Results 61 to 70 of about 3,349 (181)
Planets in Binaries: Formation and Dynamical Evolution
Binary systems are very common among field stars, yet the vast majority of known exoplanets have been detected around single stars. While this relatively small number of planets in binaries is probably partly due to strong observational biases, there is,
Francesco Marzari, Philippe Thebault
doaj +1 more source
How to build Tatooine: reducing secular excitation in Kepler circumbinary planet formation
Circumbinary planetary systems recently discovered by Kepler represent an important testbed for planet formation theories. Planetesimal growth in disks around binaries has been expected to be inhibited interior to ~10 AU by secular excitation of high ...
Rafikov, Roman R.
core +1 more source
Kepler-47: A Transiting Circumbinary Multi-Planet System [PDF]
We report the detection of Kepler-47, a system consisting of two planets orbiting around an eclipsing pair of stars. The inner and outer planets have radii 3.0 and 4.6 times that of the Earth, respectively. The binary star consists of a Sun-like star and
A. P. Boss +43 more
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Planet migration in massive circumbinary discs
ABSTRACT Most stars are in multiple systems, with the majority of those being binaries. A large number of planets have been confirmed in binary stars and, therefore, it is important to understand their formation and dynamical evolution. We perform simulations to investigate the migration of wide-orbit giant planets (semimajor axis 100 au)
Matthew Teasdale, Dimitris Stamatellos
openaire +2 more sources
Habitability Properties of Circumbinary Planets
Abstract It is shown that several habitability conditions (in fact, at least seven such conditions) appear to be fulfilled automatically by circumbinary planets of main-sequence stars (CBP-MS), whereas on Earth, these conditions are fulfilled only by chance.
openaire +2 more sources
FORMATION OF CIRCUMBINARY PLANETS IN A DEAD ZONE [PDF]
Circumbinary planets have been observed at orbital radii where binary perturbations may have significant effects on the gas disk structure, on planetesimal velocity dispersion, and on the coupling between turbulence and planetesimals. Here, we note that the impact of all of these effects on planet formation is qualitatively altered if the circumbinary ...
Martin, Rebecca G. +2 more
openaire +2 more sources
Near-Infrared Imaging Polarimetry of Inner Region of GG Tau A Disk
By performing non-masked polarization imaging with Subaru/HiCIAO, polarized scattered light from the inner region of the disk around the GG Tau A system was successfully detected in the $H$ band with a spatial resolution of approximately 0.07$\arcsec ...
Abe, Lyu +53 more
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On the migration of protoplanets embedded in circumbinary disks
We present the results of hydrodynamical simulations of low mass protoplanets embedded in circumbinary accretion disks. The aim is to examine the migration and long term orbital evolution of the protoplanets, in order to establish the stability ...
A. Pierens +48 more
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Terrestrial Planet Formation Surrounding Close Binary Stars [PDF]
Disk material has been observed around both components of some young close binary star systems. It has been shown that if planets form at the right places within such disks, they can remain dynamically stable for very long times.
Lissauer, Jack J., Quintana, Elisa V.
core +3 more sources
Regions of Dynamical Stability for Discs and Planets in Binary Stars of the Solar Neighborhood
Using the results of Pichardo \et (2005,2008), we determine regions of dynamical stability where planets (or discs in general) could survive in stable orbits around binary stellar systems.
Aguilar, Luis +2 more
core +1 more source

