[PDF] Top 20 Theory of planet formation and comparison with observation

... the planet, one gets the planetary mass-radius diagram, which is an observational result of similar importance as the semimajor axis-mass ...the planet, which constrains, at least to some extent, the ... See full document

... easier comparison with zonal cross sections, and the corresponding OLR perturbation values at the grid point nearest to the sta- tion are also given for each ... See full document

... core-accretion theory of planet ...disks. Planet cores form more quickly in a higher metallicity disk, allowing accretion of a gas giant envelope before the disk ...form planet cores more ... See full document

... have shown giant convective storms in Saturn’s atmosphere with diameter around a few thousand kilometers and lifetime around a few weeks. In addition, observations (Beebe, et al., 1992; Sanchez-Lavega, et al., 1991,1996) ... See full document

... In contrast to that, the eclipsing, short-period sdB binary J0820+0008, discovered in the course of the MUCHFUSS project, turned out to have a brown dwarf companion [49]. Additionally, at least one more similar system ... See full document

... The study of clusters by using the empirical formula k = ½ (E-V) revealed the existence of cluster series. This gave rise to the design of a cluster table that has been highly refined to its current form in this paper. ... See full document

... DOI: 10.4236/acs.2017.74036 499 Atmospheric and Climate Sciences particles. The model takes into account heating/cooling of the air due to absorp- tion/emission of infrared radiation, as well as due to phase transitions ... See full document

... 6.2 International Education as Self-Formation Theory (IESF) and the findings of this research. 6.2.1 Revisting Self-Formation Theory, Second Language Acquisition (SLA) Theory and int[r] ... See full document

... In this investigation, the SOLA-VOF code was used to simulate the nano-bubble formation. In this code, it was used a variable grid to solve above equations using finite difference method. The geometry is shown ... See full document

... single theory to deal with all forms of the winds of change: social, political, academic, military and economic – those that have created new histories in societies across the globe (Slemon ...postcolonial ... See full document

... We used the near-infrared imaging camera NIRC2 at the Keck II 10 m telescope for all of our observations. Adaptive optics imaging was carried out in natural guide star mode using the narrow camera. Due to the realignment ... See full document

... The formation of the planets around the giant gaseous ball of the Sun began a sorting process: light gases were blown to the far reaches of orbiting debris by solar wind, leaving behind concentrations of heavy ... See full document

... The formation of low-mass stars begins with the fragmentation of a molecular cloud into one or more gravitationally bound cores, internally supported by the contribution of thermal pressure, magnetic fields and ... See full document

... 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 ... See full document

... Both models for the origin of Titan’s methane argue that the ongoing enrichment of deuterium in methane would be far slower once the local temperature fell below 200K, suggesting that the bulk of processing experienced ... See full document

... 4.2 Formation mechanism of inclusions in NiTi alloy The results shown in ...situ observation revealed that the in- clusions form and grow in the residual melt where solutes concentrate during ...the ... See full document

... (i.e. the gas retained by giant planets or lost in winds is negligible). A substantial fraction of the stellar mass that constitutes the IMF is assembled by disc accretion, even at relatively large stellar masses (cf. ... See full document

... gap formation process in laminar viscous disks(Takeuchi et ...size planet may not be able to open a gap(Baruteau et ...giant planet could not open a ... See full document

... the observation in the K band for each KOI for the same reason stated in Section ...PHARO observation: we ensured that the peak fl ux is at least 10,000 ADU for each ... See full document

... massive planet or multiple planets interact with the disk ...massive planet opens a gap, particles stop their inward migration due to the positive pressure gradient at the outer edge of that ...erent ... See full document