Planet-disk interaction and orbital evolution
W Kley, RP Nelson - Annual Review of Astronomy and …, 2012 - annualreviews.org
As planets form and grow within gaseous protoplanetary disks, the mutual gravitational
interaction between the disk and planet leads to the exchange of angular momentum and …
interaction between the disk and planet leads to the exchange of angular momentum and …
Planet-disc interactions and early evolution of planetary systems
C Baruteau, A Crida, SJ Paardekooper… - arXiv preprint arXiv …, 2013 - arxiv.org
The great diversity of extrasolar planetary systems has challenged our understanding of how
planets form, and how their orbits evolve as they form. Among the various processes that …
planets form, and how their orbits evolve as they form. Among the various processes that …
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 …
Hints for a turnover at the snow line in the giant planet occurrence rate
RB Fernandes, GD Mulders, I Pascucci… - The Astrophysical …, 2019 - iopscience.iop.org
The orbital distribution of giant planets is crucial for understanding how terrestrial planets
form and predicting yields of exoplanet surveys. Here, we derive giant planets occurrence …
form and predicting yields of exoplanet surveys. Here, we derive giant planets occurrence …
The PLATO 2.0 mission
H Rauer, C Catala, C Aerts, T Appourchaux… - Experimental …, 2014 - Springer
PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …
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 …
Planet occurrence within 0.25 AU of solar-type stars from Kepler
We report the distribution of planets as a function of planet radius, orbital period, and stellar
effective temperature for orbital periods less than 50 days around solar-type (GK) stars …
effective temperature for orbital periods less than 50 days around solar-type (GK) stars …
Giant planet occurrence in the stellar mass-metallicity plane
Correlations between stellar properties and the occurrence rate of exoplanets can be used
to inform the target selection of future planet-search efforts and provide valuable clues about …
to inform the target selection of future planet-search efforts and provide valuable clues about …
The Ophiuchus DIsc Survey Employing ALMA (ODISEA)–I: project description and continuum images at 28 au resolution
LA Cieza, D Ruíz-Rodríguez, A Hales… - Monthly Notices of …, 2019 - academic.oup.com
Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
The occurrence and mass distribution of close-in super-Earths, Neptunes, and Jupiters
The questions of how planets form and how common Earth-like planets are can be
addressed by measuring the distribution of exoplanet masses and orbital periods. We report …
addressed by measuring the distribution of exoplanet masses and orbital periods. We report …