems.
Revista, Zen, ASTRO, 10
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, 2021 Studies of planet migration derived from disc planet interactions began before the discovery of exoplanets. The potential importance of migration for determining orbital architectures being realised, the field received greater attention soon after the initial discoveries of exoplanets.
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Evidence for Hidden Nearby Companions to Hot Jupiters
The Astronomical Journal, 2023 The first discovered extrasolar worlds—giant, “hot Jupiter” planets on short-period orbits—came as a surprise to solar system–centric models of planet formation, prompting the development of new theories for planetary system evolution.
Dong-Hong Wu, Malena Rice, Songhu Wang
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