formation of planetary systems
Moon formation and orbital evolution in extrasolar planetary systems - A literature review
... It is believed that the regular satellites of Jupiter, Saturn and Uranus formed within a circumplanetary disk, as this explains the circular orbits of the regular satellites and their low inclination with respect to ...
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Understanding the Origin of Planetary Systems: Studying the Kuiper Belt and the Dynamics of Planet Formation
... tion scenario yields a velocity dispersion of ∼ 190 m / s among the family members. This is in good agreement with the measured dispersion ∼ 140 m/s in semi-major axis, eccentricity, and inclination of the family members ...
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DESTINY: Database for the Effects of STellar encounters on dIsks and plaNetary sYstems
... formed planetary systems might be influenced by the gravita- tional interactions with neighbouring stars, even though this is much less frequent (Thies et ...
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Revolution evolution : tracing angular momentum during star and planetary system formation
... disc formation, evolution, and dispersal through comparison of the protoplanetary disc angular momentum with that contained within cores and the Solar System ...within planetary systems other than ...
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Doppler monitoring of five k2 transiting planetary systems
... selected systems containing sub- Neptunes ( R < 4 R ⊕ ) , because their internal compositions and formation pathways are poorly ...the planetary radius, we combined the measured transit depth with ...
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Relating binary star planetary systems to central configurations
... the formation of the Solar Sys- tem (Chiang & Lithwick 2005; Morbidelli et ...real planetary system. Extrasolar planetary systems potentially provide other op- portunities, with their ...
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Overcoming Diminished Motivation
... planet formation were informed largely by the only planetary system of which we knew—our own Solar ...of planetary systems produced in ...of planetary systems, including rich ...
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Truly eccentric - I. Revisiting eight single-eccentric planetary systems
... those systems studied by RV surveys, where there is a clear and well-established degeneracy between eccentricity and multiplicity, especially for planets close to or in mean motion ...situ formation ...
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The formation of retrograde planetary orbits by close stellar encounters
... Abstract. We consider the growing number of observations of the Rossiter- McLaughlin effect in transiting planets, which seem to suggest that ∼ 30% of transiting planets are in highly inclined or retrograde orbits. We ...
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The effects of tidal interactions on the properties and evolution of hot Jupiter planetary systems
... the systems, anal- ysis of the global properties of the full population, and simulations of possible routes for the formation and evolution of planetary ...
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Forever alone? Testing single eccentric planetary systems for multiple companions
... of planetary parame- ters from sparsely sampled radial-velocity data, especially if the amplitude (K) of the signal is ...the formation and dynamical history of planetary systems (Zhou et ...
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Survivability of planetary systems in young and dense star clusters
... The majority of free-floating planets appear as part of the field population, but this may be a selection effect of the methods used to find them (Winn & Fabrycky 2015). To some degree, however, their relatively high ...
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The fate of exomoons in white dwarf planetary systems
... the formation of the moons themselves and their subsequent evolution around their parent planet; in our Solar system, there ex- ist several relevant examples ...
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Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models
... the systems confirmed principally via this method ...the systems presented in Papers II and III, as these systems show anticorrelated TTVs at the timescale predicted by the nominal ...
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Tidal dissipation in stars and fluid planetary layers and its impact on the evolution of star-planet systems
... Abstract. Tidal dissipation in stars and planets is one of the key physical mechanisms that drive the evolution of planetary systems. It intrinsically depends on the nature of the tidal response of ...
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Atmospheres of brown dwarfs
... dust formation (nucleation, growth/evaporation, element depletion), turbulence and radiative heat- ing/cooling (Helling et al 2001, 2004), and by large-scale 2D radiative-convection simulations that included the ...
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Low-cost, multi-agent systems for planetary surface exploration
... ing twice the maximum distance between axle centre (around which the robot rotates) and the farthest point of the robot chassis from this one. Finally the sensitivity to positioning errors is defined as the er- ror on ...
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Eclipse, transit and occultation geometry of planetary systems at exo syzygy
... Exo-planetary systems are now known to host a wide variety of exo-planets, with masses ranging from ...multiple-planet systems, which lead to eclipses of Type ...
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Role of components in the formation of self-microemulsifying drug delivery systems
... delivery systems to improve the bioavailability of poorly water soluble ...delivery systems, one among the lipid-based dosage forms were proven to be promising in improving the oral bioavailability of such ...
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Expect the unexpected : non equilibrium processes in brown dwarf atmospheres
... Brown dwarfs seemed the perfect example for a static atmosphere, until it was understood that cloud formation plays a major role for their atmospheres (Tsuji et al. 19). Then, older brown dwarfs were though to be ...
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