Solving protoplanetary structure equations using Adomian decomposition method [PDF]
In this paper, the distribution of thermodynamic variables in the protoplanets formed by gravitational instability in the mass range 0.3−10MJ (1MJ=1 Jupiter mass = 1.8986×1030 gm) is investigated in their initial state by solving the structure equations ...
Gour Chandra Paul +6 more
doaj +2 more sources
An effective method in investigating structures of polytropic protoplanets formed via gravitational instability [PDF]
In this article, we have reinvestigated the initial distribution of thermodynamic variables inside the protoplanets formed via gravitational instability having mass range 0.3−10MJ (1MJ=1.8986×1030 gm) by an embedded RKACeM(4,4) method assuming that the ...
Gour Chandra Paul +2 more
doaj +2 more sources
Formation of bridgmanite-enriched layer at the top lower-mantle during magma ocean solidification [PDF]
Following the impact of the protoplanet Theia, planet Earth likely transformed into a magma ocean. New high temperature and pressure experiments by Xie et al.
Longjian Xie +9 more
doaj +2 more sources
Unveiling protoplanetary structure equations: Semi-analytical solutions via the homotopy analysis method [PDF]
This paper revisits the distribution of thermodynamic variables within initial protoplanets formed via gravitational instability (GI) across a broad mass spectrum ranging from 0.3MJ to 10MJ (where 1MJ denotes 1 Jupiter mass, equal to 1.8986×1030 g ...
Gour Chandra Paul +5 more
doaj +2 more sources
Accreting protoplanets are windows into planet formation processes, and high-contrast differential imaging is an effective way to identify them. We report results from the Giant Accreting Protoplanet Survey (GAPlanetS), which collected H α differential ...
Katherine B. Follette +23 more
doaj +1 more source
UV-optical Emission of AB Aur b Is Consistent with Scattered Stellar Light
The proposed protoplanet AB Aur b is a spatially concentrated emission source imaged in the millimeter-wavelength disk gap of the Herbig Ae/Be star AB Aur. Its near-infrared spectrum and absence of strong polarized light have been interpreted as evidence
Yifan Zhou +14 more
doaj +1 more source
MagAO-X and HST High-contrast Imaging of the AS209 Disk at Hα
The detection of emission lines associated with accretion processes is a direct method for studying how and where gas giant planets form, how young planets interact with their natal protoplanetary disk, and how volatile delivery to their atmosphere takes
Gabriele Cugno +24 more
doaj +1 more source
Prograde rotation of protoplanets by accretion of pebbles in a gaseous environment [PDF]
We perform hydrodynamical simulations of the accretion of pebbles and rocks onto protoplanets of a few hundred kilometres in radius, including two-way drag force coupling between particles and the protoplanetary disc gas.
Adachi +50 more
core +2 more sources
Planet migration: self-gravitating radiation hydrodynamical models of protoplanets with surfaces [PDF]
We calculate radial migration rates of protoplanets in laminar minimum mass solar nebula discs using three-dimensional self-gravitating radiation hydrodynamical (RHD) models.
Alexander +74 more
core +1 more source
Evolution of Stars on The Establishment of The Solar System and Planetary System
This research is the literature studies that provide an introduction to the theory of the formation and early evolution of solar system and planetary systems.
Khilyatul Khoiriyah
doaj +1 more source

