Results 31 to 40 of about 36,303 (299)
Metallicity effect and planet mass function in pebble-based planet formation models [PDF]
, 2018 One of the main scenarios of planet formation is the core accretion model where a massive core forms first and then accretes a gaseous envelope. This core forms by accreting solids, either planetesimals, or pebbles. A key constraint in this model is that
Alibert, Yann +7 more
core +1 more source
Early planet formation as a trigger for further planet formation [PDF]
Nature, 1999 Nature in press ...
Armitage, Philip J., Hansen, Brad M. S.
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Planet Formation and Disk-Planet Interactions [PDF]
, 2019 This review is based on lectures given at the 45th Saas-Fee Advanced Course 'From Protoplanetary Disks to Planet Formation' held in March 2015 in Les Diablerets, Switzerland. Starting with an overview of the main characterictics of the Solar System and extrasolar planets, we describe the planet formation process in terms of the sequential accretion ...
openaire +2 more sources
The Astrophysical Journal, 2023 We construct a one-dimensional protoplanetary disk model to investigate long-term disk evolution from molecular cloud core collapse. To obtain details of disk evolution, instead of solving the traditional diffusion equation for disk surface density, we ...
Xin-Ming Wang
doaj +1 more source
Gap formation in a self-gravitating disk and the associated migration of the embedded giant planet [PDF]
, 2014 We present the results of our recent study on the interactions between a giant planet and a self-gravitating gas disk. We investigate how the disk's self-gravity affects the gap formation process and the migration of the giant planet.
Zhang, Hui +3 more
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Global models of planet formation and evolution [PDF]
, 2015 Despite the strong increase in observational data on extrasolar planets, the processes that led to the formation of these planets are still not well understood. However, thanks to the high number of extrasolar planets that have been discovered, it is now
Dittkrist, K. M. +7 more
core +1 more source
Planetesimal formation at the gas pressure bump following a migrating planet [PDF]
, 2020 Context. Many scenarios have been proposed to avoid known difficulties in planetesimal formation such as drift or fragmentation barriers. However, in these scenarios planetesimals in general only form at some specific locations in protoplanetary discs ...
Y. Shibaike +3 more
core +1 more source
The Astrophysical Journal, 2023 Recent observations suggest that the first stages of planet formation likely take place in the Class 0/I phase of young stellar object evolution, when the star and the disk are still embedded in an infalling envelope.
Wenrui Xu, Philip J. Armitage
doaj +1 more source
Planet Formation via Gravitational Instability
, 2021 Some observed exoplanets cannot be explained in the standard core accretion paradigm. An alternative formation model, planet formation via gravitational instability (GI), has been proposed as a formation mechanism instead.
Schib, Oliver
core
Disk evolution, element abundances and cloud properties of young gas giant planets [PDF]
, 2014 ChHc and PBR highlights financial support of the European Community under the FP7 program by an ERC starting grant. PW, IK, and WFT acknowledge funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement No.
Kamp, I. +19 more
core +1 more source