Results 1 to 10 of about 2,834 (210)

Solving protoplanetary structure equations using Adomian decomposition method [PDF]

open access: yesHeliyon, 2021
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]

open access: yesHeliyon, 2022
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]

open access: yesNature Communications, 2020
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]

open access: yesHeliyon
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

The Giant Accreting Protoplanet Survey (GAPlanetS)—Results from a 6 yr Campaign to Image Accreting Protoplanets

open access: yesThe Astronomical Journal, 2023
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

open access: yesThe Astronomical Journal, 2023
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

open access: yesThe Astronomical Journal, 2023
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]

open access: yes, 2010
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]

open access: yes, 2010
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

open access: yesJurnal Ilmiah Pendidikan Fisika Al-Biruni, 2016
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

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